STAR Correlations and Fluctuations PWG

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

Dear Ke,

Please find here my comments to you nice slides:

S2: at 3 GeV -> at \sqrt{s_{NN}} - 3 GeV; and the same comment for 200 GeV

S6: Please extend what you mean by the role of NN, YN and YY interaction in EoS of neutron stars, I guess you want to refer to the puzzling phenomena of the neutron star’s mass but add more details here

Slide 6:

k -> K (as for kaon)

Slide 8: I am not sure if p-d and d-d are measured by STAR for the first time. It is saver to mention at these energy domain or something similar

L-L formula and the reference to it would help here

S11: You mention here that for p-d interaction the results is consistent with theory calculation, however no overlap region is seen on the figure, please change wording the more accurate

Femtoscopy -> femtoscopy

S12: add L-L formula for d-\Lambda

S14: shift a bit the descriptio of the slide as it partially covers the are rea of the figure

Why don’t you discuss p-\Lambda results?

S15: Add reference to HAL included in these calculations

S17: Add physics conclusion from \Lambda-\Lambda studies

S18: it would help if you highlight from where you conclude about the possible existence of the bound state

 

S19: again, please change wording to the statetemt first determination of p-d and d-d interactions (e.g. HADES shows p-d as well)

Outlook for future will help to understand what are next perspectives related to this topic.

Kind regards,

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 webmaster AT star.bnl.gov w dniu 27.10.2024, o godz. 03:48:

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

Ke Mi (mike1996 AT mails.ccnu.edu.cn) has submitted a material for a review,  
please have a look:
https://drupal.star.bnl.gov/STAR/node/69693

Deadline: 2024-11-04
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