Measurements of the chiral magnetic effect with background isolation in 200 GeV Au+Au collisions at STAR
Abstract
Using two novel methods, pair invariant mass (minv) and comparative measurements with respect to reaction plane (ΨRP) and participant plane (ΨPP), we isolate the possible chiral magnetic effect (CME) from backgrounds in 200 GeV Au+Au collisions at STAR. The invariant mass method identifies the resonance background contributions, coupled with the elliptic flow (ν2), to the charge correlator CME observable (Δγ). At high mass (minv > 1.5 GeV/c2) where resonance contribution is small, we obtain the average Δγ magnitude. In the low mass region (minv > 1.5 GeV/c2), resonance peaks are observed in Δγ(minv). An event shape engineering (ESE) method is used to model the background shape in minv to extract the potential CME signal at low minv. In the comparative method, the ΨRP is assessed by spectator neutrons measured by the ZDCs, and the ΨPP by the 2nd-harmonic event plane measured by the TPC. The ν2 is stronger along ΨPP and weaker along ΨRP; in contrast, the magnetic field, mainly from spectator protons, is weaker along ΨPP and stronger along ΨRP. As a result, the Δγ measured with respect to ΨRP and ΨPP contain different amounts of CME and background, and can thus determine these two contributions. It is foundmore »
- Authors:
-
- Purdue Univ., West Lafayette, IN (United States)
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Nuclear Physics (NP)
- Contributing Org.:
- STAR Collaboration
- OSTI Identifier:
- 1580374
- Grant/Contract Number:
- AC02-05CH11231; SC0012910
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Nuclear Physics. A
- Additional Journal Information:
- Journal Volume: 982; Journal Issue: C; Journal ID: ISSN 0375-9474
- Publisher:
- Elsevier
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 73 NUCLEAR PHYSICS AND RADIATION PHYSICS; QCD; heavy-ion collisions; chiral magnetic effect; invariant mass; reaction plane; participant plane
Citation Formats
Zhao, Jie. Measurements of the chiral magnetic effect with background isolation in 200 GeV Au+Au collisions at STAR. United States: N. p., 2019.
Web. doi:10.1016/j.nuclphysa.2018.08.035.
Zhao, Jie. Measurements of the chiral magnetic effect with background isolation in 200 GeV Au+Au collisions at STAR. United States. https://doi.org/10.1016/j.nuclphysa.2018.08.035
Zhao, Jie. Tue .
"Measurements of the chiral magnetic effect with background isolation in 200 GeV Au+Au collisions at STAR". United States. https://doi.org/10.1016/j.nuclphysa.2018.08.035. https://www.osti.gov/servlets/purl/1580374.
@article{osti_1580374,
title = {Measurements of the chiral magnetic effect with background isolation in 200 GeV Au+Au collisions at STAR},
author = {Zhao, Jie},
abstractNote = {Using two novel methods, pair invariant mass (minv) and comparative measurements with respect to reaction plane (ΨRP) and participant plane (ΨPP), we isolate the possible chiral magnetic effect (CME) from backgrounds in 200 GeV Au+Au collisions at STAR. The invariant mass method identifies the resonance background contributions, coupled with the elliptic flow (ν2), to the charge correlator CME observable (Δγ). At high mass (minv > 1.5 GeV/c2) where resonance contribution is small, we obtain the average Δγ magnitude. In the low mass region (minv > 1.5 GeV/c2), resonance peaks are observed in Δγ(minv). An event shape engineering (ESE) method is used to model the background shape in minv to extract the potential CME signal at low minv. In the comparative method, the ΨRP is assessed by spectator neutrons measured by the ZDCs, and the ΨPP by the 2nd-harmonic event plane measured by the TPC. The ν2 is stronger along ΨPP and weaker along ΨRP; in contrast, the magnetic field, mainly from spectator protons, is weaker along ΨPP and stronger along ΨRP. As a result, the Δγ measured with respect to ΨRP and ΨPP contain different amounts of CME and background, and can thus determine these two contributions. It is found that the possible CME signals with background isolation by these two novel methods are small, on the order of a few percent of the inclusive Δγ measurements.},
doi = {10.1016/j.nuclphysa.2018.08.035},
journal = {Nuclear Physics. A},
number = C,
volume = 982,
place = {United States},
year = {Tue Jan 22 00:00:00 EST 2019},
month = {Tue Jan 22 00:00:00 EST 2019}
}
Web of Science
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Works referencing / citing this record:
Back-to-back relative-excess observable to identify the chiral magnetic effect
journal, January 2020
- Feng, Yicheng; Zhao, Jie; Wang, Fuqiang
- Physical Review C, Vol. 101, Issue 1