Noise and ultraviolet divergences in the dynamics of the chiral condensate in QCD
Autor(a) principal: | |
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Data de Publicação: | 2012 |
Tipo de documento: | Artigo de conferência |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1088/1742-6596/378/1/012032 http://hdl.handle.net/11449/24654 |
Resumo: | The time evolution of the matter produced in high energy heavy-ion collisions seems to be well described by relativistic viscous hydrodynamics. In addition to the hydrodynamic degrees of freedom related to energy-momentum conservation, degrees of freedom associated with order parameters of broken continuous symmetries must be considered because they are all coupled to each other. of particular interest is the coupling of degrees of freedom associated with the chiral symmetry of QCD. Quantum and thermal fluctuations of the chiral fields act as noise sources in the classical equations of motion, turning them into stochastic differential equations in the form of Ginzburg-Landau-Langevin (GLL) equations. Analytic solutions of GLL equations are attainable only in very special circumstances and extensive numerical simulations are necessary, usually by discretizing the equations on a spatial lattice. However, a not much appreciated issue in the numerical simulations of GLL equations is that ultraviolet divergences in the form of lattice-spacing dependence plague the solutions. The divergences are related to the well-known Rayleigh-Jeans catastrophe in classical field theory. In the present communication we present a systematic lattice renormalization method to control the catastrophe. We discuss the implementation of the method for a GLL equation derived in the context of a model for the QCD chiral phase transition and consider the nonequilibrium evolution of the chiral condensate during the hydrodynamic flow of the quark-gluon plasma. |
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Noise and ultraviolet divergences in the dynamics of the chiral condensate in QCDThe time evolution of the matter produced in high energy heavy-ion collisions seems to be well described by relativistic viscous hydrodynamics. In addition to the hydrodynamic degrees of freedom related to energy-momentum conservation, degrees of freedom associated with order parameters of broken continuous symmetries must be considered because they are all coupled to each other. of particular interest is the coupling of degrees of freedom associated with the chiral symmetry of QCD. Quantum and thermal fluctuations of the chiral fields act as noise sources in the classical equations of motion, turning them into stochastic differential equations in the form of Ginzburg-Landau-Langevin (GLL) equations. Analytic solutions of GLL equations are attainable only in very special circumstances and extensive numerical simulations are necessary, usually by discretizing the equations on a spatial lattice. However, a not much appreciated issue in the numerical simulations of GLL equations is that ultraviolet divergences in the form of lattice-spacing dependence plague the solutions. The divergences are related to the well-known Rayleigh-Jeans catastrophe in classical field theory. In the present communication we present a systematic lattice renormalization method to control the catastrophe. We discuss the implementation of the method for a GLL equation derived in the context of a model for the QCD chiral phase transition and consider the nonequilibrium evolution of the chiral condensate during the hydrodynamic flow of the quark-gluon plasma.Univ Estadual Paulista, Inst Fis Teor, BR-01140070 São Paulo, BrazilUniv Estadual Paulista, Inst Fis Teor, BR-01140070 São Paulo, BrazilIop Publishing LtdUniversidade Estadual Paulista (Unesp)Krein, Gastão Inácio [UNESP]2013-09-30T19:02:15Z2014-05-20T14:13:44Z2013-09-30T19:02:15Z2014-05-20T14:13:44Z2012-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObject10application/pdfhttp://dx.doi.org/10.1088/1742-6596/378/1/012032Xiii Mexican Workshop on Particles and Fields. Bristol: Iop Publishing Ltd, v. 378, p. 10, 2012.1742-6588http://hdl.handle.net/11449/2465410.1088/1742-6596/378/1/012032WOS:000307540500032WOS000307540500032.pdf5704289678296630Web of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengXiii Mexican Workshop on Particles and Fields0,241info:eu-repo/semantics/openAccess2023-12-10T06:14:57Zoai:repositorio.unesp.br:11449/24654Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T19:53:33.002146Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Noise and ultraviolet divergences in the dynamics of the chiral condensate in QCD |
title |
Noise and ultraviolet divergences in the dynamics of the chiral condensate in QCD |
spellingShingle |
Noise and ultraviolet divergences in the dynamics of the chiral condensate in QCD Krein, Gastão Inácio [UNESP] |
title_short |
Noise and ultraviolet divergences in the dynamics of the chiral condensate in QCD |
title_full |
Noise and ultraviolet divergences in the dynamics of the chiral condensate in QCD |
title_fullStr |
Noise and ultraviolet divergences in the dynamics of the chiral condensate in QCD |
title_full_unstemmed |
Noise and ultraviolet divergences in the dynamics of the chiral condensate in QCD |
title_sort |
Noise and ultraviolet divergences in the dynamics of the chiral condensate in QCD |
author |
Krein, Gastão Inácio [UNESP] |
author_facet |
Krein, Gastão Inácio [UNESP] |
author_role |
author |
dc.contributor.none.fl_str_mv |
Universidade Estadual Paulista (Unesp) |
dc.contributor.author.fl_str_mv |
Krein, Gastão Inácio [UNESP] |
description |
The time evolution of the matter produced in high energy heavy-ion collisions seems to be well described by relativistic viscous hydrodynamics. In addition to the hydrodynamic degrees of freedom related to energy-momentum conservation, degrees of freedom associated with order parameters of broken continuous symmetries must be considered because they are all coupled to each other. of particular interest is the coupling of degrees of freedom associated with the chiral symmetry of QCD. Quantum and thermal fluctuations of the chiral fields act as noise sources in the classical equations of motion, turning them into stochastic differential equations in the form of Ginzburg-Landau-Langevin (GLL) equations. Analytic solutions of GLL equations are attainable only in very special circumstances and extensive numerical simulations are necessary, usually by discretizing the equations on a spatial lattice. However, a not much appreciated issue in the numerical simulations of GLL equations is that ultraviolet divergences in the form of lattice-spacing dependence plague the solutions. The divergences are related to the well-known Rayleigh-Jeans catastrophe in classical field theory. In the present communication we present a systematic lattice renormalization method to control the catastrophe. We discuss the implementation of the method for a GLL equation derived in the context of a model for the QCD chiral phase transition and consider the nonequilibrium evolution of the chiral condensate during the hydrodynamic flow of the quark-gluon plasma. |
publishDate |
2012 |
dc.date.none.fl_str_mv |
2012-01-01 2013-09-30T19:02:15Z 2013-09-30T19:02:15Z 2014-05-20T14:13:44Z 2014-05-20T14:13:44Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/conferenceObject |
format |
conferenceObject |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1088/1742-6596/378/1/012032 Xiii Mexican Workshop on Particles and Fields. Bristol: Iop Publishing Ltd, v. 378, p. 10, 2012. 1742-6588 http://hdl.handle.net/11449/24654 10.1088/1742-6596/378/1/012032 WOS:000307540500032 WOS000307540500032.pdf 5704289678296630 |
url |
http://dx.doi.org/10.1088/1742-6596/378/1/012032 http://hdl.handle.net/11449/24654 |
identifier_str_mv |
Xiii Mexican Workshop on Particles and Fields. Bristol: Iop Publishing Ltd, v. 378, p. 10, 2012. 1742-6588 10.1088/1742-6596/378/1/012032 WOS:000307540500032 WOS000307540500032.pdf 5704289678296630 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Xiii Mexican Workshop on Particles and Fields 0,241 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
10 application/pdf |
dc.publisher.none.fl_str_mv |
Iop Publishing Ltd |
publisher.none.fl_str_mv |
Iop Publishing Ltd |
dc.source.none.fl_str_mv |
Web of Science reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
instname_str |
Universidade Estadual Paulista (UNESP) |
instacron_str |
UNESP |
institution |
UNESP |
reponame_str |
Repositório Institucional da UNESP |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
|
_version_ |
1808129135129657344 |