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Re: [Star-fcv-l] STAR presentation by Li-ke Liu for CPOD 2024 got commented by Subhash Singha
- From: LikeLiu <likeliu AT mails.ccnu.edu.cn>
- To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
- Cc: connectsubhash <connectsubhash AT gmail.com>, zhenyuchen <zhenyuchen AT sdu.edu.cn>
- Subject: Re: [Star-fcv-l] STAR presentation by Li-ke Liu for CPOD 2024 got commented by Subhash Singha
- Date: Fri, 10 May 2024 18:42:51 +0200
Hi Subhash and Zhenyu,
Many thanks for your suggestions and comments!
The draft has modified accordingly, below is my reply:
s#4: remove v1: and v2: from the bullet. IMO, the bullets are valid forYes, I mean v2 is sensitive to the partonic/hadronic interaction, while I am not sure it’s also valid for v1 in my knowledge.
both vn'sBTW, by "constituent interaction" do you mean partonic/hadronic
interactions?
s#19: You mentioned 4.5 GeV is the onset of partonic collectivity, what
happened to the ratios above 4.5, is it possible to include in the figure?
Yes, I have added the 7.7 GeV ratio.
Since we don’t have the Preliminary results at 7.7 GeV, these data are taken from BES-I, Phys. Rev. C 88 (2013).
The NCQ scaled v2 and ratios can be found in the attachment.
For s#19 figure, we want to focus on pT integrated v2 and NCQ scaled v2 ratio at 3-4.5 GeV,
The X-axis extend to 7.7 GeV would make the pT integrated v2 overlapped too much, thus I add 7.7 GeV ratio in the edge.
Kindly let me know if you have further comments.
Thanks,
Li-Ke
Attachment:
g_Ratiov2_nqKEt_nq10-40%.pdf
Description: Adobe PDF document
On May 9, 2024, at 08:05, webmaster--- via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:Dear star-fcv-l AT lists.bnl.gov members,
Subhash Singha ( connectsubhash AT gmail.com ) has commented on a material
originally submitted by Li-ke Liu ( likeliu AT mails.ccnu.edu.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/CPOD-2024/Collectivity-High-Baryon-Density-STAR-BES-II
Comment:
Dear Li-Ke,
Very nice and clean slides. I have a few additional questions/suggestions:
s#4: remove v1: and v2: from the bullet. IMO, the bullets are valid for
both vn'sBTW, by "constituent interaction" do you mean partonic/hadronic
interactions?
s#6: "Hadronic dominates" --> can you re-word e.g. dominant hadronic
interaction or hadronic interaction dominates
s#8: "Hundreds of millions events recorded at Au+Au 3.0 - 4.5 GeV" --> the
line is redundant, you already have events listed in the table. You can
probably mention e.g. FXT data provide good precision for collectivity
measurement
s#13: is not need --> is not necessary
s#14: baryonic Mean FIeld
s#19: You mentioned 4.5 GeV is the onset of partonic collectivity, what
happened to the ratios above 4.5, is it possible to include in the figure?
I sign off with these addressed.
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[Star-fcv-l] STAR presentation by Li-ke Liu for CPOD 2024 got commented by Subhash Singha,
webmaster, 05/09/2024
- Re: [Star-fcv-l] STAR presentation by Li-ke Liu for CPOD 2024 got commented by Subhash Singha, LikeLiu, 05/10/2024
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