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Sample records for ramesh dandekar smg

  1. Ramamoorthy Ramesh | Department of Energy

    Energy Savers [EERE]

    Ramamoorthy Ramesh About Us Ramamoorthy Ramesh - Former Director, SunShot Initiative & Solar Energy Technologies Program Ramamoorthy Ramesh is the former Director of the SunShot Initiative and Solar Energy Technologies Program. Most Recent Making the Impossible Possible: From Kennedy's Moonshot to Solar's SunShot June 21 SunShot Grand Challenge Highlights Ambitious Efforts along the Entire Solar Spectrum June 13 SunShot Shoots for the Moon with First Grand Challenge Event May 23

  2. Ramesh Balakrishnan | Argonne Leadership Computing Facility

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

    National Laboratory 9700 South Cass Avenue Building 240 - Rm. 1128 Argonne, Illinois 60439 630-252-4191 bramesh@anl.gov Areas of Interest: CFD, Numerical Methods, Turbulence...

  3. Carbon Cycle 2.0: Ramamoorthy Ramesh: Low-cost Solar

    ScienceCinema (OSTI)

    Ramamoorthy Ramesh:

    2010-09-01

    Feb. 4, 2010: Humanity emits more carbon into the atmosphere than natural processes are able to remove - an imbalance with negative consequences. Carbon Cycle 2.0 is a Berkeley Lab initiative to provide the science needed to restore this balance by integrating the Labs diverse research activities and delivering creative solutions toward a carbon-neutral energy future.

  4. Microsoft Word - LM SMG Jan 2016 Update 18 Draft 12 no links...

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

    ... LM Site Name Pre-LM Name Category Transferring Organization Regulatory Driver 1 Curtis Bay, MD, Site W.R. Grace at Curtis Bay Site 2 USACE FUSRAP 2 Ford, WA, Disposal Site Dawn - ...

  5. Search for: All records | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    ... Subedi, Ramesh R. ; Wang, Diancheng ; Pan, Kai ; Deng, Xiaoyan ; Michaels, Robert W. ... Nucleon Resonance Region Wang, Diancheng ; Pan, Kai ; Subedi, Ramesh R. ; Deng, Xiaoyan We ...

  6. untitled

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

    The SMGSMU acronyms are: NW: Nuclear Weapons SMG & SMU ITS: Integrated Technologies & Systems SMG DS&A: Defense Systems & Assessments SMU ER&N: Energy, Resources, & ...

  7. Microsoft Word - UserSurvey09results.docx

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

    use of ALCF resources. Our catalyst team: Charles Bacon, Ramesh Balakrishnan, Graham Fletcher, Kumar Kalyan, Ray Loy, Vitali Morozov, James Osborn, Scott Parker, Katherine Riley,...

  8. Search for: All records | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    ... A scaler-based data acquisition system for measuring parity-violating asymmetry in deep inelastic scattering Subedi, Ramesh R. ; Wang, Diancheng ; Pan, Kai ; Deng, Xiaoyan ; ...

  9. Search for: All records | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    Subedi, Ramesh R. ; Wang, Diancheng ; Pan, Kai ; Deng, Xiaoyan ; Michaels, Robert W. ... ; Zheng Xiaochao ; Michaels, Robert ; Pan Kai ; Reimer, Paul E. The 6 GeV Parity ...

  10. A Solar Re-Skin at FedEx Field | Department of Energy

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

    Ramamoorthy Ramesh Former Director, SunShot Initiative & Solar Energy Technologies Program ... fans interested in joining the Redskins as they move toward a clean energy future. ...

  11. untitled

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

    7, as submitted by center offices and selected by the division offices. Each citation is followed by the center numbers of centers that contributed most directly to the effort described. An acronym after each accomplishment indicates which of Sandia's strategic management units (SMUs) or strategic management groups (SMGs) the work most directly supported. The SMG/SMU acronyms are: NW: Nuclear Weapons SMG & SMU ITS: Integrated Technologies & Systems SMG LT: Laboratory Transformation SMG

  12. Synthetic and Mechanistic Chemistry

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

    22(3), 189-198 (2009). Ramesh R. Kale, Harshini Mukundan, Dominique N. Price, J. Foster Harris, Daniel M. Lewallen, Basil I. Swanson, Jurgen G. Schmidt, and Suri S. Iyer,...

  13. Browse by Discipline -- E-print Network Subject Pathways: Fossil Fuels --

    Office of Scientific and Technical Information (OSTI)

    Energy, science, and technology for the research community -- hosted by the Office of Scientific and Technical Information, U.S. Department of Energy S T U V W X Y Z Rabinowitz, Joshua D. (Joshua D. Rabinowitz) - Lewis-Sigler Institute for Integrative Genomics & Department of Molecular Biology, Princeton University Raina, Ramesh (Ramesh Raina) - Department of Biology, Syracuse University Ratner, Daniel M. (Daniel M. Ratner) - Department of Bioengineering, University of Washington at

  14. Tuesday Opening Address | Department of Energy

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

    Tuesday Opening Address Tuesday Opening Address May 20, 2014 12:30PM to 1:00PM PDT Pacific Ballroom Featuring Minh Le, Director of the SunShot Initiative, and Ramamoorthy Ramesh, Deputy Director for Science and Technology at Oak Ridge National Laboratory

  15. LM Releases Update of Site Management Guide

    Broader source: Energy.gov [DOE]

    A new edition of the U.S. Department of Energy (DOE) Office of Legacy Management (LM) Site Management Guide (SMG) was posted to the LM website, February 24, 2015.

  16. Sandia Labs Accomplishments 2010

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

    The SMGSMU acronyms are: NW: Nuclear Weapons SMG & SMU DS&A: Defense Systems & Assessments SMU ER&N: Energy, Resources, & Nonproliferation SMU HS&D: Homeland Security & Defense ...

  17. Sandia Labs Accomplishments 2010

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

    9, as submitted by center offices and selected by division offices. Each citation is followed by the numbers of centers that contributed most directly to the effort described. An acronym after each accomplishment indicates which of Sandia's strategic management units (SMUs) or strategic management groups (SMGs) the work most directly supported. The SMG/SMU acronyms are: NW: Nuclear Weapons SMG & SMU DS&A: Defense Systems & Assessments SMU ER&N: Energy, Resources, &

  18. Summary of the Fall 2005 ASA Meetings

    Gasoline and Diesel Fuel Update (EIA)

    0 and 21, 2005 with the Energy Information Administration 1000 Independence Ave., SW. Washington, D.C. 20585 Introductory Sessions: Opening Remarks: Guy Caruso, EIA Administrator to include: 1. Update on the External Review Team 2. New EIA Homepages 3. EIA-914 Data 4. Hurricane Katrina Updates: 5. Since the Spring Meeting, Nancy Kirkendall, Director, SMG 6. Results of the Simulation Study for the EIA-914, Preston McDowney, SMG 7. Update: EIA's Regional Short-Term Energy Outlook, Margot Anderson,

  19. untitled

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

    Accomplishments publication recognizes some of Sandia's best work during 2008, as submitted by center offices and selected by division offices. Each citation is followed by the center numbers of centers that contributed most directly to the effort described. An acronym after each accomplishment indicates which of Sandia's strategic management units (SMUs) or strategic management groups (SMGs) the work most directly supported. The SMG/SMU acronyms are: NW: Nuclear Weapons SMG & SMU ITS:

  20. STUDY OF USING OXYGEN-ENRICHED COMBUSTION AIR FOR LOCOMOTIVE DIESEL ENGINES

    Office of Scientific and Technical Information (OSTI)

    STUDY OF USING OXYGEN-ENRICHED COMBUSTION AIR FOR LOCOMOTIVE DIESEL ENGINES Ramesh B. Poola and Raj Sekar Argonne National Laboratory Argonne, Illinois Dennis N. Assanis The University of Michigan Ann Arbor, Michigan G. Richard Cataldi Association of American Railroads Washington, D.C. ABSTRACT A thermodynamic simulation is used to study the effects of oxygen-enriched intake air on the performance and nitrogen oxide (NO) emissions of a locomotive diesel engine. The parasitic power of the air

  1. Carbon Nanohoops: Molecular Templates for Precision Nanotube Synthesis -

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

    Energy Innovation Portal Find More Like This Return to Search Carbon Nanohoops: Molecular Templates for Precision Nanotube Synthesis Lawrence Berkeley National Laboratory Contact LBL About This Technology Technology Marketing SummaryRamesh Jasti and Carolyn Bertozzi of Berkeley Lab have developed a technique to build carbon-ring "nanohoops," molecular building blocks for the formation of carbon nanotubes. Carbon nanohoops might serve as seeds, or templates, for the efficient and

  2. Center for Nanophase Materials Sciences (CNMS) - CNMS User Research

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

    Intrinsic Nucleation Mechanism of Polarization Switching on Ferroelectric Surfaces Peter Maksymovych,1 Stephen Jesse,1 Mark Huijben,2 Ramamoorthy Ramesh,2 Anna Morozovska,3 Samrat Choudhury,4 Long-Qing Chen,4 Arthur P. Baddorf,1 and Sergei V. Kalinin1 1Center for Nanophase Materials Sciences, Oak Ridge National Laboratory; 2Department of Materials Sciences and Engineering and Department of Physics, University of California Berkeley; 3Lashkaryov Institute for Semiconductor Physics, National

  3. Center for Nanophase Materials Sciences (CNMS) - CNMS User Research

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

    Polarization Control of Electron Tunneling into Ferroelectric Surfaces Peter Maksymovych1, Stephen Jesse1, Pu Yu2, Ramamoorthy Ramesh2, Arthur P. Baddorf,1 and Sergei V. Kalinin1 1 The Center for Nanophase Materials Sciences, Oak Ridge National Laboratory, Oak Ridge, TN 37831 2Department of Materials Sciences and Engineering and Department of Physics, University of California Berkeley Achievement We have discovered that polarization switching in 30-50 nm oxide films of lead-zirconate and bismuth

  4. Large Eddy Simulation of Airfoil SelfNoise | Argonne Leadership Computing

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

    Facility Large Eddy Simulation of Airfoil SelfNoise Event Sponsor: Argonne Leadership Computing Facility Seminar Start Date: Feb 4 2016 - 10:30am Building/Room: Building 240/Room 4301 Location: Argonne National Laboratory Speaker(s): Joseph George Kocheemoolayil Speaker(s) Title: Stanford University Host: Ramesh Balakrishnan Over the past 15 years, significant strides have been made towards using large eddy simulations (LES) for predicting airfoil self-noise. However, they have largely been

  5. Staff Directory | Argonne Leadership Computing Facility

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

    About Overview History Staff Directory Our Teams User Advisory Council Careers Margaret Butler Fellowship Visiting Us Contact Us Staff Directory Yury Alekseev Yuri Alexeev Assistant Computational Scientist Catalyst 630-252-0157 yuri@alcf.anl.gov Bill Allcock Bill Allcock Manager, Advanced Integration Group Leadership, AIG 630-252-7573 allcock@anl.gov Ben Allen HPC Systems Administration Specialist Systems 630-252-0554 allen@alcf.anl.gov Ramesh Balakrishnan Computational Scientist Catalyst

  6. Search for: All records | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    Subedi, Ramesh" Name Name ORCID Search Authors Type: All Book/Monograph Conference/Event Journal Article Miscellaneous Patent Program Document Software Manual Technical Report Thesis/Dissertation Subject: Identifier Numbers: Site: All Alaska Power Administration, Juneau, Alaska (United States) Albany Research Center (ARC), Albany, OR (United States) Albuquerque Complex - NNSA Albuquerque Operations Office, Albuquerque, NM (United States) Amarillo National Resource Center for Plutonium,

  7. Revitalizing American Competitiveness in Solar Technologies | Department of

    Energy Savers [EERE]

    Energy Revitalizing American Competitiveness in Solar Technologies Revitalizing American Competitiveness in Solar Technologies These slides correspond to a presentation given by Oak Ridge National Laboratory Deputy Director for Science and Technology and former SunShot Initiative Director, Dr. Ramamoorthy Ramesh at the 2014 SunShot Grand Challenge Summit and Peer Review in Anaheim, CA. This presentation is about revitalizing American competitiveness in solar technologies. PDF icon

  8. Full Electroresistance Modulation in a Mixed-Phase Metallic Alloy (Journal

    Office of Scientific and Technical Information (OSTI)

    Article) | SciTech Connect Full Electroresistance Modulation in a Mixed-Phase Metallic Alloy Citation Details In-Document Search This content will become publicly available on March 3, 2017 Title: Full Electroresistance Modulation in a Mixed-Phase Metallic Alloy Authors: Liu, Z. Q. ; Li, L. ; Gai, Z. ; Clarkson, J. D. ; Hsu, S. L. ; Wong, A. T. ; Fan, L. S. ; Lin, M.-W. ; Rouleau, C. M. ; Ward, T. Z. ; Lee, H. N. ; Sefat, A. S. ; Christen, H. M. ; Ramesh, R. Publication Date: 2016-03-03 OSTI

  9. An Update on White House Solar Panels and Our Solar Program | Department of

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

    Energy White House Solar Panels and Our Solar Program An Update on White House Solar Panels and Our Solar Program June 20, 2011 - 6:11pm Addthis Ramamoorthy Ramesh Former Director, SunShot Initiative & Solar Energy Technologies Program We cannot win the future without winning the clean energy race, which is why President Obama laid out a clear goal to increase our nation's clean energy share and continue to build a 21st century clean energy economy. Last fall, to underscore the Obama

  10. Center for Nanophase Materials Sciences (CNMS) - CNMS Research

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

    Tunable Metallic Conductance in Ferroelectric Nanodomains Peter Maksymovych,1 Anna N. Morozovska,2,3 Pu Yu,4 Eugene A. Eliseev,3 Ying-Hao Chu,4,5 Ramamoorthy Ramesh,4 Arthur P. Baddorf,1 and Sergei V. Kalinin1 1 Center for Nanophase Materials Science, Oak Ridge National Laboratory, Oak Ridge, TN, 37831 2 Institute of Semiconductor Physics, National Academy of Science of Ukraine,41, pr. Nauki, 03028 Kiev, Ukraine 3 Institute for Problems of Materials Science, National Academy of Science of

  11. Center for Nanophase Materials Sciences (CNMS) - CNMS Research

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

    Dynamic Conductivity of Ferroelectric Domain Walls in BiFeO3 Peter Maksymovych,1 Jan Seidel,2-3 Ying Hao Chu,4 Pingping Wu,5 Arthur P. Baddorf,1 Long-Qing Chen,5 Sergei V. Kalinin,1 and Ramamoorthy Ramesh2-3 1 Center for Nanophase Materials Science, Oak Ridge National Laboratory 2 Lawrence Berkeley National Laboratory 3 University of California, Berkeley 4 National Chiao Tung University, Taiwan 5 Pennsylvania State University Achievement Two years ago, electrical conductivity was discovered in

  12. Center for Nanophase Materials Sciences (CNMS) - News

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

    CNMS News Enhanced Electric Conductivity at Ferroelectric Vortex Cores in BiFeO3 Nina Balke,1 Benjamin Winchester,2 Wei Ren,3 Ying Hao Chu,4,5 Anna N. Morozovska,6 Eugene A. Eliseev,7 Mark Huijben,8 Rama K. Vasudevan,9 Petro Maksymovych,1 Jason Britson,2 Stephen Jesse,1 Igor Kornev,10 Ramamoorthy Ramesh,5 Laurent Bellaiche,3 Long Qing Chen,2 and Sergei V. Kalinin1 1 The Center for Nanophase Materials Sciences, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831 2 Department of Materials

  13. Low Cost Solar Energy Conversion (Carbon Cycle 2.0)

    SciTech Connect (OSTI)

    Ramesh, Ramamoorthy

    2010-02-04

    Ramamoorthy Ramesh from LBNL's Materials Science Division speaks at the Carbon Cycle 2.0 kick-off symposium Feb. 2, 2010. We emit more carbon into the atmosphere than natural processes are able to remove - an imbalance with negative consequences. Carbon Cycle 2.0 is a Berkeley Lab initiative to provide the science needed to restore this balance by integrating the Labs diverse research activities and delivering creative solutions toward a carbon-neutral energy future. http://carboncycle2.lbl.gov/

  14. Slide 1

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

    Ramesh, Former Director, SunShot Deputy Director for Science and Technology Oak Ridge National Laboratory Revitalizing American Competitiveness in Solar Technologies 2 Lunar Landing: 1969 3 "We choose to go to the moon in this decade and do the other things, not because they are easy, but because they are hard....Because that challenge is one that we are willing to accept, one we are unwilling to postpone, and one which we intend to win..." - President Kennedy September 12, 1962 4

  15. CMI Success Stories | Critical Materials Institute

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

    CMI Success Stories signing ceremony for first license of CMI technology Update: The license agreement was announced in August, and the official signing at Oak Ridge National Laboratory was November 19. Shown, front row: Kevin M. Cassidy, president and CEO of U.S. Rare Earths, and Dr. Thom Mason, Director of Oak Ridge National Laboratory (ORNL). Back row: Nestor Franco, ORNL Tech Transfer; Preston Bryant, U.S. Rare Earths; Dr. Ramesh Bhave, ORNL; and Dr. Daejin Kim, ORNL. collage image for first

  16. Low Cost Solar Energy Conversion (Carbon Cycle 2.0)

    ScienceCinema (OSTI)

    Ramesh, Ramamoorthy

    2011-06-08

    Ramamoorthy Ramesh from LBNL's Materials Science Division speaks at the Carbon Cycle 2.0 kick-off symposium Feb. 2, 2010. We emit more carbon into the atmosphere than natural processes are able to remove - an imbalance with negative consequences. Carbon Cycle 2.0 is a Berkeley Lab initiative to provide the science needed to restore this balance by integrating the Labs diverse research activities and delivering creative solutions toward a carbon-neutral energy future. http://carboncycle2.lbl.gov/

  17. 3C 220.3: A radio galaxy lensing a submillimeter galaxy

    SciTech Connect (OSTI)

    Haas, Martin; Westhues, Christian; Chini, Rolf; Leipski, Christian; Klaas, Ulrich; Meisenheimer, Klaus; Barthel, Peter; Koopmans, Lιon V. E.; Wilkes, Belinda J.; Bussmann, R. Shane; Willner, S. P.; Ashby, Matthew L. N.; Kuraszkiewicz, Joanna; Vegetti, Simona; Clements, David L.; Fassnacht, Christopher D.; Horesh, Assaf; Lagattuta, David J.; Stern, Daniel; Wylezalek, Dominika

    2014-07-20

    Herschel Space Observatory photometry and extensive multiwavelength follow-up have revealed that the powerful radio galaxy (PRG) 3C 220.3 at z = 0.685 acts as a gravitational lens for a background submillimeter galaxy (SMG) at z = 2.221. At an observed wavelength of 1 mm, the SMG is lensed into three distinct images. In the observed near infrared, these images are connected by an arc of ?1''.8 radius forming an Einstein half-ring centered near the radio galaxy. In visible light, only the arc is apparent. 3C 220.3 is the only known instance of strong galaxy-scale lensing by a PRG not located in a galaxy cluster and therefore it offers the potential to probe the dark matter content of the radio galaxy host. Lens modeling rejects a single lens, but two lenses centered on the radio galaxy host A and a companion B, separated by 1''.5, provide a fit consistent with all data and reveal faint candidates for the predicted fourth and fifth images. The model does not require an extended common dark matter halo, consistent with the absence of extended bright X-ray emission on our Chandra image. The projected dark matter fractions within the Einstein radii of A (1''.02) and B (0''.61) are about 0.4 ± 0.3 and 0.55 ± 0.3. The mass to i-band light ratios of A and B, M/L{sub i}?8±4 M{sub ?} L{sub ?}{sup ?1}, appear comparable to those of radio-quiet lensing galaxies at the same redshift in the CfA-Arizona Space Telescope LEns Survey, Lenses Structure and Dynamics, and Strong Lenses in the Legacy Survey samples. The lensed SMG is extremely bright with observed f(250 ?m) = 440 mJy owing to a magnification factor ? ? 10. The SMG spectrum shows luminous, narrow C IV ?1549 Ε emission, revealing that the SMG houses a hidden quasar in addition to a violent starburst. Multicolor image reconstruction of the SMG indicates a bipolar morphology of the emitted ultraviolet (UV) light suggestive of cones through which UV light escapes a dust-enshrouded nucleus.

  18. Summary of the Fall 2004 ASA Meeting

    Gasoline and Diesel Fuel Update (EIA)

    8 and 29, 2004 with the Energy Information Administration 1000 Independence Ave., SW. Washington, D.C. 20585 Thursday, October 28, 2004 1. EIA Program to Evaluate Form EIA-920, Combined Heat and Power Plant Report, Robert Rutchik, SMG, EIA In early 2004, EIA disseminated the new survey, Form EIA-920, Combined Heat and Power Plant (CHP) Report to CHP facilities to collect data on their total fuel used, fuel used to generate electricity, generation, and fossil fuel stocks. The survey's primary

  19. Super Bowl City Leads on Energy Efficient Forefront | Department of Energy

    Energy Savers [EERE]

    Bowl City Leads on Energy Efficient Forefront Super Bowl City Leads on Energy Efficient Forefront February 2, 2013 - 11:30am Addthis New Orleans' Mercedes-Benz Superdome features more than 26,000 LED lights on the building's exterior. The system uses only 10 kilowatts of electricity, equivalent to powering a small home. | Photo courtesy of SMG. New Orleans' Mercedes-Benz Superdome features more than 26,000 LED lights on the building's exterior. The system uses only 10 kilowatts of electricity,

  20. Just Say No to Carbon Emissions (LBNL Science at the Theater)

    ScienceCinema (OSTI)

    Ramesh, Ramamoorthy; Zhou, Nan; Oldenburg, Curt

    2011-04-28

    Learn about three efforts our grandchildren may thank us for: cheap solar energy, bringing energy efficiency to China, and learning how to store carbon deep underground. Can solar energy be dirt cheap? We're all potentially billionaires when it comes to solar energy. The trick is learning how to convert sunlight to electricity using cheap and plentiful materials. Ramamoorthy Ramesh, an innovative materials scientist at Berkeley Lab, will discuss how he and other researchers are working to make photovoltaic cells using the most abundant elements in the Earth's crust -- materials that are literally as common as dirt. Energy efficiency in China: Nan Zhou is a researcher with Berkeley Labs China Energy Group. She will speak about Chinas energy use and the policies that have been implemented to increase energy efficiency and reduce CO2 emission growth. Her work focuses on building China's capacity to evaluate, adopt and implement low-carbon development strategies. Zhou has an architecture degree from China, and a Master and Ph.D. in Engineering from Japan. Understanding geologic carbon sequestration: Even with continued growth of renewable energy sources such as wind and solar, fossil fuels will likely remain cheap and plentiful for decades to come. Geologist Curt Oldenburg, who heads Berkeley Lab's Geologic Carbon Sequestration Program, will discuss a strategy to reduce carbon emissions from coal and natural gas. It involves pumping compressed CO2 captured from large stationary sources into underground rock formations that can store it for geological time scales.

  1. Just Say No to Carbon Emissions (LBNL Science at the Theater)

    SciTech Connect (OSTI)

    Ramesh, Ramamoorthy; Zhou, Nan; Oldenburg, Curt

    2010-04-26

    Learn about three efforts our grandchildren may thank us for: cheap solar energy, bringing energy efficiency to China, and learning how to store carbon deep underground. Can solar energy be dirt cheap? We're all potentially billionaires when it comes to solar energy. The trick is learning how to convert sunlight to electricity using cheap and plentiful materials. Ramamoorthy Ramesh, an innovative materials scientist at Berkeley Lab, will discuss how he and other researchers are working to make photovoltaic cells using the most abundant elements in the Earth's crust -- materials that are literally as common as dirt. Energy efficiency in China: Nan Zhou is a researcher with Berkeley Labs China Energy Group. She will speak about Chinas energy use and the policies that have been implemented to increase energy efficiency and reduce CO2 emission growth. Her work focuses on building China's capacity to evaluate, adopt and implement low-carbon development strategies. Zhou has an architecture degree from China, and a Master and Ph.D. in Engineering from Japan. Understanding geologic carbon sequestration: Even with continued growth of renewable energy sources such as wind and solar, fossil fuels will likely remain cheap and plentiful for decades to come. Geologist Curt Oldenburg, who heads Berkeley Lab's Geologic Carbon Sequestration Program, will discuss a strategy to reduce carbon emissions from coal and natural gas. It involves pumping compressed CO2 captured from large stationary sources into underground rock formations that can store it for geological time scales.

  2. ALMA imaging of gas and dust in a galaxy protocluster at redshift 5.3: [C II] emission in 'typical' galaxies and dusty starbursts ?1 billion years after the big bang

    SciTech Connect (OSTI)

    Riechers, Dominik A.; Carilli, Christopher L.; Capak, Peter L.; Yan, Lin; Scoville, Nicholas Z.; Smol?i?, Vernesa; Schinnerer, Eva; Yun, Min; Cox, Pierre; Bertoldi, Frank; Karim, Alexander

    2014-12-01

    We report interferometric imaging of [C II]({sup 2} P {sub 3/2}?{sup 2} P {sub 1/2}) and OH({sup 2}?{sub 1/2} J = 3/2?1/2) emission toward the center of the galaxy protocluster associated with the z = 5.3 submillimeter galaxy (SMG) AzTEC-3, using the Atacama Large (sub)Millimeter Array (ALMA). We detect strong [C II], OH, and rest-frame 157.7 ?m continuum emission toward the SMG. The [C II]({sup 2} P {sub 3/2}?{sup 2} P {sub 1/2}) emission is distributed over a scale of 3.9 kpc, implying a dynamical mass of 9.7 Χ 10{sup 10} M {sub ?}, and a star formation rate (SFR) surface density of ?{sub SFR} = 530 M {sub ?} yr{sup –1} kpc{sup –2}. This suggests that AzTEC-3 forms stars at ?{sub SFR} approaching the Eddington limit for radiation pressure supported disks. We find that the OH emission is slightly blueshifted relative to the [C II] line, which may indicate a molecular outflow associated with the peak phase of the starburst. We also detect and dynamically resolve [C II]({sup 2} P {sub 3/2}?{sup 2} P {sub 1/2}) emission over a scale of 7.5 kpc toward a triplet of Lyman-break galaxies with moderate UV-based SFRs in the protocluster at ?95 kpc projected distance from the SMG. These galaxies are not detected in the continuum, suggesting far-infrared SFRs of <18-54 M {sub ?} yr{sup –1}, consistent with a UV-based estimate of 22 M {sub ?} yr{sup –1}. The spectral energy distribution of these galaxies is inconsistent with nearby spiral and starburst galaxies, but resembles those of dwarf galaxies. This is consistent with expectations for young starbursts without significant older stellar populations. This suggests that these galaxies are significantly metal-enriched, but not heavily dust-obscured, 'normal' star-forming galaxies at z > 5, showing that ALMA can detect the interstellar medium in 'typical' galaxies in the very early universe.

  3. SPITZER IMAGING OF HERSCHEL-ATLAS GRAVITATIONALLY LENSED SUBMILLIMETER SOURCES

    SciTech Connect (OSTI)

    Hopwood, R.; Negrello, M.; Wardlow, J.; Cooray, A.; Khostovan, A. A.; Kim, S.; Barton, E.; Da Cunha, E.; Cooke, J.; Burgarella, D.; Aretxaga, I.; Auld, R.; Baes, M.; Bertoldi, F.; Bonfield, D. G.; Blundell, R.; Buttiglione, S.; Cava, A.; Dannerbauer, H.

    2011-02-10

    We present physical properties of two submillimeter selected gravitationally lensed sources, identified in the Herschel Astrophysical Terahertz Large Area Survey. These submillimeter galaxies (SMGs) have flux densities >100 mJy at 500 {mu}m, but are not visible in existing optical imaging. We fit light profiles to each component of the lensing systems in Spitzer IRAC 3.6 and 4.5 {mu}m data and successfully disentangle the foreground lens from the background source in each case, providing important constraints on the spectral energy distributions (SEDs) of the background SMG at rest-frame optical-near-infrared wavelengths. The SED fits show that these two SMGs have high dust obscuration with A{sub V} {approx} 4-5 and star formation rates of {approx}100 M{sub sun} yr{sup -1}. They have low gas fractions and low dynamical masses compared with 850 {mu}m selected galaxies.

  4. UNITED STATE% ENGINEER OFFICE I" RaCLI MANHATTAN D' ISTRICT

    Office of Legacy Management (LM)

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  5. A COMPREHENSIVE VIEW OF A STRONGLY LENSED PLANCK-ASSOCIATED SUBMILLIMETER GALAXY

    SciTech Connect (OSTI)

    Fu Hai; Cooray, A.; Jullo, E.; Bussmann, R. S.; Ivison, R. J.; Perez-Fournon, I.; Djorgovski, S. G.; Scoville, N.; Yan, L.; Riechers, D. A.; Bradford, M.; Aguirre, J.; Auld, R.; Baes, M.; Baker, A. J.; Cava, A.; Clements, D. L.; Dannerbauer, H.; Dariush, A.; De Zotti, G.; and others

    2012-07-10

    We present high-resolution maps of stars, dust, and molecular gas in a strongly lensed submillimeter galaxy (SMG) at z = 3.259. HATLAS J114637.9-001132 is selected from the Herschel-Astrophysical Terahertz Large Area Survey (H-ATLAS) as a strong lens candidate mainly based on its unusually high 500 {mu}m flux density ({approx}300 mJy). It is the only high-redshift Planck detection in the 130 deg{sup 2} H-ATLAS Phase-I area. Keck Adaptive Optics images reveal a quadruply imaged galaxy in the K band while the Submillimeter Array and the Jansky Very Large Array show doubly imaged 880 {mu}m and CO(1{yields}0) sources, indicating differentiated distributions of the various components in the galaxy. In the source plane, the stars reside in three major kpc-scale clumps extended over {approx}1.6 kpc, the dust in a compact ({approx}1 kpc) region {approx}3 kpc north of the stars, and the cold molecular gas in an extended ({approx}7 kpc) disk {approx}5 kpc northeast of the stars. The emissions from the stars, dust, and gas are magnified by {approx}17, {approx}8, and {approx}7 times, respectively, by four lensing galaxies at z {approx} 1. Intrinsically, the lensed galaxy is a warm (T{sub dust} {approx} 40-65 K), hyper-luminous (L{sub IR} {approx} 1.7 Multiplication-Sign 10{sup 13} L{sub Sun }; star formation rate (SFR) {approx}2000 M{sub Sun} yr{sup -1}), gas-rich (M{sub gas}/M{sub baryon} {approx} 70%), young (M{sub stellar}/SFR {approx} 20 Myr), and short-lived (M{sub gas}/SFR {approx} 40 Myr) starburst. With physical properties similar to unlensed z > 2 SMGs, HATLAS J114637.9-001132 offers a detailed view of a typical SMG through a powerful cosmic microscope.

  6. A DETAILED GRAVITATIONAL LENS MODEL BASED ON SUBMILLIMETER ARRAY AND KECK ADAPTIVE OPTICS IMAGING OF A HERSCHEL-ATLAS SUBMILLIMETER GALAXY AT z = 4.243 {sup ,} {sup ,}

    SciTech Connect (OSTI)

    Bussmann, R. S.; Gurwell, M. A.; Fu Hai; Cooray, A.; Smith, D. J. B.; Bonfield, D.; Dunne, L.; Dye, S.; Eales, S.; Auld, R.; Baes, M.; Fritz, J.; Baker, A. J.; Cava, A.; Clements, D. L.; Dariush, A.; Coppin, K.; Dannerbauer, H.; De Zotti, G.; Hopwood, R.; and others

    2012-09-10

    We present high-spatial resolution imaging obtained with the Submillimeter Array (SMA) at 880 {mu}m and the Keck adaptive optics (AO) system at the K{sub S}-band of a gravitationally lensed submillimeter galaxy (SMG) at z = 4.243 discovered in the Herschel Astrophysical Terahertz Large Area Survey. The SMA data (angular resolution Almost-Equal-To 0.''6) resolve the dust emission into multiple lensed images, while the Keck AO K{sub S}-band data (angular resolution Almost-Equal-To 0.''1) resolve the lens into a pair of galaxies separated by 0.''3. We present an optical spectrum of the foreground lens obtained with the Gemini-South telescope that provides a lens redshift of z{sub lens} = 0.595 {+-} 0.005. We develop and apply a new lens modeling technique in the visibility plane that shows that the SMG is magnified by a factor of {mu} = 4.1 {+-} 0.2 and has an intrinsic infrared (IR) luminosity of L{sub IR} = (2.1 {+-} 0.2) Multiplication-Sign 10{sup 13} L{sub Sun }. We measure a half-light radius of the background source of r{sub s} = 4.4 {+-} 0.5 kpc which implies an IR luminosity surface density of {Sigma}{sub IR} (3.4 {+-} 0.9) Multiplication-Sign 10{sup 11} L{sub Sun} kpc{sup -2}, a value that is typical of z > 2 SMGs but significantly lower than IR luminous galaxies at z {approx} 0. The two lens galaxies are compact (r{sub lens} Almost-Equal-To 0.9 kpc) early-types with Einstein radii of {theta}{sub E1} 0.57 {+-} 0.01 and {theta}{sub E2} = 0.40 {+-} 0.01 that imply masses of M{sub lens1} = (7.4 {+-} 0.5) Multiplication-Sign 10{sup 10} M{sub Sun} and M{sub lens2} = (3.7 {+-} 0.3) Multiplication-Sign 10{sup 10} M{sub Sun }. The two lensing galaxies are likely about to undergo a dissipationless merger, and the mass and size of the resultant system should be similar to other early-type galaxies at z {approx} 0.6. This work highlights the importance of high spatial resolution imaging in developing models of strongly lensed galaxies discovered by Herschel.

  7. DYNAMICAL STRUCTURE OF THE MOLECULAR INTERSTELLAR MEDIUM IN AN EXTREMELY BRIGHT, MULTIPLY LENSED z {approx_equal} 3 SUBMILLIMETER GALAXY DISCOVERED WITH HERSCHEL

    SciTech Connect (OSTI)

    Riechers, Dominik A.; Cooray, A.; Carpenter, J. M.; Bock, J.; Omont, A.; Neri, R.; Cox, P.; Harris, A. I.; Baker, A. J.; Frayer, D. T.; Auld, R.; Aussel, H.; Chanial, P.; Blundell, R.; Brisbin, D.; Burgarella, D.; Chapman, S. C.; Clements, D. L.

    2011-05-20

    We report the detection of CO(J = 5 {yields} 4), CO(J = 3 {yields} 2), and CO(J = 1 {yields} 0) emission in the strongly lensed, Herschel/SPIRE-selected submillimeter galaxy (SMG) HERMES J105751.1+573027 at z = 2.9574 {+-} 0.0001, using the Plateau de Bure Interferometer, the Combined Array for Research in Millimeter-wave Astronomy, and the Green Bank Telescope. The observations spatially resolve the molecular gas into four lensed images with a maximum separation of {approx}9'' and reveal the internal gas dynamics in this system. We derive lensing-corrected CO line luminosities of L'{sub CO(1-0)} = (4.17 {+-} 0.41), L'{sub CO(3-2)} = (3.96 {+-} 0.20), and L'{sub CO(5-4)} = (3.45 {+-} 0.20) x 10{sup 10} ({mu}{sub L}/10.9){sup -1} K km s{sup -1} pc{sup 2}, corresponding to luminosity ratios of r{sub 31} = 0.95 {+-} 0.10, r{sub 53} = 0.87 {+-} 0.06, and r{sub 51} = 0.83 {+-} 0.09. This suggests a total molecular gas mass of M{sub gas} = 3.3x10{sup 10} ({alpha}{sub CO}/0.8) ({mu}{sub L}/10.9){sup -1} M{sub sun}. The gas mass, gas mass fraction, gas depletion timescale, star formation efficiency, and specific star formation rate are typical for an SMG. The velocity structure of the gas reservoir suggests that the brightest two lensed images are dynamically resolved projections of the same dust-obscured region in the galaxy that are kinematically offset from the unresolved fainter images. The resolved kinematics appear consistent with the complex velocity structure observed in major, 'wet' (i.e., gas-rich) mergers. Major mergers are commonly observed in SMGs and are likely to be responsible for fueling their intense starbursts at high gas consumption rates. This study demonstrates the level of detail to which galaxies in the early universe can be studied by utilizing the increase in effective spatial resolution and sensitivity provided by gravitational lensing.

  8. MODELING OF THE HERMES SUBMILLIMETER SOURCE LENSED BY A DARK MATTER DOMINATED FOREGROUND GROUP OF GALAXIES

    SciTech Connect (OSTI)

    Gavazzi, R.; Cooray, A.; Conley, A.; Aguirre, J. E.; Amblard, A.; Auld, R.; Beelen, A.; Blain, A.; Bock, J.; Bradford, C. M.; Bridge, C.; Djorgovski, S. G.; Blundell, R.; Brisbin, D.; Burgarella, D.; Chanial, P.; Christopher, N.; Clements, D. L.; Cox, P.

    2011-09-10

    We present the results of a gravitational lensing analysis of the bright z{sub s} = 2.957 submillimeter galaxy (SMG) HERMES found in the Herschel/SPIRE science demonstration phase data from the Herschel Multi-tiered Extragalactic Survey (HerMES) project. The high-resolution imaging available in optical and near-IR channels, along with CO emission obtained with the Plateau de Bure Interferometer, allows us to precisely estimate the intrinsic source extension and hence estimate the total lensing magnification to be {mu} = 10.9 {+-} 0.7. We measure the half-light radius R{sub eff} of the source in the rest-frame near-UV and V bands that characterize the unobscured light coming from stars and find R{sub eff,*} = [2.0 {+-} 0.1] kpc, in good agreement with recent studies on the SMG population. This lens model is also used to estimate the size of the gas distribution (R{sub eff,gas} = [1.1 {+-} 0.5] kpc) by mapping back in the source plane the CO (J = 5 {yields} 4) transition line emission. The lens modeling yields a relatively large Einstein radius R{sub Ein} = 4.''10 {+-} 0.''02, corresponding to a deflector velocity dispersion of [483 {+-} 16] km s{sup -1}. This shows that HERMES is lensed by a galaxy group-size dark matter halo at redshift z{sub l} {approx} 0.6. The projected dark matter contribution largely dominates the mass budget within the Einstein radius with f{sub dm}(< R{sub Ein}) {approx} 80%. This fraction reduces to f{sub dm}(< R{sub eff,G1} {approx_equal} 4.5 kpc) {approx} 47% within the effective radius of the main deflecting galaxy of stellar mass M{sub *,G1} = [8.5 {+-} 1.6] x 10{sup 11} M{sub sun}. At this smaller scale the dark matter fraction is consistent with results already found for massive lensing ellipticals at z {approx} 0.2 from the Sloan Lens ACS Survey.

  9. Karl G. Jansky very large array observations of cold dust and molecular gas in starbursting quasar host galaxies at z ? 4.5

    SciTech Connect (OSTI)

    Wagg, J.; Carilli, C. L.; Lentati, L.; Maiolino, R.; Hills, R.; Aravena, M.; Cox, P.; McMahon, R. G.; Riechers, D.; Walter, F.; Andreani, P.; Wolfe, A.

    2014-03-10

    We present Karl G. Jansky Very Large Array (VLA) observations of 44 GHz continuum and CO J = 2-1 line emission in BRI 1202–0725 at z = 4.7 (a starburst galaxy and quasar pair) and BRI 1335–0417 at z = 4.4 (also hosting a quasar). With the full 8 GHz bandwidth capabilities of the upgraded VLA, we study the (rest-frame) 250 GHz thermal dust continuum emission for the first time along with the cold molecular gas traced by the low-J CO line emission. The measured CO J = 2-1 line luminosities of BRI 1202–0725 are L{sub CO}{sup ?}=(8.7±0.8)Χ10{sup 10} K km s{sup –1} pc{sup 2} and L{sub CO}{sup ?}=(6.0 ± 0.5)Χ10{sup 10} K km s{sup –1} pc{sup 2} for the submillimeter galaxy (SMG) and quasar, respectively, which are equal to previous measurements of the CO J = 5-4 line luminosities implying thermalized line emission, and we estimate a combined cold molecular gas mass of ?9Χ10{sup 10} M {sub ?}. In BRI 1335–0417 we measure L{sub CO}{sup ?}=(7.3±0.6)Χ10{sup 10} K km s{sup –1} pc{sup 2}. We detect continuum emission in the SMG BRI 1202–0725 North (S {sub 44} {sub GHz} = 51 ± 6 ?Jy), while the quasar is detected with S {sub 44} {sub GHz} = 24 ± 6 ?Jy and in BRI 1335–0417 we measure S {sub 44} {sub GHz} = 40 ± 7 ?Jy. Combining our continuum observations with previous data at (rest-frame) far-infrared and centimeter wavelengths, we fit three-component models in order to estimate the star formation rates. This spectral energy distribution fitting suggests that the dominant contribution to the observed 44 GHz continuum is thermal dust emission, while either thermal free-free or synchrotron emission contributes less than 30%.

  10. GREEN BANK TELESCOPE ZPECTROMETER CO(1-0) OBSERVATIONS OF THE STRONGLY LENSED SUBMILLIMETER GALAXIES FROM THE HERSCHEL ATLAS

    SciTech Connect (OSTI)

    Frayer, D. T.; Maddalena, R.; Harris, A. I.; Baker, A. J.; Ivison, R. J.; Smail, Ian; Negrello, M.; Aretxaga, I.; Baes, M.; Birkinshaw, M.; Bonfield, D. G.; Burgarella, D.; Buttiglione, S.; Cava, A.; Cooray, A.; Dannerbauer, H.

    2011-01-10

    The Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) has uncovered a population of strongly lensed submillimeter galaxies (SMGs). The Zpectrometer instrument on the Green Bank Telescope (GBT) was used to measure the redshifts and constrain the masses of the cold molecular gas reservoirs for two candidate high-redshift lensed sources. We derive CO(1-0) redshifts of z = 3.042 {+-} 0.001 and z = 2.625 {+-} 0.001, and measure molecular gas masses of (1-3) x10{sup 10} M{sub sun}, corrected for lens amplification and assuming a conversion factor of {alpha} = 0.8 M{sub sun}( K km s{sup -1} pc{sup 2}){sup -1}. We find typical L(IR)/L'(CO) ratios of 120 {+-} 40 and 140 {+-} 50 L{sub sun}( K km s{sup -1} pc{sup 2}){sup -1}, which are consistent with those found for local ultraluminous infrared galaxies (ULIRGs) and other high-redshift SMGs. From analysis of published data, we find no evidence for enhanced L(IR)/L'(CO(1-0)) ratios for the SMG population in comparison to local ULIRGs. The GBT results highlight the power of using the CO lines to derive blind redshifts, which is challenging for the SMGs at optical wavelengths given their high obscuration.

  11. Submillimeter galaxies as progenitors of compact quiescent galaxies

    SciTech Connect (OSTI)

    Toft, S.; Zirm, A.; Krogager, J.-K.; Man, A. W. S.; Smol?i?, V.; Krpan, J.; Magnelli, B.; Karim, A.; Michalowski, M.; Capak, P.; Sheth, K.; Schawinski, K.; Wuyts, S.; Lutz, D.; Staguhn, J.; Berta, S.; Sanders, D.; Mccracken, H.; Riechers, D.

    2014-02-20

    Three billion years after the big bang (at redshift z = 2), half of the most massive galaxies were already old, quiescent systems with little to no residual star formation and extremely compact with stellar mass densities at least an order of magnitude larger than in low-redshift ellipticals, their descendants. Little is known about how they formed, but their evolved, dense stellar populations suggest formation within intense, compact starbursts 1-2 Gyr earlier (at 3 < z < 6). Simulations show that gas-rich major mergers can give rise to such starbursts, which produce dense remnants. Submillimeter-selected galaxies (SMGs) are prime examples of intense, gas-rich starbursts. With a new, representative spectroscopic sample of compact, quiescent galaxies at z = 2 and a statistically well-understood sample of SMGs, we show that z = 3-6 SMGs are consistent with being the progenitors of z = 2 quiescent galaxies, matching their formation redshifts and their distributions of sizes, stellar masses, and internal velocities. Assuming an evolutionary connection, their space densities also match if the mean duty cycle of SMG starbursts is 42{sub ?29}{sup +40} Myr (consistent with independent estimates), which indicates that the bulk of stars in these massive galaxies were formed in a major, early surge of star formation. These results suggest a coherent picture of the formation history of the most massive galaxies in the universe, from their initial burst of violent star formation through their appearance as high stellar-density galaxy cores and to their ultimate fate as giant ellipticals.

  12. Concordant plutonium-241-americium-241 dating of environmental samples: results from forest fire ash

    SciTech Connect (OSTI)

    Goldstein, Steven J; Oldham, Warren J; Murrell, Michael T; Katzman, Danny

    2010-12-07

    We have measured the Pu, {sup 237}Np, {sup 241}Am, and {sup 151}Sm isotopic systematics for a set of forest fire ash samples from various locations in the western U.S. including Montana, Wyoming, Idaho, and New Mexico. The goal of this study is to develop a concordant {sup 241}Pu (t{sub 1/2} = 14.4 y)-{sup 241}Am dating method for environmental collections. Environmental samples often contain mixtures of components including global fallout. There are a number of approaches for subtracting the global fallout component for such samples. One approach is to use {sup 242}/{sup 239}Pu as a normalizing isotope ratio in a three-isotope plot, where this ratio for the nonglobal fallout component can be estimated or assumed to be small. This study investigates a new, complementary method of normalization using the long-lived fission product, {sup 151}Sm (t{sub 1/2} = 90 y). We find that forest fire ash concentrates actinides and fission products with {approx}1E10 atoms {sup 239}Pu/g and {approx}1E8 atoms {sup 151}Sm/g, allowing us to measure these nuclides by mass spectrometric (MIC-TIMS) and radiometric (liquid scintillation counting) methods. The forest fire ash samples are characterized by a western U.S. regional isotopic signature representing varying mixtures of global fallout with a local component from atmospheric testing of nuclear weapons at the Nevada Test Site (NTS). Our results also show that {sup 151}Sm is well correlated with the Pu nuclides in the forest fire ash, suggesting that these nuclides have similar geochemical behavior in the environment. Results of this correlation indicate that the {sup 151}Sm/{sup 239}Pu atom ratio for global fallout is {approx}0.164, in agreement with an independent estimate of 0.165 based on {sup 137}Cs fission yields for atmospheric weapons tests at the NTS. {sup 241}Pu-{sup 241}Am dating of the non-global fallout component in the forest fire ash samples yield ages in the late 1950's-early 1960's, consistent with a peak in NTS weapons testing at that time. The age results for this component are in agreement using both {sup 242}Pu and {sup 151}Sm normalizations, although the errors for the {sup 151}Sm correction are currently larger due to the greater uncertainty of their measurements. Additional efforts to develop a concordant {sup 241}Pu-{sup 241}Am dating method for environmental collections are underway with emphasis on soil cores.