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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Junyi Han for SQM-2024 got commented by Subhash Singha

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: "Junyi Han" <jyhan AT mails.ccnu.edu.cn>
  • To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>, "subhash" <subhash AT rcf.rhic.bnl.gov>
  • Cc: "webmaster" <webmaster AT star.bnl.gov>
  • Subject: Re: [Star-fcv-l] STAR presentation by Junyi Han for SQM-2024 got commented by Subhash Singha
  • Date: Thu, 23 May 2024 15:07:34 +0200

Dear Subhash,

Thanks for your nice comments! I have update my slides based on your suggestions: https://drupal.star.bnl.gov/STAR/system/files/SQM2024_Junyi_v3.pdf

Best regards,
Junyi 
 
------------------ Original ------------------
From:  "STAR Flow, Chirality and Vortici"<star-fcv-l AT lists.bnl.gov>;
Date:  Thu, May 23, 2024 03:51 AM
To:  "STAR Flow, Chirality and Vortici"<star-fcv-l AT lists.bnl.gov>;
Cc:  "webmaster"<webmaster AT star.bnl.gov>;
Subject:  [Star-fcv-l] STAR presentation by Junyi Han for SQM-2024 got commented by Subhash Singha
 
Dear star-fcv-l AT lists.bnl.gov members,

Subhash Singha ( connectsubhash AT gmail.com ) has commented on a material 
originally submitted by Junyi Han ( jyhan AT mails.ccnu.edu.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/SQM-2024/Directed-Flow-Hyper-Nuclei-High-Baryon-Density-STAR

Comment:
Hi Junyi,
Nice slides. I have a few comments for your consideration:
s#1: we usually have a DOE support logo in all STAR talks.
s#3: "difficulty to reconcile" --> difficult to reconcile
s#4: "helps to explore" --> help explore
s#5: considered as a sensitive
s#8: Events --> Analyzed events (?)I think it is the number of good/accepted 
events, right? You can consider adding a reference of flow method paper
s#12: You may write the right bottom blue equation math form like you have in 
the left
s#13: Is the v1 fitting range same for all particles, it might be good to 
indicate.
You do not have "p0" in the linear equations inside the table, pls correct it
s#16: I suggest "high baryon density in STAR" --> for sNN = X.X - X.X GeV in 
STAR (at high baryon density)
You can remove "in 3.0 – 4.5 GeV collisions" in the 2nd bullet

I sign-off with these being addressed.

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