STAR Correlations and Fluctuations PWG

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

Dear Boyang,

Thanks for submitting your slides on time.

Please find here my comments to your nice presentation:

General remark: please consider adding an agenda / plan  of your talk,

Slide 1:

In 200 GeV -> in \sqrt{s_{NN}} = 200 GeV

With STAR Detector -> with the STAR Detector

Slide 2: I suggest mentioning what do you mean that the description of dense objects in astrophysics is not well understood (I assume you mean neutron star puzzle related to the mass of neutron stars, please add it to the motivation).

Add a reference(s) to some works done by HAL QCD Collaboration.

Shift a reference to the ALICE Nature paper below cited results.

As you discuss results from isobars and Au+Au collisions, I suggest to explain the motivation of their choice

Slide 3:

You can point at the figure r* and k*

I suggest adding that the wave function \Psi(r*, k*) describes correlations that are present due to interactions at the final states, including the strong one that you determine

Slide 5:

As you discuss Au+Au collisions as well, can you add them to the slide about PID too?

Slide 6:

I suggest to write „two-track effects” instead of Corrections.

Briefly explain what they mean (splitting and merging)

Slide 7:

I suggest to change „Corrections” to „additional effects"

Slide 9:

Please define used all symbols here

Slide 10:

Spin averaged method: assume two spin states are the same -> does not distinguish between spin states

Slide 13 (when you add UrQMD + HAL predictions), please add references to the models and more datails about configuration you used (to avoid questions what exactly is meant as UrQMD + HAL)

Slide 14: 

It will be good to mention which datasets you included in the linear fit (I assume that all, but please clarify).

Thanks,

Hanna

Prof. Hanna Zbroszczyk, PhD, DSc, Eng.

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 Nu Xu via Star-cf-l <star-cf-l AT lists.bnl.gov> w dniu 26.05.2024, o godz. 06:29:

Dear Boyang,

Thank you for the slides. Here are my comments:
slide 13 - 2nd bullet: I am not sure what do you want to state here. I suggest to remove it;

Thank you,

Nu

On May 25, 2024, at 2:49 AM, 付博洋 via Star-cf-l <star-cf-l AT lists.bnl.gov> wrote:

Dear Nu and Hanna,

This is a kindly reminder that I have submitted my sqm slide.

Please kindly have a look!

Any comments or suggestions are highly welcome!

Best regards,
Boyang
------------------ Original ------------------
From:  "STAR Correlations and Fluctuatio"<star-cf-l AT lists.bnl.gov>;
Date:  Mon, May 20, 2024 10:36 PM
To:  "STAR Correlations and Fluctuatio"<star-cf-l AT lists.bnl.gov>;
Cc:  "webmaster"<webmaster AT star.bnl.gov>;
Subject:  [Star-cf-l] STAR presentation by Boyang Fu for SQM-2024 submitted for review
Dear star-cf-l AT lists.bnl.gov members,

Boyang Fu (boyangfu AT mails.ccnu.edu.cn) has submitted a material for a review,  
please have a look:
https://drupal.star.bnl.gov/STAR/node/67909

Deadline: 2024-06-03
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If you have any problems with the review process, please contact  
webmaster AT www.star.bnl.gov
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