STAR Correlations and Fluctuations PWG

["Yu Zhang" <yuz AT ccnu.edu.cn>]

Dear Hanna,

Thank you very much for your comments. I've enriched the abstract and updated 

in the same link.

https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2023/Baryon-Strangeness-Correlations-3-GeV-AuAu-Collisions-RHIC-STAR-Fixe

Best regards,

Yu 

 

------------------ Original ------------------

From:  "star-cf-l AT lists.bnl.gov"<star-cf-l AT lists.bnl.gov>;

Date:  Wed, Apr 19, 2023 10:58 PM

To:  "star-cf-l AT lists.bnl.gov"<star-cf-l AT lists.bnl.gov>;

Subject:  Re: [Star-cf-l] STAR presentation by Yu Zhang for Quark Matter 2023 submitted for review

 

Dear Yu,

Please find below my comments to your nice abstract:

Title: in 3 GeV -> in \sqrt{s_{NN}} = 3 GeV

It will help if you extend description of physics motivation: nature of strongly interacting mater, etc..

You mention that B-S correlations can be sensitive to the signature of QGP phase.

However your abstract describes results from collision energy 3 GeV where we do not expect formation of QGP.

Please modify your physics motivation.

My general comment is that your abstract is very short and does nor explain too much.

I suggest to extend significantly.

Thanks,

Hanna

Hanna Paulina Zbroszczyk

PhD DSc Eng, Professor WUT

E-mail: hanna.zbroszczyk AT pw.edu.pl

Tel: +48 22 234 5851 (office)

Address:

Warsaw University of Technology

Faculty of Physics

Nuclear Physics Division

Koszykowa 75

Office: 117b (via 115)

00-662 Warsaw, Poland

Wiadomość napisana przez webmaster--- via Star-cf-l <star-cf-l AT lists.bnl.gov> w dniu 19.04.2023, o godz. 09:46:

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/63473

Deadline: 2023-05-01
---
If you have any problems with the review process, please contact  
webmaster AT www.star.bnl.gov
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