2013
DOI: 10.1016/j.nuclphysa.2013.01.069
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Search for Chiral Magnetic Effects in High-Energy Nuclear Collisions

Abstract: We present measurements of pion elliptic flow (v 2 ) in Au+Au collisions at √ s NN = 200, 62.4, 39, 27 and 19.6 GeV, as a function of event-by-event charge asymmetry (A ± ), based on data from the STAR experiment at RHIC. We find that π − (π + ) elliptic flow linearly increases (decreases) with charge asymmetry for most centrality bins and for all the beam energies under study. The slope parameter (r) from v 2 (A ± ) difference between π − and π + shows a centrality dependency similar to calculations of the … Show more

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Cited by 85 publications
(71 citation statements)
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“…On the other hand, including also a strong and long-lived magnetic field but neglecting the Lorentz force can lead to a splitting between the elliptic flows of negatively and positively charged particles. However, the slope parameter in the charge asymmetry dependence of the elliptic flow splitting is smaller than the experimental data, while the positive intercept at zero charge asymmetry is larger than the experimental value [31]. Unfortunately, as in our previous study including only the magnetic field [22], the inclusion of the Lorentz force cancells the chiral effects due to the magnetic and vorticity fields and leads instead to a negative slope parameter in the charge symmetry dependence of the elliptic flow splitting of negatively and positively charged particles, contrary to that observed in experiments.…”
Section: Discussioncontrasting
confidence: 57%
“…On the other hand, including also a strong and long-lived magnetic field but neglecting the Lorentz force can lead to a splitting between the elliptic flows of negatively and positively charged particles. However, the slope parameter in the charge asymmetry dependence of the elliptic flow splitting is smaller than the experimental data, while the positive intercept at zero charge asymmetry is larger than the experimental value [31]. Unfortunately, as in our previous study including only the magnetic field [22], the inclusion of the Lorentz force cancells the chiral effects due to the magnetic and vorticity fields and leads instead to a negative slope parameter in the charge symmetry dependence of the elliptic flow splitting of negatively and positively charged particles, contrary to that observed in experiments.…”
Section: Discussioncontrasting
confidence: 57%
“…for some p T selection and, more importantly, some η acceptance. Indeed, this observable has been proposed theoretically [4] and measured experimentally in Au-Au collisions at √ s NN = 200 GeV by the STAR collaboration [5]. However, one of the issues with this observable is that the slope of v n vs A is not independent of experimental effects (for example tracking efficiency) and therefore requires a correction factor.…”
Section: Methodology and Observablesmentioning
confidence: 98%
“…In the theoretical work on the CMW [22][23][24]28,29] as well as the analysis published by STAR [30] of Au-Au collisions at √ s NN = 200 GeV, the observable has been the charge-dependent flow coefficient v ± n as a function of the charge asymmetry A. Experimentally, the charge asymmetry defined in a specified kinematic region must be corrected for detector efficiency, as discussed in [30][31][32]. The effect of the correction is to increase the slope of positive or negative particle v ± n vs A.…”
Section: Analysis Methodologymentioning
confidence: 99%