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Re: [[Star-cf-l] ] STAR presentation by Ke Mi for WPCF 2024 submitted for review

From: Nu Xu <nxu AT lbl.gov>
To: STAR Correlations and Fluctuations PWG <star-cf-l AT lists.bnl.gov>
Cc: Nu Xu <nxu AT lbl.gov>
Subject: Re: [[Star-cf-l] ] STAR presentation by Ke Mi for WPCF 2024 submitted for review
Date: Thu, 31 Oct 2024 07:38:31 -0700

Hi All,

I am sorry that I was dropped off from the network at the end of the meeting.
Here is the list we discussed today:


CF PWG: STAR BES-II workshop talks:
I Public:
(1) Correlations from 200 GeV Isobar Collisions:
Kehao (2) Correlations from 200 GeV Isobar
Collisions: Ke/Boyang
(3) Correlations from 3 GeV AuAu Collisions (2018): Chuan/Qin/Yinjie
(4) 3rd-body Coulomb Corrected Pion HBT from FXT Collisions:
Vinh
(5) pT-pT Correlations from 3.0, 3.2 GeV AuAu Collisions:
Rutik
(6) Net-proton Hyper Moments C5 and C6 from BES-II 7.7 – 27 GeV AuAu
Collisions: Bappa
(7) Rapidity and pT Scan of Net-proton High Moments BES-II 7.7 – 27 GeV AuAu
Collisions: Yige
(8) Energy Dependence of the Strangeness-Baryon Correlation (BSC) from
BES-II: Hanwen
(9) Pion HBT with Levy Funciotn ??????
II Closed:
(1) FXT proton high moments: “Rapidity Scan of the Proton High Moments Ratios
C4/C2 from 3.2 GeV Au+Au Collisions”, Xin Zhang
(2) FXT proton high moments: “Energy Dependence of Mid-Rapidity Dependence of
Proton High Moments from 3.2, 3.5, 3.9 GeV AuAu Collisions”, Zach

> On Oct 31, 2024, at 7:14 AM, Rutik Manikandhan
> <manikandhan.rutik AT gmail.com> wrote:
>
> Hello Conveners,
>
> Please add me for the agenda next week,
> I’d like to give an update on “Energy dependence of pT-pT correlations”
>
> Best,
> Rutik Manikandhan
> PhD Candidate, Experimental Nuclear High Energy Group
> Physics Dept.
> University of Houston
>
>
> On Thu, Oct 31, 2024 at 8:06 AM Hanna Zbroszczyk <star-cf-l AT lists.bnl.gov>
> wrote:
> https://urldefense.com/v3/__https://cern.zoom.us/j/67357482915?pwd=NTEzV0lJc2o1UDRoMVMzQnk0YTBxUT09__;!!P4SdNyxKAPE!GrZG6gn3h72bPzi24BiBaTD25N8x4e3Saa87oiRNkWm_zAaJgNntPcNaxQ0qKm3LUIwbd6TJSwKsln3VVd8$
>
>
> prof. dr hab. inż. Hanna Zbroszczyk
> E-mail: hanna.zbroszczyk AT pw.edu.pl
> Tel: +48 22 234 5851 (biuro)
>
> Adres:
> Poltechnika Warszawska
> Wydział Fizyki
> Zakład Fizyki Jądrowej
> ul. Koszykowa 75
> Biuro: 117b (via 115)
> 00-662 Warszawa
>
>
>
>
>> Wiadomość napisana przez Nu Xu <nxu AT lbl.gov> w dniu 31.10.2024, o godz.
>> 14:04:
>>
>>
>> Hi all,
>>
>> Can someone send me the zoom link?
>>
>> Thank you,
>> Nu
>> Sent from my iPhone
>>
>> On Oct 31, 2024, at 8:54 PM, Hanna Zbroszczyk <star-cf-l AT lists.bnl.gov>
>> wrote:
>>
>> 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
>>> ---
>>> If you have any problems with the review process, please contact
>>> webmaster AT www.star.bnl.gov
>>>
>>
>

[[Star-cf-l] ] STAR presentation by Ke Mi for WPCF 2024 submitted for review, webmaster, 10/26/2024
- Re: [[Star-cf-l] ] STAR presentation by Ke Mi for WPCF 2024 submitted for review, Hanna Zbroszczyk, 10/31/2024
  - Re: [[Star-cf-l] ] STAR presentation by Ke Mi for WPCF 2024 submitted for review, Nu Xu, 10/31/2024
    - Re: [[Star-cf-l] ] STAR presentation by Ke Mi for WPCF 2024 submitted for review, Hanna Zbroszczyk, 10/31/2024
      - Re: [[Star-cf-l] ] STAR presentation by Ke Mi for WPCF 2024 submitted for review, Rutik Manikandhan, 10/31/2024
        
        Re: [[Star-cf-l] ] STAR presentation by Ke Mi for WPCF 2024 submitted for review, Nu Xu, 10/31/2024
        
        Re: [[Star-cf-l] ] STAR presentation by Ke Mi for WPCF 2024 submitted for review, Hanna Zbroszczyk, 10/31/2024
        
        Re: [[Star-cf-l] ] STAR presentation by Ke Mi for WPCF 2024 submitted for review, Mate Csanad, 10/31/2024
        
        Re: [[Star-cf-l] ] STAR presentation by Ke Mi for WPCF 2024 submitted for review, Nu Xu, 10/31/2024
        
        Re: [[Star-cf-l] ] STAR presentation by Ke Mi for WPCF 2024 submitted for review, Csanad Mate, 10/31/2024