Blind analysis of isobar data and search for the Chiral Magnetic Effect by the STAR collaboration

Date: 
10/14/2021 - 2:00pm to 3:00pm
Location: 
Virtual/Zoom
Speaker(s) / Presenter(s): 
Prithwish Tribedy (Brookhaven National Laboratory)
Type of Event (for grouping events):

Relativistic heavy ion collisions (HICs) at the modern accelerators like the Relativistic Heavy Ion Collider and the Large Hadron Collider provide unique testing ground for the Quantum Chromodynamics (QCD) at high energies. The early stages of such collisions generate highest densities allowed by QCD and eventually leads to the formation of a liquid-like quark-gluon matter that filled the microsecond-old universe. Interestingly, the early stages of HICs also generate the strongest known electromagnetic fields (10^18 Gauss) in the universe. The quantum fluctuations in the early stages of such collisions amidst such strong fields can lead to violation of local P and CP symmetries of strong interaction. As a consequence of such extreme conditions one expects to observe novel phenomena such as the Chiral Magnetic Effect (CME). Previous measurements of the CME remain inconclusive because of large background contributions. In order to better control the influence of signal and backgrounds, the STAR collaboration has recently performed a blind analysis on a large data sample of approximately 3.8 billion isobar Ru+Ru and Zr+Zr collisions at √sNN=200 GeV at the Relativistic Heavy Ion Collider. In this seminar I will discuss the findings and conclusions from the isobar blind analysis. 

 

Meeting Recording:
 
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