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star-cf-l - Re: [Star-cf-l] STAR presentation by Yu Zhang for QPT 2023 submitted for review

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Subject: STAR Correlations and Fluctuations PWG

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  • From: "Yu Zhang" <yuz AT ccnu.edu.cn>
  • To: "STAR Correlations and Fluctuations PWG" <star-cf-l AT lists.bnl.gov>
  • Subject: Re: [Star-cf-l] STAR presentation by Yu Zhang for QPT 2023 submitted for review
  • Date: Fri, 15 Sep 2023 13:43:20 +0800

Dear Toshihiro,

Thank you very much for your detailed comments.
I've updated my abstract accordingly at the same link.
https://drupal.star.bnl.gov/STAR/node/65129

Best regards,
Yu 
 
------------------ Original ------------------
From:  "star-cf-l AT lists.bnl.gov"<star-cf-l AT lists.bnl.gov>;
Date:  Fri, Sep 15, 2023 01:07 PM
To:  "star-cf-l AT lists.bnl.gov"<star-cf-l AT lists.bnl.gov>;
Cc:  "Toshihiro Nonaka"<nonaka.toshihiro.ge AT u.tsukuba.ac.jp>;
Subject:  Re: [Star-cf-l] STAR presentation by Yu Zhang for QPT 2023 submitted for review
 
Dear Yu,

Please find some comments below on your nice abstract.

With these considered, I sign off.

Best regards,
Toshihiro

General:
Given that the conference title is "QCD phase transition (QPT)" and many of the audience could be familiar with this field, I wonder if the introduction part on the QCD phase diagram may not needed.
I would remove L1-L5 (... by various theories). But I do not have a strong feeling on this, so you could keep the current introduction if you think it is needed.

Title: Baryon-Strangeness Correlations...

L2-3: ... chemical potential, $\mu_B=0$~MeV, the transition between .... matter is a smooth crossover.

L10: proton cumulants

L12: could exist at higher collision energies.

L12-L13: of the QGP signal

L13: baryon-strangeness correlations

L14: , K^{\pm}, and hyperons. (add comma before "and", remove "included")
- Better to specify which hyperons are included in the measurement.

L14-L15: ... and have measured the ratio C_{BS} = <BS>_c/<S^2>_c, where <BS>_c represents the 2nd-order mix-cumulant
between net-baryon and net-strangeness while <S^2>_c is the 2nd-order net-strangeness cumulant.

L15-L16: In this talk, we present the centrality dependence of the C_BS ratio from \sqrt{s_{\rm NN}} = 3 and 200 GeV....
(you could add rapidity/pT acceptance or anything else depending on your plan for the analysis)

L17-L18: ... and discuss about the physics...



差出人: Star-cf-l <star-cf-l-bounces AT lists.bnl.gov> が webmaster--- via Star-cf-l <star-cf-l AT lists.bnl.gov> の代理で送信
送信日時: 2023年9月14日 15:31
宛先: star-cf-l AT lists.bnl.gov <star-cf-l AT lists.bnl.gov>
CC: webmaster AT star.bnl.gov <webmaster AT star.bnl.gov>
件名: [Star-cf-l] STAR presentation by Yu Zhang for QPT 2023 submitted for review
 
Dear star-cf-l AT lists.bnl.gov members,

Yu Zhang (yuz AT ccnu.edu.cn) has submitted a material for a review, please have 
a look:
https://drupal.star.bnl.gov/STAR/node/65129

Deadline: 2023-10-10
---
If you have any problems with the review process, please contact 
webmaster AT www.star.bnl.gov
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