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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Shengli Huang for ISMD2021 submitted for review

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: ShinIchi Esumi <esumi.shinichi.gn AT u.tsukuba.ac.jp>
  • To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] STAR presentation by Shengli Huang for ISMD2021 submitted for review
  • Date: Thu, 8 Jul 2021 13:52:31 +0900

Dear Shengli
Since results are all previously approved preliminary, so I do not see any
issue
and therefore, would sign off. So please confirm everything are already shown
and approved before. I think I’ve mentioned earlier, I would like to know how
the
choice of beta2 (x-axis) values for AuAu and UU for 3 different centralities
(0-5 /
0-1 / 0-0.5 %) is made for the plot in page 14, are they also calculated
separately
for 3 different centralities for one system, although it looks like it is
just plotted
slightly shifted? While the model calculations are given as band as a
function of
beta2, so that you might need to explain how it was done.
Best regards, ShinIchi

> On Jul 8, 2021, at 0:40, webmaster--- via Star-fcv-l
> <star-fcv-l AT lists.bnl.gov> wrote:
>
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Shengli Huang (shengli.huang AT stonybrook.edu) has submitted a material for a
>
> review, please have a look:
> https://drupal.star.bnl.gov/STAR/node/55551
>
> ---
> If you have any problems with the review process, please contact
> webmaster AT www.star.bnl.gov
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