STAR Correlations and Fluctuations PWG

[Nu Xu <nxu AT lbl.gov>]

Hi Ke and All,

Thank you for the updated proceedings. 

I have the following suggestions for consideration:
1) Remove Fig. 2 where p-p and p-Xi- correlation functions are shown. This is 
because these results are obsolete and new results (cannot show here) will 
replace them in the paper publication;

2) We should add some PID information to demonstrate the quality of the 
analysis, especially for the new results for p-d and d-d correlation 
functions.

Hope this is helpful. 

Nu 


> On Jul 25, 2022, at 2:55 AM, Ke Mi via Star-cf-l <star-cf-l AT lists.bnl.gov> 
> wrote:
> 
> Dear Convenors,
> 
> Please find the revise draft through this link:
> https://drupal.star.bnl.gov/STAR/system/files/QM2022_Proceeding_KeMi_v3.pdf
> In this draft, we try to include all results presented at QM2022.
> 
> Your further comments and suggestions are welcome.
> Thank you.
> 
> Best regards,
> Ke
> 
>> On 25. Jul 2022, at 00:09, Hanna Paulina Zbroszczyk 
>> <hanna.zbroszczyk AT pw.edu.pl> wrote:
>> 
>> Dear Ke,
>> 
>> Meantime, please find my comments to your proceedings. Keep in mind I have 
>> commented on the version that is current now. When you will work on new 
>> draft, please include my comments regarding p-d and d-d system. Having new 
>> draft, I will comment more.
>> 
>> Line 1: this proceedings -> these proceedings
>> 
>> Linę 12: it would be nice to just mention which scenarios you consider: 
>> thermal production and / or coalescence
>> 
>> Line 21: density[3] -> density [3] 
>> 
>> Somewhere in the Results part, close to the discussion, it would be nice 
>> mention possible reasons in the correlation strengths between scenarios 
>> including / excluding the coalescence mechanism (e.g. for p-d you see a 
>> stronger correlations  with DIRECT (no coalescence) scenarios, while in 
>> d-d the coalescence scenarios leads to the stronger correlation effect).
>> Line 92-94: I would be very careful and avoid the statements that: „Those 
>> observations imply that at √sNN = 3GeV Au+Au collisions, deuterons are 
>> formed via the nucleon coalescence processes” as you don’t discuss any 
>> size dependences. You just take pure SMASH data assuming that the source 
>> size simply agrees. If you change your source size, you might get 
>> different  interpretation. This conclusion should be left for further 
>> investigation. Meantime, I suggest to make your conclusion lighter.
>> 
>> 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 Ke Mi via Star-cf-l <star-cf-l AT lists.bnl.gov> w 
>>> dniu 24.07.2022, o godz. 13:51:
>>> 
>>> Dear Hanna and Takafumi,
>>> 
>>> Thank you for the suggestion.
>>> We will revise the draft and update soon.
>>> 
>>> Best regards,
>>> Ke
>>> 
>>>> On 24. Jul 2022, at 19:49, Takafumi Niida <niida AT bnl.gov> wrote:
>>>> 
>>>> Hi Ke, 
>>>> 
>>>> I would focus more on final physics results. For example, I’m not sure 
>>>> if you need Fig. 1 and lines 54-59. If needed, Section 1 and 2 could be 
>>>> combined with some modifications. It may be helpful to make more space 
>>>> if you put Figs. 2 and 3 into one figure, upper and bottom plots, 
>>>> because of the similarity of the figures the captions can be reduced.
>>>> 
>>>> Best regards,
>>>> Takafumi
>>>> 
>>>> 
>>>>> On Jul 25, 2022, at 2:30, Hanna Paulina Zbroszczyk 
>>>>> <hanna.zbroszczyk AT pw.edu.pl> wrote:
>>>>> 
>>>>> Dear Ke and All,
>>>>> 
>>>>> As Takafumi wrote, as your talk was based on merged abstract, the 
>>>>> proceedings should also include other's results.
>>>>> I understand that in case of p-p results that changed after preliminary 
>>>>> labels had been granted, old results should not be considered any 
>>>>> longer. With p-p @ 3 GeV we should wait until final publication. 
>>>>> However, for other results, we appreciate if you include them in  your 
>>>>> proceedings.
>>>>> 
>>>>> Thank you,
>>>>> Best regards,
>>>>> 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 Ke Mi via Star-cf-l <star-cf-l AT lists.bnl.gov> 
>>>>>> w dniu 24.07.2022, o godz. 13:10:
>>>>>> 
>>>>>> Dear Hanna and Takafumi,
>>>>>> 
>>>>>> Thank you for the suggestion.
>>>>>> 
>>>>>> The main reason is due to the page limitation. We presented many of 
>>>>>> Femtoscopy results at STAR (baryon CF, meson CF, light nuclei CF..), 
>>>>>> it’s quite hard to include all of them into 6 page.
>>>>>> 
>>>>>> Beside, for the ks0-ks0 CF, since Diana has presented them at SQM2022 
>>>>>> and HYP, we think it might be much better to discuss ks0-ks0 as well 
>>>>>> as kch-ks0 in a single proceeding. (The time slot may be very close to 
>>>>>> QM proceeding). That will help to declare this important physics much 
>>>>>> more clear. For the p-p CF, since the newest results is quiet 
>>>>>> different from preliminary one and p-p/p-Xi results have been proposed 
>>>>>> a paper, so here we did not include them. 
>>>>>> 
>>>>>> Since I did not include strangeness, so I changed the title into 
>>>>>> “Femtoscopy of proton-deuteron and deuteron-deuteron in Au+Au 
>>>>>> collisions at #sqrt(sNN) = 3 GeV from RHIC-STAR”. The original title 
>>>>>> is “Femtoscopy of proton, light nuclei and strangeness from STAR”, I’m 
>>>>>> sorry about no previous notification about this change. 
>>>>>> 
>>>>>> If needed, we are willing to revise the proceedings, both title and 
>>>>>> contents. 
>>>>>> 
>>>>>> Your further suggestions are welcome. 
>>>>>> 
>>>>>> Thank you.
>>>>>> 
>>>>>> Best regards,
>>>>>> Ke
>>>>>> 
>>>>>> 
>>>>>>> On 24. Jul 2022, at 19:01, Takafumi Niida <niida AT bnl.gov> wrote:
>>>>>>> 
>>>>>>> Dear Ke,
>>>>>>> 
>>>>>>> I also agree with Hana. Since your talk was based on merged abstract, 
>>>>>>> the proceedings should also include other's results. I understand you 
>>>>>>> have many materials and page limit the proceedings should reflect 
>>>>>>> what was presented in your talk.
>>>>>>> 
>>>>>>> Best regards,
>>>>>>> Takafumi
>>>>>>> 
>>>>>>>> On Jul 25, 2022, at 0:03, Hanna Paulina Zbroszczyk via Star-cf-l 
>>>>>>>> <star-cf-l AT lists.bnl.gov> wrote:
>>>>>>>> 
>>>>>>>> Dear Ke,
>>>>>>>> 
>>>>>>>> May I ask why among of many STAR results presented in your talk you 
>>>>>>>> discuss only p-d and d-d correlations?
>>>>>>>> I understand the page limit up to 6 but your proceeding refers to 
>>>>>>>> only some part of your presentation..
>>>>>>>> You even changed the title of your contribution.. which I don’t 
>>>>>>>> understand. Please explain what happened as I am confused.
>>>>>>>> 
>>>>>>>> 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 Ke Mi via Star-cf-l 
>>>>>>>>> <star-cf-l AT lists.bnl.gov> w dniu 24.07.2022, o godz. 06:13:
>>>>>>>>> 
>>>>>>>>> Dear Xiaofeng,
>>>>>>>>> 
>>>>>>>>> Thank you for the detailed comments and sign-off, I’ve implemented 
>>>>>>>>> them and update the draft.
>>>>>>>>> Please find through same link:
>>>>>>>>> https://drupal.star.bnl.gov/STAR/node/60334
>>>>>>>>> 
>>>>>>>>> Best regards,
>>>>>>>>> Ke
>>>>>>>>> 
>>>>>>>>> 
>>>>>>>>>> On 24. Jul 2022, at 08:39, Xiaofeng Luo via Star-cf-l 
>>>>>>>>>> <star-cf-l AT lists.bnl.gov> wrote:
>>>>>>>>>> 
>>>>>>>>>> Hi Ke，
>>>>>>>>>> 
>>>>>>>>>>     Nice proceedings.
>>>>>>>>>>     Please find my minor suggestions :
>>>>>>>>>> 
>>>>>>>>>>     1. Line 73, proton and neutron production -> particle 
>>>>>>>>>> production
>>>>>>>>>>     2. Reference 9, the "sNN=" can be removed.
>>>>>>>>>>     3. You may add a reference of BES deuteron production at STAR.
>>>>>>>>>> 
>>>>>>>>>>     With those implemented, I sign off.
>>>>>>>>>> 
>>>>>>>>>> Thank you,
>>>>>>>>>> Best Regards,
>>>>>>>>>> Xiaofeng
>>>>>>>>>> 
>>>>>>>>>> On 2022/7/19 9:34 PM, webmaster--- via Star-cf-l wrote:
>>>>>>>>>>> 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/60334
>>>>>>>>>>> 
>>>>>>>>>>> ---
>>>>>>>>>>> If you have any problems with the review process, please contact
>>>>>>>>>>> webmaster AT www.star.bnl.gov
>>>>>>>>>>> _______________________________________________
>>>>>>>>>>> Star-cf-l mailing list
>>>>>>>>>>> Star-cf-l AT lists.bnl.gov
>>>>>>>>>>> https://lists.bnl.gov/mailman/listinfo/star-cf-l
>>>>>>>>>> 
>>>>>>>>>> -- 
>>>>>>>>>> Xiaofeng Luo
>>>>>>>>>> Professor of Physics
>>>>>>>>>> College of Physical Science and Technology
>>>>>>>>>> Central China Normal University
>>>>>>>>>> Luoyu Road 152, Wuhan China
>>>>>>>>>> Office Phone #: +86-27-67867500
>>>>>>>>>> 
>>>>>>>>>> _______________________________________________
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>>>>>>>>>> Star-cf-l AT lists.bnl.gov
>>>>>>>>>> https://lists.bnl.gov/mailman/listinfo/star-cf-l
>>>>>>>>> 
>>>>>>>>> _______________________________________________
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>>>>>>>> 
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>>>>>>> 
>>>>>> 
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>>>>> 
>>>> 
>>> 
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