Importance of non-flow background on the chiral magnetic wave search
arXiv:2002.05220 · doi:10.1016/j.nuclphysa.2020.121770
Abstract
An observable sensitive to the chiral magnetic wave (CMW) is the charge asymmetry dependence of the and anisotropic flow difference, . We show that, due to non-flow correlations, the flow measurements by the Q-cumulant method using all charged particles as reference introduce a trivial linear term to . The trivial slope contribution to the triangle flow difference can be negative if the non-flow is dominated by back-to-back pairs. This can explain the observed negative slope in the preliminary STAR data. We further find that the non-flow correlations give rise to additional backgrounds to the slope of from the competition among different pion sources and from the larger multiplicity dilution to () at positive (negative) .
arXiv comment4 pages, 2 figures, contribution to the proceedings of the 28th international conference on ultrarelativistic nucleus-nucleus collisions (Quark Matter 2019)
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- Chiral Magnetic Effect in Heavy Ion Collisions: The Present and Future
- Anomalous magnetohydrodynamics with temperature-dependent electric conductivity and application to the global polarization
- Global constraint on the magnitude of anomalous chiral effects in heavy-ion collisions
- Interpreting the charge-dependent flow and constraining the chiral magnetic wave with event shape engineering
- Charge-dependent transverse momentum and its impact on the search for the chiral magnetic wave
- Search for the chiral magnetic wave using anisotropic flow of identified particles at RHIC
- Probing the Chiral Magnetic Wave with charge-dependent flow measurements in Pb-Pb collisions at the LHC