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Title: Chiral drag force

Abstract

Here, we provide a holographic evaluation of novel contributions to the drag force acting on a heavy quark moving through strongly interacting plasma. The new contributions are chiral in the sense that they act in opposite directions in plasmas containing an excess of left- or right-handed quarks. The new contributions are proportional to the coefficient of the axial anomaly, and in this sense also are chiral. These new contributions to the drag force act either parallel to or antiparallel to an external magnetic field or to the vorticity of the fluid plasma. In all these respects, these contributions to the drag force felt by a heavy quark are analogous to the chiral magnetic effect (CME) on light quarks. However, the new contribution to the drag force is independent of the electric charge of the heavy quark and is the same for heavy quarks and antiquarks, meaning that these novel effects do not in fact contribute to the CME current. We show that although the chiral drag force can be non-vanishing for heavy quarks that are at rest in the local fluid rest frame, it does vanish for heavy quarks that are at rest in a suitably chosen frame. In thismore » frame, the heavy quark at rest sees counterpropagating momentum and charge currents, both proportional to the axial anomaly coefficient, but feels no drag force. This provides strong concrete evidence for the absence of dissipation in chiral transport, something that has been predicted previously via consideration of symmetries. Along the way to our principal results, we provide a general calculation of the corrections to the drag force due to the presence of gradients in the flowing fluid in the presence of a nonzero chemical potential. We close with a consequence of our result that is at least in principle observable in heavy ion collisions, namely an anticorrelation between the direction of the CME current for light quarks in a given event and the direction of the kick given to the momentum of all the heavy quarks and antiquarks in that event.« less

Authors:
 [1];  [2]
  1. Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)
  2. Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States); ITEP, Moscow (Russia)
Publication Date:
Research Org.:
Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)
Sponsoring Org.:
USDOE
OSTI Identifier:
1435622
Grant/Contract Number:  
SC0011090
Resource Type:
Accepted Manuscript
Journal Name:
Journal of High Energy Physics (Online)
Additional Journal Information:
Journal Name: Journal of High Energy Physics (Online); Journal Volume: 2015; Journal Issue: 10; Journal ID: ISSN 1029-8479
Publisher:
Springer Berlin
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; Quark-Gluon Plasma; Holography and quark-gluon plasmas; Anomalies in Field and String Theories

Citation Formats

Rajagopal, Krishna, and Sadofyev, Andrey V. Chiral drag force. United States: N. p., 2015. Web. doi:10.1007/JHEP10(2015)018.
Rajagopal, Krishna, & Sadofyev, Andrey V. Chiral drag force. United States. doi:10.1007/JHEP10(2015)018.
Rajagopal, Krishna, and Sadofyev, Andrey V. Mon . "Chiral drag force". United States. doi:10.1007/JHEP10(2015)018. https://www.osti.gov/servlets/purl/1435622.
@article{osti_1435622,
title = {Chiral drag force},
author = {Rajagopal, Krishna and Sadofyev, Andrey V.},
abstractNote = {Here, we provide a holographic evaluation of novel contributions to the drag force acting on a heavy quark moving through strongly interacting plasma. The new contributions are chiral in the sense that they act in opposite directions in plasmas containing an excess of left- or right-handed quarks. The new contributions are proportional to the coefficient of the axial anomaly, and in this sense also are chiral. These new contributions to the drag force act either parallel to or antiparallel to an external magnetic field or to the vorticity of the fluid plasma. In all these respects, these contributions to the drag force felt by a heavy quark are analogous to the chiral magnetic effect (CME) on light quarks. However, the new contribution to the drag force is independent of the electric charge of the heavy quark and is the same for heavy quarks and antiquarks, meaning that these novel effects do not in fact contribute to the CME current. We show that although the chiral drag force can be non-vanishing for heavy quarks that are at rest in the local fluid rest frame, it does vanish for heavy quarks that are at rest in a suitably chosen frame. In this frame, the heavy quark at rest sees counterpropagating momentum and charge currents, both proportional to the axial anomaly coefficient, but feels no drag force. This provides strong concrete evidence for the absence of dissipation in chiral transport, something that has been predicted previously via consideration of symmetries. Along the way to our principal results, we provide a general calculation of the corrections to the drag force due to the presence of gradients in the flowing fluid in the presence of a nonzero chemical potential. We close with a consequence of our result that is at least in principle observable in heavy ion collisions, namely an anticorrelation between the direction of the CME current for light quarks in a given event and the direction of the kick given to the momentum of all the heavy quarks and antiquarks in that event.},
doi = {10.1007/JHEP10(2015)018},
journal = {Journal of High Energy Physics (Online)},
number = 10,
volume = 2015,
place = {United States},
year = {2015},
month = {10}
}

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Works referenced in this record:

Drag force in SYM plasma with B field from AdS/CFT
journal, October 2006


Observation of charge-dependent azimuthal correlations and possible local strong parity violation in heavy-ion collisions
journal, May 2010


Fluid dynamics of R-charged black holes
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Testing the Chiral Magnetic and Chiral Vortical Effects in Heavy Ion Collisions
journal, February 2011


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font-size:0.75rem;"><br/> <span class="type">journal</span>, <span class="date" data-date="2013-09-01">September 2013</span></small> </h2> <ul id="references-list" class="small references-list" style="list-style-type:none; margin-top: 0.5em; padding-left: 0; line-height:1.8em;"> <li> <span style="color:#7cb342;"> Kalaydzhyan, Tigran</span> </li> <li> Nuclear Physics A, Vol. 913</li> <li> <span class="text-muted related-url">DOI: <a href="https://doi.org/10.1016/j.nuclphysa.2013.06.009" class="text-muted" target="_blank" rel="noopener noreferrer">10.1016/j.nuclphysa.2013.06.009<span class="fa fa-external-link" aria-hidden="true"></span></a></span> </li> </ul> <hr/> </div><div> <h2 class="title" style="margin-bottom:0;" data-apporder=""> <a href="https://doi.org/10.1088/1126-6708/2009/11/117" target="_blank" rel="noopener noreferrer" class="name">D3-D7 quark-gluon plasmas<span class="fa fa-external-link" aria-hidden="true"></span></a> <small class="text-muted" style="text-transform:uppercase; font-size:0.75rem;"><br/> <span class="type">journal</span>, <span class="date" data-date="2009-11-01">November 2009</span></small> </h2> <ul id="references-list" class="small references-list" style="list-style-type:none; margin-top: 0.5em; padding-left: 0; line-height:1.8em;"> <li> <span style="color:#7cb342;"> Bigazzi, Francesco; Cotrone, Aldo L.; Mas, Javier</span> </li> <li> Journal of High Energy Physics, Vol. 2009, Issue 11</li> <li> <span class="text-muted related-url">DOI: <a href="https://doi.org/10.1088/1126-6708/2009/11/117" class="text-muted" target="_blank" rel="noopener noreferrer">10.1088/1126-6708/2009/11/117<span class="fa fa-external-link" aria-hidden="true"></span></a></span> </li> </ul> <hr/> </div><div> <h2 class="title" style="margin-bottom:0;" data-apporder=""> <a href="https://doi.org/10.1007/JHEP10(2011)084" target="_blank" rel="noopener noreferrer" class="name">A chiral magnetic effect from AdS/CFT with flavor<span class="fa fa-external-link" aria-hidden="true"></span></a> <small class="text-muted" style="text-transform:uppercase; 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line-height:1.8em;"> <li> <span style="color:#7cb342;"> Nata Atmaja, A.; Schalm, K.</span> </li> <li> Journal of High Energy Physics, Vol. 2011, Issue 4</li> <li> <span class="text-muted related-url">DOI: <a href="https://doi.org/10.1007/JHEP04(2011)070" class="text-muted" target="_blank" rel="noopener noreferrer">10.1007/JHEP04(2011)070<span class="fa fa-external-link" aria-hidden="true"></span></a></span> </li> </ul> <hr/> </div><div> <h2 class="title" style="margin-bottom:0;" data-apporder=""> <a href="https://doi.org/10.1016/j.nuclphysa.2014.08.108" target="_blank" rel="noopener noreferrer" class="name"><math altimg="si4.gif" overflow="scroll"> <mi>Λ</mi> <mo stretchy="false">(</mo> <msubsup> <mrow> <mi>K</mi> </mrow> <mrow> <mi>S</mi> </mrow> <mrow> <mn>0</mn> </mrow> </msubsup> <mo stretchy="false">)</mo> <mtext>–</mtext> <msup> <mrow> <mi>h</mi> </mrow> <mrow> <mo>±</mo> </mrow> </msup> </math> and <math altimg="si5.gif" overflow="scroll"> <mi>Λ</mi> <mtext>–</mtext> <mi>p</mi> </math> azimuthal correlations with respect to event plane and search for chiral magnetic and vortical effects<span class="fa fa-external-link" aria-hidden="true"></span></a> <small class="text-muted" style="text-transform:uppercase; font-size:0.75rem;"><br/> <span class="type">journal</span>, <span class="date" data-date="2014-11-01">November 2014</span></small> </h2> <ul id="references-list" class="small references-list" style="list-style-type:none; margin-top: 0.5em; padding-left: 0; line-height:1.8em;"> <li> <span style="color:#7cb342;"> Zhao, Feng</span> </li> <li> Nuclear Physics A, Vol. 931</li> <li> <span class="text-muted related-url">DOI: <a href="https://doi.org/10.1016/j.nuclphysa.2014.08.108" class="text-muted" target="_blank" rel="noopener noreferrer">10.1016/j.nuclphysa.2014.08.108<span class="fa fa-external-link" aria-hidden="true"></span></a></span> </li> </ul> <hr/> </div><div> <h2 class="title" style="margin-bottom:0;" data-apporder=""> <a href="https://doi.org/10.1088/1126-6708/2006/12/068" target="_blank" rel="noopener noreferrer" class="name">On drag forces and jet quenching in strongly-coupled plasmas<span class="fa fa-external-link" aria-hidden="true"></span></a> <small class="text-muted" style="text-transform:uppercase; font-size:0.75rem;"><br/> <span class="type">journal</span>, <span class="date" data-date="2006-12-01">December 2006</span></small> </h2> <ul id="references-list" class="small references-list" style="list-style-type:none; margin-top: 0.5em; padding-left: 0; line-height:1.8em;"> <li> <span style="color:#7cb342;"> Cáceres, Elena; Güijosa, Alberto</span> </li> <li> Journal of High Energy Physics, Vol. 2006, Issue 12</li> <li> <span class="text-muted related-url">DOI: <a href="https://doi.org/10.1088/1126-6708/2006/12/068" class="text-muted" target="_blank" rel="noopener noreferrer">10.1088/1126-6708/2006/12/068<span class="fa fa-external-link" aria-hidden="true"></span></a></span> </li> </ul> <hr/> </div><div> <h2 class="title" style="margin-bottom:0;" data-apporder=""> <a href="https://doi.org/10.1007/JHEP05(2013)115" target="_blank" rel="noopener noreferrer" class="name">Holographic gravitational anomaly in first and second order hydrodynamics<span class="fa fa-external-link" aria-hidden="true"></span></a> <small class="text-muted" style="text-transform:uppercase; font-size:0.75rem;"><br/> <span class="type">journal</span>, <span class="date" data-date="2013-05-01">May 2013</span></small> </h2> <ul id="references-list" class="small references-list" style="list-style-type:none; margin-top: 0.5em; padding-left: 0; line-height:1.8em;"> <li> <span style="color:#7cb342;"> Megías, Eugenio; Pena-Benitez, Francisco</span> </li> <li> Journal of High Energy Physics, Vol. 2013, Issue 5</li> <li> <span class="text-muted related-url">DOI: <a href="https://doi.org/10.1007/JHEP05(2013)115" class="text-muted" target="_blank" rel="noopener noreferrer">10.1007/JHEP05(2013)115<span class="fa fa-external-link" aria-hidden="true"></span></a></span> </li> </ul> <hr/> </div><div> <h2 class="title" style="margin-bottom:0;" data-apporder=""> <a href="https://doi.org/10.1007/JHEP05(2011)081" target="_blank" rel="noopener noreferrer" class="name">Anomalous transport coefficients from Kubo formulas in Holography<span class="fa fa-external-link" aria-hidden="true"></span></a> <small class="text-muted" style="text-transform:uppercase; font-size:0.75rem;"><br/> <span class="type">journal</span>, <span class="date" data-date="2011-05-01">May 2011</span></small> </h2> <ul id="references-list" class="small references-list" style="list-style-type:none; margin-top: 0.5em; padding-left: 0; line-height:1.8em;"> <li> <span style="color:#7cb342;"> Amado, Irene; Landsteiner, Karl; Pena-Benitez, Francisco</span> </li> <li> Journal of High Energy Physics, Vol. 2011, Issue 5</li> <li> <span class="text-muted related-url">DOI: <a href="https://doi.org/10.1007/JHEP05(2011)081" class="text-muted" target="_blank" rel="noopener noreferrer">10.1007/JHEP05(2011)081<span class="fa fa-external-link" aria-hidden="true"></span></a></span> </li> </ul> <hr/> </div><div> <h2 class="title" style="margin-bottom:0;" data-apporder=""> <a href="https://doi.org/10.1088/1126-6708/1999/04/024" target="_blank" rel="noopener noreferrer" class="name">Phases of R-charged black holes, spinning branes and strongly coupled gauge theories<span class="fa fa-external-link" aria-hidden="true"></span></a> <small class="text-muted" style="text-transform:uppercase; font-size:0.75rem;"><br/> <span class="type">journal</span>, <span class="date" data-date="1999-04-01">April 1999</span></small> </h2> <ul id="references-list" class="small references-list" style="list-style-type:none; margin-top: 0.5em; padding-left: 0; line-height:1.8em;"> <li> <span style="color:#7cb342;"> Cvetic, Mirjam; Gubser, Steven S.</span> </li> <li> Journal of High Energy Physics, Vol. 1999, Issue 04</li> <li> <span class="text-muted related-url">DOI: <a href="https://doi.org/10.1088/1126-6708/1999/04/024" class="text-muted" target="_blank" rel="noopener noreferrer">10.1088/1126-6708/1999/04/024<span class="fa fa-external-link" aria-hidden="true"></span></a></span> </li> </ul> <hr/> </div></div> <ul class="pagination"></ul> </div> </div> <div class="col-sm-3 order-sm-3"> <ul class="nav nav-stacked"> <li class="active"><a href="" class="reference-type-filter tab-nav" data-tab="biblio-references" data-filter="type" data-pattern="*"><span class="fa fa-angle-right"></span> All References</a></li> <li class="small" style="margin-left:.75em; 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float:none;">[ × clear filter / sort ]</a> </div> </form> </div> </div> </div> </section> <section id="biblio-related" class="tab-content tab-content-sec " data-tab="biblio"> <div class="row"> <div class="col-sm-9 order-sm-9"> <section id="biblio-similar" class="tab-content tab-content-sec active" data-tab="related"> <div class="padding"> <p class="lead text-muted" style="font-size: 18px; margin-top:0px;">Similar records in OSTI.GOV collections:</p> <aside> <ul class="item-list" itemscope itemtype="http://schema.org/ItemList" style="padding-left:0; list-style-type: none;"> <li> <div class="article item document" itemprop="itemListElement" itemscope itemtype="http://schema.org/WebPage"><meta itemprop="position" content="0" /><div class="item-info"> <h2 class="title" itemprop="name headline"><a href="/pages/biblio/897585-measurement-charge-asymmetry-boson-helicity-top-antitop-quark-events-cdf-ii-experiment" itemprop="url">Measurement of the charge asymmetry and the W boson helicity in top-antitop quark events with the CDF II experiment</a></h2> <div class="metadata"> <small class="text-muted" style="text-transform:uppercase;display:block;line-height:2.5em;">Thesis/Dissertation</small><span class="authors"> <span class="author">Hirschbuehl, Dominic</span> <span class="text-muted pubdata"></span> </span> </div> <div class="abstract">In 1995 the heaviest elementary particle, top quark, was discovered at the Tevatron collider in top-antitop quark pair production. Since the top quark mass is of the same order as the electroweak symmetry breaking scale, measurements of the properties of the top quark like mass, charge, spin or the production mechanism, offer a good opportunity to test the Standard Model at such high energies. Top quarks at the Tevatron are predominantly pair-produced through light quark-antiquark annihilation. Higher order perturbative QCD calculations predict a sizeable asymmetry between the number of top quarks and antitop quarks produced in forward direction. This asymmetry<a href='#' onclick='$(this).hide().next().show().next().show();return false;' style='margin-left:10px;'>more »</a><span style='display:none;'> is induced through radiative corrections. A measurement of the asymmetry can check the perturbative QCD predictions. Due to the high mass of the top quark, nearly the mass of a gold nucleus, the life time of the top quark is much shorter than the hadronization time-scale. This means that the top quark decays before it has a chance to form a bound state. The Standard Model predicts that the top quark decays in nearly 100% of the cases into a W boson and a b quark via a charge-current weak interaction. The measurement of the W boson helicity probes the V-A structure of the weak interaction and differences to the expectation would give evidence for new physics. Until the start of the Large Hadron Collider at CERN, the Tevatron is the only experiment where top quarks can be directly produced and their properties be measured. The Tevatron reaches a center-of-mass energy of 1.96 TeV in proton antiproton collisions. The data used in this analysis were taken in Run II of the Tevatron with the Collider Detector at Fermilab (CDF) in the years 2001-2004 and represent an integrated luminosity of 319 pb{sup -1}. The thesis is organized in the following way: In the first chapter a short overview of the Standard Model is given. The theoretical aspects of the top quark decay are described with particular emphasis on the different helicities of the W boson. The second focus lies on the production process and the higher order QCD effect causing the charge asymmetry. In the following three chapters the experimental techniques of the CDF detector, hardware and the used software are introduced as well as. In this thesis t{bar t} candidates are selected in the decay mode t {yields} bl{nu}, {bar t} {yields} bjj and the charge conjugated state. An important ingredient for this measurement is the complete reconstruction of the top-antitop partonic process. The reconstruction of the partonic process requires the assignment of reconstructed objects, such as jets, the charged lepton and the missing transverse energy to parton level objects. This assignment implies a certain number of possible permutations and ambiguities. To achieve the optimal reconstruction of the event all combinations have to be considered and evaluated. To measure a t{bar t}-quantity one hypothesis has to be chosen. In chapter five we present a novel technique to fully reconstruct t{bar t} events. The technique is investigated in great detail by comparing to the Monte Carlo truth information. In the sixth chapter the background estimation is given. The identification and selection procedure on data is checked with Monte Carlo samples. Chapter seven describes the measurement of the W boson helicity in the top quark decay. The helicity of the W boson is measured via the angle between the W boson momentum in the top quark rest frame and the lepton momentum in the W boson rest frame. After correcting for acceptance and reconstruction effects the different helicity fractions are extracted by fitting the theoretical expected distribution. The systematic error is determined using the technique of pseudo experiments. In chapter eight the measurement of the charge asymmetry in top-pair production is presented. The measurement of the asymmetry is performed by using the difference of the top quark rapidities times the charge of the lepton, to distinguish between top and anti-top quarks. The results and an outlook are given in the last chapter.</span><a href='#' onclick='$(this).hide().prev().hide().prev().show();return false;' style='margin-left:10px;display:none;'>« less</a></div><div class="metadata-links small clearfix text-muted" style="margin-top:15px;"> <div class="pure-menu pure-menu-horizontal pull-right" style="width:unset;"> <ul class="pure-menu-list"> <li class="pure-menu-item"><span class="item-info-ftlink">DOI: <a class="misc doi-link " href="https://doi.org/10.2172/897585" target="_blank" rel="noopener" title="Link to document DOI" data-ostiid="897585" data-product-type="Thesis/Dissertation" data-product-subtype="" >10.2172/897585</a></span></li> <li class="pure-menu-item"><span class="item-info-ftlink"><a class="misc fulltext-link " href="/pages/servlets/purl/897585" title="Link to document media" target="_blank" rel="noopener" data-ostiid="897585" data-product-type="Thesis/Dissertation" data-product-subtype="" >Full Text Available</a></span></li> </ul> </div> </div> </div> <div class="clearfix"></div> </div> </li> <li> <div class="article item document" itemprop="itemListElement" itemscope itemtype="http://schema.org/WebPage"><meta itemprop="position" content="1" /><div class="item-info"> <h2 class="title" itemprop="name headline"><a href="/pages/biblio/21532295-testing-chiral-magnetic-chiral-vortical-effects-heavy-ion-collisions" itemprop="url">Testing the Chiral Magnetic and Chiral Vortical Effects in Heavy Ion Collisions</a></h2> <div class="metadata"> <small class="text-muted" style="text-transform:uppercase;display:block;line-height:2.5em;">Journal Article</small><span class="authors"> <span class="author">Kharzeev, Dmitri E.</span> ; <span class="author">Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000</span> ; <span class="author">Son, Dam T.</span> <span class="text-muted pubdata"> - Physical Review Letters</span> </span> </div> <div class="abstract">We devise a test of the chiral magnetic and chiral vortical effects (CME and CVE) in relativistic heavy ion collisions that relies only on the general properties of triangle anomalies. We show that the ratio R{sub EB}=J{sub E}/J{sub B} of charge J{sub E} and baryon J{sub B} currents for CME is R{sub EB}{sup CME}{yields}{infinity} for three light flavors of quarks (N{sub f}=3), and R{sub EB}{sup CME}=5 for N{sub f}=2, whereas for CVE it is R{sub EB}{sup CVE}=0 for N{sub f}=3 and R{sub EB}{sup CME}=1/2 for N{sub f}=2. The physical world with light u,d quarks and a heavier s quark is<a href='#' onclick='$(this).hide().next().show().next().show();return false;' style='margin-left:10px;'>more »</a><span style='display:none;'> in between the N{sub f}=2 and N{sub f}=3 cases; therefore, the ratios R{sub EB} for CME and CVE should differ by over an order of magnitude providing a possibility to separate clearly the CME and CVE contributions. In both cases, there has to be a positive correlation between the charge and baryon number asymmetries that can be tested on the event-by-event basis.</span><a href='#' onclick='$(this).hide().prev().hide().prev().show();return false;' style='margin-left:10px;display:none;'>« less</a></div><div class="metadata-links small clearfix text-muted" style="margin-top:15px;"> <div class="pure-menu pure-menu-horizontal pull-right" style="width:unset;"> <ul class="pure-menu-list"> <li class="pure-menu-item"><span class="item-info-ftlink">DOI: <a class="misc doi-link " href="https://doi.org/10.1103/PHYSREVLETT.106.062301" target="_blank" rel="noopener" title="Link to document DOI" data-ostiid="21532295" data-product-type="Journal Article" data-product-subtype="" >10.1103/PHYSREVLETT.106.062301</a></span></li> </ul> </div> </div> </div> <div class="clearfix"></div> </div> </li> <li> <div class="article item document" itemprop="itemListElement" itemscope itemtype="http://schema.org/WebPage"><meta itemprop="position" content="2" /><div class="item-info"> <h2 class="title" itemprop="name headline"><a href="/pages/biblio/1236438-charmonium-dissociation-anomalous-wind" itemprop="url">The charmonium dissociation in an ''anomalous wind''</a></h2> <div class="metadata"> <small class="text-muted" style="text-transform:uppercase;display:block;line-height:2.5em;">Journal Article</small><span class="authors"> <span class="author">Sadofyev, Andrey V.</span> ; <span class="author">Yin, Yi</span> <span class="text-muted pubdata"> - Journal of High Energy Physics (Online)</span> </span> </div> <div class="abstract">We study the charmonium dissociation in a strongly coupled chiral plasma in the presence of magnetic field and axial charge imbalance. This type of plasma carries "anomalous flow" induced by the chiral anomaly and exhibits novel transport phenomena such as chiral magnetic effect. We found that the "anomalous flow" would modify the charmonium color screening length by using the gauge/gravity correspondence. We derive an analytical expression quantifying the "anomalous flow" experienced by a charmonium for a large class of chiral plasma with a gravity dual. We elaborate on the similarity and it qualitative difference between anomalous effects on the charmonium<a href='#' onclick='$(this).hide().next().show().next().show();return false;' style='margin-left:10px;'>more »</a><span style='display:none;'> color screening length which are model-dependent and those on the heavy quark drag force which are fixed by the second law of thermodynamics. As a result, we speculate on the possible charmonium dissociation induced by the chiral anomaly in heavy ion collisions.</span><a href='#' onclick='$(this).hide().prev().hide().prev().show();return false;' style='margin-left:10px;display:none;'>« less</a></div><div class="metadata-links small clearfix text-muted" style="margin-top:15px;"> <span class="fa fa-book text-muted" aria-hidden="true"></span> Cited by 8<div class="pure-menu pure-menu-horizontal pull-right" style="width:unset;"> <ul class="pure-menu-list"> <li class="pure-menu-item"><span class="item-info-ftlink">DOI: <a class="misc doi-link " href="https://doi.org/10.1007/JHEP01(2016)052" target="_blank" rel="noopener" title="Link to document DOI" data-ostiid="1236438" data-product-type="Journal Article" data-product-subtype="AM" >10.1007/JHEP01(2016)052</a></span></li> <li class="pure-menu-item"><span class="item-info-ftlink"><a class="misc fulltext-link " href="/pages/servlets/purl/1236438" title="Link to document media" target="_blank" rel="noopener" data-ostiid="1236438" data-product-type="Journal Article" data-product-subtype="AM" >Full Text Available</a></span></li> </ul> </div> </div> </div> <div class="clearfix"></div> </div> </li> <li> <div class="article item document" itemprop="itemListElement" itemscope itemtype="http://schema.org/WebPage"><meta itemprop="position" content="3" /><div class="item-info"> <h2 class="title" itemprop="name headline"><a href="/pages/biblio/1253275-charmonium-dissociation-anomalous-wind" itemprop="url">The charmonium dissociation in an "anomalous wind"</a></h2> <div class="metadata"> <small class="text-muted" style="text-transform:uppercase;display:block;line-height:2.5em;">Journal Article</small><span class="authors"> <span class="author">Andrey V. Sadofyev</span> ; <span class="author">Yin, Yi</span> <span class="text-muted pubdata"> - Journal of High Energy Physics (Online)</span> </span> </div> <div class="abstract">We study the charmonium dissociation in a strongly coupled chiral plasma in the presence of magnetic field and axial charge imbalance. This type of plasma carries “anomalous flow” induced by the chiral anomaly and exhibits novel transport phenomena such as chiral magnetic effect. We found that the “anomalous flow” would modify the charmonium color screening length by using the gauge/gravity correspondence. We derive an analytical expression quantifying the “anomalous flow” experienced by a charmonium for a large class of chiral plasma with a gravity dual. We elaborate on the similarity and qualitative difference between anomalous effects on the charmonium color<a href='#' onclick='$(this).hide().next().show().next().show();return false;' style='margin-left:10px;'>more »</a><span style='display:none;'> screening length which are model-dependent and those on the heavy quark drag force which are fixed by the second law of thermodynamics. Here, we speculate on the possible charmonium dissociation induced by the chiral anomaly in heavy ion collisions.</span><a href='#' onclick='$(this).hide().prev().hide().prev().show();return false;' style='margin-left:10px;display:none;'>« less</a></div><div class="metadata-links small clearfix text-muted" style="margin-top:15px;"> <span class="fa fa-book text-muted" aria-hidden="true"></span> Cited by 8<div class="pure-menu pure-menu-horizontal pull-right" style="width:unset;"> <ul class="pure-menu-list"> <li class="pure-menu-item"><span class="item-info-ftlink">DOI: <a class="misc doi-link " href="https://doi.org/10.1007/JHEP01(2016)052" target="_blank" rel="noopener" title="Link to document DOI" data-ostiid="1253275" data-product-type="Journal Article" data-product-subtype="AM" >10.1007/JHEP01(2016)052</a></span></li> <li class="pure-menu-item"><span class="item-info-ftlink"><a class="misc fulltext-link " href="/pages/servlets/purl/1253275" title="Link to document media" target="_blank" rel="noopener" data-ostiid="1253275" data-product-type="Journal Article" data-product-subtype="AM" >Full Text Available</a></span></li> </ul> </div> </div> </div> <div class="clearfix"></div> </div> </li> <li> <div class="article item document" itemprop="itemListElement" itemscope itemtype="http://schema.org/WebPage"><meta itemprop="position" content="4" /><div class="item-info"> <h2 class="title" itemprop="name headline"><a href="/pages/biblio/279857-heavy-quark-hadronic-lagrangian-ital-wave-quarkonium" itemprop="url">Heavy quark hadronic Lagrangian for {ital s}-wave quarkonium</a></h2> <div class="metadata"> <small class="text-muted" style="text-transform:uppercase;display:block;line-height:2.5em;">Journal Article</small><span class="authors"> <span class="author">Pineda, A.</span> ; <span class="author">Soto, J.</span> <span class="text-muted pubdata"> - Physical Review, D</span> </span> </div> <div class="abstract">We use heavy quark effective theory (HQET) techniques to parametrize certain nonperturbative effects related to quantum fluctuations that put both heavy quarks and antiquarks in quarkonium almost on shell. The large off-shell momentum contributions are calculated using Coulomb-type states. The almost on-shell momentum contributions are evaluated using an effective {open_quote}{open_quote}chiral{close_quote}{close_quote} Lagrangian which incorporates the relevant symmetries of the HQET for quarks and antiquarks. The cutoff dependence of both contributions matches perfectly. The decay constants and the matrix elements of bilinear currents at zero recoil are calculated. Their leading nonperturbative contributions are parametrized by a single constant and turn out to<a href='#' onclick='$(this).hide().next().show().next().show();return false;' style='margin-left:10px;'>more »</a><span style='display:none;'> be {ital O}({alpha}{sup 2}/{Lambda}{sub QCD}{ital a}{sub {ital n}}), {ital a}{sub {ital n}} being the Bohr radius and {alpha} the strong coupling constant, times the nonperturbative contribution coming from the multipole expansion (gluon condensate). We discuss the physical applications to {Upsilon}, {ital J}/{psi}, and {ital B}{sub {ital c}} systems. {copyright} {ital 1996 The American Physical Society.}</span><a href='#' onclick='$(this).hide().prev().hide().prev().show();return false;' style='margin-left:10px;display:none;'>« less</a></div><div class="metadata-links small clearfix text-muted" style="margin-top:15px;"> <div class="pure-menu pure-menu-horizontal pull-right" style="width:unset;"> <ul class="pure-menu-list"> <li class="pure-menu-item"><span class="item-info-ftlink">DOI: <a class="misc doi-link " href="https://doi.org/10.1103/PhysRevD.53.3983" target="_blank" rel="noopener" title="Link to document DOI" data-ostiid="279857" data-product-type="Journal Article" data-product-subtype="AC" >10.1103/PhysRevD.53.3983</a></span></li> </ul> </div> </div> </div> <div class="clearfix"></div> </div> </li> </ul> </aside> </div> </section> </div> <div class="col-sm-3 order-sm-3"> <ul class="nav nav-stacked"> <li class="active"><a class="tab-nav disabled" data-tab="related" style="color: #636c72 !important; opacity: 1;"><span class="fa fa-angle-right"></span> Similar Records</a></li> </ul> </div> </div> </section> </div></div> </div> </div> </section> <footer class="" style="background-color:#f9f9f9; /* padding-top: 0.5rem; */"> <div class="footer-minor"> <div class="container"> <hr class="footer-separator" /> <div class="text-center" style="margin-top:1.25rem;"> <div class="pure-menu pure-menu-horizontal"> <ul class="pure-menu-list" id="footer-org-menu"> <li class="pure-menu-item"> <a href="https://energy.gov" target="_blank" rel="noopener noreferrer"> <img src="data:image/gif;base64,R0lGODlhAQABAIAAAP///wAAACH5BAEAAAAALAAAAAABAAEAAAICRAEAOw==" class="sprite sprite-footer-us-doe-min" alt="U.S. Department of Energy" /> </a> </li> <li class="pure-menu-item"> <a href="https://www.energy.gov/science/office-science" target="_blank" rel="noopener noreferrer"> <img src="data:image/gif;base64,R0lGODlhAQABAIAAAP///wAAACH5BAEAAAAALAAAAAABAAEAAAICRAEAOw==" class="sprite sprite-footer-office-of-science-min" alt="Office of Science" /> </a> </li> <li class="pure-menu-item"> <a href="/"> <img src="data:image/gif;base64,R0lGODlhAQABAIAAAP///wAAACH5BAEAAAAALAAAAAABAAEAAAICRAEAOw==" class="sprite sprite-footer-osti-min" alt="Office of Scientific and Technical Information" /> </a> </li> </ul> </div> </div> <div class="text-center small" style="margin-top:0.5em;margin-bottom:2.0rem;"> <div class="pure-menu pure-menu-horizontal"> <ul class="pure-menu-list"> <li class="pure-menu-item"><a href="/disclaim" class="pure-menu-link"><span class="fa fa-institution"></span> Website Policies <span class="hidden-xs">/ Important Links</span></a></li> <li class="pure-menu-item"><a href="/pages/contact" class="pure-menu-link"><span class="fa fa-comments-o"></span> Contact Us</a></li> <li class="d-block d-md-none"></li> <li class="pure-menu-item"><a href="https://www.facebook.com/ostigov" target="_blank" rel="noopener noreferrer" class="pure-menu-link social"><span class="fa fa-facebook" style=""></span></a></li> <li class="pure-menu-item"><a href="https://twitter.com/OSTIgov" target="_blank" rel="noopener noreferrer" class="pure-menu-link social"><span class="fa fa-twitter" style=""></span></a></li> <li class="pure-menu-item"><a href="https://www.youtube.com/user/ostigov" target="_blank" rel="noopener noreferrer" class="pure-menu-link social"><span class="fa fa-youtube-play" style=""></span></a></li> </ul> </div> </div> </div> </div> </footer> <link href="/pages/css/pages.fonts.191210.1608.css" rel="stylesheet"> <script src="/pages/js/pages.191210.1608.js"></script><noscript></noscript> <script defer src="/pages/js/pages.biblio.191210.1608.js"></script><noscript></noscript> <script defer src="/pages/js/lity.js"></script><noscript></noscript><script async type="text/javascript" src="/pages/js/Universal-Federated-Analytics-Min.js?agency=DOE" id="_fed_an_ua_tag"></script><noscript></noscript></body> <!-- DOE PAGES v.191210.1608 --> </html>