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Space-average electromagnetic fields and electromagnetic anomaly weighted by energy density in heavy-ion collisions
被引:13
|作者:
Siddique, Irfan
[1
]
Sheng, Xin-Li
[2
,3
]
Wang, Qun
[4
,5
,6
]
机构:
[1] Shandong Univ, Inst Frontier & Interdisciplinary Sci, Key Lab Particle Phys & Particle Irradiat MOE, Qingdao 266237, Shandong, Peoples R China
[2] Cent China Normal Univ, Key Lab Quark & Lepton Phys MOE, Wuhan 430079, Hubei, Peoples R China
[3] Cent China Normal Univ, Inst Particle Phys, Wuhan 430079, Hubei, Peoples R China
[4] Univ Sci & Technol China, Interdisciplinary Ctr Theoret Study, Hefei 230026, Peoples R China
[5] Univ Sci & Technol China, Dept Modern Phys, Hefei 230026, Peoples R China
[6] Peng Huanwu Ctr Fundamental Theory, Hefei 230026, Anhui, Peoples R China
基金:
中国国家自然科学基金;
关键词:
MAGNETIC-FIELD;
EVENT;
FLOW;
OBSERVABLES;
D O I:
10.1103/PhysRevC.104.034907
中图分类号:
O57 [原子核物理学、高能物理学];
学科分类号:
070202 ;
摘要:
We study the space-averaged electromagnetic (EM) fields weighted by the energy density in the central regions of heavy-ion collisions. These average quantities can serve as a barometer for the magnetic-field induced effects such as the magnetic effect, the chiral separation effect and the chiral magnetic wave. Comparing with the magnetic fields at the geometric center of the collision, the space-averaged fields weighted by the energy density are smaller in the early stage but damp slower in the later stage. The space average of squared fields as well as the EM anomaly E . B weighted by the energy density are also calculated. We give parametrized analytical formulas for these average quantities as functions of time by fitting numerical results for collisions in the collision energy range 7.7-200 GeV with different impact parameters.
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页数:11
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