STAR Flow, Chirality and Vorticity PWG

[Chunjian Zhang <czhang.phys AT gmail.com>]

Dear Subhash,

Thank you for your insightful comments and helpful suggestions. 

I slightly revised the abstract with, 1)L4, adding "collective" , 2) L12, "the" -> "such", 3) L13, add "the",  4) removing "evolution".

It might be distracting to give many details since the conference is more diverse among the low-energy and high-energy experts.

All the best,

Chunjian 

On Tue, Nov 26, 2024 at 10:40 PM <webmaster AT star.bnl.gov> wrote:

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

Subhash Singha ( connectsubhash AT gmail.com ) has commented on a material 
originally submitted by ChunJian Zhang ( chunjianzhang AT fudan.edu.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/INPC-2025/Imaging-shapes-atomic-nuclei-high-energy-nuclear-collisions-STAR-experiment

Comment:
Dear Chunjian,

Very nice abstract. I sign off with two minor suggestions:
It might be good to mention the exact method used e.g. flow-momentum 
correlation or Pearson correlations etc around line#4
l#12: it is not clear what are you going to show in O+O,  is it the same 
flow-momentum correlations or v2/e2 comparison with different IC models, may 
be you can rephrase accordingly.


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