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Subject: STAR Flow, Chirality and Vorticity PWG
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Re: [Star-fcv-l] STAR presentation by Junyi Han for SQM-2024 got commented by Subhash Singha
- 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.
---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
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Star-fcv-l mailing list
Star-fcv-l AT lists.bnl.gov
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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.
---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
_______________________________________________
Star-fcv-l mailing list
Star-fcv-l AT lists.bnl.gov
https://lists.bnl.gov/mailman/listinfo/star-fcv-l
-
[Star-fcv-l] STAR presentation by Junyi Han for SQM-2024 got commented by Subhash Singha,
webmaster, 05/22/2024
- Re: [Star-fcv-l] STAR presentation by Junyi Han for SQM-2024 got commented by Subhash Singha, Junyi Han, 05/23/2024
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