Production of multistrange hadrons, light nuclei and hypertriton in central Au plus Au collisions at root S-NN=11.5 and 200 GeV | |
Shah, N; Ma, YG; Chen, JH; Zhang, S | |
刊名 | PHYSICS LETTERS B |
2016 | |
卷号 | 754期号:-页码:6—10 |
关键词 | QUARK-GLUON PLASMA STAR COLLABORATION HYPERNUCLEUS SEARCH |
ISSN号 | 0370-2693 |
通讯作者 | Shah, N (reprint author), Chinese Acad Sci, Shanghai Inst Appl Phys, Shanghai 201800, Peoples R China. |
英文摘要 | The production of dibaryons, light nuclei and hypertriton in the most central Au+ Au collisions at root S-NN = 11.5 and 200 GeV is investigated by using a naive coalescence model. The production of light nuclei is studied and found that the production rate reduces by a factor of 330 (1200) for each extra nucleon added to nuclei at root S-NN = 11.5 (200) GeV. The p(T) integrated yield of multistrange hadrons falls exponentially as strangeness quantum number increases. We further investigate strangeness population factors S-3, S-2 as a function of transverse momentum as well as root S-NN. The calculations for root S-NN = 11.5 GeV presented here will stimulate interest to carry out these measurements during the phase-II of beam energy scan program at STAR experiment. (C) 2016 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000369601000002 |
内容类型 | 期刊论文 |
源URL | [http://ir.sinap.ac.cn/handle/331007/25815] |
专题 | 上海应用物理研究所_中科院上海应用物理研究所2011-2017年 |
推荐引用方式 GB/T 7714 | Shah, N,Ma, YG,Chen, JH,et al. Production of multistrange hadrons, light nuclei and hypertriton in central Au plus Au collisions at root S-NN=11.5 and 200 GeV[J]. PHYSICS LETTERS B,2016,754(-):6—10. |
APA | Shah, N,Ma, YG,Chen, JH,&Zhang, S.(2016).Production of multistrange hadrons, light nuclei and hypertriton in central Au plus Au collisions at root S-NN=11.5 and 200 GeV.PHYSICS LETTERS B,754(-),6—10. |
MLA | Shah, N,et al."Production of multistrange hadrons, light nuclei and hypertriton in central Au plus Au collisions at root S-NN=11.5 and 200 GeV".PHYSICS LETTERS B 754.-(2016):6—10. |
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