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Title: Three-particle correlations in a multiphase transport model

Here, we study three-particle mixed harmonic correlations in relativistic heavy ion collisions by considering the observable C m,n,m+n= cos(mφ 1+nφ 2-(m +n)φ 3), where φ 1,2,3 are azimuthal angles of all particle triplets, using a multiphase transport model. We find that except for C 123, these results on the centrality dependence of C 112, C 224 and C 235 as well as the relative pseudorapidity dependence of C 123 and C 224 in Au+Au collisions at √s=200 GeV agree reasonable well with the experimental data from the STAR Collaboration. We also discuss the implications of our results.
Authors:
 [1] ;  [1]
  1. Texas A & M Univ., College Station, TX (United States). Cyclotron Inst. and Dept. of Physics and Astronomy
Publication Date:
Grant/Contract Number:
SC0015266
Type:
Published Article
Journal Name:
Physics Letters. Section B
Additional Journal Information:
Journal Volume: 769; Journal Issue: C; Journal ID: ISSN 0370-2693
Publisher:
Elsevier
Research Org:
Texas A & M Univ., College Station, TX (United States)
Sponsoring Org:
USDOE Office of Science (SC)
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; Anisotropic flow; Two-particle cumulants; Three-particle correlations; AMPT
OSTI Identifier:
1349532
Alternate Identifier(s):
OSTI ID: 1374588

Sun, Yifeng, and Ko, Che Ming. Three-particle correlations in a multiphase transport model. United States: N. p., Web. doi:10.1016/j.physletb.2017.03.068.
Sun, Yifeng, & Ko, Che Ming. Three-particle correlations in a multiphase transport model. United States. doi:10.1016/j.physletb.2017.03.068.
Sun, Yifeng, and Ko, Che Ming. 2017. "Three-particle correlations in a multiphase transport model". United States. doi:10.1016/j.physletb.2017.03.068.
@article{osti_1349532,
title = {Three-particle correlations in a multiphase transport model},
author = {Sun, Yifeng and Ko, Che Ming},
abstractNote = {Here, we study three-particle mixed harmonic correlations in relativistic heavy ion collisions by considering the observable Cm,n,m+n= cos(mφ1+nφ2-(m +n)φ3), where φ1,2,3 are azimuthal angles of all particle triplets, using a multiphase transport model. We find that except for C123, these results on the centrality dependence of C112, C224 and C235 as well as the relative pseudorapidity dependence of C123 and C224 in Au+Au collisions at √s=200 GeV agree reasonable well with the experimental data from the STAR Collaboration. We also discuss the implications of our results.},
doi = {10.1016/j.physletb.2017.03.068},
journal = {Physics Letters. Section B},
number = C,
volume = 769,
place = {United States},
year = {2017},
month = {3}
}