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star-fcv-l - Re: [[Star-fcv-l] ] STAR presentation by Yicheng Feng for ICNFP 2024 got commented by Subhash Singha

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: "Feng, Yicheng" <feng216 AT purdue.edu>
  • To: "star-fcv-l AT lists.bnl.gov" <star-fcv-l AT lists.bnl.gov>, subhash <subhash AT rcf.rhic.bnl.gov>
  • Subject: Re: [[Star-fcv-l] ] STAR presentation by Yicheng Feng for ICNFP 2024 got commented by Subhash Singha
  • Date: Wed, 21 Aug 2024 22:21:47 +0000

Hi Subhash, 

Thank you for your comments and sign-off. 
I have implemented all your comments and uploaded the new version to the same drupal node: 
https://drupal.star.bnl.gov/STAR/presentations/ICNFP-2024/Overview-STAR-measurements-flow-chirality-and-vorticity

Sincerely,
Yicheng

From: star-fcv-l-request AT lists.bnl.gov <star-fcv-l-request AT lists.bnl.gov> on behalf of webmaster AT star.bnl.gov <webmaster AT star.bnl.gov>
Sent: Wednesday, August 21, 2024 5:45 AM
To: star-fcv-l AT lists.bnl.gov <star-fcv-l AT lists.bnl.gov>
Subject: [[Star-fcv-l] ] STAR presentation by Yicheng Feng for ICNFP 2024 got commented by Subhash Singha
 
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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 Yicheng Feng ( feng216 AT purdue.edu ) at
https://nam04.safelinks.protection.outlook.com/?url="https%3A%2F%2Fdrupal.star.bnl.gov%2FSTAR%2Fpresentations%2FICNFP-2024%2FOverview-STAR-measurements-flow-chirality-and-vorticity&data=05%7C02%7Cfeng216%40purdue.edu%7Cb49a9c6bebab44c12e8a08dcc1c612ee%7C4130bd397c53419cb1e58758d6d63f21%7C0%7C0%7C638598303672801270%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C0%7C%7C%7C&sdata=KiWgiOgQty3pjdxzu5%2FXbi1MNxpp6qbUnOdzqmuhTsQ%3D&reserved=0

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 รข?' 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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