STAR Flow, Chirality and Vorticity PWG

[webmaster AT star.bnl.gov]

Dear star-fcv-l AT lists.bnl.gov members,

Subhash Singha ( connectsubhash AT gmail.com ) has commented on a material  
originally submitted by Yicheng Feng ( feng216 AT purdue.edu ) at
https://drupal.star.bnl.gov/STAR/presentations/ICNFP-2024/Overview-STAR-measurements-flow-chirality-and-vorticity

Comment:
Dear Yicheng,

Nice slides. I am signing off and pushing it to star talks with a few minor  
suggestions:

s#6: flat scale --> scales or scales with y/y_beam ...
deviate --> deviate from scaling

Since we don't have model for higher energies here, I think we can remove  
"but higher → data to constraint model EOS".
I was wondering does the "baryon inhomogeneities" paper has any connection  
with this excess proton v1, if not we can remove it from the footer?

s#7: may be rephrased to something like gradual breaking of NCQ scaling

s#9: updates from BES-II




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