STAR Correlations and Fluctuations PWG

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

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
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