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 Xing Wu ( wuxing6218 AT mails.ccnu.edu.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/Hot-Quarks-2025/Anisotropic-Flow-Identified-Particles-AuAu-Collisions-sqrtsNN-30-45--0

Comment:
Dear Xing, Nice abstract. I sign off with a few suggestions for your  
consideration:

l#9 and in title: please spell out beam energies between 3.0 - 4.5 GeV
l#10: spell out NCQ
l#14: "The anti-flow of K0S measured by STAR is a factor of eight lower ... " 
 
--> It is not clear what do you mean? Is it v1 or v2? Why a factor of eight  
lower at similar energies?


---
If you have any problems with the review process, please contact  
webmaster AT www.star.bnl.gov