STAR Correlations and Fluctuations PWG

[Hanna Paulina Zbroszczyk <hanna.zbroszczyk AT pw.edu.pl>]

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
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