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Subject: STAR Flow, Chirality and Vorticity PWG
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Re:[[Star-fcv-l] ] STAR presentation got a comment
- 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:
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.
---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
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.
---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
- Re:[[Star-fcv-l] ] STAR presentation got a comment, wzlk AT mails.ccnu.edu.cn, 11/12/2024
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