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Investigation of experimental observables in search of the chiral magnetic effect in heavy-ion collisions in the STAR experiment
The chiral magnetic effect (CME) is a novel transport phenomenon, arising from the interplay between quantum anomalies and strong magnetic fields in chiral systems. In high-energy nuclear collisions, the CME may survive the expansion of the quark-gluon plasma fireball and be detected in experiments....
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Published in: | Chinese physics C 2022-01, Vol.46 (1), p.14101 |
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creator | Choudhury, Subikash Dong, Xin Drachenberg, Jim Dunlop, James Esumi, ShinIchi Feng, Yicheng Finch, Evan Hu, Yu Jia, Jiangyong Lauret, Jerome Li, Wei Liao, Jinfeng Lin, Yufu Lisa, Mike Niida, Takafumi Ray, Robert Lanny Sergeeva, Masha Shen, Diyu Shi, Shuzhe Sorensen, Paul Tang, Aihong Tribedy, Prithwish Van Buren, Gene Voloshin, Sergei Wang, Fuqiang Wang, Gang Xu, Haojie Xu, Zhiwan Yao, Nanxi Zhao, Jie |
description | The chiral magnetic effect (CME) is a novel transport phenomenon, arising from the interplay between quantum anomalies and strong magnetic fields in chiral systems. In high-energy nuclear collisions, the CME may survive the expansion of the quark-gluon plasma fireball and be detected in experiments. Over the past two decades, experimental searches for the CME have attracted extensive interest at the Relativistic Heavy Ion Collider (RHIC) and the Large Hadron Collider (LHC). The main goal of this study is to investigate three pertinent experimental approaches: the
correlator, the
R
correlator, and the signed balance functions. We exploit simple Monte Carlo simulations and a realistic event generator (EBE-AVFD) to verify the equivalence of the core components among these methods and to ascertain their sensitivities to the CME signal and the background contributions for the isobar collisions at the RHIC. |
doi_str_mv | 10.1088/1674-1137/ac2a1f |
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correlator, the
R
correlator, and the signed balance functions. We exploit simple Monte Carlo simulations and a realistic event generator (EBE-AVFD) to verify the equivalence of the core components among these methods and to ascertain their sensitivities to the CME signal and the background contributions for the isobar collisions at the RHIC.</description><identifier>ISSN: 1674-1137</identifier><identifier>EISSN: 2058-6132</identifier><identifier>DOI: 10.1088/1674-1137/ac2a1f</identifier><language>eng</language><ispartof>Chinese physics C, 2022-01, Vol.46 (1), p.14101</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c351t-2c93da53e8fd584c4baeaeb11679c0b6389cf6eba2da22372308f50730c2d99d3</citedby><cites>FETCH-LOGICAL-c351t-2c93da53e8fd584c4baeaeb11679c0b6389cf6eba2da22372308f50730c2d99d3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Choudhury, Subikash</creatorcontrib><creatorcontrib>Dong, Xin</creatorcontrib><creatorcontrib>Drachenberg, Jim</creatorcontrib><creatorcontrib>Dunlop, James</creatorcontrib><creatorcontrib>Esumi, ShinIchi</creatorcontrib><creatorcontrib>Feng, Yicheng</creatorcontrib><creatorcontrib>Finch, Evan</creatorcontrib><creatorcontrib>Hu, Yu</creatorcontrib><creatorcontrib>Jia, Jiangyong</creatorcontrib><creatorcontrib>Lauret, Jerome</creatorcontrib><creatorcontrib>Li, Wei</creatorcontrib><creatorcontrib>Liao, Jinfeng</creatorcontrib><creatorcontrib>Lin, Yufu</creatorcontrib><creatorcontrib>Lisa, Mike</creatorcontrib><creatorcontrib>Niida, Takafumi</creatorcontrib><creatorcontrib>Ray, Robert Lanny</creatorcontrib><creatorcontrib>Sergeeva, Masha</creatorcontrib><creatorcontrib>Shen, Diyu</creatorcontrib><creatorcontrib>Shi, Shuzhe</creatorcontrib><creatorcontrib>Sorensen, Paul</creatorcontrib><creatorcontrib>Tang, Aihong</creatorcontrib><creatorcontrib>Tribedy, Prithwish</creatorcontrib><creatorcontrib>Van Buren, Gene</creatorcontrib><creatorcontrib>Voloshin, Sergei</creatorcontrib><creatorcontrib>Wang, Fuqiang</creatorcontrib><creatorcontrib>Wang, Gang</creatorcontrib><creatorcontrib>Xu, Haojie</creatorcontrib><creatorcontrib>Xu, Zhiwan</creatorcontrib><creatorcontrib>Yao, Nanxi</creatorcontrib><creatorcontrib>Zhao, Jie</creatorcontrib><title>Investigation of experimental observables in search of the chiral magnetic effect in heavy-ion collisions in the STAR experiment</title><title>Chinese physics C</title><description>The chiral magnetic effect (CME) is a novel transport phenomenon, arising from the interplay between quantum anomalies and strong magnetic fields in chiral systems. In high-energy nuclear collisions, the CME may survive the expansion of the quark-gluon plasma fireball and be detected in experiments. Over the past two decades, experimental searches for the CME have attracted extensive interest at the Relativistic Heavy Ion Collider (RHIC) and the Large Hadron Collider (LHC). The main goal of this study is to investigate three pertinent experimental approaches: the
correlator, the
R
correlator, and the signed balance functions. 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In high-energy nuclear collisions, the CME may survive the expansion of the quark-gluon plasma fireball and be detected in experiments. Over the past two decades, experimental searches for the CME have attracted extensive interest at the Relativistic Heavy Ion Collider (RHIC) and the Large Hadron Collider (LHC). The main goal of this study is to investigate three pertinent experimental approaches: the
correlator, the
R
correlator, and the signed balance functions. We exploit simple Monte Carlo simulations and a realistic event generator (EBE-AVFD) to verify the equivalence of the core components among these methods and to ascertain their sensitivities to the CME signal and the background contributions for the isobar collisions at the RHIC.</abstract><doi>10.1088/1674-1137/ac2a1f</doi><oa>free_for_read</oa></addata></record> |
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title | Investigation of experimental observables in search of the chiral magnetic effect in heavy-ion collisions in the STAR experiment |
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