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Nonlinear evolution of density and flow perturbations on a Bjorken background

Density perturbations and their dynamic evolution from early to late times can be used for an improved understanding of interesting physical phenomena both in cosmology and in the context of heavy-ion collisions. We discuss the spectrum and bispectrum of these perturbations around a longitudinally e...

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Autores principales: Brouzakis, Nikolaos, Floerchinger, Stefan, Tetradis, Nikolaos, Wiedemann, Urs Achim
Lenguaje:eng
Publicado: 2014
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.91.065007
http://cds.cern.ch/record/1969230
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author Brouzakis, Nikolaos
Floerchinger, Stefan
Tetradis, Nikolaos
Wiedemann, Urs Achim
author_facet Brouzakis, Nikolaos
Floerchinger, Stefan
Tetradis, Nikolaos
Wiedemann, Urs Achim
author_sort Brouzakis, Nikolaos
collection CERN
description Density perturbations and their dynamic evolution from early to late times can be used for an improved understanding of interesting physical phenomena both in cosmology and in the context of heavy-ion collisions. We discuss the spectrum and bispectrum of these perturbations around a longitudinally expanding fireball after a heavy-ion collision. The time-evolution equations couple the spectrum and bispectrum to each other, as well as to higher-order correlation functions through nonlinear terms. A non-trivial bispectrum is thus always generated, even if absent initially. For initial conditions corresponding to a model of independent sources, we discuss the linear and nonlinear evolution is detail. We show that, if the initial conditions are sufficiently smooth for fluid dynamics to be applicable, the nonlinear effects are relatively small.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2014
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spelling cern-19692302023-03-14T17:48:22Zdoi:10.1103/PhysRevD.91.065007http://cds.cern.ch/record/1969230engBrouzakis, NikolaosFloerchinger, StefanTetradis, NikolaosWiedemann, Urs AchimNonlinear evolution of density and flow perturbations on a Bjorken backgroundParticle Physics - PhenomenologyDensity perturbations and their dynamic evolution from early to late times can be used for an improved understanding of interesting physical phenomena both in cosmology and in the context of heavy-ion collisions. We discuss the spectrum and bispectrum of these perturbations around a longitudinally expanding fireball after a heavy-ion collision. The time-evolution equations couple the spectrum and bispectrum to each other, as well as to higher-order correlation functions through nonlinear terms. A non-trivial bispectrum is thus always generated, even if absent initially. For initial conditions corresponding to a model of independent sources, we discuss the linear and nonlinear evolution is detail. We show that, if the initial conditions are sufficiently smooth for fluid dynamics to be applicable, the nonlinear effects are relatively small.Density perturbations and their dynamic evolution from early to late times can be used for an improved understanding of interesting physical phenomena both in cosmology and in the context of heavy-ion collisions. We discuss the spectrum and bispectrum of these perturbations around a longitudinally expanding fireball after a heavy-ion collision. The time-evolution equations couple the spectrum and bispectrum to each other, as well as to higher-order correlation functions through nonlinear terms. A nontrivial bispectrum is thus always generated, even if absent initially. For initial conditions corresponding to a model of independent sources, we discuss the linear and nonlinear evolution in detail. We show that, if the initial conditions are sufficiently smooth for fluid dynamics to be applicable, the nonlinear effects are relatively small.Density perturbations and their dynamic evolution from early to late times can be used for an improved understanding of interesting physical phenomena both in cosmology and in the context of heavy-ion collisions. We discuss the spectrum and bispectrum of these perturbations around a longitudinally expanding fireball after a heavy-ion collision. The time-evolution equations couple the spectrum and bispectrum to each other, as well as to higher-order correlation functions through nonlinear terms. A non-trivial bispectrum is thus always generated, even if absent initially. For initial conditions corresponding to a model of independent sources, we discuss the linear and nonlinear evolution is detail. We show that, if the initial conditions are sufficiently smooth for fluid dynamics to be applicable, the nonlinear effects are relatively small.arXiv:1411.2912CERN-PH-TH-2014-223CERN-PH-TH-2014-223oai:cds.cern.ch:19692302014-11-11
spellingShingle Particle Physics - Phenomenology
Brouzakis, Nikolaos
Floerchinger, Stefan
Tetradis, Nikolaos
Wiedemann, Urs Achim
Nonlinear evolution of density and flow perturbations on a Bjorken background
title Nonlinear evolution of density and flow perturbations on a Bjorken background
title_full Nonlinear evolution of density and flow perturbations on a Bjorken background
title_fullStr Nonlinear evolution of density and flow perturbations on a Bjorken background
title_full_unstemmed Nonlinear evolution of density and flow perturbations on a Bjorken background
title_short Nonlinear evolution of density and flow perturbations on a Bjorken background
title_sort nonlinear evolution of density and flow perturbations on a bjorken background
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1103/PhysRevD.91.065007
http://cds.cern.ch/record/1969230
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AT wiedemannursachim nonlinearevolutionofdensityandflowperturbationsonabjorkenbackground