Possible origin of RHIC Rout/Rsid HBT results
| Main Author: | |
|---|---|
| Publication Date: | 2003 |
| Format: | Conference object |
| Language: | eng |
| Source: | Repositório Institucional da UNESP |
| Download full: | http://dx.doi.org/10.1016/S0375-9474(02)01550-6 http://hdl.handle.net/11449/67230 |
Summary: | The effects of opacity of the nuclei together with a blackbody type of emission along the system history are considered as a means to explain the ratio Rout/Rsid observed by STAR and PHENIX collaborations at RHIC. Within our model, no flow is required to explain the data trend of this ratio for large surface emissivities. © 2003 Elsevier Science B.V. All rights reserved. |
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Possible origin of RHIC Rout/Rsid HBT resultsThe effects of opacity of the nuclei together with a blackbody type of emission along the system history are considered as a means to explain the ratio Rout/Rsid observed by STAR and PHENIX collaborations at RHIC. Within our model, no flow is required to explain the data trend of this ratio for large surface emissivities. © 2003 Elsevier Science B.V. All rights reserved.Institute de Física Teórica Universidade Estadual Paulista, São Paulo - SPTheoretical Physics FERMILAB MS106, P.O. Box 500, Batavia, IL 60510Nuclear Theory Group Brookhaven National Laboratory, Upton, NY 11973Institute de Física Teórica Universidade Estadual Paulista, São Paulo - SPUniversidade Estadual Paulista (Unesp)MS106Brookhaven National LaboratoryPadula, Sandra S. [UNESP]2014-05-27T11:20:38Z2014-05-27T11:20:38Z2003-03-10info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjecthttp://dx.doi.org/10.1016/S0375-9474(02)01550-6Nuclear Physics A, v. 715, p. 637C-640C, 2003.0375-9474http://hdl.handle.net/11449/6723010.1016/S0375-9474(02)01550-6WOS:0001817375000902-s2.0-17544372927Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengNuclear Physics A1.9920,938info:eu-repo/semantics/openAccess2021-10-23T21:44:16Zoai:repositorio.unesp.br:11449/67230Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462021-10-23T21:44:16Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
| dc.title.none.fl_str_mv |
Possible origin of RHIC Rout/Rsid HBT results |
| title |
Possible origin of RHIC Rout/Rsid HBT results |
| spellingShingle |
Possible origin of RHIC Rout/Rsid HBT results Padula, Sandra S. [UNESP] |
| title_short |
Possible origin of RHIC Rout/Rsid HBT results |
| title_full |
Possible origin of RHIC Rout/Rsid HBT results |
| title_fullStr |
Possible origin of RHIC Rout/Rsid HBT results |
| title_full_unstemmed |
Possible origin of RHIC Rout/Rsid HBT results |
| title_sort |
Possible origin of RHIC Rout/Rsid HBT results |
| author |
Padula, Sandra S. [UNESP] |
| author_facet |
Padula, Sandra S. [UNESP] |
| author_role |
author |
| dc.contributor.none.fl_str_mv |
Universidade Estadual Paulista (Unesp) MS106 Brookhaven National Laboratory |
| dc.contributor.author.fl_str_mv |
Padula, Sandra S. [UNESP] |
| description |
The effects of opacity of the nuclei together with a blackbody type of emission along the system history are considered as a means to explain the ratio Rout/Rsid observed by STAR and PHENIX collaborations at RHIC. Within our model, no flow is required to explain the data trend of this ratio for large surface emissivities. © 2003 Elsevier Science B.V. All rights reserved. |
| publishDate |
2003 |
| dc.date.none.fl_str_mv |
2003-03-10 2014-05-27T11:20:38Z 2014-05-27T11:20:38Z |
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info:eu-repo/semantics/publishedVersion |
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info:eu-repo/semantics/conferenceObject |
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conferenceObject |
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publishedVersion |
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http://dx.doi.org/10.1016/S0375-9474(02)01550-6 Nuclear Physics A, v. 715, p. 637C-640C, 2003. 0375-9474 http://hdl.handle.net/11449/67230 10.1016/S0375-9474(02)01550-6 WOS:000181737500090 2-s2.0-17544372927 |
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http://dx.doi.org/10.1016/S0375-9474(02)01550-6 http://hdl.handle.net/11449/67230 |
| identifier_str_mv |
Nuclear Physics A, v. 715, p. 637C-640C, 2003. 0375-9474 10.1016/S0375-9474(02)01550-6 WOS:000181737500090 2-s2.0-17544372927 |
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eng |
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eng |
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Nuclear Physics A 1.992 0,938 |
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info:eu-repo/semantics/openAccess |
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openAccess |
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Scopus reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
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Universidade Estadual Paulista (UNESP) |
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UNESP |
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UNESP |
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Repositório Institucional da UNESP |
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Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
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