DBI scalar field theory for QGP hydrodynamics
Autor(a) principal: | |
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Data de Publicação: | 2016 |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1103/PhysRevD.94.025014 http://hdl.handle.net/11449/173218 |
Resumo: | A way to describe the hydrodynamics of the quark-gluon plasma using a Dirac-Born-Infeld (DBI) action is proposed, based on the model found by Heisenberg for high energy scattering of nucleons. The expanding plasma is described as a shockwave in a DBI model for a real scalar standing in for the pion, and I show that one obtains a fluid description in terms of a relativistic fluid that near the shock is approximately ideal (η≃0) and conformal. One can introduce an extra term inside the square root of the DBI action that generates a shear viscosity term in the energy-momentum tensor near the shock, as well as a bulk viscosity, and regulates the behavior of the energy density at the shock, making it finite. The resulting fluid satisfies the relativistic Navier-Stokes equation with uμ,ρ,P,η defined in terms of φ and its derivatives. One finds a relation between the parameters of the theory and the quark-gluon plasma thermodynamics, α/β2=η/(sT), and by fixing α and β from usual (low multiplicity) particle scattering, one finds Ta mπ. |
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Repositório Institucional da UNESP |
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DBI scalar field theory for QGP hydrodynamicsA way to describe the hydrodynamics of the quark-gluon plasma using a Dirac-Born-Infeld (DBI) action is proposed, based on the model found by Heisenberg for high energy scattering of nucleons. The expanding plasma is described as a shockwave in a DBI model for a real scalar standing in for the pion, and I show that one obtains a fluid description in terms of a relativistic fluid that near the shock is approximately ideal (η≃0) and conformal. One can introduce an extra term inside the square root of the DBI action that generates a shear viscosity term in the energy-momentum tensor near the shock, as well as a bulk viscosity, and regulates the behavior of the energy density at the shock, making it finite. The resulting fluid satisfies the relativistic Navier-Stokes equation with uμ,ρ,P,η defined in terms of φ and its derivatives. One finds a relation between the parameters of the theory and the quark-gluon plasma thermodynamics, α/β2=η/(sT), and by fixing α and β from usual (low multiplicity) particle scattering, one finds Ta mπ.Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Instituto de Física Teórica UNESP-Universidade Estadual Paulista, R. Dr. Bento T. Ferraz 271Instituto de Física Teórica UNESP-Universidade Estadual Paulista, R. Dr. Bento T. Ferraz 271FAPESP: 2014/18634-9CNPq: 301709/2013-0Universidade Estadual Paulista (Unesp)Nastase, Horatiu [UNESP]2018-12-11T17:04:11Z2018-12-11T17:04:11Z2016-07-08info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://dx.doi.org/10.1103/PhysRevD.94.025014Physical Review D, v. 94, n. 2, 2016.2470-00292470-0010http://hdl.handle.net/11449/17321810.1103/PhysRevD.94.0250142-s2.0-849784189812-s2.0-84978418981.pdfScopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D1,8011,801info:eu-repo/semantics/openAccess2023-11-25T06:15:27Zoai:repositorio.unesp.br:11449/173218Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T18:40:35.281803Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
DBI scalar field theory for QGP hydrodynamics |
title |
DBI scalar field theory for QGP hydrodynamics |
spellingShingle |
DBI scalar field theory for QGP hydrodynamics Nastase, Horatiu [UNESP] |
title_short |
DBI scalar field theory for QGP hydrodynamics |
title_full |
DBI scalar field theory for QGP hydrodynamics |
title_fullStr |
DBI scalar field theory for QGP hydrodynamics |
title_full_unstemmed |
DBI scalar field theory for QGP hydrodynamics |
title_sort |
DBI scalar field theory for QGP hydrodynamics |
author |
Nastase, Horatiu [UNESP] |
author_facet |
Nastase, Horatiu [UNESP] |
author_role |
author |
dc.contributor.none.fl_str_mv |
Universidade Estadual Paulista (Unesp) |
dc.contributor.author.fl_str_mv |
Nastase, Horatiu [UNESP] |
description |
A way to describe the hydrodynamics of the quark-gluon plasma using a Dirac-Born-Infeld (DBI) action is proposed, based on the model found by Heisenberg for high energy scattering of nucleons. The expanding plasma is described as a shockwave in a DBI model for a real scalar standing in for the pion, and I show that one obtains a fluid description in terms of a relativistic fluid that near the shock is approximately ideal (η≃0) and conformal. One can introduce an extra term inside the square root of the DBI action that generates a shear viscosity term in the energy-momentum tensor near the shock, as well as a bulk viscosity, and regulates the behavior of the energy density at the shock, making it finite. The resulting fluid satisfies the relativistic Navier-Stokes equation with uμ,ρ,P,η defined in terms of φ and its derivatives. One finds a relation between the parameters of the theory and the quark-gluon plasma thermodynamics, α/β2=η/(sT), and by fixing α and β from usual (low multiplicity) particle scattering, one finds Ta mπ. |
publishDate |
2016 |
dc.date.none.fl_str_mv |
2016-07-08 2018-12-11T17:04:11Z 2018-12-11T17:04:11Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1103/PhysRevD.94.025014 Physical Review D, v. 94, n. 2, 2016. 2470-0029 2470-0010 http://hdl.handle.net/11449/173218 10.1103/PhysRevD.94.025014 2-s2.0-84978418981 2-s2.0-84978418981.pdf |
url |
http://dx.doi.org/10.1103/PhysRevD.94.025014 http://hdl.handle.net/11449/173218 |
identifier_str_mv |
Physical Review D, v. 94, n. 2, 2016. 2470-0029 2470-0010 10.1103/PhysRevD.94.025014 2-s2.0-84978418981 2-s2.0-84978418981.pdf |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physical Review D 1,801 1,801 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
application/pdf |
dc.source.none.fl_str_mv |
Scopus 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_ |
1808128965843353600 |