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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Li-ke Liu for CPOD 2024 got commented by Subhash Singha

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: subhash <subhash AT rcf.rhic.bnl.gov>
  • To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Cc: LikeLiu <likeliu AT mails.ccnu.edu.cn>, 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: Tue, 28 May 2024 17:55:59 +0800

Dear Li-Ke,

Thanks for uploading the preliminary figures. They have been updated on the FCV preliminary repository page.

Thanks and regards,
Subhash

On 2024-05-28 05:31 PM, LikeLiu via Star-fcv-l wrote:
Dear Conveners and All,

I have summarized my CPOD2024 files in below link, including
presentation slides, preliminary request and figures:

star.bnl.gov [2] [2]

Thanks and best regards,
Li-Ke

On May 12, 2024, at 22:41, LikeLiu via Star-fcv-l
<star-fcv-l AT lists.bnl.gov> wrote:

Hi Subhash and Zhenyu,

I just notice there are two typos in the previous version, which
have been corrected in the version 4.

Collectivity at High Baryon Density from STAR BES-II | The STAR
experiment [1]
star.bnl.gov [1] <bluelake_favicon.ico> [1]

Thanks,
Li-Ke

On May 10, 2024, at 18:42, LikeLiu via Star-fcv-l
<star-fcv-l AT lists.bnl.gov> wrote:

Hi Subhash and Zhenyu,

Many thanks for your suggestions and comments!

Collectivity at High Baryon Density from STAR BES-II | The STAR
experiment [1]
star.bnl.gov [1] [1]

<bluelake_favicon.ico>

[1]

The draft has modified accordingly, below is my reply:

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?Yes, I mean v2 is sensitive to the partonic/hadronic
interaction, while I am not sure it’s also valid for v1 in my
knowledge.

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
<g_Ratiov2_nqKEt_nq10-40%.pdf>

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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Links:
------
[1] https://drupal.star.bnl.gov/STAR/presentations/CPOD-2024/Collectivity-High-Baryon-Density-STAR-BES-II
[2] https://drupal.star.bnl.gov/STAR/blog/lliu/CPOD-Presentation-and-Preliminary-plots
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