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star-fcv-l - Re:[[Star-fcv-l] ] STAR presentation got a comment

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: "wzlk AT mails.ccnu.edu.cn" <wzlk AT mails.ccnu.edu.cn>
  • To: "webmaster" <webmaster AT star.bnl.gov>, "star-fcv-l" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re:[[Star-fcv-l] ] STAR presentation got a comment
  • Date: Wed, 13 Nov 2024 09:34:01 +0800

Dear Subhash,

Thanks for your nice comments.

I have taken your advice, revised the title and made changes to the abstract.

The latest abstract is linked below:

https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2025/Beam-Energy-Dependence-Baryon-v1-Au-Au-Collision-RHIC-STAR

Best regards,

Zhuo Wang
 
 
------------------ Original ------------------
From:  "webmaster"<webmaster AT star.bnl.gov>;
Date:  Tue, Nov 12, 2024 09:49 PM
To:  "王卓"<wzlk AT mails.ccnu.edu.cn>;
Subject:  STAR presentation got a comment
 
Dear Zhuo Wang,

Subhash Singha (connectsubhash AT gmail.com) has commented on your submission:

https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2025/Beam-Energy-Dependence-Baryon-v1-Au-Au-Collision-RHIC-STAR

Comments:
Dear Zhuo,

I have a few more suggestions:

Title: Beam Energy Dependence of Baryon Directed Flow (v?6?9) 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 , ?0?4p , Λ and 
Λ?0?4 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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  • Re:[[Star-fcv-l] ] STAR presentation got a comment, wzlk AT mails.ccnu.edu.cn, 11/12/2024

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