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star-cf-l - Re: [Star-cf-l] STAR presentation by Jing An for NUCLEUS-2023 submitted for review

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Subject: STAR Correlations and Fluctuations PWG

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  • From: Yingjie Zhou <yingjiezhou AT mails.ccnu.edu.cn>
  • To: Hanna Paulina Zbroszczyk <hanna.zbroszczyk AT pw.edu.pl>, STAR Correlations and Fluctuations PWG <star-cf-l AT lists.bnl.gov>
  • Subject: Re: [Star-cf-l] STAR presentation by Jing An for NUCLEUS-2023 submitted for review
  • Date: Sat, 22 Apr 2023 09:53:24 +0200

Dear Hanna,

Thank you very much for your nice comments. We have implemented them in the updated version.


You may notice the subject of the email is the STAR presentation for NUCLEUS-2023. This is because we made a mistake and chose the wrong meeting at the beginning. The poster abstract is actually for Quark Matter 2023. We have corrected it on the Drupal page. I would like to apologize for any confusion this may have caused.

Best regards,
Yingjie 


On 19. Apr 2023, at 16:49, Hanna Paulina Zbroszczyk via Star-cf-l <star-cf-l AT lists.bnl.gov> wrote:

Dear Jing and Yingjie,

Please find below my comments to your nice abstract:

Line 4-7: here you have 2 statements:
  1. For example, from the p-Λ and p-Ξ− correlation functions, one could study

  2. 5. the hyperon-nucleon (Y-N) interactions in such collisions. It is particularly interesting

  3. 6  to study the dependence on the collision energy because freeze-out condition depends

  4. 7  on energy.


    Move the second statement to the next line as it looks freeze-out conditions (source sizes, I assume) are directly connected to the FSI mentioned in the previous statements, why they are two different pieces of information.


    Line 6: the dependence on the collision energy- >the dependence on the collision energy of the parameters describing source parameters at the moment of freeze-out. 


    Line 8: change to 3.0 to 7.7 GeV


    Linę 9: proton-\Lambda -> p-\Lambda; proton-\Xî^{-}  ->  p-\Xî^{-}


    Linę 10: at 3.2 -> at \sqrt{s_{NN}} = 3.2


    Linę 11: from 3 GeV -> from \sqrt{s_{NN}} =. 3 GeV


    Linę 13: add what kind of mode; calculation your mean.


    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. 08:53:

Dear star-cf-l AT lists.bnl.gov members,

Jing An (anjing19980215 AT mails.ccnu.edu.cn) has submitted a material for a  
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/63470

Deadline: 2023-10-09
---
If you have any problems with the review process, please contact  
webmaster AT www.star.bnl.gov
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