STAR Flow, Chirality and Vorticity PWG

["Zuowen Liu" <liuzw AT mails.ccnu.edu.cn>]

Dear ShinIchi, Subhash and All

Thank you very much for your nice suggestions.

Here I attach the slides about acceptance: https://drupal.star.bnl.gov/STAR/system/files/acceptance_FXT.pdf

At FXT energies, we would like to request preliminary for three figures.

1) dv1/dy vs pT for pi+/pi-, K0s at 3, 3.2, 3.5, 3.9 GeV.

2) dv1/dy vs sqrt(sNN) for pi+/pi-, K0s and lambda at 3, 3.2, 3.5, 3.9 GeV.

Please find the acceptance for pi+/pi-, K0s and lambda at p1 and p2 in the new slides.

Acceptance of these four particle species can cover the range of measured pT and rapidity.

3) NCQ scaling of pi+/pi-, K+/K-, proton, K0s and lambda at 3.2 GeV.

Kindly find the acceptance at p5 at the slides. we do get issue for proton acceptance at mid-rapidity, there is a hole which could not be covered by TPC and BTOF. And for K-, there is purity issue at high pT, we take asymmetric mass cut at high pT to ensure purity > 90%, so that you can see the color fade away at high pT.

For Subhash:

Kindly find our systematic uncertainty study at slide 7.

Thanks and Best regards,

Zuowen

 

 

------------------ Original ------------------

From:  "EsumiShinIchi via Star-fcv-l"<star-fcv-l AT lists.bnl.gov>;

Date:  Thu, Aug 10, 2023 00:15 AM

To:  "star-fcv-l"<star-fcv-l AT lists.bnl.gov>;

Cc:  "ShinIchi Esumi"<esumi.shinichi.gn AT u.tsukuba.ac.jp>;

Subject:  Re: [Star-fcv-l] FCV PWG meeting on 09/Aug/2023 Wed. 9:30 AM EDT

 

Dear Zuowen, Chengdong and all

Thanks for the nice results, similar to the questions that people were asking to Sharang,

when you compare the beam energy dependence, how do you ensure the pT and rapidity

acceptance, which would vary with beam energy. And when you plot rapidity dependence

of vn, how do you ensure the pT acceptance that changes with rapidity, or when you plot

pT dependence, how do you ensure the rapidity acceptance. You do show mT dependence

for a wide -0.5<y<0, but there are hole in the acceptance, so you will not really be able to

correct by the efficiency for the rapidity range, therefore you would need to limit rapidity

acceptance to show pT dependence or you would need to limit pT acceptance to show

rapidity dependence. What we can really present is vn(pT, rapidity) after all.  So, p18 in

Zuowen’s slide is good, but I would worry about p19 and p20, that gives the preliminary

requests at p8 and p9...

Best regards, ShinIchi

On Aug 9, 2023, at 22:01, Zuowen Liu via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:

Dear All,

Kindly find my slides by the link:

https://drupal.star.bnl.gov/STAR/system/files/QM23_flow_Zuowen.pdf

Thanks and Best regards,

Zuowen

 

------------------ Original ------------------

From:  "xgou via Star-fcv-l"<star-fcv-l AT lists.bnl.gov>;

Date:  Wed, Aug 9, 2023 07:42 PM

To:  "star-fcv-l"<star-fcv-l AT lists.bnl.gov>;

Cc:  "xgou"<xgou AT rcf.rhic.bnl.gov>;

Subject:  Re: [Star-fcv-l] FCV PWG meeting on 09/Aug/2023 Wed. 9:30 AM EDT

 

Dear All,

  Please find my slide here:
 
https://drupal.star.bnl.gov/STAR/blog/xgou/QM2023-analysis-status-and-update-Pyc2-global-polarization-Isobar-collisionsXingrui202389

Thanks!

Best regards,
Xingrui


> Dear All,
>     You can find my slide here:
> https://drupal.star.bnl.gov/STAR/blog/slhuang/Qm2023-preliminary
>
> Thanks!
> Shengli
>
> On Tue, Aug 8, 2023 at 12:25 PM Cameron Racz via Star-fcv-l
> <star-fcv-l AT lists.bnl.gov> wrote:
>
>> Hi convenors,
>>
>> I would like to present my preliminary request for proton v3 at 3.2,
>> 3.5, and 3.9 GeV if there is enough time. My slides are located
>> here:
>>
>>
> https://drupal.star.bnl.gov/STAR/blog/cracz/Preliminary-Request-v3-Protons-32-35-39-GeV
>>
>> Thank you,
>>
>> Cameron Racz
>> Ph.D. Candidate
>> Heavy-ion Physics Group
>> University of California, Riverside
>>
>>> On Aug 8, 2023, at 5:12 AM, sharangrav via Star-fcv-l
>> <star-fcv-l AT lists.bnl.gov> wrote:
>>>
>>> Dear convenors,
>>>
>>> If time permits I would also like to give some update on my
>> anisotropic flow result for fixed target energies (for QM and ISMD).
>> Please add me to the agenda. I will post my slides soon.
>>>
>>> Thanks and regards,
>>> Sharang
>>>
>>>
>>> On 2023-08-08 11:59, subhash via Star-fcv-l wrote:
>>>> Dear All,
>>>> We shall have our weekly FCV PWG meeting this Wednesday
>> (09/Aug/2023)
>>>> at 9:30 AM EDT. As you know the deadline for preliminary
>> approvals is
>>>> the week of August 14 and submission of talk/poster to FCV PWG is
>>>> August 20.  Therefore, this week and next week we would like to
>> focus
>>>> on Quark Matter related analysis updates and preliminary
>> approval. We
>>>> would like to ask the following analyzers to present an update:
>>>> Zuowen, Chengdong, Xingrui, Rishabh & Shengli
>>>> The agenda items will be collected at:
>>>> https://drupal.star.bnl.gov/STAR/blog/jjiastar/bulkcorr
>>>> We would also like to discuss the followings in order to assess
>> your
>>>> analysis status:
>>>> -- list of promised results observables, collision system, beam
>> energies
>>>> -- status/readiness of your analysis, new preliminary requests
>>>> -- any potential issues, show stoppers, centrality/embedding
>> etc.
>>>> For preliminary request you can use this template:
>>>>
>>
> https://drupal.star.bnl.gov/STAR/system/files/Prelim_Request_template.pdf
>>>> Zoom details are copied below.
>>>> Thanks and regards,
>>>> Prithwish, Zhenyu and Subhash
>>>> ZOOM LINK FOR FCV MEETING:
>>>> Join ZoomGov Meeting
>>>>
>>
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>>
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