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Titel:Search for the chiral magnetic wave using anisotropic flow of identified particles at energies available at the BNL Relativistic Heavy Ion Collider
Mitwirkende:Abdulhamid, Muhammad Ibrahim [VerfasserIn]   i
 Deppner, Ingo Martin [VerfasserIn]   i
 Leung, Yue [VerfasserIn]   i
 Söhngen, Yannick [VerfasserIn]   i
 Weidenkaff, Philipp [VerfasserIn]   i
Körperschaft:STAR Collaboration [VerfasserIn]   i
Verf.angabe:M.I. Abdulhamid, B.E. Aboona, J. Adam, J.R. Adams, G. Agakishiev, I. Aggarwal, M.M. Aggarwal, Z. Ahammed, A. Aitbaev, I. Alekseev, D.M. Anderson, A. Aparin, S. Aslam, J. Atchison, G.S. Averichev, V. Bairathi, W. Baker, J.G. Ball Cap, K. Barish, P. Bhagat, A. Bhasin, S. Bhatta, I.G. Bordyuzhin, J.D. Brandenburg, A.V. Brandin, X.Z. Cai, H. Caines, M. Calderón de la Barca Sánchez, D. Cebra, J. Ceska, I. Chakaberia, B.K. Chan, Z. Chang, A. Chatterjee, D. Chen, J. Chen, J.H. Chen, Z. Chen, J. Cheng, Y. Cheng, S. Choudhury, W. Christie, X. Chu, H.J. Crawford, G. Dale-Gau, A. Das, M. Daugherity, T.G. Dedovich, I.M. Deppner, A.A. Derevschikov, A. Dhamija, L. Di Carlo, L. Didenko, P. Dixit, X. Dong, J.L. Drachenberg, E. Duckworth, J.C. Dunlop, J. Engelage, G. Eppley, S. Esumi, O. Evdokimov, A. Ewigleben, O. Eyser, R. Fatemi, S. Fazio, C. J. Feng, Y. Feng, E. Finch, Y. Fisyak, F. A. Flor, C. Fu, F. Geurts, N. Ghimire, A. Gibson, K. Gopal, X. Gou, D. Grosnick, A. Gupta, A. Hamed, Y. Han, M.D. Harasty, J.W. Harris, H. Harrison-Smith, W. He, X.H. He, Y. He, C. Hu, Q. Hu, Y. Hu, H. Huang, H.Z. Huang, S.L. Huang, T. Huang, X. Huang, Y. Huang, Y. Huang, T.J. Humanic, D. Isenhower, M. Isshiki, W.W. Jacobs, A. Jalotra, C. Jena, Y. Ji, J. Jia, C. Jin, X. Ju, E.G. Judd, S. Kabana, M.L. Kabir, D. Kalinkin, K. Kang, D. Kapukchyan, D. Keane, A. Kechechyan, M. Kelsey, B. Kimelman, A. Kiselev, A. G. Knospe, H.S. Ko, L. Kochenda, A.A. Korobitsin, P. Kravtsov, L. Kumar, S. Kumar, R. Kunnawalkam Elayavalli, R. Lacey, J. M. Landgraf, A. Lebedev, R. Lednicky, J.H. Lee, Y.H. Leung, N. Lewis, C. Li, W. Li, X. Li, Y. Li, Y. Li, Z. Li, X. Liang, Y. Liang, T. Lin, C. Liu, F. Liu, G. Liu, H. Liu, H. Liu, L. Liu, T. Liu, X. Liu, Y. Liu, Z. Liu, T. Ljubicic, W.J. Llope, O. Lomicky, R.S. Longacre, E.M. Loyd, T. Lu, N. S. Lukow, X.F. Luo, V.B. Luong, L. Ma, R. Ma, Y.G. Ma, N. Magdy, D. Mallick, S. Margetis, H.S. Matis, J.A. Mazer, G. McNamara, K. Mi, N. G. Minaev, B. Mohanty, M.M. Mondal, I. Mooney, D.A. Morozov, A. Mudrokh, M.I. Nagy, A.S. Nain, J.D. Nam, M. Nasim, D. Neff, J.M. Nelson, D.B. Nemes, M. Nie, G. Nigmatkulov, T. Niida, R. Nishitani, L.V. Nogach, T. Nonaka, G. Odyniec, A. Ogawa, S. Oh, V.A. Okorokov, K. Okubo, B.S. Page, R. Pak, J. Pan, A. Pandav, A.K. Pandey, Y. Panebratsev, T. Pani, P. Parfenov, A. Paul, C. Perkins, B.R. Pokhrel, M. Posik, T. Protzman, N.K. Pruthi, J. Putschke, Z. Qin, H. Qiu, A. Quintero, C. Racz, S.K. Radhakrishnan, N. Raha, R.L. Ray, H.G. Ritter, C.W. Robertson, O.V. Rogachevsky, M.A. Rosales Aguilar, D. Roy, L. Ruan, A.K. Sahoo, N.R. Sahoo, H. Sako, S. Salur, E. Samigullin, S. Sato, W. B. Schmidke, N. Schmitz, J. Seger, R. Seto, P. Seyboth, N. Shah, E. Shahaliev, P.V. Shanmuganathan, T. Shao, M. Sharma, N. Sharma, R. Sharma, S.R. Sharma, A.I. Sheikh, D.Y. Shen, K. Shen, S.S. Shi, Y. Shi, Q.Y. Shou, F. Si, J. Singh, S. Singha, P. Sinha, M.J. Skoby, Y. Söhngen, Y. Song, B. Srivastava, T.D. S. Stanislaus, D.J. Stewart, M. Strikhanov, B. Stringfellow, Y. Su, C. Sun, X. Sun, Y. Sun, Y. Sun, B. Surrow, D.N. Svirida, Z.W. Sweger, A. Tamis, A.H. Tang, Z. Tang, A. Taranenko, T. Tarnowsky, J.H. Thomas, D. Tlusty, T. Todoroki, M.V. Tokarev, C.A. Tomkiel, S. Trentalange, R.E. Tribble, P. Tribedy, O.D. Tsai, C.Y. Tsang, Z. Tu, J. Tyler, T. Ullrich, D.G. Underwood, I. Upsal, G. Van Buren, A.N. Vasiliev, V. Verkest, F. Videbæk, S. Vokal, S.A. Voloshin, F. Wang, G. Wang, J.S. Wang, X. Wang, Y. Wang, Y. Wang, Y. Wang, Z. Wang, J.C. Webb, P.C. Weidenkaff, G.D. Westfall, H. Wieman, G. Wilks, S.W. Wissink, J. Wu, J. Wu, X. Wu, Y. Wu, B. Xi, Z. G. Xiao, G. Xie, W. Xie, H. Xu, N. Xu, Q. H. Xu, Y. Xu, Y. Xu, Z. Xu, Z. Xu, G. Yan, Z. Yan, C. Yang, Q. Yang, S. Yang, Y. Yang, Z. Ye, Z. Ye, L. Yi, K. Yip, Y. Yu, W. Zha, C. Zhang, D. Zhang, J. Zhang, S. Zhang, W. Zhang, X. Zhang, Y. Zhang, Y. Zhang, Y. Zhang, Z.J. Zhang, Z. Zhang, Z. Zhang, F. Zhao, J. Zhao, M. Zhao, C. Zhou, J. Zhou, S. Zhou, Y. Zhou, X. Zhu, M. Zurek, and M. Zyzak (STAR Collaboration)
E-Jahr:2023
Jahr:July 2023
Umfang:11 S.
Illustrationen:Illustrationen
Fussnoten:Gesehen am 17.04.2024
Titel Quelle:Enthalten in: Physical review
Ort Quelle:Woodbury, NY : Inst., 2016
Jahr Quelle:2023
Band/Heft Quelle:108(2023), 1 vom: Juli, Artikel-ID 014908, Seite 1-11
ISSN Quelle:2469-9993
Abstract:The chiral magnetic wave (CMW) has been theorized to propagate in the deconfined nuclear medium formed in high-energy heavy-ion collisions and to cause a difference in elliptic flow (v2) between negatively and positively charged hadrons. Experimental data consistent with the CMW have been reported by the STAR Collaboration at the Relativistic Heavy Ion Collider (RHIC), based on the charge asymmetry dependence of the pion v2 from Au+Au collisions at √sNN=27 to 200 GeV. In this comprehensive study, we present the STAR measurements of elliptic flow and triangular flow of charged pions, along with the v2 of charged kaons and protons, as a function of charge asymmetry in Au+Au collisions at √sNN=27, 39, 62.4, and 200 GeV. The slope parameters extracted from the linear dependence of the v2 difference on charge asymmetry for different particle species are reported and compared in different centrality intervals. In addition, the slopes of v2 for charged pions in small systems, i.e., p+Au and d+Au at √sNN=200 GeV, are also presented and compared with those in large systems, i.e., Au+Au at √sNN=200 GeV and U+U at 193 GeV. Our results provide new insights for the possible existence of the CMW and further constrain the background contributions in heavy-ion collisions at RHIC energies.
DOI:doi:10.1103/PhysRevC.108.014908
URL:Bitte beachten Sie: Dies ist ein Bibliographieeintrag. Ein Volltextzugriff für Mitglieder der Universität besteht hier nur, falls für die entsprechende Zeitschrift/den entsprechenden Sammelband ein Abonnement besteht oder es sich um einen OpenAccess-Titel handelt.

Volltext: https://doi.org/10.1103/PhysRevC.108.014908
 Volltext: https://link.aps.org/doi/10.1103/PhysRevC.108.014908
 DOI: https://doi.org/10.1103/PhysRevC.108.014908
Datenträger:Online-Ressource
Sprache:eng
K10plus-PPN:1886086230
Verknüpfungen:→ Zeitschrift

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