STAR Correlations and Fluctuations PWG

[K.Mi <mike1996 AT mails.ccnu.edu.cn>]

Dear Hanna,

Thank you very much for the nice comments, please find the updated version in the same link:

https://drupal.star.bnl.gov/STAR/presentations/WPCF-2024/Recent-Results-Baryon-Correlations-RHIC-STAR-2

And also find the reply below.

Thank you.

Best regards,

Ke

2024年10月31日 20:54，Hanna Zbroszczyk (via star-cf-l Mailing List) <star-cf-l AT lists.bnl.gov> 写道：

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

Modified

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

Modified the sentence, and one more plot added

Slide 6:

k -> K (as for kaon)

Modified

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

Yes, it’s the first time to measure p-d and d-d CF at STAR.  LL formula is introduced in previous slide, so it’s not introduced here. And LL reference is listed.

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

Modified. 

Femtoscopy -> femtoscopy

Modified

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

LL formula is introduced in previous slide, so it’s not introduced here. 

S14: shift a bit the description of the slide as it partially covers the area of the figure

Modified

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

In this talk I aim to focus on the correlation involving light nuclei and involving pairs related to the Dibaryon. Also due to the time limitation, p-Lambda is not currently covered. I have one slide in the backup.

S15: Add reference to HAL included in these calculations

Added

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

Added

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

Added 

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)

I changed the HIC into STAR. 

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

Outlook added

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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