30 August 2022 to 12 September 2022
Conference venue: OAC conference center, Kolymbari, Crete, Greece. The conference will take place in Crete in physical form, however participation is also possible via internet
Europe/Athens timezone
"Second MODE Workshop on Differentiable Programming for Experiment Design" following after ICNFP2022 (https://indico.cern.ch/event/1145124/)

Search for the Chiral Magnetic Effect by the STAR Experiment

31 Aug 2022, 12:40
20m
Room 1

Room 1

Speaker

Prof. Gang Wang (UCLA)

Description

The quark-gluon plasma created in high-energy heavy-ion collisions has been conjectured to exhibit a spontaneous electric-charge separation in the direction of a strong magnetic field through the chiral magnetic effect (CME). The experimental confirmation of the CME in heavy-ion collisions will uncover fundamental aspects of strong interaction physics such as the QCD chiral symmetry restoration and the topological configurations of non-Abelian gauge fields. Over the past decade, the STAR experiment has performed a series of charge-separation measurements in Au+Au collisions at various beam energies from $\sqrt{s_{\rm NN}} =$ 200 GeV down to 7.7 GeV, and in different collision systems including p+Au, d+Au, Cu+Cu, Au+Au and U+U collisions, as well as the recent isobaric Ru+Ru and Zr+Zr collisions. Multiple analysis methods have also been developed to manifest the charge separation effect and suppress the flow related background. In this talk, we will review the aforementioned results, summarize our current understanding, and provide an outlook on future analyses.

Details

The STAR Collaboration was invited to present this topic, and I (Gang Wang) was selected by the STAR talk committee to give this talk.

Is this abstract from experiment? Yes
Name of experiment and experimental site STAR
Is the speaker for that presentation defined? Yes
Internet talk Maybe

Author

Prof. Gang Wang (UCLA)

Presentation materials