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 Zhuo Wang ( wzlk AT mails.ccnu.edu.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2025/Beam-Energy-Dependence-Baryon-v1-Au-Au-Collision-RHIC-STAR

Comment:
Dear Zhuo,

I have a few more suggestions:

Title: Beam Energy Dependence of Baryon Directed Flow (v₁) in Au+Au  
Collisions at RHIC-STAR

l#3-5: The first harmonic coefficient in the Fourier expansion of the  
final-state azimuthal anisotropy, relative to the reaction plane, is referred 
 
to as directed flow, v_1.

l#7-9: The v_1 slope with respect to the rapidity for net-baryons from the  
first phase of Beam Energy Scan (BES-I) exhibits a minimum around 10-20 GeV,  
a feature predicted to be sensitive to the softening of the equation of state 
 
near a first-order phase transition. [Move this line to the first paragraph]

Then in second para:
In this poster, we will present the rapidity dependence of p , ¯p , Λ and  
Λ¯ 6 v1 in Au+ Au collisions at √sNN = 7.7, 9.2, 11.5, 14.5, 17.3, and  
19.6 GeV using the high statistics data from the Beam Energy Scan Phase II  
(BES-II).

remove "The results from BES-II, with improved statistics, can help deepen  
our understanding of existing physical phenomena and potentially uncover new  
ones"

Then add: "We will compare our measurements with transport model calculations 
 
and discuss the implications for the QCD phase transition."

I sign off with these addressed.

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