Impact factor of Chinese Physics C is 3.6 in 2023 Impact factor of Chinese Physics C is 3.6 in 2022 2021 Impact Factor 2.944
Advanced Search
×
近期发现有不法分子冒充我刊与作者联系，借此进行欺诈等不法行为，请广大作者加以鉴别，如遇诈骗行为，请第一时间与我刊编辑部联系确认（《中国物理C》（英文）编辑部电话：010-88235947,010-88236950），并作报警处理。
本刊再次郑重声明：
（1）本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137
（2）本刊采编系统作者中心是投稿的唯一路径，该系统为ScholarOne远程稿件采编系统，仅在本刊投稿网网址（https://mc03.manuscriptcentral.com/cpc）设有登录入口。本刊不接受其他方式的投稿，如打印稿投稿、E-mail信箱投稿等，若以此种方式接收投稿均为假冒。
（3）所有投稿均需经过严格的同行评议、编辑加工后方可发表，本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿，并收取发表费用，均为假冒。
                  
《中国物理C》（英文）编辑部
2024年10月30日
Chinese Physics C> 2008, Vol. 32> Issue(12) : 976-983 DOI: 10.1088/1674-1137/32/12/007

Centrality dependence of pT spectra for identified hadrons in Au+Au and Cu+Cu collisions at √sNN= 200GeV

  • The centrality dependence of transverse momentum spectra for identified hadrons at midrapidity in Au+Au collisions at √sNN= 200GeV is systematically studied in a quark combination model. The pT spectra of π±, K±, p(p) and Λ(Λ) in different centrality bins and the nuclear modification factors (RCP) for these hadrons are calculated. The centrality dependence of the average collective transverse velocity 〈β(r)〉 for the hot and dense quark matter is obtained in Au+Au collisions, and it is applied to a relative smaller Cu+Cu collision system. The centrality dependence of pT spectra and the RCP for π0, Ks0 and Λ in Cu+Cu collisions at √sNN= 200GeV are well described. The results show that 〈β(r)〉 is only a function of the number of participants Npart and it is independent of the collision system.

  • 加载中

  • References

    [1] . Reisdorf W, Ritter H G. Annu. Rev. Nucl. Part. Sci., 1997,47: 663-7092. Sorge H. Phys. Rev. Lett., 1999, 82: 2048-20513. Kolb P, Sollfrank J, Heinz U. Phys. Lett. B, 1999, 459:667-6724. Teaney D, Shuryak E V. Phys. Rev. Lett., 1999, 83: 4951-49545. Kolb P, Sollfrank J, Heinz U. Phys. Rev. C, 2000, 62:0549096. Voloshin S A, Poskanzer A M. Phys. Lett. B, 2000, 474:27-327. Greco V, Ko C M, Levai P. Phys. Rev. C, 2003, 68: 0349048. Fries R J, Muller B, Nonaka C et al. Phys. Rev. C, 2003,68: 0449029. Armesto N, Salgado C A, Wiedemann U A. Phys. Rev.Lett., 2004, 93: 24230110. WANG X N, Gyulassy M. Phys. Rev. Lett. C, 1992, 68:1480-148311. Armesto N, Salgado C A, Wiedemann U A. Phys. Rev. C,2005, 72: 06491012. Adare A et al. (PHENIX Collaboration). Phys. Rev. Lett.,2007, 98: 16230113. Adare A et al. (PHENIX Collaboration). Phys. Rev. Lett.,2003, 91: 18230114. Enokizono A (the PHENIX Collaboration). Nucl. Phys. A,2007, 787: 37c-43c15. Fries R J, Müller B, Nonaka C et al. Phys. Rev. Lett., 2003,90: 20230316. Greco V, Ko C M, Levai P. Phys. Rev. Lett., 2003, 90:20230217. Hwa R C, YANG C B. Phys. Rev. C, 2003, 67: 03490218. Voloshin S A. Nucl. Phys. A, 2003, 715: 379c-388c19. Molnar D, Voloshin S A. Phys. Rev. Lett., 2003, 91: 09230120. YAO T, XIE Q B, SHAO F L. Chin. Phys. C, 2008, 32:356-36221. Hwa R C, YANG C B. Phys. Rev. C, 2004, 70: 02490522. SHAO F L, YAO T, XIE Q B. Phys. Rev. C, 2007, 75:03490423. Hwa R C, Tian Z. Phys. Rev. C, 2005, 72: 02490824. SHAO F L, XIE Q B, WANG Q. Phys. Rev. C, 2005, 71:04490325. Arsene I et al. (BRAHMS Collaboration). Phys. Rev. C,2005, 72: 01490826. Adler S S et al. (PHENIX Collaboration). Phys. Rev. C,2004, 69: 03490927. Schnedermann E, Heinz U. Phys. Rev. Lett., 1992, 69:2908-291128. Kolb P F, Rapp R. Phys. Rev. C, 2003, 67: 04490329. Nonaka C, Bass S A. Phys. Rev. C, 2007, 75: 01490230. Heinz U, Kolb P. Nucl. Phys. A, 2002, 702: 269-28031. Huovinen P. Nucl. Phys. A, 2005, 761: 296-31232. Prorok D. Phys. Rev. C, 2006, 73: 06490133. Pratt S, Pal S. Phys. Rev. C, 2005, 71: 01490534. XIE Q B, LIU X M. Phys. Rev. D, 1988, 38: 2169-217735. LIANG Z T, XIE Q B. Phys. Rev. D, 1991, 43: 751-75936. WANG Q, XIE Q B. J. Phys. G, 1995, 21: 897-90437. ZHAO J Q, WANG Q, XIE Q B. Sci. Sin. A, 1995, 38:1474-148738. WANG Q, SI Z G, XIE Q B. Int. J. Mod. Phys. A, 1996,11: 5203-521039. SI Z G, XIE Q B, WANG Q. Commun. Theor. Phys., 1997,28: 85-9440. SONG J, SHAO F L, XIE Q B et al. The Inuence of Net-Quarks on the Yields and Rapidity Spectra of Identi edHadrons. arXiv: hep-ph/0801.091841. Sjostrand T, Eden P, Friberg C et al. Comput. Phys. Commun.,2001, 135: 238-25942. Abelev B I et al. (STAR Collaboration). Phys. Rev. Lett.,2007, 99: 11230143. Schnedermann E, Sollfrank J, Heinz U. Phys. Rev. C, 1993,48: 2462-247544. Sakaguchi T. (PHENIX Collaboration). Contributions for Quark Matter 2006 Poster Session. Shanghai, China, 14-20. November, 2006. arXiv: nucl-ex/070302745. Adams J et al. (STAR, STAR-RICH Collaborations). nuclex/060104246. CHEN J H, JIN F, Gangadharan D et al. Parton Distributionat Hadronization from Bulk Dense Matter Producedat RHIC. arXiv: 0801.2265[nucl-th]47. SONG J, SHAO F L, XIE Q B et al. Rapidity Dependenceof Hadron Production in Central Au+Au Collisions at √span style="border-top: 1px solid; padding-top: 0px;"sNN/span =200 GeV. arXiv: nucl-th/070309548. Abelev B I et al. (STAR Collaboration). Phys. Rev. Lett.,2006, 97: 15230149. Admas J et al. (STAR Collaboration). Phys. Rev. Lett,2006, 98: 06230150. Adams J et al. (STAR Collaboration). Phys. Rev. Lett.,2003, 92: 05230251. Timmins A R. (STAR Collaboration). Quark Matter 2006Proceedings. Shanghai, China, 14-20 November, 2006.arXiv: nucl-ex/0708.329052. Hollis R S. (STAR Collaboration). Proceedings for the LakeLouise Winter Institute 2007. Alberta, Canada, 19-24February 2007. arXiv: nucl-ex/0705.068653. Bekele S. (BRAHMS Collaboration). arXiv: nucl-ex/060101154. LIANG Z T, WANG X N. Phys. Rev. Lett., 2005, 94:10230155. Abelev B I et al. (STAR Collaboration). Phys. Rev. C,2007, 76: 02491556. Back B B et al. (PHOBOS Collaboration). Phys. Rev.Lett., 2002, 89: 222301

  • Access

    加载中

Get Citation
WANG Yun-Fei, SHAO Feng-Lan, SONG Jun, WEI De-Ming and XIE Qu-Bing. Centrality dependence of pT spectra for identified hadrons in Au+Au and Cu+Cu collisions at √sNN= 200GeV[J]. Chinese Physics C, 2008, 32(12): 976-983. doi: 10.1088/1674-1137/32/12/007
WANG Yun-Fei, SHAO Feng-Lan, SONG Jun, WEI De-Ming and XIE Qu-Bing. Centrality dependence of pT spectra for identified hadrons in Au+Au and Cu+Cu collisions at √sNN= 200GeV[J]. Chinese Physics C, 2008, 32(12): 976-983.  doi: 10.1088/1674-1137/32/12/007 shu
Milestone
Received: 2008-04-01
Revised: 2008-06-11
Article Metric

Article Views(2936)
PDF Downloads(689)
Cited by(0)
Policy on re-use
To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.
通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

Centrality dependence of pT spectra for identified hadrons in Au+Au and Cu+Cu collisions at √sNN= 200GeV

    Corresponding author: SHAO Feng-Lan,
  • Received Date: 2008-04-01
  • Accepted Date: 2008-06-11
  • Available Online: 2008-12-05

Abstract: 

The centrality dependence of transverse momentum spectra for identified hadrons at midrapidity in Au+Au collisions at √sNN= 200GeV is systematically studied in a quark combination model. The pT spectra of π±, K±, p(p) and Λ(Λ) in different centrality bins and the nuclear modification factors (RCP) for these hadrons are calculated. The centrality dependence of the average collective transverse velocity 〈β(r)〉 for the hot and dense quark matter is obtained in Au+Au collisions, and it is applied to a relative smaller Cu+Cu collision system. The centrality dependence of pT spectra and the RCP for π0, Ks0 and Λ in Cu+Cu collisions at √sNN= 200GeV are well described. The results show that 〈β(r)〉 is only a function of the number of participants Npart and it is independent of the collision system.

    HTML

Reference (1)

目录

Link
IOPScience
SCOAP3
arXiv
Chinese Physical Society
Journal information
Introduction
Editorial Board
Others
Subscribe
Contact us
QQ: 1307685413
Tel: +86-010-88235947
Fax: +86-010-88233126
E-mail: cpc@ihep.ac.cn

  • CPC Website

  • IOP Website

  • CPC WeChat

Copyright © Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, China 京ICP备05002789号-1

Supported by: Beijing Renhe Information Technology Co. Ltd  E-mail: info@rhhz.net

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return