STAR Flow, Chirality and Vorticity PWG

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

Subhash Singha ( connectsubhash AT gmail.com ) has commented on a material  
originally submitted by Li-ke Liu ( likeliu AT mails.ccnu.edu.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/CPOD-2024/Collectivity-High-Baryon-Density-STAR-BES-II

Comment:
Dear Li-Ke,

Very nice and clean slides. I have a few additional questions/suggestions:

s#4: remove v1: and v2:Â  from the bullet. IMO, the bullets are valid for  
both vn'sBTW, by "constituent interaction" do you mean partonic/hadronic  
interactions?
s#6: "Hadronic dominates" --> can you re-word e.g. dominant hadronic  
interaction or hadronic interaction dominates
s#8: "Hundreds of millions events recorded at Au+Au 3.0 - 4.5 GeV" --> the  
line is redundant, you already have events listed in the table. You can  
probably mention e.g. FXT data provide good precision for collectivity  
measurement
s#13: is not need --> is not necessary
s#14: baryonic Mean FIeld
s#19: You mentioned 4.5 GeV is the onset of partonic collectivity, what  
happened to the ratios above 4.5, is it possible to include in the figure?

I sign off with these addressed.

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