On nonlinearity in hydrodynamic response to the initial geometry in relativistic heavy-ion collisions
Autor(a) principal: | |
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Data de Publicação: | 2020 |
Outros Autores: | , , , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1140/epja/s10050-020-00235-4 http://hdl.handle.net/11449/210406 |
Resumo: | In the context of event-by-event hydrodynamic description, we analyze the implications of two models characterized by distinct initial conditions. The initial energy density of the first model adopts a Gaussian-type distribution, while those of the second one are features by high energy peripheral tubes. We calibrate the initial conditions of both models so that their initial probability distribution of eccentricity are mostly identical. Subsequently, the resultant scaled probability distributions of collective flow and the correlations between flow harmonic and eccentricity coefficients are investigated. Besides, the calculations are carried out for particle correlations regarding the symmetric cumulant, mixed harmonics, and nonlinear response coefficients. Although the resultant two-particle correlations possess similar shapes, numerical calculations indicate a subtle difference between the two models. To be specific, the difference resides in more detailed observables such as the probability distributions of elliptic flow as well as Pearson correlation coefficient regarding higher-order harmonics. We discuss several essential aspects concerning the linearity and nonlinearity between initial eccentricities and final state anisotropies. Further implications are addressed. |
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Repositório Institucional da UNESP |
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2946 |
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On nonlinearity in hydrodynamic response to the initial geometry in relativistic heavy-ion collisionsIn the context of event-by-event hydrodynamic description, we analyze the implications of two models characterized by distinct initial conditions. The initial energy density of the first model adopts a Gaussian-type distribution, while those of the second one are features by high energy peripheral tubes. We calibrate the initial conditions of both models so that their initial probability distribution of eccentricity are mostly identical. Subsequently, the resultant scaled probability distributions of collective flow and the correlations between flow harmonic and eccentricity coefficients are investigated. Besides, the calculations are carried out for particle correlations regarding the symmetric cumulant, mixed harmonics, and nonlinear response coefficients. Although the resultant two-particle correlations possess similar shapes, numerical calculations indicate a subtle difference between the two models. To be specific, the difference resides in more detailed observables such as the probability distributions of elliptic flow as well as Pearson correlation coefficient regarding higher-order harmonics. We discuss several essential aspects concerning the linearity and nonlinearity between initial eccentricities and final state anisotropies. Further implications are addressed.Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Fundação de Amparo à Pesquisa do Estado do Rio de Janeiro (FAPERJ)Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)National Natural Science Foundation of China (NNSFC)INCT-FNAYangzhou Univ, Sch Phys Sci & Technol, Yangzhou 225002, Jiangsu, Peoples R ChinaUniv Estadual Paulista, Fac Engn Guaratingueta, BR-12516410 Guaratingueta, SP, BrazilChina Univ Geosci, Hubei Subsurface Multiscale Imaging Key Lab, Inst Geophys & Geomat, Wuhan 430074, Hubei, Peoples R ChinaUniv Sao Paulo, Escola Engn Lorena, BR-12602810 Lorena, SP, BrazilUniv Sao Paulo, Inst Fis, CP 66318, BR-05315970 Sao Paulo, SP, BrazilUniv Fed Rio de Janeiro, Inst Fis, CP 68528, BR-21945970 Rio De Janeiro, RJ, BrazilUniv Fed Fluminense, Inst Fis, BR-24210346 Niteroi, RJ, BrazilUniv Estadual Paulista, Fac Engn Guaratingueta, BR-12516410 Guaratingueta, SP, BrazilNational Natural Science Foundation of China (NNSFC): 11805166INCT-FNA: 464898/2014-5SpringerYangzhou UnivUniversidade Estadual Paulista (Unesp)China Univ GeosciUniversidade de São Paulo (USP)Universidade Federal do Rio de Janeiro (UFRJ)Universidade do Estado do Rio de Janeiro (UERJ)Wen, Dan [UNESP]Lin, KaiQian, Wei-Liang [UNESP]Wang, BinHama, YogiroKodama, Takeshi2021-06-25T15:07:33Z2021-06-25T15:07:33Z2020-09-03info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article13http://dx.doi.org/10.1140/epja/s10050-020-00235-4European Physical Journal A. New York: Springer, v. 56, n. 9, 13 p., 2020.1434-6001http://hdl.handle.net/11449/21040610.1140/epja/s10050-020-00235-4WOS:000568376700002Web of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengEuropean Physical Journal Ainfo:eu-repo/semantics/openAccess2021-10-23T20:17:28Zoai:repositorio.unesp.br:11449/210406Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T23:58:05.485679Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
On nonlinearity in hydrodynamic response to the initial geometry in relativistic heavy-ion collisions |
title |
On nonlinearity in hydrodynamic response to the initial geometry in relativistic heavy-ion collisions |
spellingShingle |
On nonlinearity in hydrodynamic response to the initial geometry in relativistic heavy-ion collisions Wen, Dan [UNESP] |
title_short |
On nonlinearity in hydrodynamic response to the initial geometry in relativistic heavy-ion collisions |
title_full |
On nonlinearity in hydrodynamic response to the initial geometry in relativistic heavy-ion collisions |
title_fullStr |
On nonlinearity in hydrodynamic response to the initial geometry in relativistic heavy-ion collisions |
title_full_unstemmed |
On nonlinearity in hydrodynamic response to the initial geometry in relativistic heavy-ion collisions |
title_sort |
On nonlinearity in hydrodynamic response to the initial geometry in relativistic heavy-ion collisions |
author |
Wen, Dan [UNESP] |
author_facet |
Wen, Dan [UNESP] Lin, Kai Qian, Wei-Liang [UNESP] Wang, Bin Hama, Yogiro Kodama, Takeshi |
author_role |
author |
author2 |
Lin, Kai Qian, Wei-Liang [UNESP] Wang, Bin Hama, Yogiro Kodama, Takeshi |
author2_role |
author author author author author |
dc.contributor.none.fl_str_mv |
Yangzhou Univ Universidade Estadual Paulista (Unesp) China Univ Geosci Universidade de São Paulo (USP) Universidade Federal do Rio de Janeiro (UFRJ) Universidade do Estado do Rio de Janeiro (UERJ) |
dc.contributor.author.fl_str_mv |
Wen, Dan [UNESP] Lin, Kai Qian, Wei-Liang [UNESP] Wang, Bin Hama, Yogiro Kodama, Takeshi |
description |
In the context of event-by-event hydrodynamic description, we analyze the implications of two models characterized by distinct initial conditions. The initial energy density of the first model adopts a Gaussian-type distribution, while those of the second one are features by high energy peripheral tubes. We calibrate the initial conditions of both models so that their initial probability distribution of eccentricity are mostly identical. Subsequently, the resultant scaled probability distributions of collective flow and the correlations between flow harmonic and eccentricity coefficients are investigated. Besides, the calculations are carried out for particle correlations regarding the symmetric cumulant, mixed harmonics, and nonlinear response coefficients. Although the resultant two-particle correlations possess similar shapes, numerical calculations indicate a subtle difference between the two models. To be specific, the difference resides in more detailed observables such as the probability distributions of elliptic flow as well as Pearson correlation coefficient regarding higher-order harmonics. We discuss several essential aspects concerning the linearity and nonlinearity between initial eccentricities and final state anisotropies. Further implications are addressed. |
publishDate |
2020 |
dc.date.none.fl_str_mv |
2020-09-03 2021-06-25T15:07:33Z 2021-06-25T15:07:33Z |
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/10.1140/epja/s10050-020-00235-4 European Physical Journal A. New York: Springer, v. 56, n. 9, 13 p., 2020. 1434-6001 http://hdl.handle.net/11449/210406 10.1140/epja/s10050-020-00235-4 WOS:000568376700002 |
url |
http://dx.doi.org/10.1140/epja/s10050-020-00235-4 http://hdl.handle.net/11449/210406 |
identifier_str_mv |
European Physical Journal A. New York: Springer, v. 56, n. 9, 13 p., 2020. 1434-6001 10.1140/epja/s10050-020-00235-4 WOS:000568376700002 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
European Physical Journal A |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
13 |
dc.publisher.none.fl_str_mv |
Springer |
publisher.none.fl_str_mv |
Springer |
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_ |
1808129567926255616 |