Beam Energy Dependence of Hanbury-Brown-Twiss Radii from a Blast-Wave Model

The beam energy dependence of correlation lengths (the Hanbury-Brown-Twiss radii) is calculated by using a blast-wave model and the results are comparable with those from RHIC-STAR beam energy scan data as well as the LHC-ALICE measurements. A set of parameters for the blast-wave model as a function...

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Main Authors: S. Zhang, Y. G. Ma, J. H. Chen, C. Zhong
Format: Article
Language:English
Published: Wiley 2016-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2016/9414239
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author S. Zhang
Y. G. Ma
J. H. Chen
C. Zhong
author_facet S. Zhang
Y. G. Ma
J. H. Chen
C. Zhong
author_sort S. Zhang
collection DOAJ
description The beam energy dependence of correlation lengths (the Hanbury-Brown-Twiss radii) is calculated by using a blast-wave model and the results are comparable with those from RHIC-STAR beam energy scan data as well as the LHC-ALICE measurements. A set of parameters for the blast-wave model as a function of beam energy under study are obtained by fit to the HBT radii at each energy point. The transverse momentum dependence of HBT radii is presented with the extracted parameters for Au+Au collision at sNN = 200 GeV and for Pb+Pb collisions at 2.76 TeV. From our study one can learn that particle emission duration cannot be ignored while calculating the HBT radii with the same parameters. And tuning kinetic freeze-out temperature in a range will result in system lifetime changing in the reverse direction as it is found in RHIC-STAR experiment measurements.
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institution Kabale University
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publishDate 2016-01-01
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series Advances in High Energy Physics
spelling doaj-art-84c092723f9a4cc8b2415a5e8e0664ff2025-02-03T06:01:40ZengWileyAdvances in High Energy Physics1687-73571687-73652016-01-01201610.1155/2016/94142399414239Beam Energy Dependence of Hanbury-Brown-Twiss Radii from a Blast-Wave ModelS. Zhang0Y. G. Ma1J. H. Chen2C. Zhong3Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Shanghai 201800, ChinaShanghai Institute of Applied Physics, Chinese Academy of Sciences, Shanghai 201800, ChinaShanghai Institute of Applied Physics, Chinese Academy of Sciences, Shanghai 201800, ChinaShanghai Institute of Applied Physics, Chinese Academy of Sciences, Shanghai 201800, ChinaThe beam energy dependence of correlation lengths (the Hanbury-Brown-Twiss radii) is calculated by using a blast-wave model and the results are comparable with those from RHIC-STAR beam energy scan data as well as the LHC-ALICE measurements. A set of parameters for the blast-wave model as a function of beam energy under study are obtained by fit to the HBT radii at each energy point. The transverse momentum dependence of HBT radii is presented with the extracted parameters for Au+Au collision at sNN = 200 GeV and for Pb+Pb collisions at 2.76 TeV. From our study one can learn that particle emission duration cannot be ignored while calculating the HBT radii with the same parameters. And tuning kinetic freeze-out temperature in a range will result in system lifetime changing in the reverse direction as it is found in RHIC-STAR experiment measurements.http://dx.doi.org/10.1155/2016/9414239
spellingShingle S. Zhang
Y. G. Ma
J. H. Chen
C. Zhong
Beam Energy Dependence of Hanbury-Brown-Twiss Radii from a Blast-Wave Model
Advances in High Energy Physics
title Beam Energy Dependence of Hanbury-Brown-Twiss Radii from a Blast-Wave Model
title_full Beam Energy Dependence of Hanbury-Brown-Twiss Radii from a Blast-Wave Model
title_fullStr Beam Energy Dependence of Hanbury-Brown-Twiss Radii from a Blast-Wave Model
title_full_unstemmed Beam Energy Dependence of Hanbury-Brown-Twiss Radii from a Blast-Wave Model
title_short Beam Energy Dependence of Hanbury-Brown-Twiss Radii from a Blast-Wave Model
title_sort beam energy dependence of hanbury brown twiss radii from a blast wave model
url http://dx.doi.org/10.1155/2016/9414239
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AT jhchen beamenergydependenceofhanburybrowntwissradiifromablastwavemodel
AT czhong beamenergydependenceofhanburybrowntwissradiifromablastwavemodel