National Library of Energy BETA

Sample records for matters online townhall

  1. Impacts of a Quality Matters™ Workshop on Faculty Who Design, Develop, and Deliver Online Courses: A Mixed Methods Study 

    E-Print Network [OSTI]

    Mercer, Rene E.

    2014-05-30

    Quality Matters™ is recognized world wide as a highly reputable method for quality assurance in online learning. While much research is available regarding Quality Matters as a tool for quality assurance, very little research exists on Quality...

  2. DOEFES_Plasma_Frontiers_Townhall_Vay.pptx

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would like submit theCovalent Bonding Low-Cost2 DOE HQSiteo n n e v i2DOEEA-0984

  3. A new aerosol collector for quasi on-line analysis of particulate organic matter: the Aerosol Collection Module (ACM) and first applications with a GC/MS-FID

    E-Print Network [OSTI]

    Hohaus, T.

    In many environments organic matter significantly contributes to the composition of atmospheric aerosol particles influencing its properties. Detailed chemical characterization of ambient aerosols is critical in order to ...

  4. Optimization Online - Coordinators

    E-Print Network [OSTI]

    Optimization Online Coordinators. Optimization Online submissions are electronically handled by a team of volunteer coordinators: Principal Coordinators.

  5. Online Resources

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefieldSulfateSciTechtail.Theory ofDid you notHeatMaRIEdioxideUser WorkEPVisitingOil & GasAdsorptionOnline

  6. Accessing Online COR Training

    Office of Energy Efficiency and Renewable Energy (EERE)

    Contracting Officer’s Representative (COR) training is now be available in an online format. "Accessing Online COR Training" provides a step-by-step guide to access the online COR course. 

  7. Optimization Online - Digest

    E-Print Network [OSTI]

    Subscribe to the Optimization Online Digest. Complete the form below to subscribe to the free Optimization Online Digest. Every month you will receive an e-mail ...

  8. Credits - Optimization Online

    E-Print Network [OSTI]

    Credits. Development Optimization Online was developed by Jean-Pierre Goux. Optimization Online was conceived by Jean-Pierre Goux, Sanjay Mehrotra, and ...

  9. Optimization Online Links

    E-Print Network [OSTI]

    Optimization Online Links. Optimization related societies. Mathematical Optimization Society · SIAM · INFORMS. Optimization related journals. Mathematical ...

  10. Matter & Energy Robotics Research

    E-Print Network [OSTI]

    Ruina, Andy L.

    Vehicles.com/Mariner Lean Six Sigma Online -- Top Ranked Purdue Now Offers Online Lean Six Sigma Certification www

  11. Dark Matters

    ScienceCinema (OSTI)

    Joseph Silk

    2010-01-08

    One of the greatest mysteries in the cosmos is that it is mostly dark.  Astronomers and particle physicists today are seeking to unravel the nature of this mysterious, but pervasive dark matter which has profoundly influenced the formation of structure in the universe.  I will describe the complex interplay between galaxy formation and dark matter detectability and review recent attempts to measure particle dark matter by direct and indirect means.

  12. Submit - Optimization Online

    E-Print Network [OSTI]

    Optimization Online E-Print Submission. Please enter the number of authors of the article: Visitors, Authors, More about us, Links. Subscribe, Unsubscribe

  13. Update - Optimization Online

    E-Print Network [OSTI]

    Optimization Online E-Print Update. Our secure versioning tool allows you to update your submission by uploading a new version of the report, changing the ...

  14. Policies - Optimization Online

    E-Print Network [OSTI]

    Mission statement. Optimization Online is a repository of eprints about optimization and related topics. It facilitates quick dissemination of new research of ...

  15. DOE Online Learning Center (OLC)

    Broader source: Energy.gov [DOE]

    DOE Online Learning Center offers SkillSoft online courses that can lead to business, desktop and IT professional certifications. The online classes can be accessed 365 days a year from any desktop and are completed at your own pace

  16. Optimization Online Digest -- June 2014

    E-Print Network [OSTI]

    Optimization Online Digest — June 2014. Applications — OR and Management Sciences Robust newsvendor problem with autoregressive demand

  17. Anticipating Patentable Subject Matter

    E-Print Network [OSTI]

    Burk, DL

    2015-01-01

    February 2013] PATENTABLE SUBJECT MATTER patentability—imports into patent law’s subject matter provisions theunder either novelty or subject matter. The proper question

  18. Matter Field, Dark Matter and Dark Energy

    E-Print Network [OSTI]

    Masayasu Tsuge

    2009-03-24

    A model concerning particle theory and cosmology is proposed. Matter field, dark matter and dark energy are created by an energy flow from space to primordial matter fields at the phase transition in the early universe.

  19. An assessment of remote sensing algorithms for colored dissolved organic matter in complex freshwater environments

    E-Print Network [OSTI]

    Yu, Qian

    An assessment of remote sensing algorithms for colored dissolved organic matter in complex October 2013 Accepted 12 October 2013 Available online xxxx Keywords: CDOM Algorithm Freshwater environments Saginaw River Lake Huron This study evaluated fifteen algorithms representing four major

  20. Optimization Online Digest -- May 2015

    E-Print Network [OSTI]

    Optimization Online Digest — May 2015. Applications — OR and Management Sciences Mathematical Models for Multi Container Loading Problems

  1. Optimization Online Digest -- August 2015

    E-Print Network [OSTI]

    Optimization Online Digest — August 2015. Applications — OR and Management Sciences Mixed Integer Second-Order Cone Programming for the Horizontal ...

  2. Optimization Online Digest -- October 2015

    E-Print Network [OSTI]

    Optimization Online Digest — October 2015. Applications — OR and Management Sciences Polynomial SDP Cuts for Optimal Power Flow Hassan Hijazi ...

  3. Optimization Online Digest -- March 2015

    E-Print Network [OSTI]

    Optimization Online Digest — March 2015. Applications — OR and Management Sciences Stochastic versus Robust Optimization for a Transportation Problem

  4. Optimization Online Digest -- September 2015

    E-Print Network [OSTI]

    Optimization Online Digest — September 2015. Applications — OR and Management Sciences An Improved MIP Formulation for the Unit Commitment Problem

  5. Optimization Online Digest -- January 2015

    E-Print Network [OSTI]

    Optimization Online Digest — January 2015. Applications — OR and Management Sciences The Continuous Time Service Network Design Problem Natashia ...

  6. Optimization Online Digest -- September 2014

    E-Print Network [OSTI]

    Optimization Online Digest — September 2014. Applications — OR and Management Sciences Multistage Adaptive Robust Optimization for the Unit ...

  7. Contexts/Motivation Online optimization

    E-Print Network [OSTI]

    Jaillet, Patrick

    with recourse, Markov decision process, stochastic optimal control, etc.) No probabilistic assumptionsContexts/Motivation Online optimization In-depth Cases Online Optimization Patrick Jaillet1 Michael funded by NSF, ONR, AFOSR, and Singapore Online Optimization, Jaillet & Wagner INFORMS, November 8, 2010

  8. Historical Maps Online 

    E-Print Network [OSTI]

    Rumsey, David Y.

    2005-01-31

    ://www.davidrumsey.com/, which currently has over 10,000 high resolution images of maps from his collection. He has also built a suite of tools for users to experience and interpret the maps online. These include GIS, which allows users to combine historical maps with modern...

  9. Matter Wave Radiation Leading to Matter Teleportation

    E-Print Network [OSTI]

    Yong-Yi Huang

    2015-02-12

    The concept of matter wave radiation is put forward, and its equation is established for the first time. The formalism solution shows that the probability density is a function of displacement and time. A free particle and a two-level system are reinvestigated considering the effect of matter wave radiation. Three feasible experimental designs, especially a modified Stern-Gerlach setup, are proposed to verify the existence of matter wave radiation. Matter wave radiation effect in relativity has been formulated in only a raw formulae, which offers another explanation of Lamb shift. A possible mechanics of matter teleportation is predicted due to the effect of matter wave radiation.

  10. Baryonic matter and beyond

    E-Print Network [OSTI]

    Kenji Fukushima

    2014-10-01

    We summarize recent developments in identifying the ground state of dense baryonic matter and beyond. The topics include deconfinement from baryonic matter to quark matter, a diquark mixture, topological effect coupled with chirality and density, and inhomogeneous chiral condensates.

  11. Optimization Online Digest -- January 2009

    E-Print Network [OSTI]

    Applications — Science and Engineering On the Optimal On-Line Management of Photovoltaic-Hydrogen Hybrid Energy Systems Victor Zavala, Mihai Anitescu, ...

  12. Give us feedback - Optimization Online

    E-Print Network [OSTI]

    The Optimization Online Team appreciates your comments and suggestions! Your Name: Your Email: Your Comments: Spam Blocker: What is 4+5? (Answer in ...

  13. Optimization Online Digest -- June 2015

    E-Print Network [OSTI]

    Optimization Online Digest — June 2015. Applications — OR and Management Sciences A data-driven, distribution-free, multivariate approach to the ...

  14. Optimization Online Digest -- February 2014

    E-Print Network [OSTI]

    Optimization Online Digest — February 2014. Applications — OR and Management Sciences Minimum Cost Path Problem for Plug-in Hybrid Electric Vehicles

  15. Hollow nuclear matter

    E-Print Network [OSTI]

    Gao-Chan Yong

    2015-12-18

    It is generally considered that an atomic nucleus is always compact. Based on the isospin-dependent Boltzmann nuclear transport model, here I show that large block nuclear matter or excited nuclear matter may both be hollow. And the size of inner bubble in these matter is affected by the charge number of nuclear matter. Existence of hollow nuclear matter may have many implications in nuclear or atomic physics or astrophysics as well as some practical applications.

  16. Hollow nuclear matter

    E-Print Network [OSTI]

    Yong, Gao-Chan

    2015-01-01

    It is generally considered that an atomic nucleus is always compact. Based on the isospin-dependent Boltzmann nuclear transport model, here I show that large block nuclear matter or excited nuclear matter may both be hollow. And the size of inner bubble in these matter is affected by the charge number of nuclear matter. Existence of hollow nuclear matter may have many implications in nuclear or atomic physics or astrophysics as well as some practical applications.

  17. Online help desk

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 Outreach Home Room NewsInformationJesseworkSURVEY UNIVERSEHowScientificOmbuds OfficeOne VaccineOnline help desk

  18. Online Test Proctoring Request Procedures

    E-Print Network [OSTI]

    Stuart, Steven J.

    Online Test Proctoring Request Procedures #12;Documentation last updated: Friday, January 17, 2014 Page | 2 of 10 Online Test Proctoring Request Form Procedures Contents Test Proctoring Center (TPC............................................................................................................................... 10 #12;Documentation last updated: Friday, January 17, 2014 Page | 3 of 10 Test Proctoring Center

  19. PC Guia Online Pas: Portugal

    E-Print Network [OSTI]

    Instituto de Sistemas e Robotica

    , monitorizados e controlados. O INNOV8 é um jogo de simulação da IBM que junta as tecnologias com os processos de Clínico MSKCC e a IBM utilizam tecnologia Watson para ajudar oncologistas Plataforma de Analítica emprego em tecnologia #12;PC Guia Online País: Portugal Period.: Diária Âmbito: Online Pag.: 2 de 3ID

  20. Asymmetric dark matter

    SciTech Connect (OSTI)

    Kumar, Jason

    2014-06-24

    We review the theoretical framework underlying models of asymmetric dark matter, describe astrophysical constraints which arise from observations of neutron stars, and discuss the prospects for detecting asymmetric dark matter.

  1. Design of programmable matter

    E-Print Network [OSTI]

    Knaian, Ara N. (Ara Nerses), 1977-

    2008-01-01

    Programmable matter is a proposed digital material having computation, sensing, actuation, and display as continuous properties active over its whole extent. Programmable matter would have many exciting applications, like ...

  2. Hot-dark matter, cold dark matter and accelerating universe

    E-Print Network [OSTI]

    Abbas Farmany; Amin Farmany; Mohammad Mahmoodi

    2006-07-07

    The Friedman equation is solved for a universe contains hotdark matter and cold dark matter. In this scenario, hot-dark matter drives an accelerating universe no cold dark matter.

  3. Dynamic Support of Government in Online Shopping

    E-Print Network [OSTI]

    Hai, Le Chi; Alam Kazmi, Syed Hasnain

    2015-01-01

    environment that makes online shopping faster and stable, the government perspective is vital with the Technology

  4. Big Questions: Dark Matter

    SciTech Connect (OSTI)

    Lincoln, Don

    2013-12-05

    Carl Sagan's oft-quoted statement that there are "billions and billions" of stars in the cosmos gives an idea of just how much "stuff" is in the universe. However scientists now think that in addition to the type of matter with which we are familiar, there is another kind of matter out there. This new kind of matter is called "dark matter" and there seems to be five times as much as ordinary matter. Dark matter interacts only with gravity, thus light simply zips right by it. Scientists are searching through their data, trying to prove that the dark matter idea is real. Fermilab's Dr. Don Lincoln tells us why we think this seemingly-crazy idea might not be so crazy after all.

  5. Big Questions: Dark Matter

    ScienceCinema (OSTI)

    Lincoln, Don

    2014-08-07

    Carl Sagan's oft-quoted statement that there are "billions and billions" of stars in the cosmos gives an idea of just how much "stuff" is in the universe. However scientists now think that in addition to the type of matter with which we are familiar, there is another kind of matter out there. This new kind of matter is called "dark matter" and there seems to be five times as much as ordinary matter. Dark matter interacts only with gravity, thus light simply zips right by it. Scientists are searching through their data, trying to prove that the dark matter idea is real. Fermilab's Dr. Don Lincoln tells us why we think this seemingly-crazy idea might not be so crazy after all.

  6. Sec. Chu Online Town Hall

    Office of Energy Efficiency and Renewable Energy (EERE)

    Secretary Steven Chu hosted an online town hall to discuss the clean energy and innovation agenda President Obama laid out in his 2011 State of the Union address. (January 26, 2011)

  7. Groundwater Report Goes Online, Interactive

    Broader source: Energy.gov [DOE]

    RICHLAND, Wash. – EM’s Richland Operations Office (RL) has moved its 1,200-page annual report on groundwater monitoring to a fully online and interactive web application.

  8. Bayesian locally weighted online learning 

    E-Print Network [OSTI]

    Edakunni, Narayanan U.

    2010-01-01

    Locally weighted regression is a non-parametric technique of regression that is capable of coping with non-stationarity of the input distribution. Online algorithms like Receptive FieldWeighted Regression and Locally ...

  9. PC Guia Online Pas: Portugal

    E-Print Network [OSTI]

    Instituto de Sistemas e Robotica

    da Computação e Tecnologias da Informação. "Turbo Parsers: Dependency Parsing by Approximate Hardware Reviews Software Downloads Especial E3 Ofertas de emprego em tecnologia #12;PC Guia Online País as últimas novidades e dicas sobre tecnologia. Apple Google And

  10. Privacy regulation and online advertising

    E-Print Network [OSTI]

    Goldfarb, Avi

    Advertisers use online customer data to target their marketing appeals. This has heightened consumers' privacy concerns, leading governments to pass laws designed to protect consumer privacy by restricting the use of data ...

  11. Buyout prices in online auctions

    E-Print Network [OSTI]

    Gupta, Shobhit

    2006-01-01

    Buyout options allow bidders to instantly purchase at a specified price an item listed for sale through an online auction. A temporary buyout option disappears once a regular bid above the reserve price is made, while a ...

  12. User Experience Research Online Tools

    Broader source: Energy.gov [DOE]

    The Office of Energy Efficiency and Renewable Energy (EERE) has a variety of online tools to help you conduct user experience (UX) research. The following tools are free for use by staff and contractors who work on the EERE website.

  13. Marine Ecological Processes Online section

    E-Print Network [OSTI]

    Hill, Jeffrey E.

    Marine Ecological Processes Online section FAS 6272 (3 credits) Fall 2014 Course Description, behavior, population dynamics, and community structure in marine and estuarine ecosystems. Prerequisite will have: · Examined how ecological processes operate in the marine environment · Compared how ecological

  14. A Model to Evaluate Online Educational Resources in Statistics

    E-Print Network [OSTI]

    Ooms, Ann; Garfield, Joan

    2008-01-01

    Improving Online Educational Resources. ” Doctoral Thesis,Model to Evaluate Online Educational Resources in Statisticsusing online educational resources has steadily increased.

  15. Matter: Space without Time

    E-Print Network [OSTI]

    Yousef Ghazi-Tabatabai

    2012-11-19

    While Quantum Gravity remains elusive and Quantum Field Theory retains the interpretational difficulties of Quantum Mechanics, we have introduced an alternate approach to the unification of particles, fields, space and time, suggesting that the concept of matter as space without time provides a framework which unifies matter with spacetime and in which we anticipate the development of complete theories (ideally a single unified theory) describing observed 'particles, charges, fields and forces' solely with the geometry of our matter-space-time universe.

  16. Cosmology with Mimetic Matter

    SciTech Connect (OSTI)

    Chamseddine, Ali H.; Mukhanov, Viatcheslav; Vikman, Alexander E-mail: viatcheslav.Mukhanov@lmu.de

    2014-06-01

    We consider minimal extensions of the recently proposed Mimetic Dark Matter and show that by introducing a potential for the mimetic non-dynamical scalar field we can mimic nearly any gravitational properties of the normal matter. In particular, the mimetic matter can provide us with inflaton, quintessence and even can lead to a bouncing nonsingular universe. We also investigate the behaviour of cosmological perturbations due to a mimetic matter. We demonstrate that simple mimetic inflation can produce red-tilted scalar perturbations which are largely enhanced over gravity waves.

  17. Energy Matters Mailbag

    Broader source: Energy.gov [DOE]

    This edition of the mailbag tackles follow-up questions from our Energy Matters discussion on breaking our reliance on foreign oil.

  18. Dipolar Dark Matter

    E-Print Network [OSTI]

    Luc Blanchet; Lavinia Heisenberg

    2015-05-19

    Massive gravity theories have been developed as viable IR modifications of gravity motivated by dark energy and the problem of the cosmological constant. On the other hand, modified gravity and modified dark matter theories were developed with the aim of solving the problems of standard cold dark matter at galactic scales. Here we propose to adapt the framework of ghost-free massive bigravity theories to reformulate the problem of dark matter at galactic scales. We investigate a promising alternative to dark matter called dipolar dark matter (DDM) in which two different species of dark matter are separately coupled to the two metrics of bigravity and are linked together by an internal vector field. We show that this model successfully reproduces the phenomenology of dark matter at galactic scales (i.e. MOND) as a result of a mechanism of gravitational polarisation. The model is safe in the gravitational sector, but because the two types of dark matter interact through the vector field, a ghostly degree of freedom in the decoupling limit is reintroduced in the dark matter sector. Crucial questions to address in future work is whether the polarisation mechanism can be realized in absence of ghosts, and what are the cosmological implications of the model.

  19. Energy and matter

    E-Print Network [OSTI]

    Gobato, Ricardo; Fedrigo, Desire Francine Gobato

    2015-01-01

    Our work is an approach between matter and energy. Using the famous equation E = mc^2, Einstein and the Law of Universal Gravitation of Newton, we estimate that a small amount matter converted into energy is needed to lift, using the gravitational potential energy equation on the surface, a mountain of solid iron or even Mount Everest.

  20. PUBLISHED ONLINE: 11 AUGUST 2013 | DOI: 10.1038/NPHYS2715 Molecular motors robustly drive active gels to a

    E-Print Network [OSTI]

    Loss, Daniel

    ARTICLES PUBLISHED ONLINE: 11 AUGUST 2013 | DOI: 10.1038/NPHYS2715 Molecular motors robustly drive a fascinating class of internally driven matter, in which molecular motors exert localized stresses inside polymer networks. There is evidence that network crosslinking is required to allow motors to induce

  1. Therapist and Adolescent Behavior in Online Therapy 

    E-Print Network [OSTI]

    Cepeda, Lisa Marie

    2009-05-15

    and repeated opportunities (anticipate future communications) to exchange information and build relationships. To examine the extent to which the process of online therapy resembles face-to-face therapy, online therapy transcripts were examined through a...

  2. Online Energy Generation Scheduling for Microgrids with

    E-Print Network [OSTI]

    Zhang, Junshan

    Online Energy Generation Scheduling for Microgrids with Intermittent Energy Sources and Co entitled: Online Energy Generation Scheduling for Microgrids with Intermittent Energy Sources and Co schedul- ing. However, accurate prediction cannot be guaranteed due to the small scale of microgrids

  3. Photovoltaic Online Training Course for Code Officials

    Broader source: Energy.gov [DOE]

    The Photovoltaic Online Training Course for Code Officials is a free online training tool for those officials who conduct reviews and inspections of residential PV systems. Throughout the course's...

  4. Policy -Online Business Management Certificate Program

    E-Print Network [OSTI]

    Hanson, Stephen José

    Advisor-Instructor's assignments. Refund Policy (for Online Certificate program only - Lean Six Sigma programs. Grievance Policy If you are a participant in our Online Certificate Program or Lean/Six Sigma

  5. Dark matter searches

    E-Print Network [OSTI]

    Baudis, Laura

    2015-01-01

    One of the major challenges of modern physics is to decipher the nature of dark matter. Astrophysical observations provide ample evidence for the existence of an invisible and dominant mass component in the observable universe, from the scales of galaxies up to the largest cosmological scales. The dark matter could be made of new, yet undiscovered elementary particles, with allowed masses and interaction strengths with normal matter spanning an enormous range. Axions, produced non-thermally in the early universe, and weakly interacting massive particles (WIMPs), which froze out of thermal equilibrium with a relic density matching the observations, represent two well-motivated, generic classes of dark matter candidates. Dark matter axions could be detected by exploiting their predicted coupling to two photons, where the highest sensitivity is reached by experiments using a microwave cavity permeated by a strong magnetic field. WIMPs could be directly observed via scatters off atomic nuclei in underground, ultr...

  6. Dark matter axions

    E-Print Network [OSTI]

    P. Sikivie

    2009-09-04

    The hypothesis of an `invisible' axion was made by Misha Shifman and others, approximately thirty years ago. It has turned out to be an unusually fruitful idea, crossing boundaries between particle physics, astrophysics and cosmology. An axion with mass of order $10^{-5}$ eV (with large uncertainties) is one of the leading candidates for the dark matter of the universe. It was found recently that dark matter axions thermalize and form a Bose-Einstein condensate (BEC). Because they form a BEC, axions differ from ordinary cold dark matter (CDM) in the non-linear regime of structure formation and upon entering the horizon. Axion BEC provides a mechanism for the production of net overall rotation in dark matter halos, and for the alignment of cosmic microwave anisotropy multipoles. Because there is evidence for these phenomena, unexplained with ordinary CDM, an argument can be made that the dark matter is axions.

  7. Dissipation of dark matter

    E-Print Network [OSTI]

    Hermano Velten; Dominik J. Schwarz

    2012-10-01

    Fluids often display dissipative properties. We explore dissipation in the form of bulk viscosity in the cold dark matter fluid. We constrain this model using current data from supernovae, baryon acoustic oscillations and the cosmic microwave background. Considering the isotropic and homogeneous background only, viscous dark matter is allowed to have a bulk viscosity $\\lesssim 10^7$ Pa$\\cdot$s, also consistent with the expected integrated Sachs-Wolfe effect (which plagues some models with bulk viscosity). We further investigate the small-scale formation of viscous dark matter halos, which turns out to place significantly stronger constraints on the dark matter viscosity. The existence of dwarf galaxies is guaranteed only for much smaller values of the dark matter viscosity, $\\lesssim 10^{-3}$ Pa$\\cdot$s.

  8. Dynamic Support of Government in Online Shopping

    E-Print Network [OSTI]

    Hai, Le Chi; Alam Kazmi, Syed Hasnain

    2015-01-01

    predict the impact of the behavior, its context and socialusefulness impact on online www.ccsenet.org/ass Asian Social

  9. Online Master of Science in Applied Psychology

    E-Print Network [OSTI]

    Zhou, Xianghong Jasmine

    Online Master of Science in Applied Psychology #12;Online Master of Science in Applied Psychology of psychology to today's changing business environment. On behalf of the University of Southern California, I Psychology online program. Here at USC, we recognize the importance of applying psychology in many areas

  10. Canal Superior Online Pas: Portugal

    E-Print Network [OSTI]

    Instituto de Sistemas e Robotica

    -se a promotores que já tenham constituído a empresa ou que pretendam avançar com um negócio na área da energia NOTÍCIAS PROGRAMASDEINFORMAÇÃO REPORTAGEM ÚLTIMAS 1,5 MILHÕES DE EUROS PARA PROJETOS NA ÁREA DA ENERGIA Online 1,5 MILHÕES DE EUROS PARA PROJETOS NA ÁREA DA ENERGIA A Fundação Repsol lança uma nova edição do

  11. Free Energy Code Online Discussion

    E-Print Network [OSTI]

    Free Energy Code Online Discussion for Building Department Personnel Join us for this FREE 90 Bruce Cheney from Anchors Aweigh Energy, LLC want to hear from YOU on residential HVAC changeout issues of the California Energy Commission. Date: 3 dates currently offered, choose the one that works for you

  12. Online Search Aids Petroleum Abstracts

    E-Print Network [OSTI]

    Reynolds, Albert C.

    to enter the words for the query. The center frame will display the list of terms resulting from the queryOnline Search Aids User Guide Petroleum Abstracts® A Division of The University of Tulsa July 1. A compilation of relevant E&P technical index terms and their relationships, covering the areas of geology

  13. PC Guia Online Pas: Portugal

    E-Print Network [OSTI]

    Instituto de Sistemas e Robotica

    Satélites, Jogos e Tecnologias no IST Taguspark Instituto Superior Técnico promove Career Sessions Autor Reviews Software Assinaturas Downloads Ofertas de emprego em tecnologia #12;PC Guia Online País: Portugal as últimas novidades e dicas sobre tecnologia. Apple Google Android Microsoft Samsung Facebook Asus iPad Sony

  14. Marine Ecological Processes Online section

    E-Print Network [OSTI]

    Hill, Jeffrey E.

    Marine Ecological Processes Online section FAS 4270 (3 credits) Fall 2012 Course Description The course covers the ecology of marine organisms and habitats with focus on how general ecological principles and those unique to the marine environment drive patterns and processes. Prerequisite: Two

  15. Relativistic Laser-Matter Interactions

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Relativistic Laser-Matter Interactions Relativistic Laser-Matter Interactions Enabling the next generation of intense particle accelerators Contact Juan Fernandez (505) 667-6575...

  16. Axion BEC Dark Matter

    E-Print Network [OSTI]

    Erken, Ozgur; Tam, Heywood; Yang, Qiaoli

    2011-01-01

    Cold dark matter axions thermalize through gravitational self-interactions and form a Bose-Einstein condensate when the photon temperature reaches approximately 500 eV. Axion Bose-Einstein condensation provides an opportunity to distinguish axions from the other dark matter candidates on the basis of observation. The rethermalization of axions that are about to fall in a galactic potential well causes them to acquire net overall rotation, whereas ordinary cold dark matter falls in with an irrotational velocity field. The inner caustics of galactic halos are different in the two cases.

  17. Axion BEC Dark Matter

    E-Print Network [OSTI]

    Ozgur Erken; Pierre Sikivie; Heywood Tam; Qiaoli Yang

    2011-11-16

    Cold dark matter axions thermalize through gravitational self-interactions and form a Bose-Einstein condensate when the photon temperature reaches approximately 500 eV. Axion Bose-Einstein condensation provides an opportunity to distinguish axions from the other dark matter candidates on the basis of observation. The rethermalization of axions that are about to fall in a galactic potential well causes them to acquire net overall rotation, whereas ordinary cold dark matter falls in with an irrotational velocity field. The inner caustics of galactic halos are different in the two cases.

  18. Dark Matter 2014

    E-Print Network [OSTI]

    Marc Schumann

    2015-01-06

    This article gives an overview on the status of experimental searches for dark matter at the end of 2014. The main focus is on direct searches for weakly interacting massive particles (WIMPs) using underground-based low-background detectors, especially on the new results published in 2014. WIMPs are excellent dark matter candidates, predicted by many theories beyond the standard model of particle physics, and are expected to interact with the target nuclei either via spin-independent (scalar) or spin-dependent (axial-vector) couplings. Non-WIMP dark matter candidates, especially axions and axion-like particles are also briefly discussed.

  19. Matter & Energy Civil Engineering

    E-Print Network [OSTI]

    Rogers, John A.

    See Also: Matter & Energy Detectors· Optics· Civil Engineering· Engineering· Nature of Water Yonggang Huang, Joseph Cummings Professor of Civil and Environmental Engineering and Mechanical Engineering· Electronics· Reference Photography· Infrared· Mechanical engineering · Optics· ScienceDaily (Jan. 17, 2011

  20. Gaseous dark matter detectors

    E-Print Network [OSTI]

    Martoff, C. J.

    Dark matter (DM) detectors with directional sensitivity have the potential of yielding an unambiguous positive observation of WIMPs as well as discriminating between galactic DM halo models. In this paper, we introduce the ...

  1. Matter & Energy Electronics

    E-Print Network [OSTI]

    Suslick, Kenneth S.

    See also: Matter & Energy Detectors· Electronics· Technology· Medical Technology· Weapons Technology · Organic Chemistry· Reference Hydrogen chloride· Photography· Catalytic converter· Nanomedicine a series of tiny colored dots ­ each a different pigment ­ on an inert backing such as paper, plastic

  2. The Heart of Matter

    E-Print Network [OSTI]

    Rohini M. Godbole

    2010-06-30

    In this article I trace the development of the human understanding of the "Heart of Matter" from early concepts of "elements" (or alternatively "Panchmahabhootas") to the current status of "quarks" and "leptons" as the fundamental constituents of matter, interacting together via exchange of the various force carrier particles called "gauge bosons" such as the photon, W/Z-boson etc. I would like to show how our understanding of the fundamental constituents of matter has gone hand in hand with our understanding of the fundamental forces in nature. I will also outline how the knowledge of particle physics at the "micro" scale of less than a Fermi(one millionth of a nanometer), enables us to offer explanations of Cosmological observations at the "macro" scale. Consequently these observations, may in turn, help us address some very fundamental questions of the Physics at the "Heart of the Matter".

  3. Hot and dark matter

    E-Print Network [OSTI]

    D'Eramo, Francesco

    2012-01-01

    In this thesis, we build new Effective Field Theory tools to describe the propagation of energetic partons in hot and dense media, and we propose two new reactions for dark matter in the early universe. In the first part, ...

  4. Dark matter searches

    E-Print Network [OSTI]

    Laura Baudis

    2015-09-02

    One of the major challenges of modern physics is to decipher the nature of dark matter. Astrophysical observations provide ample evidence for the existence of an invisible and dominant mass component in the observable universe, from the scales of galaxies up to the largest cosmological scales. The dark matter could be made of new, yet undiscovered elementary particles, with allowed masses and interaction strengths with normal matter spanning an enormous range. Axions, produced non-thermally in the early universe, and weakly interacting massive particles (WIMPs), which froze out of thermal equilibrium with a relic density matching the observations, represent two well-motivated, generic classes of dark matter candidates. Dark matter axions could be detected by exploiting their predicted coupling to two photons, where the highest sensitivity is reached by experiments using a microwave cavity permeated by a strong magnetic field. WIMPs could be directly observed via scatters off atomic nuclei in underground, ultra low-background detectors, or indirectly, via secondary radiation produced when they pair annihilate. They could also be generated at particle colliders such as the LHC, where associated particles produced in the same process are to be detected. After a brief motivation and an introduction to the phenomenology of particle dark matter detection, I will discuss the most promising experimental techniques to search for axions and WIMPs, addressing their current and future science reach, as well as their complementarity.

  5. Single-Pass Online Learning: Performance, Voting Schemes and Online Feature Selection

    E-Print Network [OSTI]

    Cohen, William W.

    of averaging, a.k.a. vot- ing, on online learning. Finally, we describe how the new Modified Margin Balanced and achieves results comparable to Linear SVM in several NLP tasks. Voting (a.k.a. averaging) an online

  6. Axion Dark Matter Searches

    E-Print Network [OSTI]

    I. Stern

    2014-03-21

    Nearly all astrophysical and cosmological data point convincingly to a large component of cold dark matter in the Universe. The axion particle, first theorized as a solution to the strong charge-parity problem of quantum chromodynamics, has been established as a prominent CDM candidate. Cosmic observation and particle physics experiments have bracketed the unknown mass of the axion between approximately a $\\mu$eV and a meV. The Axion Dark Matter eXperiement (ADMX) has successfully completed searches between 1.9 and 3.7 $\\mu$eV down to the KSVZ photon-coupling limit. ADMX and the Axion Dark Matter eXperiement High-Frequency (ADMX-HF) will search for axions at weaker coupling and/or higher frequencies within the next few years. Status of the experiments, current research and development, and projected mass-coupling exclusion limits are presented.

  7. Axion Dark Matter Searches

    E-Print Network [OSTI]

    Stern, I

    2014-01-01

    Nearly all astrophysical and cosmological data point convincingly to a large component of cold dark matter in the Universe. The axion particle, first theorized as a solution to the strong charge-parity problem of quantum chromodynamics, has been established as a prominent CDM candidate. Cosmic observation and particle physics experiments have bracketed the unknown mass of the axion between approximately a $\\mu$eV and a meV. The Axion Dark Matter eXperiement (ADMX) has successfully completed searches between 1.9 and 3.7 $\\mu$eV down to the KSVZ photon-coupling limit. ADMX and the Axion Dark Matter eXperiement High-Frequency (ADMX-HF) will search for axions at weaker coupling and/or higher frequencies within the next few years. Status of the experiments, current research and development, and projected mass-coupling exclusion limits are presented.

  8. Thermodynamics of clusterized matter

    E-Print Network [OSTI]

    Ad. R. Raduta; F. Gulminelli

    2009-08-26

    Thermodynamics of clusterized matter is studied in the framework of statistical models with non-interacting cluster degrees of freedom. At variance with the analytical Fisher model, exact Metropolis simulation results indicate that the transition from homogeneous to clusterized matter lies along the $\\rho=\\rho_0$ axis at all temperatures and the limiting point of the phase diagram is not a critical point even if the surface energy vanishes at this point. Sensitivity of the inferred phase diagram to the employed statistical framework in the case of finite systems is discussed by considering the grand-canonical and constant-pressure canonical ensembles. A Wigner-Seitz formalism in which the fragment charge is neutralized by an uniform electron distribution allows to build the phase diagram of neutron star matter.

  9. Natural minimal dark matter

    E-Print Network [OSTI]

    Fabbrichesi, Marco

    2015-01-01

    We show how the Higgs boson mass is protected from the potentially large corrections due to the introduction of minimal dark matter if the new physics sector is made supersymmetric. The fermionic dark matter candidate (a 5-plet of $SU(2)_L$) is accompanied by a scalar state. The weak gauge sector is made supersymmetric and the Higgs boson is embedded in a supersymmetric multiplet. The remaining standard model states are non-supersymmetric. Non vanishing corrections to the Higgs boson mass only appear at three-loop level and the model is natural for dark matter masses up to 15 TeV--a value larger than the one required by the cosmological relic density. The construction presented stands as an example of a general approach to naturalness that solves the little hierarchy problem which arises when new physics is added beyond the standard model at an energy scale around 10 TeV.

  10. Axion Dark Matter Searches

    E-Print Network [OSTI]

    I. Stern

    2015-11-17

    Nearly all astrophysical and cosmological data point convincingly to a large component of cold dark matter in the Universe. The axion particle, first theorized as a solution to the strong charge-parity problem of quantum chromodynamics, has been established as a prominent CDM candidate. Cosmic observation and particle physics experiments have bracketed the unknown mass of the axion between approximately a $\\mu$eV and a meV. The Axion Dark Matter eXperiement (ADMX) has successfully completed searches between 1.9 and 3.7 $\\mu$eV down to the KSVZ photon-coupling limit. ADMX and the Axion Dark Matter eXperiement High-Frequency (ADMX-HF) will search for axions at weaker coupling and/or higher frequencies within the next few years. Status of the experiments, current research and development, and projected mass-coupling exclusion limits are presented.

  11. Cold nuclear matter

    E-Print Network [OSTI]

    C. O. Dorso; P. A. Giménez Molinelli; J. I. Nichols; J. A. López

    2013-05-09

    The behavior of nuclear matter is studied at low densities and temperatures using classical molecular dynamics with three different sets of potentials with different compressibility. Nuclear matter is found to arrange in crystalline structures around the saturation density and in non-homogeneous (i.e. pasta-like) structures at lower densities. Similar results were obtained with a simple Lennard-Jones potential. Finite size effects are analysed and the existence of the non-homogeneous structures is shown to be inherent to the use of periodic boundary conditions and the finitude of the system. For large enough systems the non-homogeneous structures are limited to one sphere, one rod or one slab per simulation cell, which are shown to be minimal surface structures under cubic periodic boundary conditions at the corresponding volume fraction. The relevance of these findings to the simulations of neutron star and supernovae matter is discussed.

  12. Asymptotically Safe Dark Matter

    E-Print Network [OSTI]

    Francesco Sannino; Ian M. Shoemaker

    2015-08-05

    We introduce a new paradigm for dark matter (DM) interactions in which the interaction strength is asymptotically safe. In models of this type, the coupling strength is small at low energies but increases at higher energies, and asymptotically approaches a finite constant value. The resulting phenomenology of this "asymptotically safe DM" is quite distinct. One interesting effect of this is to partially offset the low-energy constraints from direct detection experiments without affecting thermal freeze-out processes which occur at higher energies. High-energy collider and indirect annihilation searches are the primary ways to constrain or discover asymptotically safe dark matter.

  13. Safe Dark Matter

    E-Print Network [OSTI]

    Francesco Sannino; Ian M. Shoemaker

    2015-07-29

    We introduce a new paradigm for dark matter (DM) interactions in which the interaction strength is asymptotically safe. In models of this type, the coupling strength is small at low energies but increases at higher energies, and asymptotically approaches a finite constant value. The resulting phenomenology of this "safe DM" is quite distinct. One interesting effect of this is to partially offset the low-energy constraints from direct detection experiments without affecting thermal freeze-out processes which occur at higher energies. High-energy collider and indirect annihilation searches are the primary ways to constrain or discover safe dark matter.

  14. Optimization Online - All Areas Submissions - January 2009

    E-Print Network [OSTI]

    Hybrid MPI/OpenMP parallel support vector machine training ... On the Optimal On-Line Management of Photovoltaic-Hydrogen Hybrid Energy Systems

  15. Optimization Online - Enter Your Password to Continue

    E-Print Network [OSTI]

    On the Optimal On-Line Management of Photovoltaic-Hydrogen Hybrid Energy Systems. Enter the Article Password: If you forgot your password, select your ...

  16. Optimization Online - Search or Browse Submissions

    E-Print Network [OSTI]

    Search or Browse Optimization Online Submissions. Google Search. Enter your search terms: name of author(s), title, keywords, journal, etc. The Web

  17. Dynamic Support of Government in Online Shopping

    E-Print Network [OSTI]

    Hai, Le Chi; Alam Kazmi, Syed Hasnain

    2015-01-01

    also say that the use of new technology to complete theirperceived usefulness of new technologies affect individualinfrastructure, leading to new technologies such as online

  18. Statistics Online Computational Resource for Education

    E-Print Network [OSTI]

    Dinov, Ivo D; Christou, Nicolas

    2009-01-01

    and assess- ment of the statistic online computationalintroductory probability and statistics courses. Computers &Leslie, M. (2003). Statistics starter kit. Science, © 2009

  19. Optimal Online Learning with Matrix Parameters

    E-Print Network [OSTI]

    Nie, Jiazhong

    2015-01-01

    Learning Problem: the Expert Setting 1.2 Learning Matrixwith Dense Instance Matrices . . . . . . . . .Optimal Online Learning with Matrix Parameters by Jiazhong

  20. Social Features of Online Networks: The Strength of Intermediary Ties in Online Social Media

    E-Print Network [OSTI]

    Moro, Esteban

    as communication channels. Recent worldwide events, such as social movements in Spain or revolts in the Middle EastSocial Features of Online Networks: The Strength of Intermediary Ties in Online Social Media Abstract An increasing fraction of today's social interactions occur using online social media

  1. Ethan Burns (UNH) Anticipatory On-line Planning 1 / 22 Anticipatory On-line Planning

    E-Print Network [OSTI]

    Ruml, Wheeler

    Ethan Burns (UNH) Anticipatory On-line Planning ­ 1 / 22 Anticipatory On-line Planning Ethan Burns1 Formalization Hindsight Opt. Experiments Conclusion Ethan Burns (UNH) Anticipatory On-line Planning ­ 2 / 22'd s Contributions Formalization Hindsight Opt. Experiments Conclusion Ethan Burns (UNH) Anticipatory On

  2. Quantum Condensed Matter | Neutron Science | ORNL

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Quantum Condensed Matter SHARE Quantum Condensed Matter Neutron scattering is a uniquely powerful probe for measuring the structure and dynamics of condensed matter. As such it is...

  3. Quantum Condensed Matter | More Science | ORNL

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Quantum Condensed Matter SHARE Quantum Condensed Matter Neutron scattering is a uniquely powerful probe for measuring the structure and dynamics of condensed matter. As such it is...

  4. Investigation of Direct Injection Vehicle Particulate Matter...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Direct Injection Vehicle Particulate Matter Emissions Investigation of Direct Injection Vehicle Particulate Matter Emissions This study focuses primarily on particulate matter mass...

  5. Asymmetric condensed dark matter

    E-Print Network [OSTI]

    Aguirre, Anthony

    2015-01-01

    We explore the viability of a boson dark matter candidate with an asymmetry between the number densities of particles and antiparticles. A simple thermal field theory analysis confirms that, under certain general conditions, this component would develop a Bose-Einstein condensate in the early universe that, for appropriate model parameters, could survive the ensuing cosmological evolution until now. The condensation of a dark matter component in equilibrium with the thermal plasma is a relativistic process, hence the amount of matter dictated by the charge asymmetry is complemented by a hot relic density frozen out at the time of decoupling. Contrary to the case of ordinary WIMPs, dark matter particles in a condensate can be very light, $10^{-22}\\,{\\rm eV} \\lesssim m \\lesssim 10^2\\,{\\rm eV}$; the lower limit arises from constraints on small-scale structure formation, while the upper bound ensures that the density from thermal relics is not too large. Big-Bang nucleosynthesis constrains the temperature of deco...

  6. Tunguska Dark Matter Ball

    E-Print Network [OSTI]

    C. D. Froggatt; H. B. Nielsen

    2015-05-10

    It is suggested that the Tunguska event in June 1908 cm-large was due to a cm-large ball of a condensate of bound states of 6 top and 6 anti-top quarks containing highly compressed ordinary matter. Such balls are supposed to make up the dark matter as we earlier proposed. The expected rate of impact of this kind of dark matter ball with the earth seems to crudely match a time scale of 200 years between the impacts. The main explosion of the Tunguska event is explained in our picture as material coming out from deep within the earth, where it has been heated and compressed by the ball penetrating to a depth of several thousand km. Thus the effect has some similarity with volcanic activity as suggested by Kundt. We discuss the possible identification of kimberlite pipes with earlier Tunguska-like events. A discussion of how the dark matter balls may have formed in the early universe is also given.

  7. Energy Matters - Spring 2002

    SciTech Connect (OSTI)

    2002-03-01

    Quarterly newsletter from DOE's Industrial Technologies Program to promote the use of energy-efficient industrial systems. The focus of the Spring 2002 Issue of Energy Matters focuses on premium energy efficiency systems, with articles on new gas technologies, steam efficiency, the Augusta Newsprint Showcase, and more.

  8. Energy Matters - Fall 2002

    SciTech Connect (OSTI)

    2002-09-01

    Quarterly newsletter from DOE's Industrial Technologies Program to promote the use of energy-efficient industrial systems. This issue focus of this edition of the Energy Matters Newsletter is on energy and environmental issues. Read more about compressed air's role in productivity, making good motor decisions, and more.

  9. Subject Matters Introduction

    E-Print Network [OSTI]

    Subject Matters Introduction The AS and A Level subject choices you make when in Year 11 (or assessing applicants at the University of Cambridge, we consider not only the individual A Level subjects taken but also the combination of these. We generally prefer applicants to have taken certain subjects

  10. Matter & Energy Solar Energy

    E-Print Network [OSTI]

    Rogers, John A.

    See Also: Matter & Energy Solar Energy· Electronics· Materials Science· Earth & Climate Energy at the University of Illinois, the future of solar energy just got brighter. Although silicon is the industry Electronics Over 1.2 Million Electronics Parts, Components and Equipment. www.AlliedElec.com solar energy

  11. Dark Matter Searches

    E-Print Network [OSTI]

    Laura Baudis

    2005-11-29

    More than 90% of matter in the Universe could be composed of heavy particles, which were non-relativistic, or 'cold', when they froze-out from the primordial soup. I will review current searches for these hypothetical particles, both via interactions with nuclei in deep underground detectors, and via the observation of their annihilation products in the Sun, galactic halo and galactic center.

  12. Anatomy of the visual word form area: Adjacent cortical circuits and long-range white matter connections

    E-Print Network [OSTI]

    Wandell, Brian A.

    Anatomy of the visual word form area: Adjacent cortical circuits and long-range white matter, United States a r t i c l e i n f o Article history: Available online xxxx Keywords: Visual word form t Circuitry in ventral occipital-temporal cortex is essential for seeing words. We analyze the circuitry

  13. Energy Matters in Washington State Page 1 Energy Matters

    E-Print Network [OSTI]

    Collins, Gary S.

    Energy Matters in Washington State ­ Page 1 Energy Matters in Washington State June 2008 Updated November 2009 Updated and Revised October 2013 Grand Coulee Dam #12;Energy Matters in Washington State ­ Page 2 Copyright © 2013 Washington State University Energy Program. 905 Plum Street SE, P.O. Box 43169

  14. The Search for Dark Matter

    SciTech Connect (OSTI)

    Orrell, John

    2013-11-20

    More than 25 years ago, PNNL scientists began the first underground measurements searching for dark matter using specialized radiation detector technology. Dark matter is yet to be discovered says Physicist John L. Orrell.

  15. The Search for Dark Matter

    ScienceCinema (OSTI)

    Orrell, John

    2014-07-24

    More than 25 years ago, PNNL scientists began the first underground measurements searching for dark matter using specialized radiation detector technology. Dark matter is yet to be discovered says Physicist John L. Orrell.

  16. Photovoltaic Online Training Course for Code Officials

    Broader source: Energy.gov [DOE]

    The Photovoltaic Online Training Course for Code Officials is a free online training tool for those officials who conduct reviews and inspections of residential PV systems. Throughout the course's 7 page-turner lessons and 3D interactive Capstone lesson, major topics of concern for field inspection and expedited permitting are covered.

  17. STATISTICS FOR GRADUATE STUDENTS ONLINE RESOURCES

    E-Print Network [OSTI]

    Fletcher, Robin

    1 STATISTICS FOR GRADUATE STUDENTS ONLINE RESOURCES Introduction to Data Analysis Exploring Data Pitfalls of Data Analysis (or How to Avoid Lies and Damned Lies) Statistics notes and related articles published in British Medical Journal Statistical literacy HyperStat Online Statistics Textbook Electronic

  18. Online Effects of Offline Ads Diane Lambert

    E-Print Network [OSTI]

    Cortes, Corinna

    Online Effects of Offline Ads Diane Lambert Google, Inc. 76 Ninth Ave New York, NY 10011 dlambert a methodology for assessing how ad campaigns in offline media such as print, audio and TV affect online in ad appeared suggests heightened interest in the advertised product, as long as there would have been

  19. Competition and Fraud in Online Advertising Markets

    E-Print Network [OSTI]

    Cortes, Corinna

    Competition and Fraud in Online Advertising Markets Bob Mungamuru1 and Stephen Weis2 1 Stanford of the online advertising market is presented, fo- cusing on the effect of ad fraud. In the model, the market is comprised of three classes of players: publishers, advertising networks, and advertisers. The central

  20. Online Deadline Scheduling with Bounded Energy Efficiency

    E-Print Network [OSTI]

    Wong, Prudence W.H.

    Online Deadline Scheduling with Bounded Energy Efficiency Joseph Wun-Tat Chan1 , Tak-Wah Lam 2 concern when compared to throughput and the schedules targeted may be very poor in energy efficiency subject to a user-defined threshold of energy efficiency. We first show that all deterministic online

  1. Corporate Training On-Site Online Global

    E-Print Network [OSTI]

    Barrett, Jeffrey A.

    MAKE THE RIGHT MOVE Corporate Training On-Site · Online · Global IMPROVE YOUR COMPETITIVE ADVANTAGE WITH WORLD-CLASS ON-SITE AND ONLINE SOLUTIONS TAILORED TO MEET YOUR BUSINESS AND EMPLOYEE TRAINING NEEDS a competitive advantage depends on how well your staff executes. UCIrvineExtension's Corporate Training helps

  2. Online optimization of storage ring nonlinear beam dynamics ...

    Office of Scientific and Technical Information (OSTI)

    Online optimization of storage ring nonlinear beam dynamics Citation Details In-Document Search Title: Online optimization of storage ring nonlinear beam dynamics Authors: Huang,...

  3. Online optimization of storage ring nonlinear beam dynamics ...

    Office of Scientific and Technical Information (OSTI)

    Online optimization of storage ring nonlinear beam dynamics Citation Details In-Document Search Title: Online optimization of storage ring nonlinear beam dynamics You are...

  4. Ground Rules for MA 30300 Summer 2015 (Online class) Instructor ...

    E-Print Network [OSTI]

    2015-05-05

    Ground Rules for MA 30300 Summer 2015 (Online class). Instructor: Prof. Veronica Quitalo (vquitalo@purdue.edu). Online lectures: Recorded/livestream ...

  5. New Online Tools Showcase Efficient Technologies and Deployment...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    New Online Tools Showcase Efficient Technologies and Deployment Case Studies New Online Tools Showcase Efficient Technologies and Deployment Case Studies September 29, 2015 -...

  6. DOE Jobs Online (Hiring Manager), Office of Human Capitol Management...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Jobs Online (Hiring Manager), Office of Human Capitol Management Innovation and Solutions DOE Jobs Online (Hiring Manager), Office of Human Capitol Management Innovation and...

  7. FACTSHEET: Energy Department Launches Open-Source Online Training...

    Energy Savers [EERE]

    FACTSHEET: Energy Department Launches Open-Source Online Training Resource to Help Students, Workers Gain Valuable Skills FACTSHEET: Energy Department Launches Open-Source Online...

  8. NERSC Online Training May 3: Navigating NERSC File Systems

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Online Training May 3: Navigating NERSC File Systems NERSC Online Training May 3: Navigating NERSC File Systems April 26, 2011 by Richard Gerber A NERSC training event, "Navigating...

  9. Levitating Dark Matter

    E-Print Network [OSTI]

    Nemanja Kaloper; Antonio Padilla

    2009-10-07

    A sizable fraction of the total energy density of the universe may be in heavy particles with a net dark $U(1)'$ charge comparable to its mass. When the charges have the same sign the cancellation between their gravitational and gauge forces may lead to a mismatch between different measures of masses in the universe. Measuring galactic masses by orbits of normal matter, such as galaxy rotation curves or lensing, will give the total mass, while the flows of dark matter agglomerates may yield smaller values if the gauge repulsion is not accounted for. If distant galaxies which house light beacons like SNe Ia contain such dark particles, the observations of their cosmic recession may mistake the weaker forces for an extra `antigravity', and infer an effective dark energy equation of state smaller than the real one. In some cases, including that of a cosmological constant, these effects can mimic $wdark energy, or superhorizon effects.

  10. Rigid particulate matter sensor

    DOE Patents [OSTI]

    Hall, Matthew (Austin, TX)

    2011-02-22

    A sensor to detect particulate matter. The sensor includes a first rigid tube, a second rigid tube, a detection surface electrode, and a bias surface electrode. The second rigid tube is mounted substantially parallel to the first rigid tube. The detection surface electrode is disposed on an outer surface of the first rigid tube. The detection surface electrode is disposed to face the second rigid tube. The bias surface electrode is disposed on an outer surface of the second rigid tube. The bias surface electrode is disposed to face the detection surface electrode on the first rigid tube. An air gap exists between the detection surface electrode and the bias surface electrode to allow particulate matter within an exhaust stream to flow between the detection and bias surface electrodes.

  11. Self-Interacting Dark Matter

    E-Print Network [OSTI]

    Benjamin D. Wandelt; Romeel Dave; Glennys R. Farrar; Patrick C. McGuire; David N. Spergel; Paul J. Steinhardt

    2000-06-28

    Spergel and Steinhardt have recently proposed the concept of dark matter with strong self-interactions as a means to address numerous discrepancies between observations of dark matter halos on subgalactic scales and the predictions of the standard collisionless dark matter picture. We review the motivations for this scenario and discuss some recent, successful numerical tests. We also discuss the possibility that the dark matter interacts strongly with ordinary baryonic matter, as well as with itself. We present a new analysis of the experimental constraints and re-evaluate the allowed range of cross-section and mass.

  12. Hidden vector dark matter

    E-Print Network [OSTI]

    Thomas Hambye

    2010-03-16

    We show that dark matter could be made of massive gauge bosons whose stability doesn't require to impose by hand any discrete or global symmetry. Stability of gauge bosons can be guaranteed by the custodial symmetry associated to the gauge symmetry and particle content of the model. The particle content we consider to this end is based on a hidden sector made of a vector multiplet associated to a non-abelian gauge group and of a scalar multiplet charged under this gauge group. The hidden sector interacts with the Standard Model particles through the Higgs portal quartic scalar interaction in such a way that the gauge bosons behave as thermal WIMPS. This can lead easily to the observed dark matter relic density in agreement with the other various constraints, and can be tested experimentally in a large fraction of the parameter space. In this model the dark matter direct detection rate and the annihilation cross section can decouple if the Higgs portal interaction is weak.

  13. Cosmology with matter diffusion

    SciTech Connect (OSTI)

    Calogero, Simone; Velten, Hermano E-mail: velten@cce.ufes.br

    2013-11-01

    We construct a viable cosmological model based on velocity diffusion of matter particles. In order to ensure the conservation of the total energy-momentum tensor in the presence of diffusion, we include a cosmological scalar field ? which we identify with the dark energy component of the universe. The model is characterized by only one new degree of freedom, the diffusion parameter ?. The standard ?CDM model can be recovered by setting ? = 0. If diffusion takes place (? > 0) the dynamics of the matter and of the dark energy fields are coupled. We argue that the existence of a diffusion mechanism in the universe may serve as a theoretical motivation for interacting models. We constrain the background dynamics of the diffusion model with Supernovae, H(z) and BAO data. We also perform a perturbative analysis of this model in order to understand structure formation in the universe. We calculate the impact of diffusion both on the CMB spectrum, with particular attention to the integrated Sachs-Wolfe signal, and on the matter power spectrum P(k). The latter analysis places strong constraints on the magnitude of the diffusion mechanism but does not rule out the model.

  14. Superconnections and Matter

    E-Print Network [OSTI]

    Roepstorff, G

    1998-01-01

    In a previous paper, the superconnection formalism was used to naturally fit the Higgs field into a U(n) gauge theory where we aimed at the reconstruction of the standard model. The approach provides an alternative to non-commutative geometry. This work is now continued by including matter field (leptons). The essentially new ingredient is the right-handed neutrino field and a new kind of interaction that goes with it. All interactions follow from one Dirac operator associated to a superconnection.

  15. Superconnections and Matter

    E-Print Network [OSTI]

    G. Roepstorff

    2000-08-17

    In a previous paper (hep-th/9801040), the superconnection formalism was used to fit the Higgs field into a U(n) gauge theory with particular emphasis on the n=2 case, aiming at the reconstruction of certain parts of the Standard Model. The approach provides an alternative to the one bases on non-commutative geometry. This work is continued by including matter fields (leptons only). We extend the Standard Model by including the right-handed neutrino field. The possibility of a finite neutrino mass is thus accounted for.

  16. Discrete dark matter

    SciTech Connect (OSTI)

    Hirsch, M.; Morisi, S.; Peinado, E.; Valle, J. W. F. [AHEP Group, Institut de Fisica Corpuscular--C.S.I.C./Universitat de Valencia, Edificio Institutos de Paterna, Apartado 22085, E-46071 Valencia (Spain)

    2010-12-01

    We propose a new motivation for the stability of dark matter (DM). We suggest that the same non-Abelian discrete flavor symmetry which accounts for the observed pattern of neutrino oscillations, spontaneously breaks to a Z{sub 2} subgroup which renders DM stable. The simplest scheme leads to a scalar doublet DM potentially detectable in nuclear recoil experiments, inverse neutrino mass hierarchy, hence a neutrinoless double beta decay rate accessible to upcoming searches, while {theta}{sub 13}=0 gives no CP violation in neutrino oscillations.

  17. Thermodynamics of electroweak matter

    E-Print Network [OSTI]

    A. Gynther

    2006-09-21

    This paper is a slightly modified version of the introductory part of a PhD thesis, also containing the articles hep-ph/0303019, hep-ph/0510375 and hep-ph/0512177. We provide a short history of the research of electroweak thermodynamics and a brief introduction to the theory as well as to the necessary theoretical tools needed to work at finite temperatures. We then review computations regarding the pressure of electroweak matter at high temperatures (the full expression of the perturbative expansion of the pressure is given in the appendix) and the electroweak phase diagram at finite chemical potentials. Finally, we compare electroweak and QCD thermodynamics.

  18. Dark Matter Velocity Spectroscopy

    E-Print Network [OSTI]

    Eric G. Speckhard; Kenny C. Y. Ng; John F. Beacom; Ranjan Laha

    2015-07-31

    Dark matter decays or annihilations that produce line-like spectra may be smoking-gun signals. However, even such distinctive signatures can be mimicked by astrophysical or instrumental causes. We show that velocity spectroscopy-the measurement of energy shifts induced by relative motion of source and observer-can separate these three causes with minimal theoretical uncertainties. The principal obstacle has been energy resolution, but upcoming experiments will reach the required 0.1% level. As an example, we show that the imminent Astro-H mission can use Milky Way observations to separate possible causes of the 3.5-keV line. We discuss other applications.

  19. Dark matter axions

    SciTech Connect (OSTI)

    Sikivie, P. (California Univ., Santa Barbara, CA (United States). Inst. for Theoretical Physics Florida Univ., Gainesville, FL (United States). Dept. of Physics)

    1992-01-01

    The physics of axions is briefly reviewed theoretically, and various constraints on the axion mass are recounted. Then the two main contributions to the present cosmological axion energy density, that due to the realignment of the vacuum during the QCD phase transition and that from axions radiated by cosmic axion strings, are discussed. Next, two detection schemes for axions that are sensitive to different mass ranges, an electromagnetic cavity permeated by a strong magnetic field and a system of superconducting wires embedded in a material transparent to microwave radiation, are described. Finally, the phase space structure of cold dark matter galactic halos is considered. (RWR)

  20. Dark matter axions

    SciTech Connect (OSTI)

    Sikivie, P. [California Univ., Santa Barbara, CA (United States). Inst. for Theoretical Physics]|[Florida Univ., Gainesville, FL (United States). Dept. of Physics

    1992-09-01

    The physics of axions is briefly reviewed theoretically, and various constraints on the axion mass are recounted. Then the two main contributions to the present cosmological axion energy density, that due to the realignment of the vacuum during the QCD phase transition and that from axions radiated by cosmic axion strings, are discussed. Next, two detection schemes for axions that are sensitive to different mass ranges, an electromagnetic cavity permeated by a strong magnetic field and a system of superconducting wires embedded in a material transparent to microwave radiation, are described. Finally, the phase space structure of cold dark matter galactic halos is considered. (RWR)

  1. Materials/Condensed Matter

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 Outreach Home Room NewsInformationJesse BergkampCentermillion toMSDSMaterials andMaterials/Condensed Matter Print

  2. Double-Disk Dark Matter

    E-Print Network [OSTI]

    Fan, JiJi; Randall, Lisa; Reece, Matthew

    2013-01-01

    Based on observational tests and constraints on halo structure, dark matter is generally taken to be cold and essentially collisionless. On the other hand, given the large number of particles and forces in the visible world, a more complex dark sector could be a reasonable or even likely possibility. This hypothesis leads to testable consequences, perhaps portending the discovery of a rich hidden world neighboring our own. We consider a scenario that readily satisfies current bounds that we call Partially Interacting Dark Matter (PIDM). This scenario contains self-interacting dark matter, but it is not the dominant component. Even if PIDM contains only a fraction of the net dark matter density, comparable to the baryonic fraction, the subdominant component's interactions can lead to interesting and potentially observable consequences. Our primary focus will be the special case of Double-Disk Dark Matter (DDDM), in which self-interactions allow the dark matter to lose enough energy to lead to dynamics similar ...

  3. Visualizing remixes in an online programming community

    E-Print Network [OSTI]

    Liu, Di, M. Eng. Massachusetts Institute of Technology

    2013-01-01

    Scratch is a block-based programming language and associated online community that allows children and young adults to learn to build interactive games and animations - and share their creations with one another. Scratch's ...

  4. Personnel / Human Resource Management MGTK 302 Online

    E-Print Network [OSTI]

    Diestel, Geoff

    competencies: Strategic Human Resource Management: Knowledge of strategic management concepts (strategyPersonnel / Human Resource Management MGTK 302 Online Fall 2014 YOUR INSTRUCTOR Name: Ms. Amanda of human resource management; relationship between personnel management and organizations' emerging role

  5. Activity based interfaces in online social networks

    E-Print Network [OSTI]

    Laraqui, Jawad

    2007-01-01

    The goal of the project is to explore how activity-based interfaces can create more meaningful experiences for the users and builders of online social networking sites. Medina, a social-networking site based on the idea ...

  6. "Prime" Advertising Space: Measuring Implict Memory Online 

    E-Print Network [OSTI]

    Barratt, Madeleine

    2012-05-25

    In marketing literature, click-through-rates are generally employed to measure the success of banner advertisements online. This measure has led to the banner blindness hypothesis, which posits that internet users ignore banner advertisements...

  7. Online Display Advertising: Targeting and Intrusiveness

    E-Print Network [OSTI]

    Tucker, Catherine Elizabeth

    We use data from a large-scale field experiment to explore what influences the effectiveness of online advertising. We find that matching an ad to website content and increasing an ad's obtrusiveness independently increase ...

  8. Online independent film distribution : what is missing?

    E-Print Network [OSTI]

    AbouZeid, Perihan

    2015-01-01

    This thesis proposes a new model for online platforms for independent films. Today, platforms such as Netflix, iTunes, and YouTube are in the face of major industry challenges: more competitors are entering the market; ...

  9. Online Raman spectroscopy for bioprocess monitoring

    E-Print Network [OSTI]

    Gil, Gustavo Adolfo

    2005-01-01

    Online monitoring of bioprocesses is essential to expanding the potential of biotechnology. In this thesis, a system to estimate concentrations of chemical components of an Escherichia Coli fermentation growth medium via ...

  10. On-line chemical composition analyzer development

    SciTech Connect (OSTI)

    Garrison, A.A.

    1993-01-01

    This report relates to the development of an on-line Raman analyzer for control of a distillation column. It is divided into: program issues, experimental control system evaluation, energy savings analysis, and reliability analysis. (DLC)

  11. Monthly Weather Review EARLY ONLINE RELEASE

    E-Print Network [OSTI]

    Majda, Andrew J.

    Monthly Weather Review EARLY ONLINE RELEASE This is a preliminary PDF of the author Institute of Mathematical Sciences5 New York University6 New York, NY7 Submitted to Monthly Weather Review8

  12. Monthly Weather Review EARLY ONLINE RELEASE

    E-Print Network [OSTI]

    Collett Jr., Jeffrey L.

    Monthly Weather Review EARLY ONLINE RELEASE This is a preliminary PDF of the author to Monthly Weather Review25 Revised 16 May 201426 Manuscript (non-LaTeX) Click here to download Manuscript

  13. Internet Exchanges: Enabling Local Online Communities

    E-Print Network [OSTI]

    Mitchell, Keith

    Interconnect Principles Internet Exchange History Internet Exchange Models Internet Exchange Security Setting, Foundry #12;Internet Exchanges History #12;A decade+ of Internet Exchanges The London Internet ExchangeInternet Exchanges: Enabling Local Online Communities Keith Mitchell Chair, United Kingdom Network

  14. Online social network sensors for influenza outbreaks

    E-Print Network [OSTI]

    Everett, Katie Elizabeth

    2013-01-01

    Previous research has shown strong correlations between postings on the online social network Twitter where users complain of influenza-like symptoms, and clinical data on actual influenza rates. In addition, previous ...

  15. Dark matter burners

    E-Print Network [OSTI]

    Moskalenko, I V

    2006-01-01

    We show that a star orbiting close enough to an adiabatically grown supermassive black hole can capture a large number of weakly interacting massive particles (WIMPs) during its lifetime. WIMP annihilation energy release in low- to medium-mass stars is comparable with or even exceeds the luminosity of such stars due to thermonuclear burning. The excessive energy release in the stellar core may result in an evolution scenario different from what is expected for a regular star. The model thus predicts the existence of unusual stars within the central parsec of galactic nuclei. If found, such stars would provide evidence for the existence of particle dark matter. The excess luminosity of such stars attributed to WIMP "burning" can be used to infer the local WIMP matter density. A white dwarf with a highly eccentric orbit around the central black hole may exhibit variations in brightness correlated with the orbital phase. On the other hand, white dwarfs shown to lack such orbital brightness variations can be used...

  16. Condensed Matter and Magnet Science

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    helimagnets and the development of a cryogen-free apparatus for spherical neutron polarimetry." Read more... Cutting-edge condensed matter physics research, high magnetic field...

  17. Solving the Dark Matter Problem

    ScienceCinema (OSTI)

    Baltz, Ted

    2009-09-01

    Cosmological observations have firmly established that the majority of matter in the universe is of an unknown type, called 'dark matter'. A compelling hypothesis is that the dark matter consists of weakly interacting massive particles (WIMPs) in the mass range around 100 GeV. If the WIMP hypothesis is correct, such particles could be created and studied at accelerators. Furthermore they could be directly detected as the primary component of our galaxy. Solving the dark matter problem requires that the connection be made between the two. We describe some theoretical and experimental avenues that might lead to this connection.

  18. Nuclear Matter and Nuclear Dynamics

    E-Print Network [OSTI]

    M Colonna

    2009-02-26

    Highlights on the recent research activity, carried out by the Italian Community involved in the "Nuclear Matter and Nuclear Dynamics" field, will be presented.

  19. MEASURING AGENDA SETTING WITH ONLINE SEARCH TRAFFIC: INFLUENCES OF ONLINE AND TRADITIONAL MEDIA

    E-Print Network [OSTI]

    Cortes, Corinna

    consumption amongst the electorate. In fact, one working hypothesis is the increased choice online may simply in their routine news consumption, the abundance of choice online may simply make it easier for the disinterested on differences in political knowledge based on an individual's self-reported media preferences for soft news

  20. Dark matter burners

    E-Print Network [OSTI]

    Moskalenko, I V; Moskalenko, Igor V.; Wai, Lawrence L.

    2007-01-01

    We show that a star orbiting close enough to an adiabatically grown supermassive black hole (SMBH) can capture weakly interacting massive particles (WIMPs) at an extremely high rate. The stellar luminosity due to annihilation of captured WIMPs in the stellar core may be comparable to or even exceed the luminosity of the star due to thermonuclear burning. The model thus predicts the existence of unusual stars, essentially WIMP burners, in the vicinity of a SMBH. We find that the most efficient WIMP burners are stars with degenerate electron cores, e.g. white dwarfs (WDs); such WDs may have a very high surface temperature. If found, such stars would provide evidence for the existence of particle dark matter and can possibly be used to establish its density profile. On the other hand, the lack of such unusual stars may provide constraints on the WIMP density near the SMBH, as well as the WIMP-nucleus scattering and pair annihilation cross-sections.

  1. Dark matter burners

    E-Print Network [OSTI]

    Igor V. Moskalenko; Lawrence L. Wai

    2007-02-24

    We show that a star orbiting close enough to an adiabatically grown supermassive black hole (SMBH) can capture weakly interacting massive particles (WIMPs) at an extremely high rate. The stellar luminosity due to annihilation of captured WIMPs in the stellar core may be comparable to or even exceed the luminosity of the star due to thermonuclear burning. The model thus predicts the existence of unusual stars, essentially WIMP burners, in the vicinity of a SMBH. We find that the most efficient WIMP burners are stars with degenerate electron cores, e.g. white dwarfs (WDs); such WDs may have a very high surface temperature. If found, such stars would provide evidence for the existence of particle dark matter and can possibly be used to establish its density profile. On the other hand, the lack of such unusual stars may provide constraints on the WIMP density near the SMBH, as well as the WIMP-nucleus scattering and pair annihilation cross-sections.

  2. Energy Matters in Washington State

    E-Print Network [OSTI]

    Collins, Gary S.

    Energy Matters in Washington State Energy Matters in Washington State www.energy.wsu.edu/library/ November 2009 #12;905 Plum Street SE, Building 3 P.O. Box 43169 Olympia, Washington 98504-3169 Energy University Extension Energy Program. 905 Plum Street SE, Building 3, P.O. Box 43169, Olympia, Washington

  3. Astronomical Evidence for Dark Matter

    E-Print Network [OSTI]

    Golwala, Sunil

    dark matter (assumed non-baryonic) #12;A word about constitutes an energy density from the Friedmann Equation: (Assuming no curvature) #12;Definitions C Critical Density X X/C = 1 => flat universe, what Rotation curve: Virial Theorem: #12;Spiral Galaxies Luminous Matter ~ follows: Asymptotes to constant value

  4. dark matter dark energy inflation

    E-Print Network [OSTI]

    Hu, Wayne

    theory dark matter dark energy inflation The National Science Foundation The Kavli Foundation NSF Site Review November 28-29, 2005 #12;dark matter dark energy inflation NSF Site Visit ­ November 28 - 29, 2005The National Science Foundation The Kavli Foundation The Theoretical Web UHE cosmic rays B

  5. Dark matter on the lattice

    E-Print Network [OSTI]

    Randy Lewis

    2014-11-26

    Several collaborations have recently performed lattice calculations aimed specifically at dark matter, including work with SU(2), SU(3), SU(4) and SO(4) gauge theories to represent the dark sector. Highlights of these studies are presented here, after a reminder of how lattice calculations in QCD itself are helping with the hunt for dark matter.

  6. Charmonium mass in nuclear matter 

    E-Print Network [OSTI]

    Lee, S. H.; Ko, Che Ming.

    2003-01-01

    The mass shift of charmonium states in nuclear matter is studied in the perturbative QCD approach. The leading-order effect due to the change of gluon condensate in nuclear matter is evaluated using the leading-order QCD formula, while the higher...

  7. Quantum vacuum and dark matter

    E-Print Network [OSTI]

    Dragan Slavkov Hajdukovic

    2011-11-21

    Recently, the gravitational polarization of the quantum vacuum was proposed as alternative to the dark matter paradigm. In the present paper we consider four benchmark measurements: the universality of the central surface density of galaxy dark matter haloes, the cored dark matter haloes in dwarf spheroidal galaxies, the non-existence of dark disks in spiral galaxies and distribution of dark matter after collision of clusters of galaxies (the Bullet cluster is a famous example). Only some of these phenomena (but not all of them) can (in principle) be explained by the dark matter and the theories of modified gravity. However, we argue that the framework of the gravitational polarization of the quantum vacuum allows the understanding of the totality of these phenomena.

  8. 0045-2068/$ -see front matter 2004 Elsevier Inc. All rights reserved. doi:10.1016/j.bioorg.2004.04.002

    E-Print Network [OSTI]

    Theodorakis, Emmanuel

    0045-2068/$ - see front matter 2004 Elsevier Inc. All rights reserved. doi:10.1016/j.bioorg.2004.04.002 Bioorganic Chemistry 32 (2004) 274­289 www.elsevier.com/locate/bioorg Hydrophilic molecular rotor derivatives 22 March 2004 Available online 13 May 2004 Abstract Recent research shows high potential for some p

  9. GOLD: The Genomes Online Database

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    Kyrpides, Nikos; Liolios, Dinos; Chen, Amy; Tavernarakis, Nektarios; Hugenholtz, Philip; Markowitz, Victor; Bernal, Alex

    Since its inception in 1997, GOLD has continuously monitored genome sequencing projects worldwide and has provided the community with a unique centralized resource that integrates diverse information related to Archaea, Bacteria, Eukaryotic and more recently Metagenomic sequencing projects. As of September 2007, GOLD recorded 639 completed genome projects. These projects have their complete sequence deposited into the public archival sequence databases such as GenBank EMBL,and DDBJ. From the total of 639 complete and published genome projects as of 9/2007, 527 were bacterial, 47 were archaeal and 65 were eukaryotic. In addition to the complete projects, there were 2158 ongoing sequencing projects. 1328 of those were bacterial, 59 archaeal and 771 eukaryotic projects. Two types of metadata are provided by GOLD: (i) project metadata and (ii) organism/environment metadata. GOLD CARD pages for every project are available from the link of every GOLD_STAMP ID. The information in every one of these pages is organized into three tables: (a) Organism information, (b) Genome project information and (c) External links. [The Genomes On Line Database (GOLD) in 2007: Status of genomic and metagenomic projects and their associated metadata, Konstantinos Liolios, Konstantinos Mavromatis, Nektarios Tavernarakis and Nikos C. Kyrpides, Nucleic Acids Research Advance Access published online on November 2, 2007, Nucleic Acids Research, doi:10.1093/nar/gkm884]

    The basic tables in the GOLD database that can be browsed or searched include the following information:

    • Gold Stamp ID
    • Organism name
    • Domain
    • Links to information sources
    • Size and link to a map, when available
    • Chromosome number, Plas number, and GC content
    • A link for downloading the actual genome data
    • Institution that did the sequencing
    • Funding source
    • Database where information resides
    • Publication status and information

    (Specialized Interface)

  10. Nuclear-matter--quark-matter phase diagram with strangeness

    SciTech Connect (OSTI)

    Barz, H. W.; Friman, B. L.; Knoll, J.; Schulz, H.

    1989-07-01

    A phenomenological equation of state of strongly interacting matter, including strange degrees of freedom, is presented. It is shown that the hyperon and kaon interactions must be included, in order to obtain a reasonable description of the deconfinement transition at high baryon densities. The consequences of kaon condensation on the nuclear-matter--quark-matter phase diagram are explored. The relative particle abundances obtained in an isentropic expansion of a blob of quark-gluon plasma are presented for different initial conditions. Implications for ultrarelativistic heavy-ion collisions are briefly discussed.

  11. Laser Driven Dynamic Loading of Condensed Matter

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Laser Driven Dynamic Loading of Condensed Matter Laser Driven Dynamic Loading of Condensed Matter Advanced diagnostics of experiments covering many orders of magnitude in strain...

  12. MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY; SOLID STATE...

    Office of Scientific and Technical Information (OSTI)

    Open problems in condensed matter physics, 1987 Falicov, L.M. 75 CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY; SOLID STATE PHYSICS; RESEARCH PROGRAMS;...

  13. Ultrafast Spectroscopy of Warm Dense Matter

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    of planet formation and structures as well as the evolution of an imploding inertial fusion capsule depends on our understanding of matter in the complex warm dense matter...

  14. Prokaryotic Genomes from Microbes Online Database

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    Alm, Eric J.; Huang, Katherine H.; Price, Morgan N.; Koche, Richard P.; Keller, Keith; Dubchak, Inna L.; Arkin, Adam P.

    To describe the potential functions of genes, MicrobesOnline includes protein family analyses (from InterPro and COG), metabolic maps (from KEGG), links to research papers (from UniProt and PubMed), and operon predictions for every genome. To examine each gene's evolutionary history, MicrobesOnline includes precomputed phylogenetic trees for all the gene families. It displays gene trees with genomic context or it compares the gene tree to the species tree. The tools provided with MicrobesOnline allow users to: compute customized motifs, sequence alignments, and phylogenetic trees change expression patterns in metabolic maps annotate genes in various ways The database contains more than 430 genomes. A browse tree tool and a genome browser are available, along with specialized search capabilities. (Specialized Interface)

  15. Casting Light on Dark Matter

    E-Print Network [OSTI]

    John Ellis

    2011-06-15

    The prospects for detecting a candidate supersymmetric dark matter particle at the LHC are reviewed, and compared with the prospects for direct and indirect searches for astrophysical dark matter. The discussion is based on a frequentist analysis of the preferred regions of the Minimal supersymmetric extension of the Standard Model with universal soft supersymmetry breaking (the CMSSM). LHC searches may have good chances to observe supersymmetry in the near future - and so may direct searches for astrophysical dark matter particles, whereas indirect searches may require greater sensitivity, at least within the CMSSM.

  16. The Unification and Cogeneration of Dark Matter and Baryonic Matter

    E-Print Network [OSTI]

    S. M. Barr

    2011-09-18

    In grand unified theories with gauge groups larger than SU(5), the multiplets that contain the known quarks and leptons also contain fermions that are singlets under the Standard Model gauge group. Some of these could be the dark matter of the universe. Grand unified theories can also have accidental U(1) global symmetries (analogous to B-L in minimal SU(5)) that can stabilize dark matter. These ideas are illustrated in an SU(6) model.

  17. The Unification and Cogeneration of Dark Matter and Baryonic Matter

    E-Print Network [OSTI]

    Barr, S M

    2011-01-01

    In grand unified theories with gauge groups larger than SU(5), the multiplets that contain the known quarks and leptons also contain fermions that are singlets under the Standard Model gauge group. Some of these could be the dark matter of the universe. Grand unified theories can also have accidental U(1) global symmetries (analogous to B-L in minimal SU(5)) that can stabilize dark matter. These ideas are illustrated in an SU(6) model.

  18. Online interaction database: What have we learned

    E-Print Network [OSTI]

    Zadezensky, I.; de Castro, W.; Meyer, J.; Butterweck, V.; Derendorf, H.

    2006-10-25

    ?[Citrus?Reference?Book] 1Center?for?Food?and?Drug?Interaction?Research?and?Education,?University?of?Florida,?Gainesville,?FL Online?Database?For?Grapefruit?Juice?Drug?Interactions:?What?Have?We?Learned?? I.?Zadezensky1,?W.V.?de?Castro1,??J.?Meyer1,?V...?[Citrus?Reference?Book] 1Center?for?Food?and?Drug?Interaction?Research?and?Education,?University?of?Florida,?Gainesville,?FL Online?Database?For?Grapefruit?Juice?Drug?Interactions:?What?Have?We?Learned?? I.?Zadezensky1,?W.V.?de?Castro1,??J.?Meyer1,?V...

  19. Romantic regressions : an analysis of behavior in online dating systems

    E-Print Network [OSTI]

    Fiore, Andrew Rocco Tresolini, 1979-

    2004-01-01

    Online personal advertisements have shed their stigma as matchmakers for the awkward to claim a prominent role in the social lives of millions of people. Web sites for online dating allow users to post lengthy personal ...

  20. AmiGO: online access to ontology and annotation data

    E-Print Network [OSTI]

    Carbon, Seth

    2009-01-01

    Genet. , 25, 25–29. GO Online SQL Environment (GOOSE) Thisusers the ability to perform SQL queries directly on the GOSlimmer tools, the GO Online SQL Environment and a user help

  1. Inventory planning for low demand items in online retailing

    E-Print Network [OSTI]

    Chhaochhria, Pallav

    2007-01-01

    A large online retailer strategically stocks inventory for SKUs with low demand. The motivations are to provide a wide range of selections and faster customer fulfillment service. We assume the online retailer has the ...

  2. An on-line human signature verification system 

    E-Print Network [OSTI]

    Simsek, Burc A

    2000-01-01

    A study on human signature verification is presented. A literature survey of current and past methodologies for on-line signature verification is followed by a new approach to the problem of on-line signature verification. ...

  3. A Dynamic Near-Optimal Algorithm for Online Linear Programming

    E-Print Network [OSTI]

    Ye, Yinyu

    -time forward dynamic pricing for PEVs charging/discharging on smart-grid; Yinyu Ye Online Linear Program 2009

  4. Peer-to-Peer Architecture for Massively Multiplayer Online Games

    E-Print Network [OSTI]

    for real games. #12;ii #12;Resum´e Online spil med massivt deltagerantal kræver i dag store datacentre som

  5. Free Online Training on the DVU Learning Channel!

    Broader source: Energy.gov [DOE]

    Free online courses are now available through the DOE Virtual University (DVU) website on the new DVU Learning Channel

  6. X-ray elemental online analyzer measures volatiles

    SciTech Connect (OSTI)

    Klein, A.; Pilz, K.; Reich, K. [Indutech Instruments GmbH, Simmersfeld (Germany)

    2008-04-15

    The use of an online XRF analyser for determining the volatiles content of coal is outlined. 3 figs.

  7. Physical Protection of Classified Matter

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    1988-02-03

    The order establishes policy and objectives for physical protection of classified matter. This directive does not cancel another directive. Chg 1, 7-30-93. Canceled by 5632.1C.

  8. Lorentz-violating dark matter 

    E-Print Network [OSTI]

    Mondragon, Antonio Richard

    2009-05-15

    was originally motivated by an unconventional fundamental theory, but which in this dissertation is defined as matter which has a nonzero minimum velocity. Furthermore, the present investigation evolved into the broader goal of exploring the properties of Lorentz...

  9. Energy Matters: Our Energy Independence

    Office of Energy Efficiency and Renewable Energy (EERE)

    In this installment of the livechat series "Energy Matters," Dr. Arun Majumdar takes questions from the public about the investments we're making today that will move us off of foreign oil and...

  10. Strongly interacting parton matter equilibration

    SciTech Connect (OSTI)

    Ozvenchuk, V.; Linnyk, O.; Bratkovskaya, E.; Gorenstein, M.; Cassing, W.

    2012-07-15

    We study the kinetic and chemical equilibration in 'infinite' parton matter within the Parton-Hadron-String Dynamics transport approach. The 'infinite' matter is simulated within a cubic box with periodic boundary conditions initialized at different energy densities. Particle abundances, kinetic energy distributions, and the detailed balance of the off-shell quarks and gluons in the strongly-interacting quarkgluon plasma are addressed and discussed.

  11. Dark Matter Triggers of Supernovae

    E-Print Network [OSTI]

    Peter W. Graham; Surjeet Rajendran; Jaime Varela

    2015-05-17

    The transit of primordial black holes through a white dwarf causes localized heating around the trajectory of the black hole through dynamical friction. For sufficiently massive black holes, this heat can initiate runaway thermonuclear fusion causing the white dwarf to explode as a supernova. The shape of the observed distribution of white dwarfs with masses up to $1.25 M_{\\odot}$ rules out primordial black holes with masses $\\sim 10^{19}$ gm - $10^{20}$ gm as a dominant constituent of the local dark matter density. Black holes with masses as large as $10^{24}$ gm will be excluded if recent observations by the NuStar collaboration of a population of white dwarfs near the galactic center are confirmed. Black holes in the mass range $10^{20}$ gm - $10^{22}$ gm are also constrained by the observed supernova rate, though these bounds are subject to astrophysical uncertainties. These bounds can be further strengthened through measurements of white dwarf binaries in gravitational wave observatories. The mechanism proposed in this paper can constrain a variety of other dark matter scenarios such as Q balls, annihilation/collision of large composite states of dark matter and models of dark matter where the accretion of dark matter leads to the formation of compact cores within the star. White dwarfs, with their astronomical lifetimes and sizes, can thus act as large space-time volume detectors enabling a unique probe of the properties of dark matter, especially of dark matter candidates that have low number density. This mechanism also raises the intriguing possibility that a class of supernova may be triggered through rare events induced by dark matter rather than the conventional mechanism of accreting white dwarfs that explode upon reaching the Chandrasekhar mass.

  12. Cosmology, Thermodynamics and Matter Creation

    E-Print Network [OSTI]

    J. A. S. Lima; M. O. Calvao; I. Waga

    2007-08-24

    Several approaches to the matter creation problem in the context of cosmological models are summarily reviewed. A covariant formulation of the general relativistic imperfect simple fluid endowed with a process of matter creation is presented. By considering the standard big bang model, it is shown how the recent results of Prigogine et alii \\cite{1} can be recovered and, at the same time their limits of validity are explicited.

  13. A Practical Application of Differential Privacy to Personalized Online Advertising

    E-Print Network [OSTI]

    International Association for Cryptologic Research (IACR)

    A Practical Application of Differential Privacy to Personalized Online Advertising Yehuda Lindell@cs.biu.ac.il,omrier@gmail.com Abstract Online advertising plays an important role in supporting many Internet services. Person- alized online advertising offers marketers a way to direct ads at very specific audiences. The vast body

  14. INNOVATIVE CONCEPTS FOR ON-LINE SYNCHRONOUS GENERATOR PARAMETER ESTIMATION

    E-Print Network [OSTI]

    INNOVATIVE CONCEPTS FOR ON-LINE SYNCHRONOUS GENERATOR PARAMETER ESTIMATION by Elias Kyriakides FOR ON-LINE SYNCHRONOUS GENERATOR PARAMETER ESTIMATION by Elias Kyriakides has been approved December ABSTRACT A method to identify synchronous generator parameters from on-line measurements is presented

  15. Hands-on online : towards experiential product design education with online resources

    E-Print Network [OSTI]

    Ramos, Joshua D

    2013-01-01

    This pilot study investigates the potential for teaching experiential, hands-on product design online. Specifically, the work is a first attempt to elucidate differences in outcomes between residential, hands-on educational ...

  16. Integrating the Digital Library into an Online

    E-Print Network [OSTI]

    de Lijser, Peter

    Integrating the Digital Library into an Online MS IDT Program JoAnn Carter-Wells, Ph.D. Karen Ivers #12; History and Structure of MISDT Program and Library Involvement Program Strands, Orientation Meetings, Program/Course Activities Range of Library Services for Distance Students Emerging Issues

  17. Bacon butty cancer risk ONLINE REPORTER

    E-Print Network [OSTI]

    Lega, Joceline

    Bacon butty cancer risk ONLINE REPORTER Published: 31st October 2007 0 PROCESSED meats, including ham and bacon are such a high risk factor for bowel cancer they should be avoided completely, bacon, pastrami, salami, and frankfurters. However, not all minced meats and hamburgers were considered

  18. ONLINE OPTIMIZATION AND SELECTION OF MEASUREMENTS

    E-Print Network [OSTI]

    Skogestad, Sigurd

    117 Chapter 7 ON­LINE OPTIMIZATION AND SELECTION OF MEASUREMENTS This is the last of three chapters that discuss optimal operation of a general heat exchanger network. A method that combines the use of steady state optimization and decentralized feedback control is proposed. A general steady state model

  19. gifted.msu.edu Apply online at

    E-Print Network [OSTI]

    curriculum for motivated, intelligent middle school and high school students. Our programs aim to enhancegifted.msu.edu Apply online at On the banks of the Red Cedar, There's a school that's known to all; Its specialty is winning, And those Spartans play good ball; Spartan teams are never beaten, All

  20. TOEFL TUTORIAL now ONLINE with East Tennessee

    E-Print Network [OSTI]

    Karsai, Istvan

    to ETSU is NOT required. The course is being offered as a five-week ses- sion three times: Jan. 17 ­ Feb for the reading, QUESTIONS? EMAIL the instructor at mcgarry@etsu.edu or visit the web site at: http://www.etsu.edu/ professionaldevelopment ETSU On-line Registration: http://etsuaw.etsu.edu/wconnect/ace/home.htm #12;

  1. Online Advertising Insertion Order Form Company name

    E-Print Network [OSTI]

    McReynolds, Ben

    Online Advertising Insertion Order Form Advertiser Company name: Address: City: State: Zip: Contact: Billing Instructions Gross Amount : $ Net Amount: $ Please refer to 2014 Advertising Rate Sheet Less 15% agency discount or other applicable discount (please specify below): Send invoices to: Advertiser

  2. A "Poisoning" Attack Against Online Anomaly Detection

    E-Print Network [OSTI]

    Freytag, Johann-Christoph

    A "Poisoning" Attack Against Online Anomaly Detection Marius Kloft Department of Computer Science it is robust against targeted "poisoning" attacks. The latter have been first investigated by Nelson et al. [1 of all data points observed so far. The key idea of a poisoning attack is to insert specially crafted

  3. Weather and Forecasting EARLY ONLINE RELEASE

    E-Print Network [OSTI]

    Weather and Forecasting EARLY ONLINE RELEASE This is a preliminary PDF of the author, Guangzhou 510301, China9 2. State Key Laboratory of Severe Weather, Chinese Academy of Meteorological10, China20 21 22 23 24 Submitted to Weather and Forecasting25 2014. 12. 2826 27 Corresponding author: Dr

  4. Monthly Weather Review EARLY ONLINE RELEASE

    E-Print Network [OSTI]

    Collett Jr., Jeffrey L.

    Monthly Weather Review EARLY ONLINE RELEASE This is a preliminary PDF of the author into numerical weather4 prediction models can improve precipitation forecasts and extend prediction capabilities5 that assimilates precipitation-affected microwave radiances into the7 Weather Research and Forecasting (WRF) model

  5. Weather and Forecasting EARLY ONLINE RELEASE

    E-Print Network [OSTI]

    Johnson, Richard H.

    Weather and Forecasting EARLY ONLINE RELEASE This is a preliminary PDF of the author Fort Collins, Colorado7 October 20128 (submitted to Weather and Forecasting)9 1 Corresponding author address: Rebecca D. Adams-Selin, HQ Air Force Weather Agency 16th Weather Squadron, 101 Nelson Dr., Offutt

  6. Monthly Weather Review EARLY ONLINE RELEASE

    E-Print Network [OSTI]

    Johnson, Richard H.

    Monthly Weather Review EARLY ONLINE RELEASE This is a preliminary PDF of the author, Colorado5 December 20126 (submitted to Monthly Weather Review)7 1 Corresponding author address: Rebecca D. Adams-Selin, HQ Air Force Weather Agency 16th Weather Squadron, 101 Nelson Dr., Offutt AFB, NE, 68113

  7. Monthly Weather Review EARLY ONLINE RELEASE

    E-Print Network [OSTI]

    Johnson, Richard H.

    Monthly Weather Review EARLY ONLINE RELEASE This is a preliminary PDF of the author and have been linked to severe weather and flooding in northern Mexico and the southwest United States 2001; Douglas and Leal 2003; Gochis et al. 2004; Higgins et al. 2004) and severe weather outbreaks

  8. Monthly Weather Review EARLY ONLINE RELEASE

    E-Print Network [OSTI]

    Heinselman, Pamela L.

    Monthly Weather Review EARLY ONLINE RELEASE This is a preliminary PDF of the author its first bow echo was captured by9 the National Weather Radar Testbed Phased Array Radar (NWRT PAR weather events, such as quasi-linear convective systems (QLCSs). Trapp et al.29 (2005) found that 18

  9. Geographies of an online social network

    E-Print Network [OSTI]

    Lengyel, Balázs; Ságvári, Bence; Jakobi, Ákos; Kertész, János

    2015-01-01

    How is online social media activity structured in the geographical space? Recent studies have shown that in spite of earlier visions about the "death of distance", physical proximity is still a major factor in social tie formation and maintenance in virtual social networks. Yet, it is unclear, what are the characteristics of the distance dependence in online social networks. In order to explore this issue the complete network of the former major Hungarian online social network is analyzed. We find that the distance dependence is weaker for the online social network ties than what was found earlier for phone communication networks. For a further analysis we introduced a coarser granularity: We identified the settlements with the nodes of a network and assigned two kinds of weights to the links between them. When the weights are proportional to the number of contacts we observed weakly formed, but spatially based modules resembling to the borders of macro-regions, the highest level of regional administration in...

  10. PROBING DENSE NUCLEAR MATTER VIA NUCLEAR COLLISIONS

    E-Print Network [OSTI]

    Stocker, H.

    2012-01-01

    shocked nuclear matter during the compression and expansionand isentropic expansion were valid in nuclear collisions.

  11. ArcGIS Explorer Online Extended Use Quick Guide ArcGIS Explorer Online--GIS for Everyone

    E-Print Network [OSTI]

    Wright, Dawn Jeannine

    ArcGIS Explorer Online Extended Use Quick Guide ArcGIS Explorer Online--GIS for Everyone Creating notes, photo links, and presentations ArcGIS Explorer Online (AGXO) is a browser-based GIS viewer, perform queries and create presentations. This quick guide is an extension of the Introduction to ArcGIS

  12. On-line Module Selection Student Guidelines On-line module selection opens on Wed 18th

    E-Print Network [OSTI]

    Harman, Neal.A.

    On-line Module Selection Student Guidelines Step 1 On-line module selection opens on Wed 18th March' followed by the tab `Next Year's Module Pre-selections'. Please note that any modules that are compulsory programme, you will need to submit the paper-work for this in-advance of selecting modules as your online

  13. Window in the dark matter exclusion limits

    SciTech Connect (OSTI)

    Zaharijas, Gabrijela; Farrar, Glennys R. [Center for Cosmology and Particle Physics, New York University, New York, New York 10003 (United States)

    2005-10-15

    We consider the cross section limits for light dark matter cadnidates (m=0.4 to 10 GeV). We calculate the interaction of dark matter in the crust above underground dark matter detectors and find that in the intermediate cross section range, the energy loss of dark matter is sufficient to fall below the energy threshold of current underground experiments. This implies the existence of a window in the dark matter exclusion limits in the micro-barn range.

  14. Double-Disk Dark Matter

    E-Print Network [OSTI]

    JiJi Fan; Andrey Katz; Lisa Randall; Matthew Reece

    2013-07-31

    Based on observational constraints on large scale structure and halo structure, dark matter is generally taken to be cold and essentially collisionless. On the other hand, given the large number of particles and forces in the visible world, a more complex dark sector could be a reasonable or even likely possibility. This hypothesis leads to testable consequences, perhaps portending the discovery of a rich hidden world neighboring our own. We consider a scenario that readily satisfies current bounds that we call Partially Interacting Dark Matter (PIDM). This scenario contains self-interacting dark matter, but it is not the dominant component. Even if PIDM contains only a fraction of the net dark matter density, comparable to the baryonic fraction, the subdominant component's interactions can lead to interesting and potentially observable consequences. Our primary focus will be the special case of Double-Disk Dark Matter (DDDM), in which self-interactions allow the dark matter to lose enough energy to lead to dynamics similar to those in the baryonic sector. We explore a simple model in which DDDM can cool efficiently and form a disk within galaxies, and we evaluate some of the possible observational signatures. The most prominent signal of such a scenario could be an enhanced indirect detection signature with a distinctive spatial distribution. Even though subdominant, the enhanced density at the center of the galaxy and possibly throughout the plane of the galaxy can lead to large boost factors, and could even explain a signature as large as the 130 GeV Fermi line. Such scenarios also predict additional dark radiation degrees of freedom that could soon be detectable and would influence the interpretation of future data, such as that from Planck and from the Gaia satellite. We consider this to be the first step toward exploring a rich array of new possibilities for dark matter dynamics.

  15. Bimetric gravity and dark matter

    E-Print Network [OSTI]

    Laura Bernard; Luc Blanchet; Lavinia Heisenberg

    2015-07-10

    We review some recent proposals for relativistic models of dark matter in the context of bimetric gravity. The aim is to solve the problems of cold dark matter (CDM) at galactic scales, and to reproduce the phenomenology of the modified Newtonian dynamics (MOND), while still being in agreement with the standard cosmological model $\\Lambda$-CDM at large scales. In this context a promising alternative is dipolar dark matter (DDM) in which two different species of dark matter particles are separately coupled to the two metrics of bigravity and are linked together by an internal vector field. The phenomenology of MOND then results from a mechanism of gravitational polarization. Probably the best formulation of the model is within the framework of recently developed massive bigravity theories. Then the gravitational sector of the model is safe by construction, but a ghostly degree of freedom in the decoupling limit is still present in the dark matter sector. Future work should analyse the cosmological solutions of the model and check the post-Newtonian parameters in the solar system.

  16. The DAMIC dark matter experiment

    E-Print Network [OSTI]

    Aguilar-Arevalo, A; Bertou, X; Bole, D; Butner, M; Cancelo, G; Vázquez, A Castañeda; Chavarria, A E; Neto, J R T de Mello; Dixon, S; D'Olivo, J C; Estrada, J; Moroni, G Fernandez; Torres, K P Hernández; Izraelevitch, F; Kavner, A; Kilminster, B; Lawson, I; Liao, J; López, M; Molina, J; Moreno-Granados, G; Pena, J; Privitera, P; Sarkis, Y; Scarpine, V; Schwarz, T; Haro, M Sofo; Tiffenberg, J; Machado, D Torres; Trillaud, F; You, X; Zhou, J

    2015-01-01

    The DAMIC (Dark Matter in CCDs) experiment uses high resistivity, scientific grade CCDs to search for dark matter. The CCD's low electronic noise allows an unprecedently low energy threshold of a few tens of eV that make it possible to detect silicon recoils resulting from interactions of low mass WIMPs. In addition the CCD's high spatial resolution and the excellent energy response results in very effective background identification techniques. The experiment has a unique sensitivity to dark matter particles with masses below 10 GeV/c$^2$. Previous results have demonstrated the potential of this technology, motivating the construction of DAMIC100, a 100 grams silicon target detector currently being installed at SNOLAB. In this contribution, the mode of operation and unique imaging capabilities of the CCDs, and how they may be exploited to characterize and suppress backgrounds will be discussed, as well as physics results after one year of data taking.

  17. Dark Matter in 3D

    SciTech Connect (OSTI)

    Alves, Daniele S.M.; Hedri, Sonia El; Wacker, Jay G.

    2012-04-01

    We discuss the relevance of directional detection experiments in the post-discovery era and propose a method to extract the local dark matter phase space distribution from directional data. The first feature of this method is a parameterization of the dark matter distribution function in terms of integrals of motion, which can be analytically extended to infer properties of the global distribution if certain equilibrium conditions hold. The second feature of our method is a decomposition of the distribution function in moments of a model independent basis, with minimal reliance on the ansatz for its functional form. We illustrate our method using the Via Lactea II N-body simulation as well as an analytical model for the dark matter halo. We conclude that O(1000) events are necessary to measure deviations from the Standard Halo Model and constrain or measure the presence of anisotropies.

  18. Static Response of Neutron Matter

    E-Print Network [OSTI]

    Buraczynski, Mateusz

    2015-01-01

    We generalize the problem of strongly interacting neutron matter by adding a periodic external modulation. This allows us to study from first principles a neutron system that is extended and inhomogeneous, with connections to the physics of both neutron-star crusts and neutron-rich nuclei. We carry out fully non-perturbative microscopic Quantum Monte Carlo calculations of the energy of neutron matter at different densities, as well as different strengths and periodicities of the external potential. In order to remove systematic errors, we examine finite-size effects and the impact of the wave function ansatz. We also make contact with energy-density functional theories of nuclei and disentangle isovector gradient contributions from bulk properties. Finally, we calculate the static density-density linear response function of neutron matter and compare it with the response of other physical systems.

  19. Chiral condensate in neutron matter

    E-Print Network [OSTI]

    N. Kaiser; W. Weise

    2008-08-06

    A recent chiral perturbation theory calculation of the in-medium quark condensate $$ is extended to the isospin-asymmetric case of pure neutron matter. In contrast to the behavior in isospin-symmetric nuclear matter we find only small deviations from the linear density approximation. This feature originates primarily from the reduced weight factors (e.g. 1/6 for the dominant contributions) of the $2\\pi$-exchange mechanisms in pure neutron matter. Our result suggests therefore that the tendencies for chiral symmetry restoration are actually favored in systems with large neutron excess (e.g. neutron stars). We also analyze the behavior of the density-dependent quark condensate $(\\rho_n)$ in the chiral limit $m_\\pi\\to 0$.

  20. Online Social Activity Reflects Economic Status

    E-Print Network [OSTI]

    Liu, Jin-Hu; Shao, Junming; Zhou, Tao

    2015-01-01

    To characterize economic development and diagnose the economic health condition, several popular indices such as gross domestic product (GDP), industrial structure and income growth are widely applied. However, computing these indices based on traditional economic census is usually costly and resources consuming, and more importantly, following a long time delay. In this paper, we analyzed nearly 200 million users' activities for four consecutive years in the largest social network (Sina Microblog) in China, aiming at exploring latent relationships between the online social activities and local economic status. Results indicate that online social activity has a strong correlation with local economic development and industrial structure, and more interestingly, allows revealing the macro-economic structure instantaneously with nearly no cost. Beyond, this work also provides a new venue to identify risky signal in local economic structure.

  1. Automatic identification of abstract online groups

    DOE Patents [OSTI]

    Engel, David W; Gregory, Michelle L; Bell, Eric B; Cowell, Andrew J; Piatt, Andrew W

    2014-04-15

    Online abstract groups, in which members aren't explicitly connected, can be automatically identified by computer-implemented methods. The methods involve harvesting records from social media and extracting content-based and structure-based features from each record. Each record includes a social-media posting and is associated with one or more entities. Each feature is stored on a data storage device and includes a computer-readable representation of an attribute of one or more records. The methods further involve grouping records into record groups according to the features of each record. Further still the methods involve calculating an n-dimensional surface representing each record group and defining an outlier as a record having feature-based distances measured from every n-dimensional surface that exceed a threshold value. Each of the n-dimensional surfaces is described by a footprint that characterizes the respective record group as an online abstract group.

  2. Benford's Law Applies To Online Social Networks

    E-Print Network [OSTI]

    Golbeck, Jennifer

    2015-01-01

    Benford's Law states that the frequency of first digits of numbers in naturally occurring systems is not evenly distributed. Numbers beginning with a 1 occur roughly 30\\% of the time, and are six times more common than numbers beginning with a 9. We show that Benford's Law applies to social and behavioral features of users in online social networks. We consider social data from five major social networks: Facebook, Twitter, Google Plus, Pinterest, and Live Journal. We show that the distribution of first significant digits of friend and follower counts for users in these systems follow Benford's Law. The same holds for the number of posts users make. We extend this to egocentric networks, showing that friend counts among the people in an individual's social network also follow the expected distribution. We discuss how this can be used to detect suspicious or fraudulent activity online and to validate datasets.

  3. Discourse indicators of culture in online courses 

    E-Print Network [OSTI]

    Gazi, Yakut

    2009-05-15

    , for giving me the opportunity to have my hands in the ?real thing?. Ravi, I also particularly thank you for your encouragement and support during the last phase of my writing. I still have the daily text messages you sent me on my cell phone. Do not think... levels, unwavering support from the host institution and a real commitment to student learning? (1998, p. 159). Globalization of education and online education initiatives go hand in hand, most recently through higher education institutions offering...

  4. Massivizing Online Games: Distributed Computing Challenges and

    E-Print Network [OSTI]

    Langendoen, Koen

    .st.ewi.tudelft.nl #12;(TU) Delft ­ the Netherlands ­ Europe founded 13th century pop: 100,000 pop.: 100,000 pop: 16.5 M founded 1842 pop: 13,000 pop.: 100,000 (We are here) #12;Why Social Gaming? Massivizing Social Games Gaming used to be art, may now be computingOnline Gaming used to be art, may now be computing Massivizing

  5. Photometry from online Digitized Sky Survey Plates

    E-Print Network [OSTI]

    A. Bacher; S. Kimeswenger; P. Teutsch

    2005-07-22

    Online Digital Sky Survey (DSS) material is often used to obtain information on newly discovered variable stars for older epochs (e.g. Nova progenitors, flare stars, ...). We present here the results of an investigation of photometry on online digital sky survey material in small fields calibrated by CCD sequences. We compared different source extraction mechanisms and found, that even down near to the sensitivity limit, despite the H-compression used for the online material, photometry with an accuracy better than 0\\fm1 rms is possible on DSS-II. Our investigation shows that the accuracy depends strongly on the source extraction method. The SuperCOSMOS scans, although retrieved with an higher spatial resolution, do not give us better results. The methods and parameters presented here, allow the user to obtain good plate photometry in small fields down to the Schmidt plate survey limits with a few bright CCD calibrators, which may be calibrated with amateur size telescopes. Especially for the events mentioned above, new field photometry for calibration purposes mostly exists, but the progenitors were not measured photometrically before. Also the follow up whether stellar concentrations are newly detected clusters or similar work may be done without using mid size telescopes. The calibration presented here is a "local" one for small fields. We show that this method presented here gives higher accuracies than "global" calibrations of surveys (e.g. GSC-II, SuperCOSMOS and USNO-B)

  6. Pump Systems Matter Mission and Vision | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    ionofPumpSystemsMatter.pdf More Documents & Publications Overview of Pump Systems Matter Hydraulic Institute Mission and Vision Course Overview Pump Systems Matter Optimization...

  7. Why Geology Matters: Decoding the Past, Anticipating the Future

    E-Print Network [OSTI]

    Anderson, Byron P.

    2011-01-01

    Review: Why Geology Matters: Decoding the Past, AnticipatingUSA Macdougall, Doug. Why Geology Matters: Decoding theE-book available. Why Geology Matters pursues two goals: to

  8. Apparatus for particulate matter analysis

    DOE Patents [OSTI]

    Gundel, Lara A.; Apte, Michael G.; Hansen, Anthony D.; Black, Douglas R.

    2007-01-30

    The apparatus described herein is a miniaturized system for particle exposure assessment (MSPEA) for the quantitative measurement and qualitative identification of particulate content in gases. The present invention utilizes a quartz crystal microbalance (QCM) or other mass-sensitive temperature compensated acoustic wave resonator for mass measurement. Detectors and probes and light sources are used in combination for the qualitative determination of particulate matter.

  9. Laser Cooling of Matter INTRODUCTION

    E-Print Network [OSTI]

    Kaiser, Robin

    Laser Cooling of Matter INTRODUCTION Laser cooling of neutral atoms in the past decades has been a breakthrough in the understanding of their dy- namics and led to the seminal proposals of laser cooling-Doppler and subrecoil cooling, as well as new technologies, such as semiconductor diode lasers. Most of those

  10. States of Matter Deepak Dhar

    E-Print Network [OSTI]

    Udgaonkar, Jayant B.

    - logical classification of different animal species) or some mixture of these (e.g. books in a library answer in this case is that states of matter is a classification scheme, like filing cabinets classification schemes could be alphabetical (e.g. in a dictionary), or based on some common properties ( zoo

  11. Wino dark matter under siege

    SciTech Connect (OSTI)

    Cohen, Timothy; Lisanti, Mariangela; Pierce, Aaron; Slatyer, Tracy R. E-mail: mlisanti@princeton.edu E-mail: tslatyer@mit.edu

    2013-10-01

    A fermion triplet of SU(2){sub L} — a wino — is a well-motivated dark matter candidate. This work shows that present-day wino annihilations are constrained by indirect detection experiments, with the strongest limits coming from H.E.S.S. and Fermi. The bounds on wino dark matter are presented as a function of mass for two scenarios: thermal (winos constitute a subdominant component of the dark matter for masses less than 3.1 TeV) and non-thermal (winos comprise all the dark matter). Assuming the NFW halo model, the H.E.S.S. search for gamma-ray lines excludes the 3.1 TeV thermal wino; the combined H.E.S.S. and Fermi results completely exclude the non-thermal scenario. Uncertainties in the exclusions are explored. Indirect detection may provide the only probe for models of anomaly plus gravity mediation where the wino is the lightest superpartner and scalars reside at the 100 TeV scale.

  12. Solar Neutrino Matter Effects Redux

    E-Print Network [OSTI]

    A. B. Balantekin; A. Malkus

    2011-12-19

    Following recent low-threshold analysis of the Sudbury Neutrino Observatory and asymmetry measurements of the BOREXINO Collaboration of the solar neutrino flux, we revisit the analysis of the matter effects in the Sun. We show that solar neutrino data constrains the mixing angle $\\theta_{13}$ poorly and that subdominant Standard Model effects can mimic the effects of the physics beyond the Standard Model.

  13. Neutrino Mass and Dark Matter

    E-Print Network [OSTI]

    David O. Caldwell

    1998-12-01

    Despite direct observations favoring a low mass density, a critical density universe with a neutrino component of dark matter provides the best existing model to explain the observed structure of the universe over more than three orders of magnitude in distance scale. In principle this hot dark matter could consist of one, two, or three species of active neutrinos. If all present indications for neutrino mass are correct, however, only the two-species (muon neutrino and tau neutrino) possibility works. This requires the existence of at least one light sterile neutrino to explain the solar electron neutrino deficit via nu(e)->nu(s), leaving nu(mu)->nu(tau) as the explanation for the anomalous nu(mu)/nu(e) ratio produced by atmospheric neutrinos, and having the LSND experiment demonstrating via anti-nu(mu)-> anti-nu(e) the mass difference between the light nu(e)-nu(s) pair and the heavier nu(mu)-nu(tau) pair required for dark matter. Other experiments do not conflict with the LSND results when all the experiments are analyzed in the same way, and when analyzed conservatively the LSND data is quite compatible with the mass difference needed for dark matter. Further support for this mass pattern is provided by the need for a sterile neutrino to rescue heavy-element nucleosynthesis in supernovae, and it could even aid the concordance in light element abundances from the early universe.

  14. Cold quark matter in compact stars

    SciTech Connect (OSTI)

    Franzon, B.; Fogaca, D. A.; Navarra, F. S.; Horvath, J. E.

    2013-03-25

    We used an equation of state for the cold quark matter to the study of properties of quark stars. We also discuss the absolute stability of quark matter and compute the mass-radius relation for self-bound stars.

  15. Microfiltration of colloids and natural organic matter 

    E-Print Network [OSTI]

    Schäfer, Andrea; Schwicke, U.; Fischer, M. M.; Fane, Anthony G.; Waite, T. D.

    2000-01-01

    Surface waters contain colloids and natural organic matter, largely composed of humic substances. In this work the effect of natural organic matter (NOM) and humic substances (IHSS stream humic and fulvic acid reference ...

  16. Strongly Interacting Matter at High Energy Density

    E-Print Network [OSTI]

    Larry McLerran

    2008-12-08

    This lecture concerns the properties of strongly interacting matter (which is described by Quantum Chromodynamics) at very high energy density. I review the properties of matter at high temperature, discussing the deconfinement phase transition . At high baryon density and low temperature, large $N_c$ arguments are developed which suggest that high baryonic density matter is a third form of matter, Quarkyonic Matter, that is distinct from confined hadronic matter and deconfined matter. I finally discuss the Color Glass Condensate which controls the high energy limit of QCD, and forms the low x part of a hadron wavefunction. The Glasma is introduced as matter formed by the Color Glass Condensate which eventually thermalizes into a Quark Gluon Plasma.

  17. Indirect searches for neutralino dark matter

    E-Print Network [OSTI]

    Joakim Edsjo

    2002-11-15

    There is mounting evidence for dark matter in the Universe and one of the favourite dark matter candidates is the neutralino, which naturally appears as the lightest supersymmetric particle (LSP) in many supersymmetric extensions of the standard model. The neutralino has the desired properties to be a good dark matter candidate and we will here review the different indirect searches for neutralino dark matter and discuss the implications on these from recent direct searches.

  18. Operations & Maintenance Best Practices Guide: Front Matter

    Broader source: Energy.gov [DOE]

    Guide describes the front matter of the Operations and Maintenance Best Practices: a Guide to Achieving Operational Efficiency.

  19. Nuclear matter to strange matter transition in holographic QCD

    E-Print Network [OSTI]

    Youngman Kim; Yunseok Seo; Sang-Jin Sin

    2009-11-19

    We construct a simple holographic QCD model to study nuclear matter to strange matter transition. The interaction of dense medium and hadrons is taken care of by imposing the force balancing condition for stable D4/D6/D6 configuration. By considering the intermediate and light flavor branes interacting with baryon vertex homogeneously distributed along R^3 space and requesting the energy minimization, we find that there is a well defined transition density as a function of current quark mass. We also find that as density goes up very high, intermediate (or heavy) and light quarks populate equally as expected from the Pauli principle. In this sense, the effect of the Pauli principle is realized as dynamics of D-branes.

  20. Microbes Online: an integrated portal for comparative functional genomics

    E-Print Network [OSTI]

    Arkin, Adam P.

    2014-01-01

    understand mechanisms by which microbes survive in uncertainMicrobes Online: an integrated portal for comparativecerevisiae to environmental microbes such as Desulfovibrio

  1. Leave any noise at the signal : participation art online

    E-Print Network [OSTI]

    Frid-Jimenez, Amber

    2007-01-01

    Online participatory media holds the promise of activating otherwise passive audiences by providing spaces that encourage creative collaboration among diverse participants. The thesis traces the history of participation ...

  2. Dark Matter Searches with Representing the

    E-Print Network [OSTI]

    California at Santa Cruz, University of

    · Supernova Remnants · Unidentified Gamma-ray Sources · Gamma-Ray Bursts · Solar Physics · Dark Matter #12;SCIPP talk Larry Wai / SLAC 4 Talk overview 1. What is GLAST? 2. How does dark matter shine in gamma rays? 3. Where should we look for dark matter with GLAST? #12;SCIPP talk Larry Wai / SLAC 5 GLAST

  3. Personal Finance Make Your Money Matter

    E-Print Network [OSTI]

    Stevenson, Mark

    Personal Finance Make Your Money Matter Name: Registration number: Department: Year of study of your portfolio. #12;Personal Finance Make Your Money Matter2 Contents Timetable Page 3 Introduction 16 #12;Personal Finance Make Your Money Matter3 Timetable Friday 6.00 pm Introduction

  4. The Impact of Visual Appearance on User Response in Online Display Advertising

    E-Print Network [OSTI]

    Azimi, Javad; Zhou, Yang; Navalpakkam, Vidhya; Mao, Jianchang; Fern, Xiaoli

    2012-01-01

    Display advertising has been a significant source of revenue for publishers and ad networks in online advertising ecosystem. One of the main goals in display advertising is to maximize user response rate for advertising campaigns, such as click through rates (CTR) or conversion rates. Although in the online advertising industry we believe that the visual appearance of ads (creatives) matters for propensity of user response, there is no published work so far to address this topic via a systematic data-driven approach. In this paper we quantitatively study the relationship between the visual appearance and performance of creatives using large scale data in the world's largest display ads exchange system, RightMedia. We designed a set of 43 visual features, some of which are novel and some are inspired by related work. We extracted these features from real creatives served on RightMedia. We also designed and conducted a series of experiments to evaluate the effectiveness of visual features for CTR prediction, ra...

  5. Online Application Process | netl.doe.gov

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 Outreach Home Room NewsInformationJesseworkSURVEY UNIVERSEHowScientificOmbuds OfficeOne Vaccine LeadsOneOnline

  6. Online Legal Resources | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious Rank EERE: Alternative Fuelsof EnergyApril 2014DepartmentCouncilOffice of the ChiefResearchOilOnline

  7. Exploring online retailing strategies : case studies of leading firms in the U.S. and China

    E-Print Network [OSTI]

    Chen, Jian, S.M. Massachusetts Institute of Technology, Sloan School of Management

    2012-01-01

    Online retailing has been a significant part of people's daily life. Research shows that 85% of internet users have purchased online. In China, with the increased penetration rate of internet and adoption of online payment, ...

  8. On the Summarization of Dynamically Introduced Information: Online Discussions and Blogs

    E-Print Network [OSTI]

    Hovy, Eduard

    On the Summarization of Dynamically Introduced Information: Online Discussions and Blogs Liang Zhou approaches to summarizing dynamically introduced information: online discussions and blogs.aaai.org). All rights reserved. Online discussion forums and personal blogs are "dynamic", involving frequent

  9. Effects of Advanced Combustion Technologies on Particulate Matter...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Advanced Combustion Technologies on Particulate Matter Emissions Characteristics Effects of Advanced Combustion Technologies on Particulate Matter Emissions Characteristics...

  10. Superconducting Detectors for Super Light Dark Matter

    E-Print Network [OSTI]

    Yonit Hochberg; Yue Zhao; Kathryn M. Zurek

    2015-04-27

    We propose and study a new class of of superconducting detectors which are sensitive to O(meV) electron recoils from dark matter-electron scattering. Such devices could detect dark matter as light as the warm dark matter limit, mX > keV. We compute the rate of dark matter scattering off free electrons in a (superconducting) metal, including the relevant Pauli blocking factors. We demonstrate that classes of dark matter consistent with all astrophysical and terrestrial constraints could be detected by such detectors with a moderate size exposure.

  11. Superconducting Detectors for Super Light Dark Matter

    E-Print Network [OSTI]

    Hochberg, Yonit; Zurek, Kathryn M

    2015-01-01

    We propose and study a new class of of superconducting detectors which are sensitive to O(meV) electron recoils from dark matter-electron scattering. Such devices could detect dark matter as light as the warm dark matter limit, mX > keV. We compute the rate of dark matter scattering off free electrons in a (superconducting) metal, including the relevant Pauli blocking factors. We demonstrate that classes of dark matter consistent with all astrophysical and terrestrial constraints could be detected by such detectors with a moderate size exposure.

  12. Superconducting Detectors for Super Light Dark Matter

    E-Print Network [OSTI]

    Yonit Hochberg; Yue Zhao; Kathryn M. Zurek

    2015-11-11

    We propose and study a new class of superconducting detectors which are sensitive to O(meV) electron recoils from dark matter-electron scattering. Such devices could detect dark matter as light as the warm dark matter limit, mX > keV. We compute the rate of dark matter scattering off of free electrons in a (superconducting) metal, including the relevant Pauli blocking factors. We demonstrate that classes of dark matter consistent with terrestrial and cosmological/astrophysical constraints could be detected by such detectors with a moderate size exposure.

  13. Incompressibility of asymmetric nuclear matter

    E-Print Network [OSTI]

    Lie-Wen Chen; Bao-Jun Cai; Chun Shen; Che Ming Ko; Jun Xu; Bao-An Li

    2009-11-17

    The incompressibility $K_sat(\\delta)$ of isospin asymmetric nuclear matter at its saturation density. Our results show that in the expansion of $K_sat(\\delta)$ in powers of isospin asymmetry $\\delta$, i.e., $K_sat(\\delta )$=K_{0}+K_{sat,2}\\delta^{2}+K_{sat,4}\\delta^{4}+O(\\delta^{6})$, the magnitude of the 4th-order K_{sat,4} parameter is generally small. The 2nd-order K_{sat,2} parameter thus essentially characterizes the isospin dependence of the incompressibility of asymmetric nuclear matter at saturation density. Furthermore, the K_{sat,2} can be expressed as K_{sat,2}=K_{sym}-6L-J_{0}/{K_{0}L in terms of the slope parameter $L$ and the curvature parameter $K_{\\mathrm{sym}}$ of the symmetry energy and the third-order derivative parameter $J_0$ of the energy of symmetric nuclear matter at saturation density, and we find the higher order $J_0$ contribution to K_{sat,2} generally cannot be neglected. Also, we have found a linear correlation between K_{sym} and $L$ as well as between $J_{0}/K_{0}$ and $K_{0}$. Using these correlations together with the empirical constraints on $K_{0}$ and $L$, the nuclear symmetry energy $E_sym(\\rho_{0})$ at normal nuclear density, and the nucleon effective mass, we have obtained an estimated value of K_{sat,2}=-370 +- 120 MeV for the 2nd-order parameter in the isospin asymmetry expansion of the incompressibility of asymmetric nuclear matter at its saturation density.

  14. Two-portal Dark Matter

    E-Print Network [OSTI]

    Karim Ghorbani; Hossein Ghorbani

    2015-06-14

    We propose a renormalizable dark matter model in which a fermionic dark matter (DM) candidate communicates with the standard model particles through two distinct portals: Higgs and vector portals. The dark sector is charged under a $U(1)'$ gauge symmetry while the standard model has a leptophobic interaction with the dark vector boson. The leading contribution of DM-nucleon elastic scattering cross section begins at one-loop level. The model meets all the constraints imposed by direct detection experiments provided by LUX and XENON100, observed relic abundance according to WMAP and Planck, and the invisible Higgs decay width measured at the LHC. It turns out that the dark matter mass in the viable parameter space can take values from a few GeV up to 1 TeV. This is a new feature which is absent in the models with only one portal. In addition, we can find in the constrained regions of the parameter space a DM mass of $\\sim 34$ GeV annihilating into $b$ quark pair, which explains the Fermi-LAT gamma-ray excess.

  15. On Math, Matter and Mind

    E-Print Network [OSTI]

    Piet Hut; Mark Alford; Max Tegmark

    2006-01-15

    We discuss the nature of reality in the ontological context of Penrose's math-matter-mind triangle. The triangle suggests the circularity of the widespread view that math arises from the mind, the mind arises out of matter, and that matter can be explained in terms of math. Non-physicists should be wary of any claim that modern physics leads us to any particular resolution of this circularity, since even the sample of three theoretical physicists writing this paper hold three divergent views. Some physicists believe that current physics has already found the basic framework for a complete description of reality, and only has to fill in the details. Others suspect that no single framework, from physics or other sources, will ever capture reality. Yet others guess that reality might be approached arbitrarily closely by some form of future physics, but probably based on completely different frameworks. We will designate these three approaches as the fundamentalist, secular and mystic views of the world, as seen by practicing physicists. We present and contrast each of these views, which arguably form broad categories capturing most if not all interpretations of physics. We argue that this diversity in the physics community is more useful than an ontological monoculture, since it motivates physicists to tackle unsolved problems with a wide variety of approaches.

  16. Heavy Dark Matter Through the Higgs Portal

    E-Print Network [OSTI]

    John March-Russell; Stephen M. West; Daniel Cumberbatch; Dan Hooper

    2008-06-17

    Motivated by Higgs Portal and Hidden Valley models, heavy particle dark matter that communicates with the supersymmetric Standard Model via pure Higgs sector interactions is considered. We show that a thermal relic abundance consistent with the measured density of dark matter is possible for masses up to $\\sim 30\\tev$. For dark matter masses above $\\sim 1\\tev$, non-perturbative Sommerfeld corrections to the annihilation rate are large, and have the potential to greatly affect indirect detection signals. For large dark matter masses, the Higgs-dark-matter-sector couplings are large and we show how such models may be given a UV completion within the context of so-called "Fat-Higgs" models. Higgs Portal dark matter provides an example of an attractive alternative to conventional MSSM neutralino dark matter that may evade discovery at the LHC, while still being within the reach of current and upcoming indirect detection experiments.

  17. Online short-term solar power forecasting

    SciTech Connect (OSTI)

    Bacher, Peder; Madsen, Henrik [Informatics and Mathematical Modelling, Richard Pedersens Plads, Technical University of Denmark, Building 321, DK-2800 Lyngby (Denmark); Nielsen, Henrik Aalborg [ENFOR A/S, Lyngsoe Alle 3, DK-2970 Hoersholm (Denmark)

    2009-10-15

    This paper describes a new approach to online forecasting of power production from PV systems. The method is suited to online forecasting in many applications and in this paper it is used to predict hourly values of solar power for horizons of up to 36 h. The data used is 15-min observations of solar power from 21 PV systems located on rooftops in a small village in Denmark. The suggested method is a two-stage method where first a statistical normalization of the solar power is obtained using a clear sky model. The clear sky model is found using statistical smoothing techniques. Then forecasts of the normalized solar power are calculated using adaptive linear time series models. Both autoregressive (AR) and AR with exogenous input (ARX) models are evaluated, where the latter takes numerical weather predictions (NWPs) as input. The results indicate that for forecasts up to 2 h ahead the most important input is the available observations of solar power, while for longer horizons NWPs are the most important input. A root mean square error improvement of around 35% is achieved by the ARX model compared to a proposed reference model. (author)

  18. Online b-jets tagging at CDF

    SciTech Connect (OSTI)

    Casarsa, M.; Ristori, L.; Amerio, S.; Lucchesi, D.; Pagan Griso, S.; Torre, S.T.; Cortiana, G.; /Padua U., Astron. Dept.

    2007-04-01

    We propose a method to identify b-quark jets at trigger level which exploits recently increased CDF trigger system capabilities. b-quark jets identification is of central interest for the CDF high-P{sub T} physics program, and the possibility to select online b-jets enriched samples can extend the physics reaches especially for light Higgs boson searches where the H {yields} b{bar b} decay mode is dominant. Exploiting new trigger primitives provided by two recent trigger upgrades, the Level2 XFT stereo tracking and the improved Level2 cluster-finder, in conjunction with the existing Silicon Vertex Tracker (SVT), we design an online trigger algorithm aimed at selecting good purity b-jets samples useful for many physics measurements, the most important being inclusive H {yields} b{bar b} searches. We discuss the performances of the proposed b-tagging algorithm which must guarantee reasonable trigger rates at luminosity greater than 2 x 10{sup 32} cm{sup -2}s{sup -1} and provide high efficiency on H {yields} b{bar b} events.

  19. Optimizing Throughput and Energy in Online Deadline Scheduling

    E-Print Network [OSTI]

    Wong, Prudence W.H.

    consider a processor that can vary its speed between 0 and a maximum speed T to minimize its energy usage usage. If we ignore energy usage, the best possible online algorithm is 4-competitive on throughput jobs; O(1)-competitive online algorithms with respect to energy usage have been known [Yao et al. 1995

  20. The Online Journal "JEPT" Surface Technology | Electroplating | Electrochemistry

    E-Print Network [OSTI]

    Knobloch,Jürgen

    The Online Journal "JEPT" Surface Technology | Electroplating | Electrochemistry The scientific. Focused on electroplating and electro- chemical fundamentals. All articles are available online as well as coatings for collector rings. Friction balls were made of smooth alumina with a diameter of 6 mm. To have

  1. Chemistry 1010 -090 (Online) Chemistry, Humanity, and Environment

    E-Print Network [OSTI]

    Simons, Jack

    chemistry to environmental questions such as energy sources, air quality, water quality, mineral resourcesChemistry 1010 -090 (Online) Chemistry, Humanity, and Environment 1. Course Content The Online version of Chemistry 1010 (1010-090) supports the aims of the University of Utah General Education Mission

  2. Researching a Company Online Ready Reference D-13

    E-Print Network [OSTI]

    Researching a Company Online Ready Reference D-13 College of Engineering, Architecture & Technology information on over 50,000 public and private companies (www.hoovers.com). · CorpTech Database of High and private high-tech organizations (www.corptech.com). · Companies Online from Dun & Bradstreet and Lycos

  3. Pipelineable On-Line Encryption Farzaneh Abed1

    E-Print Network [OSTI]

    International Association for Cryptologic Research (IACR)

    Pipelineable On-Line Encryption Farzaneh Abed1 , Scott Fluhrer2 , Christian Forler1, Eik List1 chosen-ciphertext attacks with pipelineability to support efficient implementations. POE combines a block POET, a provably secure on-line AE scheme, which inherits pipelineability and chosen

  4. Request for Online Payment Site ETSU Bursar Office

    E-Print Network [OSTI]

    Karsai, Istvan

    Request for Online Payment Site ETSU Bursar Office PO Box 70732 Date*: _____________ (*allow Ustore site with inventory a credit card merchant ID will be requested for ETSU's processor, development: The requirements and responsibilities of an Online Site Manager are: 1. The site manager must be a full-time ETSU

  5. A S D F : Automated, Online Fingerpointing for Hadoop1

    E-Print Network [OSTI]

    . ASDF is an automated, online fingerpointing framework that transparently extracts and parses different. We demonstrate ASDF's online fingerpointing for documented performance problems in Hadoop, under different workloads; our results indicate that ASDF incurs an average monitoring overhead of 0.38% of CPU

  6. Follow the money Understanding economics of online aggregation and advertising

    E-Print Network [OSTI]

    Greenberg, Albert

    Follow the money Understanding economics of online aggregation and advertising Phillipa Gill Vijay-scale collection and exploitation of personal infor- mation to drive targeted online advertisements has raised much in- formation is collected and how valuable it is for advertising. We use HTTP traces consisting

  7. Micro-blogging as Online Word of Mouth Branding

    E-Print Network [OSTI]

    Jansen, James

    Micro-blogging as Online Word of Mouth Branding Abstract In this paper, we report research results investigating micro-blogging as a form of online word of mouth branding. We analyzed 149,472 micro-blog postings containing branding comments, sentiments, and opinions. We investigated the overall structure of these micro-blog

  8. Online Appendix for "Liquidity Constraints and Consumer Bankruptcy

    E-Print Network [OSTI]

    Ottino, Julio M.

    Online Appendix for "Liquidity Constraints and Consumer Bankruptcy: Evidence from Tax Rebates" Tal of Rebates Online Appendix Table OA2 reports results of an alternative specification that attempts to estimate the long-run effect of the rebates. To do so, we pursue an alternative research design

  9. The social influence factor: Impact of online product review characteristics

    E-Print Network [OSTI]

    Al Hanbali, Ahmad

    The social influence factor: Impact of online product review characteristics on consumer purchasing of reviews and consumer purchasing decisions. The impact of online consumer reviews on consumer purchasing. The research challenge therefore entails review function characteristics and its impact on consumer purchasing

  10. Privacy-Preserving Friend Search over Online Social Networks

    E-Print Network [OSTI]

    International Association for Cryptologic Research (IACR)

    characterizing one's social position and significantly impact one's daily life. Over online social networks (OSNsPrivacy-Preserving Friend Search over Online Social Networks Huang Lin , Sherman S. M. Chow Tong University Abstract--Friendships or social contacts represent an impor- tant attribute

  11. Institute of Environment & Resources Online monitoring and control

    E-Print Network [OSTI]

    Institute of Environment & Resources Online monitoring and control of the biogas process Kanokwan Boe #12;#12;Online monitoring and control of the biogas process Kanokwan Boe Ph.D. Thesis May 2006 of the biogas process Cover: Torben Dolin & Julie Camilla Middleton Printed by: DTU tryk Institute

  12. Managing References using EndNote online: Pharmacy & Pharmacology

    E-Print Network [OSTI]

    Scheichl, Robert

    . In the catalogue search box, type in Web of Science 3. The open Web of Science database by clicking view online and then the Register link (drop-down under the Customize your experience option) 2. Enter your University of Bath email. Read and agree to terms use of use to complete registration 8. To access EndNote online in the future

  13. Massivizing Online Games:g Distributed Computing Challenges and

    E-Print Network [OSTI]

    Langendoen, Koen

    used to be art, may now be computing Online Gaming used to be multimedia is now DC g , y p g Online ­ the Netherlands ­ Europe( ) op founded 13th century pop: 100,000 pop.: 100,000 pop:16.5 M founded 1842 pop: 13

  14. Supporting Online Services in Environments Constrained by Communication

    E-Print Network [OSTI]

    demonstrated the qualitative and quantitative advantages of control- oriented design as a flexible approach, 1998 CMU-CS-98-172 School of Computer Science Carnegie Mellon University Pittsburgh, PA 15213 Thesis, their approaches do not handle access to online services well. This thesis examines the problem of designing online

  15. Supporting Online Services in Environments Constrained by Communication

    E-Print Network [OSTI]

    demonstrated the qualitative and quantitative advantages of control­ oriented design as a flexible approach, 1998 CMU­CS­98­172 School of Computer Science Carnegie Mellon University Pittsburgh, PA 15213 Thesis, their approaches do not handle access to online services well. This thesis examines the problem of designing online

  16. Online Housing Application, Room Selection & Dining Plan Instructions

    E-Print Network [OSTI]

    Cantlon, Jessica F.

    1 Online Housing Application, Room Selection & Dining Plan Instructions 2014-15 Table of Contents Financial Clearance 3 On Campus Housing Requirements 4 Selecting Alone 4 Selecting as a Group 4 Mutual Requests 4 Lottery Days and Times 4 Kinds of Housing 5 On-line Application Process 6 Room Selection Process

  17. ADAPTIVE ONLINE ENERGY SAVING FOR HETEROGENEOUS SENSOR Meikang Qiu1

    E-Print Network [OSTI]

    Sha, Edwin

    ADAPTIVE ONLINE ENERGY SAVING FOR HETEROGENEOUS SENSOR NETWORKS Meikang Qiu1 Jingtong Hu2 Edwin H-to-predict environments and have limited lifetime. We use a novel adaptive online energy saving (AOES) algorithm to save as a probabilistic random variable to save energy by se- lecting the best mode assignment for each node, which

  18. Managing References using EndNote online: Chemistry

    E-Print Network [OSTI]

    Scheichl, Robert

    search box, type in Web of Science 3. The open Web of Science database by clicking view online under and then the Register link (drop-down under the Customize your experience option) 2. Enter your University of Bath email. Read and agree to terms use of use to complete registration 8. To access EndNote online in the future

  19. Health Advisor An Online Game for Managing Healthcare Delivery

    E-Print Network [OSTI]

    Li, Mo

    Health Advisor An Online Game for Managing Healthcare Delivery Tennenbaum Institute Georgia, valuable change. Health Advisor The Tennenbaum Institute is developing, with partial support from IBM, an online game for managing healthcare delivery ­ Health Advisor. Each player manages a set of clients

  20. Managing References using EndNote online -Mechanical Engineering

    E-Print Network [OSTI]

    Scheichl, Robert

    : Export from the Library catalogue into Endnote online 1. Open the Library homepage and enter a search term into the Catalogue search box 2. Select an item from the results that are returned and click. In the catalogue search box, type in Web of Science 3. Open the Web of Science database by clicking View Online

  1. Resonance ionization laser ion sources for on-line isotope separators...

    Office of Scientific and Technical Information (OSTI)

    Resonance ionization laser ion sources for on-line isotope separators (invited) Citation Details In-Document Search Title: Resonance ionization laser ion sources for on-line...

  2. Modern Models for Learning Large-Scale Highly Skewed Online Advertising Data

    E-Print Network [OSTI]

    Zhang, Qiang

    2015-01-01

    prediction for display advertising. ACM Transactions on1 Introduction Online advertising, also called onlinecommon channels for online advertising. It involves both a

  3. Gravitational confinement of photons and matter from Induced Matter theory

    E-Print Network [OSTI]

    Mauricio Bellini

    2012-04-19

    Using an Extended Scharzschild-Anti de Sitter (ESAdS) metric here introduced, where the noncompact extra dimension is time-like, we study the gravitational confinement of matter and photons from a 5D vacuum. The important result here obtained is that the photon trajectories (in general, massless particles) are periodic. They are confined to a radius $r\\leq 2 m G/c^2$ by the gravitational field. Massive test particles are also gravitationally confined, but their trajectories are not periodic.

  4. Characterizing interactions in online social networks during exceptional events

    E-Print Network [OSTI]

    Omodei, Elisa; Arenas, Alex

    2015-01-01

    Nowadays, millions of people interact on a daily basis on online social media like Facebook and Twitter, where they share and discuss information about a wide variety of topics. In this paper, we focus on a specific online social network, Twitter, and we analyze multiple datasets each one consisting of individuals' online activity before, during and after an exceptional event in terms of volume of the communications registered. We consider important events that occurred in different arenas that range from policy to culture or science. For each dataset, the users' online activities are modeled by a multilayer network in which each layer conveys a different kind of interaction, specifically: retweeting, mentioning and replying. This representation allows us to unveil that these distinct types of interaction produce networks with different statistical properties, in particular concerning the degree distribution and the clustering structure. These results suggests that models of online activity cannot discard the...

  5. Flavored dark matter beyond minimal flavor violation

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Agrawal, Prateek; Blanke, Monika; Gemmler, Katrin

    2014-10-13

    We study the interplay of flavor and dark matter phenomenology for models of flavored dark matter interacting with quarks. We allow an arbitrary flavor structure in the coupling of dark matter with quarks. This coupling is assumed to be the only new source of violation of the Standard Model flavor symmetry extended by a U(3)x associated with the dark matter. We call this ansatz Dark Minimal Flavor Violation (DMFV) and highlight its various implications, including an unbroken discrete symmetry that can stabilize the dark matter. As an illustration we study a Dirac fermionic dark matter ? which transforms asmore »triplet under U(3)x , and is a singlet under the Standard Model. The dark matter couples to right-handed down-type quarks via a colored scalar mediator ? with a coupling ?. We identify a number of “flavor-safe” scenarios for the structure of ? which are beyond Minimal Flavor Violation. For dark matter and collider phenomenology we focus on the well-motivated case of b-flavored dark matter. The combined flavor and dark matter constraints on the parameter space of ? turn out to be interesting intersections of the individual ones. LHC constraints on simplified models of squarks and sbottoms can be adapted to our case, and monojet searches can be relevant if the spectrum is compressed.« less

  6. How cold is cold dark matter?

    SciTech Connect (OSTI)

    Armendariz-Picon, Cristian; Neelakanta, Jayanth T., E-mail: armen@phy.syr.edu, E-mail: jtneelak@syr.edu [Department of Physics, Syracuse University, Syracuse, NY 13244-1130 (United States)

    2014-03-01

    If cold dark matter consists of particles, these must be non-interacting and non-relativistic by definition. In most cold dark matter models however, dark matter particles inherit a non-vanishing velocity dispersion from interactions in the early universe, a velocity that redshifts with cosmic expansion but certainly remains non-zero. In this article, we place model-independent constraints on the dark matter temperature to mass ratio, whose square root determines the dark matter velocity dispersion. We only assume that dark matter particles decoupled kinetically while non-relativistic, when galactic scales had not entered the horizon yet, and that their momentum distribution has been Maxwellian since that time. Under these assumptions, using cosmic microwave background and matter power spectrum observations, we place upper limits on the temperature to mass ratio of cold dark matter today (away from collapsed structures). These limits imply that the present cold dark matter velocity dispersion has to be smaller than 54 m/s. Cold dark matter has to be quite cold, indeed.

  7. E Tap 487 (Class # 1132)/E Tap 687 (Class # 1139) Online Learning and Massive Open Online Courses (MOOCs) (3)

    E-Print Network [OSTI]

    Alexandrova, Ivana

    . This reflects growth in online education of nearly 300% between 2003 and 2013. Last year several new online. It will include an analysis of recent developments including the entry of Ivy League and other elite institutions will engage in discussions around access, students, faculty, learning effectiveness, and cost issues

  8. Dissipative hidden sector dark matter

    E-Print Network [OSTI]

    R. Foot; S. Vagnozzi

    2014-12-15

    A simple way of explaining dark matter without modifying known Standard Model physics is to require the existence of a hidden (dark) sector, which interacts with the visible one predominantly via gravity. We consider a hidden sector containing two stable particles charged under an unbroken $U(1)^{'}$ gauge symmetry, hence featuring dissipative interactions. The massless gauge field associated with this symmetry, the dark photon, can interact via kinetic mixing with the ordinary photon. In fact, such an interaction of strength $\\epsilon \\sim 10 ^{-9}$ appears to be necessary in order to explain galactic structure. We calculate the effect of this new physics on Big Bang Nucleosynthesis and its contribution to the relativistic energy density at Hydrogen recombination. We then examine the process of dark recombination, during which neutral dark states are formed, which is important for large-scale structure formation. Galactic structure is considered next, focussing on spiral and irregular galaxies. For these galaxies we modelled the dark matter halo (at the current epoch) as a dissipative plasma of dark matter particles, where the energy lost due to dissipation is compensated by the energy produced from ordinary supernovae (the core-collapse energy is transferred to the hidden sector via kinetic mixing induced processes in the supernova core). We find that such a dynamical halo model can reproduce several observed features of disk galaxies, including the cored density profile and the Tully-Fisher relation. We also discuss how elliptical and dwarf spheroidal galaxies could fit into this picture. Finally, these analyses are combined to set bounds on the parameter space of our model, which can serve as a guideline for future experimental searches.

  9. The CRESST Dark Matter Search

    E-Print Network [OSTI]

    B. Majorovits; G. Angloher; C. Bucci; P. Christ; C. Cozzini; F. von Feilitzsch; D. Hauff; S. Henry; Th. Jagemann; J. Jochum; H. Kraus; V. Mikhailik; J. Ninkovic; F. Petricca; W. Potzel; F. Proebst; Y. Ramachers; M. Razeti; W. Rau; W. Seidel; M. Stark; L. Stodolsky; A. J. B. Tolhurst; D. Wahl; W. Westphal; H. Wulandari

    2004-11-15

    We present first competitive results on WIMP dark matter using the phonon-light-detection technique. A particularly strong limit for WIMPs with coherent scattering results from selecting a region of the phonon-light plane corresponding to tungsten recoils. The observed count rate in the neutron band is compatible with the rate expected from neutron background. CRESST is presently being upgraded with a 66 channel SQUID readout system, a neutron shield and a muon veto system. This results in a significant improvement in sensitivity.

  10. Dark Matter in the MSSM

    SciTech Connect (OSTI)

    Cotta, R.C.; Gainer, J.S.; Hewett, J.L.; Rizzo, T.G.; /SLAC

    2009-04-07

    We have recently examined a large number of points in the parameter space of the phenomenological MSSM, the 19-dimensional parameter space of the CP-conserving MSSM with Minimal Flavor Violation. We determined whether each of these points satisfied existing experimental and theoretical constraints. This analysis provides insight into general features of the MSSM without reference to a particular SUSY breaking scenario or any other assumptions at the GUT scale. This study opens up new possibilities for SUSY phenomenology both in colliders and in astrophysical experiments. Here we shall discuss the implications of this analysis relevant to the study of dark matter.

  11. BBN with light dark matter

    SciTech Connect (OSTI)

    Berezhiani, Zurab [Dipartimento di Fisica, Università dell'Aquila, Via Vetoio, 67100 Coppito, L'Aquila (Italy); Dolgov, Aleksander; Tkachev, Igor, E-mail: Zurab.Berezhiani@aquila.infn.it, E-mail: dolgov@fe.infn.it, E-mail: tkachev@ms2.inr.ac.ru [Laboratory of Cosmology and Elementary Particles, Novosibirsk State University, Pirogov street 2, 630090 Novosibirsk (Russian Federation)

    2013-02-01

    Effects of light millicharged dark matter particles on primordial nucleosynthesis are considered. It is shown that if the mass of such particles is much smaller than the electron mass, they lead to strong overproduction of Helium-4. An agreement with observations can be achieved by non-vanishing lepton asymmetry. Baryon-to-photon ratio at BBN and neutrino-to-photon ratio both at BBN and at recombination are noticeably different as compared to the standard cosmological model. The latter ratio and possible lepton asymmetry could be checked by Planck. For higher mass of new particles the effect is much less pronounced and may even have opposite sign.

  12. Geometry Matters | The Ames Laboratory

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would likeUniverse (Journalvivo Low-Dose Low LET Ionizing RadiationSNACGeographyGeometry Matters

  13. The Cosmology of Composite Inelastic Dark Matter

    SciTech Connect (OSTI)

    Spier Moreira Alves, Daniele; Behbahani, Siavosh R.; /SLAC /Stanford U., ITP; Schuster, Philip; Wacker, Jay G.; /SLAC

    2011-08-19

    Composite dark matter is a natural setting for implementing inelastic dark matter - the O(100 keV) mass splitting arises from spin-spin interactions of constituent fermions. In models where the constituents are charged under an axial U(1) gauge symmetry that also couples to the Standard Model quarks, dark matter scatters inelastically off Standard Model nuclei and can explain the DAMA/LIBRA annual modulation signal. This article describes the early Universe cosmology of a minimal implementation of a composite inelastic dark matter model where the dark matter is a meson composed of a light and a heavy quark. The synthesis of the constituent quarks into dark hadrons results in several qualitatively different configurations of the resulting dark matter composition depending on the relative mass scales in the system.

  14. Baryon Destruction by Asymmetric Dark Matter

    E-Print Network [OSTI]

    Hooman Davoudiasl; David E. Morrissey; Kris Sigurdson; Sean Tulin

    2011-06-21

    We investigate new and unusual signals that arise in theories where dark matter is asymmetric and carries a net antibaryon number, as may occur when the dark matter abundance is linked to the baryon abundance. Antibaryonic dark matter can cause {\\it induced nucleon decay} by annihilating visible baryons through inelastic scattering. These processes lead to an effective nucleon lifetime of 10^{29}-10^{32} years in terrestrial nucleon decay experiments, if baryon number transfer between visible and dark sectors arises through new physics at the weak scale. The possibility of induced nucleon decay motivates a novel approach for direct detection of cosmic dark matter in nucleon decay experiments. Monojet searches (and related signatures) at hadron colliders also provide a complementary probe of weak-scale dark-matter--induced baryon number violation. Finally, we discuss the effects of baryon-destroying dark matter on stellar systems and show that it can be consistent with existing observations.

  15. Baryon Destruction by Asymmetric Dark Matter

    E-Print Network [OSTI]

    Davoudiasl, Hooman; Sigurdson, Kris; Tulin, Sean

    2011-01-01

    We investigate new and unusual signals that arise in theories where dark matter is asymmetric and carries a net antibaryon number, as may occur when the dark matter abundance is linked to the baryon abundance. Antibaryonic dark matter can cause {\\it induced nucleon decay} by annihilating visible baryons through inelastic scattering. These processes lead to an effective nucleon lifetime of 10^{29}-10^{32} years in terrestrial nucleon decay experiments, if baryon number transfer between visible and dark sectors arises through new physics at the weak scale. The possibility of induced nucleon decay motivates a novel approach for direct detection of cosmic dark matter in nucleon decay experiments. Monojet searches (and related signatures) at hadron colliders also provide a complementary probe of weak-scale dark-matter--induced baryon number violation. Finally, we discuss the effects of baryon-destroying dark matter on stellar systems and show that it can be consistent with existing observations.

  16. On-line tritium production monitor

    DOE Patents [OSTI]

    Mihalczo, John T. (Oak Ridge, TN)

    1993-01-01

    A scintillation optical fiber system for the on-line monitoring of nuclear reactions in an event-by-event manner is described. In the measurement of tritium production one or more optical fibers are coated with enriched .sup.6 Li and connected to standard scintillation counter circuitry. A neutron generated .sup.6 Li(n )T reaction occurs in the coated surface of .sup.6 Li-coated fiber to produce energetic alpha and triton particles one of which enters the optical fiber and scintillates light through the fiber to the counting circuit. The coated optical fibers can be provided with position sensitivity by placing a mirror at the free end of the fibers or by using pulse counting circuits at both ends of the fibers.

  17. On-line tritium production monitor

    DOE Patents [OSTI]

    Mihalczo, J.T.

    1993-11-23

    A scintillation optical fiber system for the on-line monitoring of nuclear reactions in an event-by-event manner is described. In the measurement of tritium production one or more optical fibers are coated with enriched {sup 6}Li and connected to standard scintillation counter circuitry. A neutron generated {sup 6}Li(n)T reaction occurs in the coated surface of {sup 6}Li-coated fiber to produce energetic alpha and triton particles one of which enters the optical fiber and scintillates light through the fiber to the counting circuit. The coated optical fibers can be provided with position sensitivity by placing a mirror at the free end of the fibers or by using pulse counting circuits at both ends of the fibers. 5 figures.

  18. Entropy and the Predictability of Online Life

    E-Print Network [OSTI]

    Sinatra, Roberta

    2014-01-01

    Using mobile phone records and information theory measures, our daily lives have been recently shown to follow strict statistical regularities, and our movement patterns are to a large extent predictable. Here, we apply entropy and predictability measures to two data sets of the behavioral actions and the mobility of a large number of players in the virtual universe of a massive multiplayer online game. We find that movements in virtual human lives follow the same high levels of predictability as offline mobility, where future movements can to some extent be predicted well if the temporal correlations of visited places are accounted for. Time series of behavioral actions show similar high levels of predictability, even when temporal correlations are neglected. Entropy conditional on specific behavioral actions reveals that in terms of predictability negative behavior has a wider variety than positive actions. The actions which contain information to best predict an individual's subsequent action are negative,...

  19. Online Monitoring System for Performance Fault Detection

    SciTech Connect (OSTI)

    Gioiosa, Roberto; Kestor, Gokcen; Kerbyson, Darren J.

    2014-05-19

    To achieve the exaFLOPS performance within a contain power budget, next supercomputers will feature hundreds of millions of components operating at low- and near-threshold voltage. As the probability that at least one of these components fails during the execution of an application approaches certainty, it seems unrealistic to expect that any run of a scientific application will not experience some performance faults. We believe that there is need of a new generation of light-weight performance and debugging tools that can be used online even during production runs of parallel applications and that can identify performance anomalies during the application execution. In this work we propose the design and implementation of a monitoring system that continuously inspects the evolution of run

  20. Dark matter as a cancer hazard

    E-Print Network [OSTI]

    Chashchina, Olga

    2015-01-01

    We comment on the paper "Dark Matter collisions with the Human Body" by K.~Freese and C.~Savage (Phys.\\ Lett.\\ B {\\bf 717}, 25 (2012) [arXiv:1204.1339]) and describe a dark matter model for which the results of the previous paper do not apply. Within this mirror dark matter model, potentially hazardous objects, mirror micrometeorites, can exist potentially leading to diseases triggered by multiple mutations, such as cancer.

  1. Dark matter as a cancer hazard

    E-Print Network [OSTI]

    Olga Chashchina; Zurab Silagadze

    2015-09-17

    We comment on the paper "Dark Matter collisions with the Human Body" by K.~Freese and C.~Savage (Phys.\\ Lett.\\ B {\\bf 717}, 25 (2012) [arXiv:1204.1339]) and describe a dark matter model for which the results of the previous paper do not apply. Within this mirror dark matter model, potentially hazardous objects, mirror micrometeorites, can exist potentially leading to diseases triggered by multiple mutations, such as cancer.

  2. Galaxy Structure, Dark Matter, and Galaxy Formation

    E-Print Network [OSTI]

    David H. Weinberg

    1996-10-01

    The structure of galaxies, the nature of dark matter, and the physics of galaxy formation were the interlocking themes of DM 1996: Dark and Visible Matter in Galaxies and Cosmological Implications. In this conference summary report, I review recent observational and theoretical advances in these areas, then describe highlights of the meeting and discuss their implications. I include as an appendix the lyrics of The Dark Matter Rap: A Cosmological History for the MTV Generation.

  3. Maximally incompressible neutron star matter

    E-Print Network [OSTI]

    Timothy S. Olson

    2000-12-07

    Relativistic kinetic theory, based on the Grad method of moments as developed by Israel and Stewart, is used to model viscous and thermal dissipation in neutron star matter and determine an upper limit on the maximum mass of neutron stars. In the context of kinetic theory, the equation of state must satisfy a set of constraints in order for the equilibrium states of the fluid to be thermodynamically stable and for perturbations from equilibrium to propagate causally via hyperbolic equations. Application of these constraints to neutron star matter restricts the stiffness of the most incompressible equation of state compatible with causality to be softer than the maximally incompressible equation of state that results from requiring the adiabatic sound speed to not exceed the speed of light. Using three equations of state based on experimental nucleon-nucleon scattering data and properties of light nuclei up to twice normal nuclear energy density, and the kinetic theory maximally incompressible equation of state at higher density, an upper limit on the maximum mass of neutron stars averaging 2.64 solar masses is derived.

  4. Interaction of gravitational waves with matter

    E-Print Network [OSTI]

    A. Cetoli; C. J. Pethick

    2011-10-03

    We develop a unified formalism for describing the interaction of gravitational waves with matter that clearly separates the effects of general relativity from those due to interactions in the matter. Using it, we derive a general expression for the dispersion of gravitational waves in matter in terms of correlation functions for the matter in flat spacetime. The self energy of a gravitational wave is shown to have contributions analogous to the paramagnetic and diamagnetic contributions to the self energy of an electromagnetic wave. We apply the formalism to some simple systems - free particles, an interacting scalar field, and a fermionic superfluid.

  5. Dark matter annihilation or unresolved astrophysical sources...

    Office of Scientific and Technical Information (OSTI)

    should be a powerful tool for revealing the CGB origin, and potentially for the first detection of dark matter annihilation. Authors: Ando, Shin'ichiro ; Komatsu, Eiichiro ;...

  6. Does Management Matter? Evidence from India

    E-Print Network [OSTI]

    Bloom, Nicholas; Eifert, Benn; Mahajan, Aprajit; McKenzie, David; Roberts, John

    2012-01-01

    DOES MANAGEMENT MATTER? EVIDENCE FROM INDIA Nicholas Bloombadly managed? Our experiment does not directly answer thisworks, imagine a plant that does not record quality defects.

  7. Does Management Matter? Evidence from India

    E-Print Network [OSTI]

    Bloom, Nicholas; Eifert, Benn; Mahajan, Aprajit; McKenzie, David; Roberts, John

    2012-01-01

    MATTER? EVIDENCE FROM INDIA Nicholas Bloom a , Benn Eifertorganization, productivity and India. Acknowledgements:textile industry? Despite India’s recent rapid growth, total

  8. PROBING DENSE NUCLEAR MATTER VIA NUCLEAR COLLISIONS

    E-Print Network [OSTI]

    Stocker, H.

    2012-01-01

    University of California. LBL-12095 Probing Dense NuclearMatter Nuclear Collisions* v~a H. Stocker, M.Gyulassy and J. Boguta Nuclear Science Division Lawrence

  9. Dark matter from decaying topological defects

    SciTech Connect (OSTI)

    Hindmarsh, Mark [Helsinki Institute of Physics, Gustaf Hällströmin katu, P.O. Box 64, 00014 Helsinki University (Finland); Kirk, Russell; West, Stephen M., E-mail: m.b.hindmarsh@sussex.ac.uk, E-mail: russell.kirk.2008@live.rhul.ac.uk, E-mail: stephen.west@rhul.ac.uk [Dept. of Physics, Royal Holloway University of London, Egham Hill, Egham, Surrey, TW20 0EX (United Kingdom)

    2014-03-01

    We study dark matter production by decaying topological defects, in particular cosmic strings. In topological defect or ''top-down'' (TD) scenarios, the dark matter injection rate varies as a power law with time with exponent p?4. We find a formula in closed form for the yield for all p < 3/2, which accurately reproduces the solution of the Boltzmann equation. We investigate two scenarios (p = 1, p = 7/6) motivated by cosmic strings which decay into TeV-scale states with a high branching fraction into dark matter particles. For dark matter models annihilating either by s-wave or p-wave, we find the regions of parameter space where the TD model can account for the dark matter relic density as measured by Planck. We find that topological defects can be the principal source of dark matter, even when the standard freeze-out calculation under-predicts the relic density and hence can lead to potentially large ''boost factor'' enhancements in the dark matter annihilation rate. We examine dark matter model-independent limits on this scenario arising from unitarity and discuss example model-dependent limits coming from indirect dark matter search experiments. In the four cases studied, the upper bound on G? for strings with an appreciable channel into TeV-scale states is significantly more stringent than the current Cosmic Microwave Background limits.

  10. Does Management Matter? Evidence from India

    E-Print Network [OSTI]

    Bloom, Nicholas; Eifert, Benn; Mahajan, Aprajit; McKenzie, David; Roberts, John

    2012-01-01

    DOES MANAGEMENT MATTER? EVIDENCE FROM INDIA Nicholas Bloomis whether differences in management practices across firmsTo investigate this, we ran a management field experiment on

  11. Dark galactic halos without dark matter

    E-Print Network [OSTI]

    R. K. Nesbet

    2015-03-03

    Using standard Einstein theory, baryonic mass cannot account for observed galactic rotation velocities and gravitational lensing, attributed to galactic dark matter halos. In contrast, theory constrained by Weyl conformal scaling symmetry explains observed galactic rotation in the halo region without invoking dark matter. An explanation of dark halos, gravitational lensing, and structural stabilization, without dark matter and consistent with conformal theory, is proposed here. Condensation of uniform primordial matter into a material cloud or galaxy vacates a large surrounding spherical halo. Within such an extended vacancy in the original cosmic background mass-energy density, conformal theory predicts centripetal acceleration of the observed magnitude.

  12. Universal Ownership: Why Environmental Externalities Matter to...

    Open Energy Info (EERE)

    Universal Ownership: Why Environmental Externalities Matter to Institutional Investors Jump to: navigation, search Tool Summary LAUNCH TOOL Name: Universal Ownership: Why...

  13. Dark Energy and Dark Matter Models

    E-Print Network [OSTI]

    Burra G. Sidharth

    2015-08-27

    We revisit the problems of dark energy and dark matter and several models designed to explain them, in the light of some latest findings.

  14. Dark Energy and Dark Matter Models

    E-Print Network [OSTI]

    Burra G. Sidharth

    2015-11-30

    We revisit the problems of dark energy and dark matter and several models designed to explain them, in the light of some latest findings.

  15. Trends Online: A Compendium of Data on Global Change

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    Data records are presented in multipage formats, each dealing with a specific site, region, or emissions species. The data records include tables; graphs; discussions of methods for collecting, measuring, and reporting the data; trends in the data, and references to literature providing further information. Instructions for citing specific data in Trends Online are provided for each compiled data set. All data appearing in Trends Online are available, on request, on digital media from CDIAC at no cost. [Copied from the Abstract to Trends Online at http://cdiac.ornl.gov/trends/abstract.htm

  16. The design, development and introduction of the Harwell library online ordering and cataloguing system LIBCAT

    E-Print Network [OSTI]

    Haynes, E M

    1983-01-01

    The design, development and introduction of the Harwell library online ordering and cataloguing system

  17. Dark Matter Searche with GLAST

    E-Print Network [OSTI]

    E. Nuss

    2007-04-20

    The Gamma-Ray Large Area Space Telescope (GLAST), scheduled to be launched in fall 2007, is the next generation satellite for high-energy gamma-ray astronomy. The Large Area Telescope (LAT), GLAST main instrument, with a wide field of view (> 2 sr), a large effective area (> 8000 cm^2 at 1 GeV) and 20 MeV - 300 GeV energy range, will provide excellent high energy gamma-ray observations for Dark Matter searches. In this paper we examine the potential of the LAT to detect gamma-rays coming from WIMPS annihilation in the context of supersymmetry. As an example, two search regions are investigated: the galactic center and the galactic satellites.

  18. Lepton-flavored dark matter

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Kile, Jennifer; Kobach, Andrew; Soni, Amarjit

    2015-05-01

    In this work, we address two paradoxes. The first is that the measured dark-matter relic density can be satisfied with new physics at O(100 GeV–1 TeV), while the null results from direct-detection experiments place lower bounds of O(10 TeV) on a new-physics scale. The second puzzle is that the severe suppression of lepton-flavor-violating processes involving electrons, e.g. ? ? 3e, ? ? e??, etc., implies that generic new-physics contributions to lepton interactions cannot exist below O(10–100 TeV), whereas the 3.6? deviation of the muon g – 2 from the standard model can be explained by a new physics scale more »TeV). Here, we suggest that it may not be a coincidence that both the muon g – 2 and the relic density can be satisfied by a new-physics scale ?1 TeV. We consider the possibility of a gauged lepton-flavor interaction that couples at tree level only to ?- and ?-flavored leptons and the dark sector. Dark matter thus interacts appreciably only with particles of ? and ? flavor at tree level and has loop-suppressed couplings to quarks and electrons. Remarkably, if such a gauged flavor interaction exists at a scale O(100 GeV–1 TeV), it allows for a consistent phenomenological framework, compatible with the muon g – 2, the relic density, direct detection, indirect detection, charged-lepton decays, neutrino trident production, and results from hadron and e?e? colliders. We suggest experimental tests for these ideas at colliders and for low-energy observables. (author)« less

  19. Lepton-flavored dark matter

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Kile, Jennifer; Kobach, Andrew; Soni, Amarjit

    2015-05-01

    In this work, we address two paradoxes. The first is that the measured dark-matter relic density can be satisfied with new physics at O(100 GeV–1 TeV), while the null results from direct-detection experiments place lower bounds of O(10 TeV) on a new-physics scale. The second puzzle is that the severe suppression of lepton-flavor-violating processes involving electrons, e.g. ? ? 3e, ? ? e??, etc., implies that generic new-physics contributions to lepton interactions cannot exist below O(10–100 TeV), whereas the 3.6? deviation of the muon g – 2 from the standard model can be explained by a new physics scale matter thus interacts appreciably only with particles of ? and ? flavor at tree level and has loop-suppressed couplings to quarks and electrons. Remarkably, if such a gauged flavor interaction exists at a scale O(100 GeV–1 TeV), it allows for a consistent phenomenological framework, compatible with the muon g – 2, the relic density, direct detection, indirect detection, charged-lepton decays, neutrino trident production, and results from hadron and e?e? colliders. We suggest experimental tests for these ideas at colliders and for low-energy observables. (author)

  20. Advanced particulate matter control apparatus and methods

    DOE Patents [OSTI]

    Miller, Stanley J. (Grand Forks, ND); Zhuang, Ye (Grand Forks, ND); Almlie, Jay C. (East Grand Forks, MN)

    2012-01-10

    Apparatus and methods for collection and removal of particulate matter, including fine particulate matter, from a gas stream, comprising a unique combination of high collection efficiency and ultralow pressure drop across the filter. The apparatus and method utilize simultaneous electrostatic precipitation and membrane filtration of a particular pore size, wherein electrostatic collection and filtration occur on the same surface.

  1. Probing nuclear matter with jet conversions 

    E-Print Network [OSTI]

    Liu, W.; Fries, Rainer J.

    2008-01-01

    We discuss the flavor of leading jet partons as a valuable probe of nuclear matter. We point out that the coupling of jets to nuclear matter naturally leads to an alteration of jet chemistry even at high transverse momentum PT. In particular...

  2. Viability of the Matter Bounce Scenario

    E-Print Network [OSTI]

    Jaume de Haro; Jaume Amorós

    2014-11-27

    It is shown that teleparallel $F({\\mathcal T})$ theories of gravity combined with Loop Quantum Cosmology support a Matter Bounce Scenario which is an alternative to the inflation scenario in the Big Bang paradigm. It is checked thatthese bouncing models provide theoretical data that fits well with the current observational data, allowing the viability of the Matter Bounce Scenario.

  3. Vision on tap : an online computer vision toolkit

    E-Print Network [OSTI]

    Chiu, Kevin (Kevin Geeyoung)

    2011-01-01

    In this thesis, we present an online toolkit, based on a combination of a Scratch-based programming environment and computer vision libraries, manifested as blocks within the environment, integrated with a community platform ...

  4. 59LINKS TO ONLINE RESOURCES | Career and Industry Information Websites

    E-Print Network [OSTI]

    Lee, Tonghun

    Society of Training and Development www.astd.org International Foundation of Employee Benefit Plans www Illinois MSA group Illinois MSF group Illinois MSTM group www.uiaa.org On-line Illinois alumni directory

  5. Online Modeling in the Process Industry for Energy Optimization 

    E-Print Network [OSTI]

    Alexander, J.

    1988-01-01

    "This paper discusses how steady state models are being used in the process industry to perform online energy optimization of steam and electrical systems. It presents process demands commonly found in the processing industry in terms of steam...

  6. Using evidence informed approval to create online learning resources

    E-Print Network [OSTI]

    Tracy, Frances; Jordan, Katy; Johnstone, Keith; Carmichael, Patrick

    2007-06-14

    into undergraduate teaching and learning within the Department; and to develop online resources to support student learning. The research focused on the second year ‘Part IB Plant & Microbial Sciences’ (IB PMS) Course. A combination of focus groups, dual...

  7. Northeast Home Heating Oil Reserve- Online Bidding System

    Broader source: Energy.gov [DOE]

    The U.S. Department of Energy has developed an on-line bidding system - an anonymous auction program - for the sale of product from the one million barrel Northeast Home Heating Oil Reserve.

  8. #2005-03-02641A Supporting Online Material

    E-Print Network [OSTI]

    Brocks, Jochen J.

    #2005-03-02641A Supporting Online Material Biomarker evidence for green and purple sulphur bacteria Accelerated Solvent Extractor. The extracts were reduced to 100 - 500 µl under a stream of purified nitrogen

  9. Chinese online BBS sphere : what BBS has brought to China

    E-Print Network [OSTI]

    Jin, Liwen, S.M. Massachusetts Institute of Technology

    2008-01-01

    This thesis explores various aspects of the online Bulletin Board System (BBS) world as they relate to the possibilities of the public sphere in China. It addresses two major questions: what has BBS brought to China where ...

  10. When Does Retargeting Work? Information Specificity in Online Advertising

    E-Print Network [OSTI]

    Lambrecht, Anja

    Firms can now offer personalized recommendations to consumers who return to their website, using consumers' previous browsing history on that website. In addition, online advertising has greatly improved in its use of ...

  11. Dynamic Online-Advertising Auctions as Stochastic Scheduling

    E-Print Network [OSTI]

    Menache, Ishai

    We study dynamic models of online-advertising auctions in the Internet: advertisers compete for space on a web page over multiple time periods, and the web page displays ads in differentiated slots based on their bids and ...

  12. Interleaving Cryptography and Mechanism Design The Case of Online Auctions

    E-Print Network [OSTI]

    International Association for Cryptologic Research (IACR)

    Interleaving Cryptography and Mechanism Design The Case of Online Auctions Edith Elkind 1. This auction mechanism is designed to provide (in this order) security, cognitive convenience, and round explicitly with the mechanism design. Keywords: auctions, cognitive costs, cryptography, mechanism design

  13. Oxford Colleges On-line Reports for Tutorials

    E-Print Network [OSTI]

    Wallace, Mark

    OxCORT Oxford Colleges On-line Reports for Tutorials Tutorial Office Role Version 4.4 BSP Training Overview of Tutorial reports.................................................................11 Overview of Revision Class reports.....................................................12 Overview of payments

  14. Oxford Colleges On-line Reports for Tutorials

    E-Print Network [OSTI]

    Wallace, Mark

    OxCORT Oxford Colleges On-line Reports for Tutorials Organising or Personal Tutor Role Version 4 of Tutorial reports...................................................................8 Overview of Revision Class reports.......................................................8 Overview of payments

  15. Oxford Colleges On-line Reports for Tutorials

    E-Print Network [OSTI]

    Wallace, Mark

    OxCORT Oxford Colleges On-line Reports for Tutorials Senior Tutor Role Version 4.4 BSP Training of Tutorial reports...................................................................8 Overview of Revision Class reports.......................................................8 Overview of payments

  16. Oxford Colleges On-line Reports for Tutorials

    E-Print Network [OSTI]

    Wallace, Mark

    OxCORT Oxford Colleges On-line Reports for Tutorials Tutor Role Version 4.5 BSP Training Team Overview of Tutorial reports...................................................................8 Overview of Revision Class reports.......................................................8 Report states

  17. On-line hydraulic state prediction for water distribution systems

    E-Print Network [OSTI]

    Whittle, Andrew

    This paper describes and demonstrates a method for on?line hydraulic state prediction in urban water networks. The proposed method uses a Predictor?Corrector (PC) approach in which a statistical data?driven algorithm is ...

  18. Comparing Appliance and Lighting Energy Costs Online Just Got...

    Broader source: Energy.gov (indexed) [DOE]

    We read reviews, compare specs, hunt for the best prices, and consider the long-term costs. The wealth of resources available online makes most of this very easy. One thing that...

  19. Kid's Survey Network : teaching data literacy with multiplayer online games

    E-Print Network [OSTI]

    Wong, Christopher, M. Eng. Massachusetts Institute of Technology

    2009-01-01

    Current advancements in technology have permeated modern society, especially among the younger generations of computer users. Today's youth have grown up accustomed to video games and online social networking as standard ...

  20. Temporary and Permanent Buyout Prices in Online Auctions

    E-Print Network [OSTI]

    Gupta, Shobhit

    Increasingly used in online auctions, buyout prices allow bidders to instantly purchase the item listed. We distinguish two types: a temporary buyout option disappears if a bid above the reserve price is made; a permanent ...

  1. Targeted online advertising : persuasion in an era of massless communication

    E-Print Network [OSTI]

    Baird, Eleanor Coumont

    2008-01-01

    In recent years, the decline of the mass media and the growth of a participatory and fragmented audience online have forced advertisers, agencies, and publishers to revise their thinking about delivering marketing messages ...

  2. Web Mapping and Online GIS Applications for Renewable Energy...

    Energy Savers [EERE]

    Web Mapping and Online GIS Applications for Renewable Energy EERE TAP Webinar Dan Getman and Ted Quinby May 26, 2010 Innovation for Our Energy Future Innovation for Our Energy...

  3. A strategic analysis of online grocery and its future outlook

    E-Print Network [OSTI]

    Xie, Kang, 1973-

    2004-01-01

    (cont.) are suggested to help future online grocers avoid the mistakes made by the earlier attempt, align their business strategy with the growing consumer interest in specialty foods and wellness services and find the ...

  4. Online appendix for Teacher Pay Reform and Productivity

    E-Print Network [OSTI]

    Sprott, Julien Clinton

    Online appendix for Teacher Pay Reform and Productivity by Sojourner, Mykerezi & West September 26 Figure 1: Effects of P4P-centered HRM reform on reading and math achievement as measured by the MCA

  5. Strongly Interacting Matter Matter at Very High Energy Density: 3 Lectures in Zakopane

    E-Print Network [OSTI]

    Larry McLerran

    2010-11-14

    These lectures concern the properties of strongly interacting matter at very high energy density. I begin with the Color Glass Condensate and the Glasma, matter that controls the earliest times in hadronic collisions. I then describe the Quark Gluon Plasma, matter produced from the thermalized remnants of the Glasma. Finally, I describe high density baryonic matter, in particular Quarkyonic matter. The discussion will be intuitive and based on simple structural aspects of QCD. There will be some discussion of experimental tests of these ideas.

  6. Dimensionless constants, cosmology and other dark matters

    E-Print Network [OSTI]

    Max Tegmark; Anthony Aguirre; Martin J Rees; Frank Wilczek

    2006-01-11

    We identify 31 dimensionless physical constants required by particle physics and cosmology, and emphasize that both microphysical constraints and selection effects might help elucidate their origin. Axion cosmology provides an instructive example, in which these two kinds of arguments must both be taken into account, and work well together. If a Peccei-Quinn phase transition occurred before or during inflation, then the axion dark matter density will vary from place to place with a probability distribution. By calculating the net dark matter halo formation rate as a function of all four relevant cosmological parameters and assessing other constraints, we find that this probability distribution, computed at stable solar systems, is arguably peaked near the observed dark matter density. If cosmologically relevant WIMP dark matter is discovered, then one naturally expects comparable densities of WIMPs and axions, making it important to follow up with precision measurements to determine whether WIMPs account for all of the dark matter or merely part of it.

  7. Dark Matter Studies Entrain Nuclear Physics

    E-Print Network [OSTI]

    Susan Gardner; George Fuller

    2013-03-19

    We review theoretically well-motivated dark-matter candidates, and pathways to their discovery, in the light of recent results from collider physics, astrophysics, and cosmology. Taken in aggregate, these encourage broader thinking in regards to possible dark-matter candidates --- dark-matter need not be made of "WIMPs," i.e., elementary particles with weak-scale masses and interactions. Facilities dedicated to nuclear physics are well-poised to investigate certain non-WIMP models. In parallel to this, developments in observational cosmology permit probes of the relativistic energy density at early epochs and thus provide new ways to constrain dark-matter models, provided nuclear physics inputs are sufficiently well-known. The emerging confluence of accelerator, astrophysical, and cosmological constraints permit searches for dark-matter candidates in a greater range of masses and interaction strengths than heretofore possible.

  8. A reactor core on-line monitoring program - COMP

    SciTech Connect (OSTI)

    Wang, C.; Wu, H.; Cao, L.

    2012-07-01

    A program named COMP is developed for on-line monitoring PWRs' in-core power distribution in this paper. Harmonics expansion method is used in COMP. The Unit 1 reactor of Daya Bay Nuclear Power Plant (Daya Bay NPP) in China is considered for verification. The numerical results show that the maximum relative error between measurement and reconstruction results from COMP is less than 5%, and the computing time is short, indicating that COMP is capable for online monitoring PWRs. (authors)

  9. Detecting the invisible universe with neutrinos and dark matter

    E-Print Network [OSTI]

    Kaboth, Asher C. (Asher Cunningham)

    2012-01-01

    Recent work in astrophysics has show that most of the matter in the universe is non-luminous. This work investigates two searches for non-luminous matter: hot dark matter formed from cosmic relic neutrinos from the Big ...

  10. On-line subsea multiphase flow measurement

    SciTech Connect (OSTI)

    High, G.; Frantzen, K.H.; Marshall, M.

    1995-12-31

    This paper describes the final detailed design, engineering, and installation phase of a Joint Industry Program to qualify a robust subsea multiphase flowmeter module for long-term installation on a North Sea manifold tie-in. Multiphase subsea production has become a common method of hydrocarbon recovery in all areas of offshore E and P. In the North Sea, many developments are subsea satellites with multiphase well-fluids being comingled prior to processing. The system described meets this challenge by offering a cost effective solution to real-time well monitoring as an alternative to the conventional test separator, removing the need for test lines and shutting in wells for testing. The multiphase instrument allows on-line well fluid analysis, and is also an important tool for reservoir management and field analysis, and provides a means of implementing field allocation metering thereby simplifying small marginal field developments. This project is one of the first subsea multiphase flowmeter installations engineered for long-term subsea service, and designed as an integrated component of the subsea production control system.

  11. Ethan Burns (UNH) Iterative-deepening Search with On-line Tree Size Prediction 1 / 30 Iterative-deepening Search with On-line Tree Size Prediction

    E-Print Network [OSTI]

    Ruml, Wheeler

    Ethan Burns (UNH) Iterative-deepening Search with On-line Tree Size Prediction ­ 1 / 30 Iterative-deepening Search with On-line Tree Size Prediction Ethan Burns and Wheeler Ruml {eaburns, ruml} at cs Evaluation Ethan Burns (UNH) Iterative-deepening Search with On-line Tree Size Prediction ­ 2 / 30 On

  12. Reduction of Transient Particulate Matter Spikes with Decision...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Transient Particulate Matter Spikes with Decision Tree Based Control Reduction of Transient Particulate Matter Spikes with Decision Tree Based Control Using a non-parametric...

  13. Social Media and Messages that Matter - Top Tips and Tools |...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    and Messages that Matter - Top Tips and Tools Social Media and Messages that Matter - Top Tips and Tools Better Buildings Residential Network Peer Exchange Call Series: Social...

  14. How Much Do Local Regulations Matter? Exploring the Impact of...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Regulations Matter? Exploring the Impact of Permitting and Local Regulatory Processes on PV Prices in the United States How Much Do Local Regulations Matter? Exploring the Impact...

  15. How Much Do Local Regulations Matter? Exploring the Impact of...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Matter? Exploring the Impact of Permitting and Local Regulatory Processes on PV Prices in the United States How Much Do Local Regulations Matter? Exploring the Impact of...

  16. JETS OF NUCLEAR MATTER FROM HIGH ENERGY HEAVY ION COLLISIONS

    E-Print Network [OSTI]

    Stocker, H.

    2013-01-01

    of California. LBL-11774 Jets of Nuclear Matter from Highclusters. Strongly correlated jets of nuclear matter areExperimental analysis of the jet phenomena is in progress.

  17. Properties of nuclear matter within the JISP16NNinteraction ...

    Office of Scientific and Technical Information (OSTI)

    Properties of nuclear matter within the JISP16NNinteraction Citation Details In-Document Search Title: Properties of nuclear matter within the JISP16NNinteraction Authors:...

  18. The Right Technology Matters: The Importantce of Public-Private...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    The Right Technology Matters: The Importantce of Public-Private Partnerships for Engine Development The Right Technology Matters: The Importantce of Public-Private Partnerships for...

  19. Osmotic pressure of matter and vacuum energy

    E-Print Network [OSTI]

    G. E. Volovik

    2009-10-04

    The walls of the box which contains matter represent a membrane that allows the relativistic quantum vacuum to pass but not matter. That is why the pressure of matter in the box may be considered as the analog of the osmotic pressure. However, we demonstrate that the osmotic pressure of matter is modified due to interaction of matter with vacuum. This interaction induces the nonzero negative vacuum pressure inside the box, as a result the measured osmotic pressure becomes smaller than the matter pressure. As distinct from the Casimir effect, this induced vacuum pressure is the bulk effect and does not depend on the size of the box. This effect dominates in the thermodynamic limit of the infinite volume of the box. Analog of this effect has been observed in the dilute solution of 3He in liquid 4He, where the superfluid 4He plays the role of the non-relativistic quantum vacuum, and 3He atoms play the role of matter.

  20. Asymmetric dark matter in braneworld cosmology

    SciTech Connect (OSTI)

    Meehan, Michael T.; Whittingham, Ian B., E-mail: Michael.Meehan@my.jcu.edu.au, E-mail: Ian.Whittingham@jcu.edu.au [School of Engineering and Physical Sciences, James Cook University, Townsville, 4811 Australia (Australia)

    2014-06-01

    We investigate the effect of a braneworld expansion era on the relic density of asymmetric dark matter. We find that the enhanced expansion rate in the early universe predicted by the Randall-Sundrum II (RSII) model leads to earlier particle freeze-out and an enhanced relic density. This effect has been observed previously by Okada and Seto (2004) for symmetric dark matter models and here we extend their results to the case of asymmetric dark matter. We also discuss the enhanced asymmetric annihilation rate in the braneworld scenario and its implications for indirect detection experiments.

  1. Hidden photons in connection to dark matter

    SciTech Connect (OSTI)

    Andreas, Sarah; Ringwald, Andreas [Deutsches Elektronen-Synchrotron DESY, Hamburg (Germany); Goodsell, Mark D. [CPhT, Ecole Polytechnique, Palaiseau (France)

    2013-11-07

    Light extra U(1) gauge bosons, so called hidden photons, which reside in a hidden sector have attracted much attention since they are a well motivated feature of many scenarios beyond the Standard Model and furthermore could mediate the interaction with hidden sector dark matter. We review limits on hidden photons from past electron beam dump experiments including two new limits from such experiments at KEK and Orsay. In addition, we study the possibility of having dark matter in the hidden sector. A simple toy model and different supersymmetric realisations are shown to provide viable dark matter candidates in the hidden sector that are in agreement with recent direct detection limits.

  2. Baryonic pinching of galactic dark matter halos

    SciTech Connect (OSTI)

    Gustafsson, Michael; Fairbairn, Malcolm; Sommer-Larsen, Jesper [Cosmology, Particle Astrophysics and String Theory, Department of Physics, Stockholm University, AlbaNova University Center, SE-106 91, Stockholm (Sweden); Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen (Denmark)

    2006-12-15

    High resolution cosmological N-body simulations of four galaxy-scale dark matter halos are compared to corresponding N-body/hydrodynamical simulations containing dark matter, stars and gas. The simulations without baryons share features with others described in the literature in that the dark matter density slope continuously decreases towards the center, with a density {rho}{sub DM}{proportional_to}r{sup -1.3{+-}}{sup 0.2}, at about 1% of the virial radius for our Milky Way sized galaxies. The central cusps in the simulations which also contain baryons steepen significantly, to {rho}{sub DM}{proportional_to}r{sup -1.9{+-}}{sup 0.2}, with an indication of the inner logarithmic slope converging. Models of adiabatic contraction of dark matter halos due to the central buildup of stellar/gaseous galaxies are examined. The simplest and most commonly used model, by Blumenthal et al., is shown to overestimate the central dark matter density considerably. A modified model proposed by Gnedin et al. is tested and it is shown that, while it is a considerable improvement, it is not perfect. Moreover, it is found that the contraction parameters in their model not only depend on the orbital structure of the dark-matter-only halos but also on the stellar feedback prescription which is most relevant for the baryonic distribution. Implications for dark matter annihilation at the galactic center are discussed and it is found that, although our simulations show a considerable reduced dark matter halo contraction as compared to the Blumenthal et al. model, the fluxes from dark matter annihilation are still expected to be enhanced by at least a factor of a hundred, as compared to dark-matter-only halos. Finally, it is shown that, while dark-matter-only halos are typically prolate, the dark matter halos containing baryons are mildly oblate with minor-to-major axis ratios of c/a=0.73{+-}0.11, with their flattening aligned with the central baryonic disks.

  3. Brane World Dynamics and Adiabatic Matter creation

    E-Print Network [OSTI]

    P. Gopakumar; G. V. Vijayagovindan

    2006-04-10

    We have treated the adiabatic matter creation process in various three-brane models by applying thermodynamics of open systems. The matter creation rate is found to affect the evolution of scale factor and energy density of the universe. We find modification at early stages of cosmic dynamics. In GB and RS brane worlds, by chosing appropriate parameters we obtain standard scenario, while the warped DGP model has different Friedmann equations. During later stages, since the matter creation is negligible the evolution reduces to FRW expansion, in RS and GB models.

  4. Quintessence with quadratic coupling to dark matter

    SciTech Connect (OSTI)

    Boehmer, Christian G.; Chan, Nyein; Caldera-Cabral, Gabriela; Lazkoz, Ruth; Maartens, Roy

    2010-04-15

    We introduce a new form of coupling between dark energy and dark matter that is quadratic in their energy densities. Then we investigate the background dynamics when dark energy is in the form of exponential quintessence. The three types of quadratic coupling all admit late-time accelerating critical points, but these are not scaling solutions. We also show that two types of coupling allow for a suitable matter era at early times and acceleration at late times, while the third type of coupling does not admit a suitable matter era.

  5. Direct Detection of Cold Dark Matter

    E-Print Network [OSTI]

    Laura Baudis

    2007-11-25

    We know from cosmological and astrophysical observations that more than 80% of the matter density in the Universe is non-luminous, or dark. This non-baryonic dark matter could be composed of neutral, heavy particles, which were non-relativistic, or 'cold', when they decoupled from ordinary matter. I will review the direct detection methods of these hypothetical particles via their interactions with nuclei in ultra-low background, deep underground experiments. The emphasis is on most recent results and on the status of near future projects.

  6. LIGHT PHOTINOS AS DARK MATTER

    E-Print Network [OSTI]

    Glennys R. Farrar; Edward W. Kolb

    1995-04-24

    There are good reasons to consider models of low-energy supersymmetry with very light photinos and gluinos. In a wide class of models the lightest $R$-odd, color-singlet state containing a gluino, the $\\r0$, has a mass in the 1-2 GeV range and the slightly lighter photino, $\\pho$, would survive as the relic $R$-odd species. For the light photino masses considered here, previous calculations resulted in an unacceptable photino relic abundance. But we point out that processes other than photino self-annihilation determine the relic abundance when the photino and $R^0$ are close in mass. Including $\\r0\\longleftrightarrow\\pho$ processes, we find that the photino relic abundance is most sensitive to the $\\r0$-to-$\\pho$ mass ratio, and within model uncertainties, a critical density in photinos may be obtained for an $\\r0$-to-$\\pho$ mass ratio in the range 1.2 to 2.2. We propose photinos in the mass range of 500 MeV to 1.6 GeV as a dark matter candidate, and discuss a strategy to test the hypothesis.

  7. Photonic dark matter portal revisited

    E-Print Network [OSTI]

    S. A. Alavi; F S Kazemian

    2015-11-18

    In our previous paper [1], we studied a model of dark matter (DM) in which the hidden sector interacts with standard model particles via a hidden photonic portal (HP). We investigated the effects of this new interaction on the hydrogen atom and obtained an upper bound for the coupling of the model. In this work, we study the effects of HP on two interesting exotic atoms namely muonium and positronium. We obtain a tighter upper limit on the coupling. We also calculate the change (shift) in the Aharonov-Bohm phase due to HP and find that the phase shift is negligibly small (for DM particles mass in the GeV range). Recently a 3.5 keV X ray line signal observed in the spectrum of 73 galaxy clusters, reported by the XXM-Newton X ray observatory. Since in HP model the DM particles can decay directly into photons, so we finally calculate the value of the coupling constant f using the condition Delta E=3.5 keV.

  8. Dark matter burners: Preliminary estimates

    E-Print Network [OSTI]

    I. V. Moskalenko; L. L. Wai

    2007-02-24

    We show that a star orbiting close enough to an adiabatically grown supermassive black hole can capture a large number of weakly interacting massive particles (WIMPs) during its lifetime. WIMP annihilation energy release in low- to medium-mass stars is comparable with or even exceeds the luminosity of such stars due to thermonuclear burning. The excessive energy release in the stellar core may result in an evolution scenario different from what is expected for a regular star. The model thus predicts the existence of unusual stars within the central parsec of galactic nuclei. If found, such stars would provide evidence for the existence of particle dark matter. White dwarfs seem to be the most promising candidates to look for. The signature of a white dwarf burning WIMPs would be a very hot star with mass and radius characteristic for a white dwarf, but with luminosity exceeding the typical luminosity of a white dwarf by orders of magnitude <50L_sun. A white dwarf with a highly eccentric orbit around the central black hole may exhibit variations in brightness correlated with the orbital phase.

  9. DEAP-3600 Dark Matter Search

    E-Print Network [OSTI]

    P. -A. Amaudruz; M. Batygov; B. Beltran; J. Bonatt; M. G. Boulay; B. Broerman; J. F. Bueno; A. Butcher; B. Cai; M. Chen; R. Chouinard; B. T. Cleveland; K. Dering; J. DiGioseffo; F. Duncan; T. Flower; R. Ford; P. Giampa; P. Gorel; K. Graham; D. R. Grant; E. Guliyev; A. L. Hallin; M. Hamstra; P. Harvey; C. J. Jillings; M. Ku?niak; I. Lawson; O. Li; P. Liimatainen; P. Majewski; A. B. McDonald; T. McElroy; K. McFarlane; J. Monroe; A. Muir; C. Nantais; C. Ng; A. J. Noble; C. Ouellet; K. Palladino; P. Pasuthip; S. J. M. Peeters; T. Pollmann; W. Rau; F. Retière; N. Seeburn; K. Singhrao; P. Skensved; B. Smith; T. Sonley; J. Tang; E. Vázquez-Jáuregui; L. Veloce; J. Walding; M. Ward

    2014-10-27

    The DEAP-3600 experiment is located 2 km underground at SNOLAB, in Sudbury, Ontario. It is a single-phase detector that searches for dark matter particle interactions within a 1000-kg fiducial mass target of liquid argon. A first generation prototype detector (DEAP-1) with a 7-kg liquid argon target mass demonstrated a high level of pulse-shape discrimination (PSD) for reducing $\\beta$/$\\gamma$ backgrounds and helped to develop low radioactivity techniques to mitigate surface-related $\\alpha$ backgrounds. Construction of the DEAP-3600 detector is nearly complete and commissioning is starting in 2014. The target sensitivity to spin-independent scattering of Weakly Interacting Massive Particles (WIMPs) on nucleons of 10$^{-46}$ cm$^2$ will allow one order of magnitude improvement in sensitivity over current searches at 100 GeV WIMP mass. This paper presents an overview and status of the DEAP-3600 project and discusses plans for a future multi-tonne experiment, DEAP-50T.

  10. Dark Matter Triggers of Supernovae

    E-Print Network [OSTI]

    Graham, Peter W; Varela, Jaime

    2015-01-01

    The transit of primordial black holes through a white dwarf causes localized heating around the trajectory of the black hole through dynamical friction. For sufficiently massive black holes, this heat can initiate runaway thermonuclear fusion causing the white dwarf to explode as a supernova. The shape of the observed distribution of white dwarfs with masses up to $1.25 M_{\\odot}$ rules out primordial black holes with masses $\\sim 10^{19}$ gm - $10^{20}$ gm as a dominant constituent of the local dark matter density. Black holes with masses as large as $10^{24}$ gm will be excluded if recent observations by the NuStar collaboration of a population of white dwarfs near the galactic center are confirmed. Black holes in the mass range $10^{20}$ gm - $10^{22}$ gm are also constrained by the observed supernova rate, though these bounds are subject to astrophysical uncertainties. These bounds can be further strengthened through measurements of white dwarf binaries in gravitational wave observatories. The mechanism p...

  11. EPJ ESoft Matter and Biological Physics

    E-Print Network [OSTI]

    Roman, Benoît

    February 2014 Published online: 25 April 2014 ­ c EDP Sciences / Societ`a Italiana di Fisica / Springer based on a balance between stretching and curvature energies on defocused states. This criterion is made a renewed vision of elastic singularities as a thermodynamic condensed phase where stress is focused

  12. Superheavy sterile neutrinos as dark matter 

    E-Print Network [OSTI]

    Tang, Yongjun

    2000-01-01

    neutrinos as a dark matter candidate, produced through MSW conversion of active neutrinos. Recently Allen proposed a different nonthermal mechanism for the production of superheavy sterile neutrinos. Such neutrinos are predicted by an SO(10) grand...

  13. Exploring the Nature of Matter | Jefferson Lab

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    of matter." And you might ask, what do they mean? At Jefferson Laboratory, we scatter electrons like Hofstadter did in the '50s when he explored nuclei. That's why one of our roads...

  14. A Scenario of Heavy Baryonic Dark Matter

    E-Print Network [OSTI]

    Huo, Ran; Tsai, Yue-Lin Sming; Yanagida, Tsutomu T

    2015-01-01

    We consider a general class of models in which dark matter is a composite baryonic and antibaryonic particle of some hidden vector-like strong gauge theory. The model building provides simple answers to two basic questions: Annihilation between dark baryon and antibaryon saturates the unitarity bound, which in thermal freeze out predicts the scale of dark matter particle to be about 150 TeV. And the dark matter stability is a result of the accidental dark baryon number, which can still be violated by operators suppressed by large scales, leading to tiny decay rate. We show that annihilation between dark baryon and anti-baryon seems difficult to be detected in the galaxy center in the near future. On the other hand in the minimal model of $SU(3)$ hidden strong gauge group with a Planck scale suppression, the dark matter life time happens to be marginal to the current detection bound, and can explain the current AMS-02 antiproton results.

  15. Particulate matter in the central subtropical Pacific 

    E-Print Network [OSTI]

    Colgan, Annette Renee

    1995-01-01

    The distribution of particulate matter (PM) in the Central Subtropical Pacific and its relationships with water masses and currents were determined from optical and hydrographic data. Beam attenuation data were collected with a Sea Tech...

  16. Characterisation of carbonaceous particulate matter in Edinburgh 

    E-Print Network [OSTI]

    Hammonds, Mark David

    2012-06-22

    Airborne particulate matter (PM) has important harmful effects on human health, as well as a number of other important atmospheric effects. Although progress has been made in understanding the sources and effects of PM, ...

  17. Low-scale seesaw and dark matter

    E-Print Network [OSTI]

    M. Fabbrichesi; S. Petcov

    2013-04-15

    We discuss how two birds---the little hierarchy problem of low-scale type-I seesaw models and the search for a viable dark matter candidate---are (proverbially) killed by one stone: a new inert scalar state

  18. Antigravitation, Dark Energy, Dark Matter - Alternative Solution

    E-Print Network [OSTI]

    Alexeev, Boris V

    2009-01-01

    Collisional damping of gravitational waves in the Newtonian matter is investigated. The generalized theory of Landau damping is applied to the gravitational physical systems in the context of the plasma gravitational analogy.

  19. Indirect dark matter search with AMS-02

    E-Print Network [OSTI]

    S. Di Falco

    2006-07-06

    The Alpha Magnetic Spectrometer (AMS), to be installed on the International Space Station, will provide data on cosmic radiations in the energy range from 0.5 GeV to 3 TeV. The main physics goals are the anti-matter and the dark matter searches. Observations and cosmology indicate that the Universe may include a large amount of unknown Dark Matter. It should be composed of non baryonic Weakly Interacting Massive Particles (WIMP). In R-parity conserving models a good WIMP candidate is the lightest SUSY particle. AMS offers a unique opportunity to study simultaneously SUSY dark matter in three decay channels resulting from the neutralino annihilation: e+, antiproton and gamma. Either in the SUSY frame and in alternative scenarios (like extra-dimensions) the expected flux sensitivities as a function of energy in 3 year exposure for the e+/e- ratio, gamma and antiproton yields are presented.

  20. Disentangling Dark Matter Dynamics with Directional Detection

    SciTech Connect (OSTI)

    Lisanti, Mariangela; Wacker, Jay G.; /SLAC

    2009-12-16

    Inelastic dark matter reconciles the DAMA anomaly with other null direct detection experiments and points to a non-minimal structure in the dark matter sector. In addition to the dominant inelastic interaction, dark matter scattering may have a subdominant elastic component. If these elastic interactions are suppressed at low momentum transfer, they will have similar nuclear recoil spectra to inelastic scattering events. While upcoming direct detection experiments will see strong signals from such models, they may not be able to unambiguously determine the presence of the subdominant elastic scattering from the recoil spectra alone. We show that directional detection experiments can separate elastic and inelastic scattering events and discover the underlying dynamics of dark matter models.

  1. Shocking Signals of Dark Matter Annihilation

    E-Print Network [OSTI]

    Davis, Jonathan H; Boehm, Celine; Kotera, Kumiko; Norman, Colin

    2015-01-01

    We examine whether charged particles injected by self-annihilating Dark Matter into regions undergoing Diffuse Shock Acceleration (DSA) can be accelerated to high energies. We consider three astrophysical sites where shock acceleration is supposed to occur, namely the Galactic Centre, galaxy clusters and Active Galactic Nuclei (AGN). For the Milky Way, we find that the acceleration of cosmic rays injected by dark matter could lead to a bump in the cosmic ray spectrum provided that the product of the efficiency of the acceleration mechanism and the concentration of DM particles is high enough. Among the various acceleration sources that we consider (namely supernova remnants (SNRs), Fermi bubbles and AGN jets), we find that the Fermi bubbles are a potentially more efficient accelerator than SNRs. However both could in principle accelerate electrons and protons injected by dark matter to very high energies. At the extragalactic level, the acceleration of dark matter annihilation products could be responsible fo...

  2. Scalar Dark Matter From Theory Space

    SciTech Connect (OSTI)

    Birkedal-Hansen, Andreas; Wacker, Jay G.

    2003-12-26

    The scalar dark matter candidate in a prototypical theory space little Higgs model is investigated. We review all details of the model pertinent to a relic density calculation. We perform a thermal relic density calculation including couplings to the gauge and Higgs sectors of the model. We find two regions of parameter space that give acceptable dark matter abundances. The first region has a dark matter candidate with a mass {Omicron}(100 GeV), the second region has a candidate with a mass greater than {Omicron}(500 GeV). The dark matter candidate in either region is an admixture of an SU(2) triplet and an SU(2) singlet, thereby constituting a possible WIMP (weakly interacting massive particle).

  3. Light Dark Matter Annihilations into Two Photons

    E-Print Network [OSTI]

    C. Boehm; J. Orloff; P. Salati

    2006-07-19

    We compute the pair annihilation cross section of light (spin-0) dark matter particles into two photons and discuss the detectability of the monochromatic line associated with these annihilations.

  4. Modeling the strangeness content of hadronic matter

    E-Print Network [OSTI]

    G. Toledo Sanchez; J. Piekarewicz

    2001-09-06

    The strangeness content of hadronic matter is studied in a string-flip model that reproduces various aspects of the QCD-inspired phenomenology, such as quark clustering at low density and color deconfinement at high density, while avoiding long range van der Waals forces. Hadronic matter is modeled in terms of its quark constituents by taking into account its internal flavor (u,d,s) and color (red, blue, green) degrees of freedom. Variational Monte-Carlo simulations in three spatial dimensions are performed for the ground-state energy of the system. The onset of the transition to strange matter is found to be influenced by weak, yet not negligible, clustering correlations. The phase diagram of the system displays an interesting structure containing both continuous and discontinuous phase transitions. Strange matter is found to be absolutely stable in the model.

  5. Manual for Classified Matter Protection and Control

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    1998-01-09

    Provides detailed requirements for the protection and control of classified matter which supplement DOE O 471.2A. Cancels DOE M 471.2-1 dated 09/26/1995.

  6. Nuclear Matter with Relativistic Quark Dynamics

    SciTech Connect (OSTI)

    Suisso, E.F.; Batista, E.F.; Araujo, W.R.B. de; Frederico, T.; Carlson, B.V. [Dep. de Fisica, Instituto Tecnologico da Aeronautca, Centro Tecnico Aeroespacial, 12.228-901, Sao Jose dos Campos, Sao Paulo (Brazil)

    2004-12-02

    We investigate a quark-meson coupling model of the nuclear matter with a light-front nucleon model, where the quarks interact with flavor independent contact force. We found results comparable to the ones obtained with a confining interaction.

  7. Interaction of Radiation with Matter Electrons

    E-Print Network [OSTI]

    Massey, Thomas N.

    Module 2 Interaction of Radiation with Matter · Gammas · Electrons · Charged Particles · Neutron of mass. · Energy from radiation only deposited if it interacts with the material. · Only the amount;Pair Production #12;Gamma Interaction with Water #12;http://physics

  8. Scalar Dark Matter: Direct vs. Indirect Detection

    E-Print Network [OSTI]

    Michael Duerr; Pavel Fileviez Perez; Juri Smirnov

    2015-09-14

    We revisit the simplest model for dark matter. In this context the dark matter candidate is a real scalar field which interacts with the Standard Model particles through the Higgs portal. We discuss the relic density constraints as well as the predictions for direct and indirect detection. The final state radiation processes are investigated in order to understand the visibility of the gamma lines from dark matter annihilation. We find two regions where one could observe the gamma lines at gamma-ray telescopes. We point out that the region where the dark matter mass is between 100 and 300 GeV can be tested in the near future at direct and indirect detection experiments.

  9. Scalar Dark Matter: Direct vs. Indirect Detection

    E-Print Network [OSTI]

    Duerr, Michael; Smirnov, Juri

    2015-01-01

    We revisit the simplest model for dark matter. In this context the dark matter candidate is a real scalar field which interacts with the Standard Model particles through the Higgs portal. We discuss the relic density constraints as well as the predictions for direct and indirect detection. The final state radiation processes are investigated in order to understand the visibility of the gamma lines from dark matter annihilation. We find two regions where one could observe the gamma lines at gamma-ray telescopes. We point out that the region where the dark matter mass is between 100 and 300 GeV can be tested in the near future at direct and indirect detection experiments.

  10. Antigravitation, Dark Energy, Dark Matter - Alternative Solution

    E-Print Network [OSTI]

    Boris V. Alexeev

    2009-09-04

    Collisional damping of gravitational waves in the Newtonian matter is investigated. The generalized theory of Landau damping is applied to the gravitational physical systems in the context of the plasma gravitational analogy.

  11. Mechanisms of dissipation in wet granular matter

    E-Print Network [OSTI]

    A. Fingerle; S. Herminghaus

    2007-08-20

    The impact dynamics between wet surfaces, which dominates the mechanical properties of wet granular matter, is studied both experimentally and theoretically. It is shown that the hysteretic formation and rupture of liquid capillary bridges between adjacent grains accounts reasonably well for most relevant cases of wet granular matter. The various dissipation mechanisms are discussed with particular emphasis on their relevance. Variations of the rupture energy loss with the impact energy are quantified and discussed.

  12. Directional detection of galactic dark matter

    E-Print Network [OSTI]

    Mayet, F; Santos, D

    2012-01-01

    Directional detection is a promising Dark Matter search strategy. Taking advantage on the rotation of the Solar system around the galactic center through the Dark Matter halo, it allows to show a direction dependence of WIMP events that may be a powerful tool to identify genuine WIMP events as such. Directional detection strategy requires the simultaneous measurement of the energy and the 3D track of low energy recoils, which is a common challenge for all current projects of directional detectors.

  13. The C-4 Dark Matter Experiment

    SciTech Connect (OSTI)

    Bonicalzi, Ricco; Collar, J. I.; Colaresi, J.; Fast, James E.; Fields, N.; Fuller, Erin S.; Hai, M.; Hossbach, Todd W.; Kos, Marek S.; Orrell, John L.; Overman, Cory T.; Reid, Douglas J.; VanDevender, Brent A.; Wiseman, Clinton G.; Yocum, K. M.

    2013-06-01

    Abstract We describe the experimental design of C-4, an expansion of the CoGeNT dark matter search to four identical detectors each approximately three times the mass of the p-type point contact (PPC) germanium diode presently taking data at the Soudan Underground Laboratory. Expected reductions of radioactive backgrounds and energy threshold are discussed, including an estimate of the additional sensitivity to low-mass dark matter candidates to be obtained with this search.

  14. Asymmetric nuclear matter and neutron star properties

    E-Print Network [OSTI]

    L. Engvik; M. Hjorth-Jensen; E. Osnes; G. Bao; E. Oestgaard

    1994-06-23

    We calculate properties of neutron stars such as mass and radius using a relativistic Dirac-Brueckner-hartree-Fock apprach for asymmetric nuclear matter. For pure neutron matter we find the maximum mass to be 2.4 solar masses with a radius of 12 km. For a proton fraction of 30% we find a max mass of 2.1 solar masses and a radius of 10.5 km. The implications are discussed.

  15. From nuclear matter to Neutron Stars

    E-Print Network [OSTI]

    T. K. Jha

    2009-02-02

    Neutron stars are the most dense objects in the observable Universe and conventionally one uses nuclear theory to obtain the equation of state (EOS) of dense hadronic matter and the global properties of these stars. In this work, we review various aspects of nuclear matter within an effective Chiral model and interlink fundamental quantities both from nuclear saturation as well as vacuum properties and correlate it with the star properties.

  16. Cosmological effects of coupled dark matter

    E-Print Network [OSTI]

    Sophie C. F. Morris; Anne M. Green; Antonio Padilla; Ewan R. M. Tarrant

    2013-10-15

    Many models have been studied that contain more than one species of dark matter and some of these couple the Cold Dark Matter (CDM) to a light scalar field. In doing this we introduce additional long range forces, which in turn can significantly affect our estimates of cosmological parameters if not properly accounted for. It is, therefore, important to study these models and their resulting cosmological implications. We present a model in which a fraction of the total cold dark matter density is coupled to a scalar field. We study the background and perturbation evolution and calculate the resulting Cosmic Microwave Background anisotropy spectra. The greater the fraction of dark matter coupled to the scalar field and the stronger the coupling strength, the greater the deviation of the background evolution from LCDM. Previous work, with a single coupled dark matter species, has found an upper limit on the coupling strength of order O(0.1). We find that with a coupling of this magnitude more than half the dark matter can be coupled to a scalar field without producing any significant deviations from LCDM.

  17. Coupling dark energy to dark matter perturbations

    E-Print Network [OSTI]

    Valerio Marra

    2015-06-21

    This Letter proposes that dark energy in the form of a scalar field could effectively couple to dark matter perturbations. The idea is that dark matter particles could annihilate/interact inside dense clumps and transfer energy to the scalar field, which would then enter an accelerated regime. This hypothesis is interesting as it provides a natural trigger for the onset of the acceleration of the universe, since dark energy starts driving the expansion of the universe when matter perturbations become sufficiently dense. Here we study a possible realization of this general idea by coupling dark energy to dark matter via the linear growth function of matter perturbations. The numerical results show that it is indeed possible to obtain a viable cosmology with the expected series of radiation, matter and dark-energy dominated eras. Moreover, the current density of dark energy is given by the value of the coupling parameters rather than by very special initial conditions for the scalar field. In other words, this model does not suffer from the so-called "coincidence problem" and its related fine tuning of initial conditions.

  18. Coupling dark energy to dark matter perturbations

    E-Print Network [OSTI]

    Marra, Valerio

    2015-01-01

    This Letter proposes that dark energy in the form of a scalar field could effectively couple to dark matter perturbations. The idea is that dark matter particles could annihilate/interact inside dense clumps and transfer energy to the scalar field, which would then enter an accelerated regime. This hypothesis is interesting as it provides a natural trigger for the onset of the acceleration of the universe, since dark energy starts driving the expansion of the universe when matter perturbations become sufficiently dense. Here we study a possible realization of this general idea by coupling dark energy to dark matter via the linear growth function of matter perturbations. The numerical results show that it is indeed possible to obtain a viable cosmology with the expected series of radiation, matter and dark-energy dominated eras. Moreover, the current density of dark energy is given by the value of the coupling parameters rather than by very special initial conditions for the scalar field. In other words, this ...

  19. Identifying dark matter interactions in monojet searches

    SciTech Connect (OSTI)

    Agrawal, Prateek; Rentala, Vikram

    2014-05-01

    We study the discrimination of quark-initiated jets from gluon-initiated jets in monojet searches for dark matter using the technique of averaged jet energy profiles. We demonstrate our results in the context of effective field theories of dark matter interactions with quarks and gluons, but our methods apply more generally to a wide class of models. Different effective theories of dark matter and the standard model backgrounds each have a characteristic quark/gluon fraction for the leading jet. When used in conjunction with the traditional cut-and-count monojet search, the jet energy profile can be used to set stronger bounds on contact interactions of dark matter. In the event of a discovery of a monojet excess at the 14 TeV LHC, contact interactions between dark matter with quarks or with gluons can be differentiated at the 95% confidence level. For a given rate at the LHC, signal predictions at direct detection experiments for different dark matter interactions can span five orders of magnitude. The ability to identify these interactions allows us to make a tighter connection between LHC searches and direct detection experiments.

  20. Measuring the dark matter equation of state

    E-Print Network [OSTI]

    Ana Laura Serra; Mariano Javier de León Domínguez Romero

    2011-05-30

    The nature of the dominant component of galaxies and clusters remains unknown. While the astrophysics community supports the cold dark matter (CDM) paradigm as a clue factor in the current cosmological model, no direct CDM detections have been performed. Faber and Visser 2006 have suggested a simple method for measuring the dark matter equation of state that combines kinematic and gravitational lensing data to test the widely adopted assumption of pressureless dark matter. Following this formalism, we have measured the dark matter equation of state for first time using improved techniques. We have found that the value of the equation of state parameter is consistent with pressureless dark matter within the errors. Nevertheless, the measured value is lower than expected because typically the masses determined with lensing are larger than those obtained through kinematic methods. We have tested our techniques using simulations and we have also analyzed possible sources of error that could invalidate or mimic our results. In the light of this result, we can now suggest that the understanding of the nature of dark matter requires a complete general relativistic analysis.

  1. PUBLISHED ONLINE: 2 NOVEMBER 2014 | DOI: 10.1038/NPHYS3135 Collisions of matter-wave solitons

    E-Print Network [OSTI]

    Loss, Daniel

    we explore the nature of soliton collisions using Bose­Einstein condensates of atoms with attractive previously14 and are given in the Methods section. A Bose­Einstein condensate of atoms in the |F =1,mF =1

  2. RIKEN Center for Emergent Matter Science Strong Correlation Physics Division

    E-Print Network [OSTI]

    Fukai, Tomoki

    Quantum Condencsed Matter Research Group Macroscopic Quantum Coherence Research Team Superconducting

  3. Assembling thefacebook: Using heterogeneity to understand online social network assembly

    E-Print Network [OSTI]

    Jacobs, Abigail Z; Ugander, Johan; Clauset, Aaron

    2015-01-01

    Online social networks represent a popular and highly diverse class of social media systems. Despite this variety, each of these systems undergoes a general process of online social network assembly, which represents the complicated and heterogeneous changes that transform newly born systems into mature platforms. However, little is known about this process. For example, how much of a network's assembly is driven by simple growth? How does a network's structure change as it matures? How does network structure vary with adoption rates and user heterogeneity, and do these properties play different roles at different points in the assembly? We investigate these and other questions using a unique dataset of online connections among the roughly one million users at the first 100 colleges admitted to Facebook, captured just 20 months after its launch. We first show that different vintages and adoption rates across this population of networks reveal temporal dynamics of the assembly process, and that assembly is onl...

  4. Dark matter directional detection in non-relativistic effective theories

    E-Print Network [OSTI]

    Catena, Riccardo

    2015-01-01

    We extend the formalism of dark matter directional detection to arbitrary one-body dark matter-nucleon interactions. The new theoretical framework generalizes the one currently used, which is based on 2 types of dark matter-nucleon interaction only. It includes 14 dark matter-nucleon interaction operators, 8 isotope-dependent nuclear response functions, and the Radon transform of the first 2 moments of the dark matter velocity distribution. We calculate the recoil energy spectra at dark matter directional detectors made of CF$_4$, CS$_2$ and $^{3}$He for the 14 dark matter-nucleon interactions, using nuclear response functions recently obtained through numerical nuclear structure calculations. We highlight the new features of the proposed theoretical framework, and present our results for a spherical dark matter halo and for a stream of dark matter particles. This study lays the foundations for model independent analyses of dark matter directional detection experiments.

  5. Dark matter directional detection in non-relativistic effective theories

    E-Print Network [OSTI]

    Riccardo Catena

    2015-05-24

    We extend the formalism of dark matter directional detection to arbitrary one-body dark matter-nucleon interactions. The new theoretical framework generalizes the one currently used, which is based on 2 types of dark matter-nucleon interaction only. It includes 14 dark matter-nucleon interaction operators, 8 isotope-dependent nuclear response functions, and the Radon transform of the first 2 moments of the dark matter velocity distribution. We calculate the recoil energy spectra at dark matter directional detectors made of CF$_4$, CS$_2$ and $^{3}$He for the 14 dark matter-nucleon interactions, using nuclear response functions recently obtained through numerical nuclear structure calculations. We highlight the new features of the proposed theoretical framework, and present our results for a spherical dark matter halo and for a stream of dark matter particles. This study lays the foundations for model independent analyses of dark matter directional detection experiments.

  6. Incorporating on-line process data into a diagnostic knowledge-based system 

    E-Print Network [OSTI]

    Lin, Kai Hsuan

    1994-01-01

    The objective of this research was to develop and implement an on-line gypsum wallboard manufacturing expert system incorporating on-line process monitoring information and statistical process control. In support of this objective, several sub...

  7. Aalborg Universitet Photovoltaic Array Condition Monitoring Based on Online Regression of Performance

    E-Print Network [OSTI]

    Teodorescu, Remus

    Aalborg Universitet Photovoltaic Array Condition Monitoring Based on Online Regression of the 39th IEEE Photovoltaic Specialists Conference, PVSC 2013 DOI (link to publication from Publisher): 10., & Teodorescu, R. (2013). Photovoltaic Array Condition Monitoring Based on Online Regression of Performance

  8. IEA-GIA ExCo - National Geothermal Data System and Online Tools...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    IEA-GIA ExCo - National Geothermal Data System and Online Tools IEA-GIA ExCo - National Geothermal Data System and Online Tools National Geothermal Data System presentation by Jay...

  9. Young media-induced travelers: online representations of media-induced travel conversations 

    E-Print Network [OSTI]

    Scarpino, Michelle Renee

    2009-05-15

    technology, specifically how online communities and online discussion forums are utilized as important venues, which support conversations among travelers (Wang, Yu & Fesenmaier, 2002; Wang & Fesenmaier, 2004). Study results supported previous arguments...

  10. Conceptual framework of e-service quality to predict return intentions of online travel agency's user 

    E-Print Network [OSTI]

    Park, Young A

    2003-01-01

    industry has also been affected by this new business paradigm. The proliferation of Internet use has created both opportunities and challenges for online tourism agencies. As businesses and consumers increase their Internet usage, the role of the online...

  11. An Overview of NREL's Online Data Tool for Fuel Cell System-Derived...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    An Overview of NREL's Online Data Tool for Fuel Cell System-Derived Contaminants An Overview of NREL's Online Data Tool for Fuel Cell System-Derived Contaminants Download...

  12. Algorithmic and implementation aspects of on-line calibration of Dynamic Traffic Assignment

    E-Print Network [OSTI]

    Huang, Enyang

    2010-01-01

    This thesis compares alternative and proposes new candidate algorithms for the online calibration of Dynamic Traffic Assignment (DTA). The thesis presents two formulations to on-line calibration: 1) The classical statespace ...

  13. HarvardX and MITx: Two Years of Open Online Courses Fall 2012-Summer 2014

    E-Print Network [OSTI]

    Ho, Andrew Dean

    2015-03-30

    What happens when well-known universities offer online courses, assessments, and certificates of completion for free? Early descriptions of Massive Open Online Courses (MOOCs) have emphasized large enrollments, low ...

  14. A Window in the Dark Matter Exclusion Limits

    E-Print Network [OSTI]

    Gabrijela Zaharijas; Glennys R. Farrar

    2005-06-28

    We consider the cross section limits for light dark matter candidates ($m=0.4$ to 10 GeV). We calculate the interaction of dark matter in the crust above underground dark matter detectors and find that in the intermediate cross section range, the energy loss of dark matter is sufficient to fall below the energy threshold of current underground experiments. This implies the existence of a window in the dark matter exclusion limits in the micro-barn range.

  15. Dark Matter Through the Neutrino Portal

    E-Print Network [OSTI]

    Adam Falkowski; Jose Juknevich; Jessie Shelton

    2009-08-13

    We consider a model of dark matter whose most prominent signature is a monochromatic flux of TeV neutrinos from the galactic center. As an example of a general scenario, we consider a specific model where the dark matter is a fermion in the adjoint representation of a hidden SU(N) gauge group that confines at GeV energies. The absence of light fermionic states in the dark sector ensures stability of dark matter on cosmological time scales. Dark matter couples to the standard model via the neutrino portal, that is, the singlet operator H L constructed from the Higgs and lepton doublets, which is the lowest dimensional fermionic singlet operator in the standard model. This coupling prompts dark matter decay where the dominant decay channel has one neutrino (and at least one dark glueball) in the final state. Other decay channels with charged standard model particles involve more particles in the final state and are therefore suppressed by phase space. In consequence, the standard indirect detection signals like gamma-ray photons, antiprotons and positrons are suppressed with respect to the neutrino signal. This coupling via the neutrino portal is most robustly constrained by Super-Kamiokande, which restricts the dark matter lifetime to be larger than 10^25 seconds. In the near future, the scenario will be probed by the new generation of neutrino telescopes. ANTARES will be sensitive to a dark matter lifetime of order 10^26 seconds, while IceCube/DeepCore can probe a lifetime as large as 10^27 seconds.

  16. Working Group Report: Dark Matter Complementarity (Dark Matter in the Coming Decade: Complementary Paths to Discovery and Beyond)

    SciTech Connect (OSTI)

    Arrenberg, Sebastian; et al.,

    2013-10-31

    In this Report we discuss the four complementary searches for the identity of dark matter: direct detection experiments that look for dark matter interacting in the lab, indirect detection experiments that connect lab signals to dark matter in our own and other galaxies, collider experiments that elucidate the particle properties of dark matter, and astrophysical probes sensitive to non-gravitational interactions of dark matter. The complementarity among the different dark matter searches is discussed qualitatively and illustrated quantitatively in several theoretical scenarios. Our primary conclusion is that the diversity of possible dark matter candidates requires a balanced program based on all four of those approaches.

  17. On-Line Student Modeling for Coached Problem Solving Using Bayesian Networks

    E-Print Network [OSTI]

    VanLehn, Kurt

    York. © CISM, 1997. Available on-line from http://um.org. #12;the important reasoning is hidden from

  18. The University of Texas at Arlington College of Nursing Equivalency Chart for: University of Phoenix -Online

    E-Print Network [OSTI]

    Huang, Haiying

    of Phoenix - Online Catalog: 2014-2015 The following is a list of all prerequisite coursework that may

  19. Comparison of Course Completion and Academic Performance in Online vs. Traditional Courses 

    E-Print Network [OSTI]

    Atchley, Thomas Wayne

    2011-10-21

    resulted in increased semester credit hour generation. According to the Tarleton State University (n.d.) online Fact Book, online courses generated 1,581 semester credit hours in fall 2002. By fall 2008, online semester credit hours had increased to 5...

  20. arXiv:submit/0910499[stat.ML]11Feb2014 Online Nonparametric Regression

    E-Print Network [OSTI]

    Rakhlin, Alexander "Sasha"

    arXiv:submit/0910499[stat.ML]11Feb2014 Online Nonparametric Regression Alexander Rakhlin University for online regression for arbitrary classes of regression functions in terms of the sequential entropy learning with squared loss and online nonparametric regression are the same. In addition to a non

  1. Master's Thesis Growth in Online Social Networks: Sheer Volume vs Social

    E-Print Network [OSTI]

    Moon, Sue B.

    Korea Advanced Institute of Science and Technology 2008 #12; Growth in Online Social Networks: Sheer Master's Thesis Growth in Online Social Networks: Sheer Volume vs Social Interaction Volume vs Social Interaction 2 #12;Growth in Online Social Networks: Sheer Volume vs Social Interaction

  2. How do I enroll? 1. Log into WSU's online portal (Academica).

    E-Print Network [OSTI]

    Finley Jr., Russell L.

    How do I enroll? 1. Log into WSU's online portal (Academica). 2 by noon the following business day. 8. Check your account in the online portal in WSU's online portal (Academica). The first payment may include non-deferred fees. What if I add

  3. SMALL ONLINE RAMSEY NUMBERS--A NEW APPROACH PRZEMYSLAW GORDINOWICZ AND PAWEL PRALAT

    E-Print Network [OSTI]

    Pralat, Pawel

    SMALL ONLINE RAMSEY NUMBERS--A NEW APPROACH PRZEMYSLAW GORDINOWICZ AND PAWEL PRALAT Abstract. Introduction and definitions In this paper, we consider online Ramsey numbers introduced in 2005 by Kurek and Ruciski [7] and the corresponding on-line Ramsey game. (The game was considered earlier by Beck [1

  4. ONLINE AND SIZE ANTI-RAMSEY NUMBERS MARIA AXENOVICH, KOLJA KNAUER, JUDITH STUMPP, AND TORSTEN UECKERDT

    E-Print Network [OSTI]

    Felsner, Stefan

    ONLINE AND SIZE ANTI-RAMSEY NUMBERS MARIA AXENOVICH, KOLJA KNAUER, JUDITH STUMPP, AND TORSTEN of a graph H is the size anti-Ramsey number ARs(H) of H. This number in offline and online setting is investigated here. Keywords: Coloring, anti-Ramsey, rainbow, totally multicolored, proper coloring, online

  5. A NOTE ON SMALL ON-LINE RAMSEY NUMBERS FOR PATHS AND THEIR GENERALIZATION

    E-Print Network [OSTI]

    Pralat, Pawel

    A NOTE ON SMALL ON-LINE RAMSEY NUMBERS FOR PATHS AND THEIR GENERALIZATION PAWEL PRALAT Abstract. In this note, we consider the on-line Ramsey numbers R(Pn) for paths and their generalization. The standard on-line Ramsey game is played on an un- bounded set of vertices, whereas the new variant of the game we consider

  6. Multicolor on-line degree Ramsey numbers of trees William B. Kinnersley

    E-Print Network [OSTI]

    West, Douglas B.

    Multicolor on-line degree Ramsey numbers of trees William B. Kinnersley and Douglas B. West University of Illinois, Urbana IL. October 24, 2011; revised May 25, 2012 Abstract In the on-line Ramsey game can ensure that a monochromatic G arises. The s-color on-line degree Ramsey number of G, denoted °R

  7. Toward On-line Schema Evolution for Non-stop Amol Deshpande and Michael Hicks

    E-Print Network [OSTI]

    Hicks, Michael

    in the third issue. Supporting on-line evolution is non-trivial. Almost every aspect of a running database and process of on-line schema evolution more concrete, we present an example inspired by http://www.agiledata.org/essays/databaseToward On-line Schema Evolution for Non-stop Systems Amol Deshpande and Michael Hicks University

  8. Revenue Maximization in Reservation-based Online Advertising Through Dynamic Inventory

    E-Print Network [OSTI]

    Cortes, Corinna

    Revenue Maximization in Reservation-based Online Advertising Through Dynamic Inventory Management in the online advertising industry is one where advertisers pre-purchase a reservation package of online.) while trying to meet advertisers' expectations. The current process of sales is usually ad hoc

  9. doi: 10.1130/G35342.1 published online 10 January 2014;Geology

    E-Print Network [OSTI]

    Bookhagen, Bodo

    Geology doi: 10.1130/G35342.1 published online 10 January 2014;Geology Burch Fisher, Adrien Moulin for publication but have not © Geological Society of America as doi:10.1130/G35342.1Geology, published online on 10 January 2014 as doi:10.1130/G35342.1Geology, published online on 10 January 2014 #12;GEOLOGY

  10. doi: 10.1130/G35915.1 published online 15 September 2014;Geology

    E-Print Network [OSTI]

    Jones, Peter JS

    Geology doi: 10.1130/G35915.1 published online 15 September 2014;Geology and Anson W. Mackay Katy E for publication but have not © Geological Society of America as doi:10.1130/G35915.1Geology, published online on 15 September 2014 as doi:10.1130/G35915.1Geology, published online on 15 September 2014 #12;GEOLOGY

  11. The Optimal Mix of TV and Online Ads to Maximize Reach

    E-Print Network [OSTI]

    Cortes, Corinna

    The Optimal Mix of TV and Online Ads to Maximize Reach Yuxue Jin, Georg M. Goerg, Nicolas Remy, Jim allocate budget between TV and online ads in order to maximize reach or maintain the same reach at a lower budget allocation between TV and online ads to maximize reach to the target demographics. We take

  12. Color superconductivity and dense quark matter

    E-Print Network [OSTI]

    Massimo Mannarelli

    2008-12-26

    The properties of cold and dense quark matter have been the subject of extensive investigation, especially in the last decade. Unfortunately, we still lack of a complete understanding of the properties of matter in these conditions. One possibility is that quark matter is in a color superconducting phase which is characterized by the formation of a diquark condensate. We review some of the basic concepts of color superconductivity and some of the aspects of this phase of matter which are relevant for compact stars. Since quarks have color, flavor as well as spin degrees of freedom many different color superconducting phases can be realized. At asymptotic densities QCD predicts that the color flavor locked phase is favored. At lower densities where the QCD coupling constant is large, perturbative methods cannot be applied and one has to rely on some effective model, eventually trying to constrain such a model with experimental observations. The picture is complicated by the requirement that matter in the interior of compact stars is in weak equilibrium and neutral. These conditions and the (possible) large value of the strange quark mass conspire to separate the Fermi momenta of quarks with different flavors, rendering homogenous superconducting phases unstable. One of the aims of this presentation is to introduce non-experts in the field to some of the basic ideas of color superconductivity and to some of its open problems.

  13. Indirect and direct search for dark matter

    E-Print Network [OSTI]

    Michael Klasen; Martin Pohl; Günter Sigl

    2015-07-14

    The majority of the matter in the universe is still unidentified and under investigation by both direct and indirect means. Many experiments searching for the recoil of dark-matter particles off target nuclei in underground laboratories have established increasingly strong constraints on the mass and scattering cross sections of weakly interacting particles, and some have even seen hints at a possible signal. Other experiments search for a possible mixing of photons with light scalar or pseudo-scalar particles that could also constitute dark matter. Furthermore, annihilation or decay of dark matter can contribute to charged cosmic rays, photons at all energies, and neutrinos. Many existing and future ground-based and satellite experiments are sensitive to such signals. Finally, data from the Large Hadron Collider at CERN are scrutinized for missing energy as a signature of new weakly interacting particles that may be related to dark matter. In this review article we summarize the status of the field with an emphasis on the complementarity between direct detection in dedicated laboratory experiments, indirect detection in the cosmic radiation, and searches at particle accelerators.

  14. Online Distance Recovery for a Sewer Inspection Robot Marina Kolesnik

    E-Print Network [OSTI]

    Kolesnik, Marina

    Online Distance Recovery for a Sewer Inspection Robot Marina Kolesnik Institute for Autonomous computation based on images taken in a sewer by a robot-inspector is presented. Modern concrete sewers provide regular marks on the sewer images and can be used for their 3-D interpretation. After each robot

  15. A Nursery and Greenhouse Online Knowledge Center: Learning Opportunities

    E-Print Network [OSTI]

    Virginia Tech

    A Nursery and Greenhouse Online Knowledge Center: Learning Opportunities for Sustainable Practice and greenhouse operations. This is particularly important because these production facilities are typically and greenhouse industry. A web-based knowledge center provides the most cost-effective mechanism for information

  16. On-Line Machine Covering Yossi Azar1

    E-Print Network [OSTI]

    Azar, Yossi

    On-Line Machine Covering Yossi Azar1 ,Leah Epstein2 1 Dept. of Computer Science, Tel of scheduling a sequence of jobs to m parallel machines as to maximize the minimum load over the machines. This situation corresponds to a case that a system which consists of the m machines is alive (i.e. productive

  17. Predicting Emerging Social Conventions in Online Social Networks

    E-Print Network [OSTI]

    Gummadi, Krishna P.

    of massive social movements [34]. They guide everyday behaviors of the general public [1] as well as thosePredicting Emerging Social Conventions in Online Social Networks Farshad Kooti MPI-SWS farshad@mpi-sws.org Meeyoung Cha KAIST meeyoungcha@kaist.edu ABSTRACT The way in which social conventions emerge in communities

  18. Online Prediction of Battery Lifetime for Embedded and Mobile Devices

    E-Print Network [OSTI]

    Krintz, Chandra

    Online Prediction of Battery Lifetime for Embedded and Mobile Devices Ye Wen, Rich Wolski, and compare it to two similar battery prediction technologies: ACPI and Smart Battery. We employ twenty is a critical resource for battery-powered embedded systems and mobile devices. As such, battery life must

  19. Personalized Online Education --A Crowdsourcing Challenge Daniel S. Weld1

    E-Print Network [OSTI]

    Mausam

    Personalized Online Education -- A Crowdsourcing Challenge Daniel S. Weld1 Eytan Adar2 Lydia- chanical Turk, may prove useful for optimizing personalized curricula (Dai, Mausam, and Weld 2010; Shahaf and Horvitz 2010; Dai, Mausam, and Weld 2011; Lin, Mausam, and Copyright c 2012, Association

  20. Motivation for Participation in Online Neighborhood Watch Communities: An Empirical

    E-Print Network [OSTI]

    Shneiderman, Ben

    Motivation for Participation in Online Neighborhood Watch Communities: An Empirical Study Involving--This paper presents a three-part experiment de- signed to investigate the motivations of users of a community versions of an invitation email which differ by expressing one of four possible motivations for using

  1. 6 Month Internship Market Research & Development Online, Italian speakers

    E-Print Network [OSTI]

    Maróti, Miklós

    ) Paid Accommodation. 2) Paid Utility Bills (electricity, gas, water and council tax) + Internet Access 3 retailer which was established in 2008 and employs 50 staff. It sells clothes hangers, home storage. To sustain growth the company has now expanded sales into Europe and intends to have online store- fronts

  2. The Key Coal Producers ONLINE SUPPORTING MATERIALS to

    E-Print Network [OSTI]

    Patzek, Tadeusz W.

    The Key Coal Producers ONLINE SUPPORTING MATERIALS to A Global Coal Production Forecast with Multi's most important coal-producing area is North-Central China. The provinces of Inner Mongolia, Ningxia, Shaanxi and Shanxi together accounted for 83 percent of China's proven coal reserves in 2000, and Shanxi

  3. WHAT IS NANOTECHNOLOGY? Adapted from Online Materials Available from NNIN

    E-Print Network [OSTI]

    Zhigilei, Leonid V.

    1 WHAT IS NANOTECHNOLOGY? Adapted from Online Materials Available from NNIN: http://www.nnin.org/nnin_edu.html Nanotechnology is the science and technology of small things ­ in particular, things that are less than 100nm of precisely what is included in nanotechnology. In general, however, most agree that three things

  4. Adaptive Demand Response: Online Learning of Restless and Controlled Bandits

    E-Print Network [OSTI]

    Liu, Mingyan

    Adaptive Demand Response: Online Learning of Restless and Controlled Bandits Qingsi Wang, Mingyan realized curtailment, not the curtailment of each load. We develop an adaptive demand response learning like UCB1. I. INTRODUCTION Electric loads participating in demand response programs provide a variety

  5. Measuring the Longitudinal Evolution of the Online Anonymous Marketplace Ecosystem

    E-Print Network [OSTI]

    Sadeh, Norman M.

    managed to shut down Silk Road in October 2013 and arrest its operator. Far from causing the demise. Then, in early October 2013, Silk Road was shut down, its operator arrested, and all the money held the emergence of Silk Road, the first successful online anonymous marketplace, in which buy- ers and sellers

  6. Online $300 300 x 250 pixels ABOUT THE JOURNAL

    E-Print Network [OSTI]

    Mateo, Jill M.

    Online $300 300 x 250 pixels ABOUT THE JOURNAL The Journal of Legal Studies is an interdisciplinary journal of theoretical and empirical research on law and legal institutions. Economists, political. For more information contact: J-advertising@press.uchicago.edu Journal of Legal Studies A leading journal

  7. Online $300 300 x 250 pixels ABOUT THE JOURNAL

    E-Print Network [OSTI]

    Mateo, Jill M.

    Online $300 300 x 250 pixels ABOUT THE JOURNAL The Journal of Modern History is recognized as the leading American journal for the study of European history. The Journal's expansive geographical. For more information contact: J-advertising@press.uchicago.edu Journal of Modern History The leading

  8. Faculty and Student Perceptions of Online Learning in Engineering Education

    E-Print Network [OSTI]

    Thornton, Mitchell

    The concept of teaching at a distance, or distance education, has a long history. Distance education has beenFaculty and Student Perceptions of Online Learning in Engineering Education Abstract The number of distance education programs at the university level has been rapidly growing. Studies have shown

  9. Online Multicasting for Network Capacity Maximization in Energy-Constrained

    E-Print Network [OSTI]

    Liang, Weifa

    Online Multicasting for Network Capacity Maximization in Energy-Constrained Ad Hoc Networks Weifa of network capacity, network lifetime, and transmission energy consumption for each multicast request, the network capacity is proportional to the network lifetime if the transmission energy consumption for each

  10. Online Bipartite Matching with Unknown Distributions Chinmay Karande

    E-Print Network [OSTI]

    Cortes, Corinna

    Online Bipartite Matching with Unknown Distributions Chinmay Karande Google Research Mountain View, CA chinmayk@google.com Aranyak Mehta Google Research Mountain View, CA aranyak@google.com Pushkar Research, Mountain View Permission to make digital or hard copies of all or part of this work for personal

  11. Degree Ramsey and On-Line Degree Ramsey Numbers

    E-Print Network [OSTI]

    West, Douglas B.

    Degree Ramsey and On-Line Degree Ramsey Numbers Douglas B. West Department of Mathematics;Parameter Ramsey Numbers Def. H G means every 2-coloring of E(H) gives a monochromatic G. Ramsey's Theorem H exists. Ramsey number R(G) = min{n: Kn G}. #12;Parameter Ramsey Numbers Def. H G means every 2

  12. Degree Ramsey and On-Line Degree Ramsey Numbers

    E-Print Network [OSTI]

    West, Douglas B.

    Degree Ramsey and On-Line Degree Ramsey Numbers Douglas B. West Department of Mathematics Stocker #12;Parameter Ramsey Numbers Def. H G means every 2-coloring of E(H) gives a monochromatic G. Ramsey's Theorem H exists. Ramsey number R(G) = min{n: Kn G}. #12;Parameter Ramsey Numbers Def. H G

  13. A new approach for online multiobjective optimization of mechatronical systems

    E-Print Network [OSTI]

    A new approach for online multiobjective optimization of mechatronical systems K. Witting, B;1 Introduction For the optimization of mechatronical systems one has to bear in mind many things in this work are not only of theoretical interest but are also quite useful in mechatronical applications. 2

  14. Online, Asynchronous Schema Change in F1 University of

    E-Print Network [OSTI]

    Cortes, Corinna

    a protocol for schema evolution in a globally distributed database management system with shared data evolution--the ability to change a database's def- inition without the loss of data--has been studied in the database system to transition to a new schema at different times--and online--all servers can access

  15. Online Mechanism Design for Electric Vehicle Charging Enrico H. Gerding

    E-Print Network [OSTI]

    Chen, Yiling

    Online Mechanism Design for Electric Vehicle Charging Enrico H. Gerding eg@ecs.soton.ac.uk Valentin electric vehicles are expected to place a consid- erable strain on local electricity distribution networks mechanisms are evaluated in depth, using data from a real-world trial of electric vehicles in the UK

  16. An Expressive Auction Design for Online Display Advertising Sebastien Lahaie

    E-Print Network [OSTI]

    Chen, Yiling

    An Expressive Auction Design for Online Display Advertising S´ebastien Lahaie Yahoo! Research New to target within an advertising network. The design al- lows the network to differentiate impressions according to relevant attributes (e.g., geographic location of the user, topic of the webpage). Advertisers

  17. Shopping for Top Forums: Discovering Online Discussion for Product Research

    E-Print Network [OSTI]

    Cortes, Corinna

    ranked result of 85%. Categories and Subject Descriptors H.3.3 [Information Search and Retrieval Language Technologies Institute Carnegie Mellon University Pittsburgh, PA 15213 jelsas@cs.cmu.edu Natalie such as blogs, twitter and online discussion boards have been recognized as valuable sources of market intelli

  18. Automatically Constructing Semantic Web Services from Online Sources

    E-Print Network [OSTI]

    Lerman, Kristina

    of Southern California Information Sciences Institute 4676 Admiralty Way Marina del Rey, CA 90292 {ambite into Semantic Web Services. In general, the type of source that we focus on in this paper are informationAutomatically Constructing Semantic Web Services from Online Sources Jos´e Luis Ambite, Sirish

  19. Access via Science Online Site Pass ARTIFICIAL INTELLIGENCE

    E-Print Network [OSTI]

    Duckett, Tom

    Access via Science Online Site Pass ARTIFICIAL INTELLIGENCE: Autonomous Mental Development of an adult brain, such as vision, speech, and language. Nevertheless, these traditional approaches have." A Definition What is autonomous mental development? With time, a brainlike natural or an artificial embodied

  20. Published online 6 August 2003 Physical modelling in biomechanics

    E-Print Network [OSTI]

    Koehl, Mimi

    Published online 6 August 2003 Physical modelling in biomechanics M. A. R. Koehl Department@socrates.berkeley.edu) Physical models, like mathematical models, are useful tools in biomechanical research. Physical models organ- isms. Physical models also permit some aspects of the biomechanical performance of extinct

  1. Exploring big data opportunities for Online Customer Segmentation

    E-Print Network [OSTI]

    Utrecht, Universiteit

    Exploring big data opportunities for Online Customer Segmentation Georgia Fotaki Marco Spruit Sjaak University P.O. Box 80.089 3508 TB Utrecht The Netherlands #12;iii Exploring big data opportunities and analyzing the huge amount of data; and this is where the concept of "Big Data" can play an essential role

  2. Sparse Online Greedy Support Vector Yaakov Engel1

    E-Print Network [OSTI]

    Meir, Ron

    problems. 1 Introduction Kernel machines have become by now a standard tool in the arsenal of MachineSparse Online Greedy Support Vector Regression Yaakov Engel1 , Shie Mannor2 and Ron Meir2 1 Center to kernel machines and in recent years focused on Support Vector Machines (SVMs) [13]. A basic idea behind

  3. Optimal Bounds for Online Page Migration with Generalized Migration Costs

    E-Print Network [OSTI]

    Schmid, Stefan

    Optimal Bounds for Online Page Migration with Generalized Migration Costs Johannes Schneider1 to a generalized version of the classic page migration problem where migration costs are not necessarily given by the migration distance only, but may depend on prior migrations, or on the available bandwidth along

  4. Viewability Prediction for Online Display Ads Information Systems Dept.

    E-Print Network [OSTI]

    Borcea, Cristian

    Viewability Prediction for Online Display Ads Chong Wang Information Systems Dept. New Jersey. Advertisers are charged by ad serv- ing, where their ads are shown in web pages. However, re- cent studies show that about half of the ads were actually never seen by users because they do not scroll deep

  5. Situated Practices of Looking: Visual Practice in an Online World

    E-Print Network [OSTI]

    Hayes, Gillian R.

    Situated Practices of Looking: Visual Practice in an Online World Lilly Irani, Gillian R. Hayes Graphical virtual worlds are increasingly significant sites of collaborative interaction. Many argue it might at first seem; second, that we need to look beyond the virtual in understanding virtual worlds

  6. Scripted Artificially Intelligent Basic Online Tactical Simulation Jesse D. Phillips+

    E-Print Network [OSTI]

    Dascalu, Sergiu

    Scripted Artificially Intelligent Basic Online Tactical Simulation Jesse D. Phillips+ Roger V.+ Department of Computer Science and Engineering+ CAVCaM University of Nevada, Reno Desert Research Institute of the concepts. This paper presents details of the idea, specification, design, and functionality of the Scripted

  7. Online Fault Detection and Tolerance for Photovoltaic Energy Harvesting Systems

    E-Print Network [OSTI]

    Pedram, Massoud

    Online Fault Detection and Tolerance for Photovoltaic Energy Harvesting Systems Xue Lin 1 , Yanzhi, yanzhiwa, dizhu, pedram}@usc.edu, 2 naehyuck@elpl.snu.ac.kr ABSTRACT Photovoltaic energy harvesting systems, Performance, Reliability. Keywords Photovoltaic System, Fault Detection, Fault Tolerance, Photovoltaic Panel

  8. Online Energy Estimation of Relational Operations in Database Systems

    E-Print Network [OSTI]

    Tu, Yicheng

    1 Online Energy Estimation of Relational Operations in Database Systems Zichen Xu # , Yi-Cheng Tu known to consume a large amount of energy. As databases are one of the major applications in a data center, building energy-aware database systems has become an active research topic recently

  9. Building Online Corpora of Philippine Languages* Shirley N. Dita

    E-Print Network [OSTI]

    Building Online Corpora of Philippine Languages* Shirley N. Dita a , Rachel Edita O. Roxas b Avenue, Manila, Philippines shirley.dita@dlsu.edu.ph b College of Computer Studies, De La Salle University 2401 Taft Avenue, Manila, Philippines {rachel.roxas, paul.inventado}@dlsu.edu.ph Abstract

  10. Efficient On-Line Estimation of Autoregressive Department of Mathematics

    E-Print Network [OSTI]

    Sheldon, Nathan D.

    control, optimization, and signal processing. A comprehensive survey of the related results and of some allows for incorporation of auxiliary information into the estimation process and, under certain class of on-line estimating procedures for the AR(m) processes. The advantage of our approach is that

  11. Automatic setup of recommended connections for online searching

    E-Print Network [OSTI]

    Painter, Kevin

    the recommended Connections. #12;Information Services 4 July 2013 7. Select a database to search and enter search terms in the search boxes 8. Select the number of results to retrieve The records will appear in EndnoteAutomatic setup of recommended connections for online searching EndNote X6 #12;Information Services

  12. On-Line Renewals Spring 2015 Co-op Timeline

    E-Print Network [OSTI]

    On-Line Renewals Spring 2015 Co-op Timeline All students applying for Co-ops &/or Internships must for Spring 2015 Co-op ( Renewals are for Co-ops only). Also Work Term Evaluations will be accepted. November 10, 2014 Earliest date for submitting Coop Renewals to start working (on January 12th ) December 1

  13. INTERNATIONAL Available online at www.sciencedirect.com

    E-Print Network [OSTI]

    Hong, Soon Hyung

    2013 Available online 7 March 2013 Abstract Biomorphic SiC composites were fabricated by infiltration were oxidized at elevated temperatures (up to 1450 1C) in air to study their oxidation behavior. Pores (liquid-Si infiltration), and chemical vapor infiltration [3­8]. The reaction bonding process involves

  14. Online Pricing with Discounts by a Location Model

    E-Print Network [OSTI]

    Sidorov, Nikita

    , for whom it becomes uneconomic to consult on a day-to-day basis the numerous alternative suppliers of Manchester, Oxford Road, P.O.Box 88, Manchester M60 1QD Keywords: Online pricing; Supplier selection investigates a model for pricing the demand for a set of goods when multiple suppliers operate discount

  15. Online Backchannel Synthesis Evaluation with the Switching Wizard of Oz

    E-Print Network [OSTI]

    Wieringa, Roel

    synthesis algorithm in an online conversation between a human speaker and a virtual listener. We adopt watches a virtual listener that is either controlled by a human listener or by an algorithm. The source-to-face dialog with a human speaker [1]. The quality of the behavior model should be measured by how the animated

  16. Understanding Online Social Network Usage from a Network Perspective

    E-Print Network [OSTI]

    Greenberg, Albert

    actually inter- act with OSNs by extracting clickstreams from passively monitored network traffic. Our characterization of user interactions within the OSN for four different OSNs (Facebook, LinkedIn, Hi5, and Stu- di Online Social Networks (OSNs) such as Facebook, MySpace, LinkedIn, Hi5, and StudiVZ, have become popular

  17. Facebook Twitter LinkedIn Online Social Service

    E-Print Network [OSTI]

    Hung, Shih-Hao

    ­­ Facebook Twitter LinkedIn Online Social Service Social Network node edge graph corpus Facebook relational time-evolving Social Network Analysis, SNA Small Data Big Data 1960 1990 2000 Facebook Twitter 2014 Facebook 8 Application Programming Interface, API crawler Big Graph Data Mining Big Data Google

  18. By Dr David Whitehouse BBC News Online science editor

    E-Print Network [OSTI]

    By Dr David Whitehouse BBC News Online science editor Decision day for fusion project ITER - NUCLEAR FUSION PROJECT The project is estimated to cost $5bn over the next 10 years It will produce The International Thermonuclear Experimental Reactor (Iter) is the boldest nuclear initiative since the Manhattan

  19. Managing References using EndNote online-Chemical Engineering

    E-Print Network [OSTI]

    Scheichl, Robert

    the Library homepage and enter a search term into the Catalogue search box 2. Select an item from the results. In the catalogue search box, type in Web of Science 3. Open the Web of Science database by clicking View Online and then the Register link 2. Enter your University of Bath email address 3. Click Continue 4. Complete the form

  20. Asymptotic safety of gravity-matter systems

    E-Print Network [OSTI]

    Meibohm, Jan; Reichert, Manuel

    2015-01-01

    We study the ultraviolet stability of gravity-matter systems for general numbers of minimally coupled scalars and fermions. This is done within the functional renormalisation group setup put forward in \\cite{Christiansen:2015rva} for pure gravity. It includes full dynamical propagators and a genuine dynamical Newton's coupling, which is extracted from the graviton three-point function. We find ultraviolet stability of general gravity-fermion systems. Gravity-scalar systems are also found to be ultraviolet stable within validity bounds for the chosen generic class of regulators, based on the size of the anomalous dimension. Remarkably, the ultraviolet fixed points for the dynamical couplings are found to be significantly different from those of their associated background counterparts, once matter fields are included. In summary, the asymptotic safety scenario does not put constraints on the matter content of the theory within the validity bounds for the chosen generic class of regulators.

  1. Cold Positrons from Decaying Dark Matter

    SciTech Connect (OSTI)

    Boubekeur, Lotfi; Dodelson, Scott; Vives, Oscar

    2012-11-01

    Many models of dark matter contain more than one new particle beyond those in the Standard Model. Often heavier particles decay into the lightest dark matter particle as the Universe evolves. Here we explore the possibilities that arise if one of the products in a (Heavy Particle) $\\rightarrow$ (Dark Matter) decay is a positron, and the lifetime is shorter than the age of the Universe. The positrons cool down by scattering off the cosmic microwave background and eventually annihilate when they fall into Galactic potential wells. The resulting 511 keV flux not only places constraints on this class of models but might even be consistent with that observed by the INTEGRAL satellite.

  2. Bi-metric Gravity and "Dark Matter"

    E-Print Network [OSTI]

    I. T. Drummond

    2000-08-18

    We present a bi-metric theory of gravity containing a length scale of galactic size. For distances less than this scale the theory satisfies the standard tests of General Relativity. For distances greater than this scale the theory yields an effective gravitational constant much larger than the locally observed value of Newton's constant. The transition from one regime to the other through the galactic scale can explain the observed rotation curves of galaxies and hence the effects normally attributed to the presence of dark matter. Phenomena on an extragalactic scale such as galactic clusters and the expansion of the universe are controlled by the enhanced gravitational coupling. This provides an explanation of the missing matter normally invoked to account for the observed value of Hubble's constant in relation to observed matter.

  3. Exotic Matter and Space-Time

    E-Print Network [OSTI]

    Hidezumi Terazawa

    2015-04-15

    Exotic forms of matter such as carbon nanofoams, hexalambdas, super-hypernuclei, strange stars, pentaquarks, color-balls, etc. and their relations to current problems in cosmo-particle physics such as dark matter and energy are discussed in some details. This is an extended version of the invited talk presented at the International Conference on New Trends in High-Energy Physics , Yalta, Crimea(Ukraine), September 10-17, 2005, which has been published in the Proceedings, edited by P.N.Bogolyubov, P.O.Fedosenko, L.L.Jenkovszky, and Yu.A.Karpenko(Bogolyubov Institute for Theoretical Physics, Kiev, 2005). In an extended and up-dated version of the Chapters I and III, entitled "Exotic Nuclei and Strange Stars", which has been published in Nonlinear Phenomena in Complex Systems 18(2015)25-30, new forms of matter such as exotic nuclei and strange stars are discussed in some detail.

  4. Higgs Portal Vector Dark Matter : Revisited

    E-Print Network [OSTI]

    Seungwon Baek; P. Ko; Wan-Il Park; Eibun Senaha

    2013-04-15

    We revisit the Higgs portal vector dark matter model including a hidden sector Higgs field that generates the mass of the vector dark matter. The model becomes renormalizable and has two scalar bosons, the mixtures of the standard model (SM) Higgs and the hidden sector Higgs bosons. The strong bound from direct detection such as XENON100 is evaded due to the cancellation mechanism between the contributions from two scalar bosons. As a result, the model becomes still viable in large range of dark matter mass, contrary to some claims in the literature. The Higgs properties are also affected, the signal strengths for the Higgs boson search being universally suppressed relative to the SM value, which could be tested at the LHC in the future.

  5. Neutrino matter potentials induced by Earth

    E-Print Network [OSTI]

    J. Linder

    2006-01-15

    An instructive method of deriving the matter potentials felt by neutrinos propagating through matter on Earth is presented. This paper thoroughly guides the reader through the calculations involving the effective weak Hamiltonian for lepton and quark scattering. The matter potentials are well-known results since the late 70's, but a detailed and pedagogical calculation of these quantities is hard to find. We derive potentials due to charged and neutral current scattering on electrons, neutrons and protons. Intended readership is for undergraduates/graduates in the fields of relativistic quantum mechanics and quantum field theory. In addition to the derivation of the potentials for neutrinos, we explicitely study the origin of the reversed sign for potentials in the case of antineutrino-scattering.

  6. Neutralino Dark Matter in BMSSM Effective Theory

    E-Print Network [OSTI]

    Marcus Berg; Joakim Edsjo; Paolo Gondolo; Erik Lundstrom; Stefan Sjors

    2009-06-03

    We study thermal neutralino dark matter in an effective field theory extension of the MSSM, called "Beyond the MSSM" (BMSSM) in Dine, Seiberg and Thomas (2007). In this class of effective field theories, the field content of the MSSM is unchanged, but the little hierarchy problem is alleviated by allowing small corrections to the Higgs/higgsino part of the Lagrangian. We perform parameter scans and compute the dark matter relic density. The light Higgsino LSP scenario is modified the most; we find new regions of parameter space compared to the standard MSSM. This involves interesting interplay between the WMAP dark matter bounds and the LEP chargino bound. We also find some changes for gaugino LSPs, partly due to annihilation through a Higgs resonance, and partly due to coannihilation with light stops in models that are ruled in by the new effective terms.

  7. Neutralino dark matter in BMSSM effective theory

    SciTech Connect (OSTI)

    Berg, Marcus; Edsjö, Joakim; Lundström, Erik; Sjörs, Stefan; Gondolo, Paolo E-mail: edsjo@physto.se E-mail: erik@physto.se

    2009-08-01

    We study thermal neutralino dark matter in an effective field theory extension of the MSSM, called ''Beyond the MSSM'' (BMSSM) in Dine, Seiberg and Thomas (2007). In this class of effective field theories, the field content of the MSSM is unchanged, but the little hierarchy problem is alleviated by allowing small corrections to the Higgs/higgsino part of the Lagrangian. We perform parameter scans and compute the dark matter relic density. The light higgsino LSP scenario is modified the most; we find new regions of parameter space compared to the standard MSSM. This involves interesting interplay between the WMAP dark matter bounds and the LEP chargino bound. We also find some changes for gaugino LSPs, partly due to annihilation through a Higgs resonance, and partly due to coannihilation with light top squarks in models that are ruled in by the new effective terms.

  8. Symplectic gauge fields and dark matter

    E-Print Network [OSTI]

    Asorey, J; Garcia-Alvarez, D

    2015-01-01

    The dynamics of symplectic gauge fields provides a consistent framework for fundamental interactions based on spin three gauge fields. One remarkable property is that symplectic gauge fields only have minimal couplings with gravitational fields and not with any other field of the Standard Model. Interactions with ordinary matter and radiation can only arise from radiative corrections. In spite of the gauge nature of symplectic fields they acquire a mass by the Coleman-Weinberg mechanism which generates Higgs-like mass terms where the gravitational field is playing the role of a Higgs field. Massive symplectic gauge fields weakly interacting with ordinary matter are natural candidates for the dark matter component of the Universe.

  9. Symplectic gauge fields and dark matter

    E-Print Network [OSTI]

    J. Asorey; M. Asorey; D. Garcia-Alvarez

    2015-11-02

    The dynamics of symplectic gauge fields provides a consistent framework for fundamental interactions based on spin three gauge fields. One remarkable property is that symplectic gauge fields only have minimal couplings with gravitational fields and not with any other field of the Standard Model. Interactions with ordinary matter and radiation can only arise from radiative corrections. In spite of the gauge nature of symplectic fields they acquire a mass by the Coleman-Weinberg mechanism which generates Higgs-like mass terms where the gravitational field is playing the role of a Higgs field. Massive symplectic gauge fields weakly interacting with ordinary matter are natural candidates for the dark matter component of the Universe.

  10. Towards a 'Thermodynamics' of Active Matter

    E-Print Network [OSTI]

    Sho C. Takatori; John F. Brady

    2014-11-21

    Self-propulsion allows living systems to display unusual collective behavior. Unlike passive systems in thermal equilibrium, active matter systems are not constrained by conventional thermodynamic laws. A question arises however as to what extent, if any, can concepts from classical thermodynamics be applied to nonequilibrium systems like active matter. Here we use the new swim pressure perspective to develop a simple theory for predicting phase separation in active matter. Using purely mechanical arguments we generate a phase diagram with a spinodal and critical point, and define a nonequilibrium chemical potential to interpret the "binodal." We provide a generalization of thermodynamic concepts like the free energy and temperature for nonequilibrium active systems. Our theory agrees with existing simulation data both qualitatively and quantitatively and may provide a framework for understanding and predicting the behavior of nonequilibrium active systems.

  11. Unified Description of Dark Energy and Dark Matter

    E-Print Network [OSTI]

    Walter Petry

    2008-11-09

    Dark energy in the universe is assumed to be vacuum energy. The energy-momentum of vacuum is described by a scale-dependent cosmological constant. The equations of motion imply for the density of matter (dust) the sum of the usual matter density (luminous matter) and an additional matter density (dark matter) similar to the dark energy. The scale-dependent cosmological constant is given up to an exponent which is approximated by the experimentally decided density parameters of dark matter and dark energy. This yields that dark matter is one third of dark energy for all times implying an explanation of the coincidence of dark matter and dark energy. In the final state, the universe becomes dark, consisting of dark matter and dark energy.

  12. A SM Singlet Scalar as Dark Matter

    E-Print Network [OSTI]

    Tonatiuh Matos; Ricardo Lopez-Fernandez

    2014-03-20

    In this work we investigate the possibility that a simple extension of the Standard Model (SM) can be the dark matter of the universe. We postulate the existence of a scalar field singlet like the Higgs as an extra term in the SM Lagrangian. We find that from the astrophysical point of view a very small mass and self-interaction is more convenient to agree with observations and from particle detectors observations we do not see any essential constrain to this settings. Thus, we conclude that a scalar field singlet with a small mass and self-interaction is a good candidate to be the nature of the dark matter.

  13. Axions as hot and cold dark matter

    SciTech Connect (OSTI)

    Jeong, Kwang Sik; Kawasaki, Masahiro; Takahashi, Fuminobu E-mail: kawasaki@icrr.u-tokyo.ac.jp

    2014-02-01

    The presence of a hot dark matter component has been hinted at 3? by a combination of the results from different cosmological observations. We examine a possibility that pseudo Nambu-Goldstone bosons account for both hot and cold dark matter components. We show that the QCD axions can do the job for the axion decay constant f{sub a}?

  14. Microscopic calculations in asymmetric nuclear matter

    E-Print Network [OSTI]

    D. Alonso; F. Sammarruca

    2003-02-06

    A microscopic calculation of the equation of state for asymmetric nuclear matter is presented. We employ realistic nucleon-nucleon forces and operate within the Dirac-Brueckner-Hartree-Fock approach to nuclear matter. The focal point of this paper is a (momentum-space) G-matrix which properly accounts for the asymmetry between protons and neutrons. This will merge naturally into the development of an effective interaction suitable for applications to asymmetric nuclei, which will be the object of extensive study in the future.

  15. Asymmetric dark matter and the Sun

    E-Print Network [OSTI]

    Mads T. Frandsen; Subir Sarkar

    2010-06-01

    Cold dark matter particles with an intrinsic matter-antimatter asymmetry do not annihilate after gravitational capture by the Sun and can affect its interior structure. The rate of capture is exponentially enhanced when such particles have self-interactions of the right order to explain structure formation on galactic scales. A `dark baryon' of mass 5 GeV is a natural candidate and has the required relic abundance if its asymmetry is similar to that of ordinary baryons. We show that such particles can solve the `solar composition problem'. The predicted small decrease in the low energy neutrino fluxes may be measurable by the Borexino and SNO+ experiments.

  16. Particulate matter sensor with a heater

    DOE Patents [OSTI]

    Hall, Matthew (Austin, TX)

    2011-08-16

    An apparatus to detect particulate matter. The apparatus includes a sensor electrode, a shroud, and a heater. The electrode measures a chemical composition within an exhaust stream. The shroud surrounds at least a portion of the sensor electrode, exclusive of a distal end of the sensor electrode exposed to the exhaust stream. The shroud defines an air gap between the sensor electrode and the shroud and an opening toward the distal end of the sensor electrode. The heater is mounted relative to the sensor electrode. The heater burns off particulate matter in the air gap between the sensor electrode and the shroud.

  17. Gravitational mass of relativistic matter and antimatter

    E-Print Network [OSTI]

    Tigran Kalaydzhyan

    2015-07-09

    The universality of free fall, the weak equivalence principle (WEP), is a cornerstone of the general theory of relativity, the most precise theory of gravity confirmed in all experiments up to date. The WEP states the equivalence of the inertial, $m$, and gravitational, $m_g$, masses and was tested in numerous occasions with normal matter at relatively low energies. However, there is no proof for the matter and antimatter at high energies. For the antimatter the situation is even less clear -- current direct observations of trapped antihydrogen suggest the limits $-65 International Linear Collider (ILC) and Compact Linear Collider (CLIC).

  18. Wiley Online Library Books The Library has subscribed to about 310 Wiley Online Library Books, mainly covering subjects such as

    E-Print Network [OSTI]

    Po, Lai-Man

    of Hong Kong Access Search About Wiley Online Library Books 1. Enter search term(s) (Multiple words. 1. Enter search term(s) (Multiple words entered will be automatically combined with the AND operator entered will be automatically combined with the AND operator) 2. Select an operator to combine the search

  19. Dark-Matter-Induced Violation of the Weak Equivalence Principle

    SciTech Connect (OSTI)

    Carroll, Sean M.; Mantry, Sonny [California Institute of Technology, Pasadena, California 91125 (United States); Ramsey-Musolf, Michael J. [University of Wisconsin-Madison, Madison, Wisconsin 53706 (United States); California Institute of Technology, Pasadena, California 91125 (United States); Stubbs, Christoper W. [Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138 (United States)

    2009-07-03

    A long-range fifth force coupled to dark matter can induce a coupling to ordinary matter if the dark matter interacts with standard model fields. We consider constraints on such a scenario from both astrophysical observations and laboratory experiments. We also examine the case where the dark matter is a weakly interacting massive particle, and derive relations between the coupling to dark matter and the coupling to ordinary matter for different models. Currently, this scenario is most tightly constrained by galactic dynamics, but improvements in Eoetvoes experiments can probe unconstrained regions of parameter space.

  20. On the capture of dark matter by neutron stars

    SciTech Connect (OSTI)

    Güver, Tolga; Erkoca, Arif Emre; Sarcevic, Ina; Reno, Mary Hall E-mail: aeerkoca@gmail.com E-mail: ina@physics.arizona.edu

    2014-05-01

    We calculate the number of dark matter particles that a neutron star accumulates over its lifetime as it rotates around the center of a galaxy, when the dark matter particle is a self-interacting boson but does not self-annihilate. We take into account dark matter interactions with baryonic matter and the time evolution of the dark matter sphere as it collapses within the neutron star. We show that dark matter self-interactions play an important role in the rapid accumulation of dark matter in the core of the neutron star. We consider the possibility of determining an exclusion region of the parameter space for dark matter mass and dark matter interaction cross section with the nucleons as well as dark matter self-interaction cross section, based on the observation of old neutron stars. We show that for a dark matter density of 10{sup 3} GeV/cm{sup 3}and dark matter mass m{sub ?} ?< 10 GeV, there is a potential exclusion region for dark matter interactions with nucleons that is three orders of magnitude more stringent than without self-interactions. The potential exclusion region for dark matter self-interaction cross sections is many orders of magnitude stronger than the current Bullet Cluster limit. For example, for high dark matter density regions, we find that for m{sub ?} ? 10 GeV when the dark matter interaction cross section with the nucleons ranges from ?{sub ?n} ? 10{sup ?52} cm{sup 2} to ?{sub ?n} ? 10{sup ?57} cm{sup 2}, the dark matter self-interaction cross section limit is ?{sub ??} ?< 10{sup ?33} cm{sup 2}, which is about ten orders of magnitude stronger than the Bullet Cluster limit.