STAR Correlations and Fluctuations PWG

["付博洋" <boyangfu AT mails.ccnu.edu.cn>]

Dear Nu and Hanna,

Thank you very much for your comments!  We're implemented them in the updated version.

Please find the new version in the following link and reply in the below:

https://drupal.star.bnl.gov/STAR/node/67909

We would like to request a new preliminary plot for SQM which is shown in slide 16. The data points are already preliminary but we draw the plot in a new style. The link of this plot can be found via:

https://drupal.star.bnl.gov/STAR/system/files/f0_points.pdf

Please kindly let us know if you have any comments or suggestions! Thank you.

Best regards,

Boyang

 

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

From:  "STAR Correlations and Fluctuatio"<star-cf-l AT lists.bnl.gov>;

Date:  Mon, May 27, 2024 09:16 PM

To:  "STAR Correlations and Fluctuatio"<star-cf-l AT lists.bnl.gov>;

Cc:  "Hanna Paulina Zbroszczyk"<hanna.zbroszczyk AT pw.edu.pl>;

Subject:  Re: [Star-cf-l] STAR presentation by Boyang Fu for SQM-2024 submitted for review

 

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,

Outline added.

Slide 1:

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

With STAR Detector -> with the STAR Detector

Done

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).

We change the motivation a little bit by considering local comments. Now I just say that the correlation in pXi is important to study the Y-N interactions and explore the inner structure of the neutron star.

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

Done

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

Modified

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

We will explain this during the talk.

Slide 3:

You can point at the figure r* and k*

Done

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

Done

Slide 5:

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

Here we want to put an example to show the PID process. If adding AuAu's PID, this slide will be too crowded.

Slide 6:

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

Done

Briefly explain what they mean (splitting and merging)

I'll mention this during my talk.

Slide 7:

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

Done

Slide 9:

Please define used all symbols here

Done

Slide 10:

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

Done

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)

Done

Slide 14:

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

Done

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;
This sentence has been rephrase and here we want to show the enhancement of strong interaction from central to peripheral by comparing with the Coulomb.

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
---
If you have any problems with the review process, please contact  
webmaster AT www.star.bnl.gov
_______________________________________________
Star-cf-l mailing list
Star-cf-l AT lists.bnl.gov
https://lists.bnl.gov/mailman/listinfo/star-cf-l
_______________________________________________
Star-cf-l mailing list
Star-cf-l AT lists.bnl.gov
https://lists.bnl.gov/mailman/listinfo/star-cf-l

_______________________________________________
Star-cf-l mailing list
Star-cf-l AT lists.bnl.gov
https://lists.bnl.gov/mailman/listinfo/star-cf-l