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Re: [[Star-fcv-l] ] STAR presentation by Xing Wu for Quark Matter 2025 got commented by Subhash Singha
- From: "Xing Wu" <wuxing6218 AT mails.ccnu.edu.cn>
- To: "star-fcv-l" <star-fcv-l AT lists.bnl.gov>
- Subject: Re: [[Star-fcv-l] ] STAR presentation by Xing Wu for Quark Matter 2025 got commented by Subhash Singha
- Date: Wed, 30 Oct 2024 22:07:18 +0800
Dear Subhash,
Thank you for your suggestion. I have updated my abstract. Please find in the below link.
Thanks,
Xing
------------------ Original ------------------
From: "webmaster"<webmaster AT star.bnl.gov>;
Date: Wed, Oct 30, 2024 05:20 PM
To: "star-fcv-l"<star-fcv-l AT lists.bnl.gov>;
Subject: [[Star-fcv-l] ] STAR presentation by Xing Wu for Quark Matter 2025 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 Xing Wu ( wuxing6218 AT mails.ccnu.edu.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2025/Probing-QCD-phase-structure-elliptic-flow-Au-Au-collisions-%E2%88%9A-sNN-77-
Comment:
Dear Xing,
Nice poster. I have following suggestions:
"second phase of RHIC beam energy scan two" --> second phase of RHIC Beam
Energy Scan (BES-II)
Suggest the last sentence: "partonic degrees of freedom when √sNN ≥ 3.9
GeV" --> "partonic degrees of freedom when √sNN ≥ 7.7 GeV." because I
presume you are not showing results below 7.7 GeV in your poster.
---
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 a material
originally submitted by Xing Wu ( wuxing6218 AT mails.ccnu.edu.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2025/Probing-QCD-phase-structure-elliptic-flow-Au-Au-collisions-%E2%88%9A-sNN-77-
Comment:
Dear Xing,
Nice poster. I have following suggestions:
"second phase of RHIC beam energy scan two" --> second phase of RHIC Beam
Energy Scan (BES-II)
Suggest the last sentence: "partonic degrees of freedom when √sNN ≥ 3.9
GeV" --> "partonic degrees of freedom when √sNN ≥ 7.7 GeV." because I
presume you are not showing results below 7.7 GeV in your poster.
---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
-
[[Star-fcv-l] ] STAR presentation by Xing Wu for Quark Matter 2025 got commented by Subhash Singha,
webmaster, 10/30/2024
- Re: [[Star-fcv-l] ] STAR presentation by Xing Wu for Quark Matter 2025 got commented by Subhash Singha, Xing Wu, 10/30/2024
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