Search for the chiral magnetic effect in collisions between two isobars with deformed and neutron-rich nuclear structures
Xin-Li Zhao, Guo-Liang Ma

TL;DR
This study investigates the difficulty of detecting the chiral magnetic effect (CME) in isobar collisions due to background differences and final state interactions, highlighting the need for more sensitive observables.
Contribution
The paper demonstrates through modeling that current CME observables are insufficiently sensitive to weak CME signals in isobar collisions, emphasizing the importance of developing new detection methods.
Findings
Seven nuclear deformation cases match STAR reference ratios.
Final state interactions weaken CME signals significantly.
Current observables struggle to detect weak CME signals.
Abstract
Isobar collisions which were thought to have the same background and different magnetic fields provide an opportunity to verify the chiral magnetic effect (CME) in relativistic heavy-ion collisions. However, the first result from the RHIC-STAR isobar experiment did not observe the CME signal, but discovered that the backgrounds are different between and collisions. We test eighteen cases of Woods-Saxon parameter settings resulting from different nuclear deformation or nuclear structure effects using a mutiphase transport model. We find out that seven cases can reasonably reproduce three reference ratios measured by the STAR experiment. Considering both the halo-type neutron skin structure and CME-like charge separation, we demonstrate that it is difficult for the CME observables (,…
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