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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Prabhupada Dixit for SQM 2021 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 Prabhupada Dixit for SQM 2021 submitted for review
  • Date: Sat, 31 Jul 2021 21:11:50 +0900

Dear Prabhupada
Thanks for the nice write-up. I would sign off with some minor comments.
After signing off from one of other conveners, you can go to star talk.
Best regards, ShinIchi

L17 : in the azimuthal distributions, known as anisotropic flow.
L38 : Due to the finite resolution of the event plane,
(The multiplicity does determine the resolution together with the vn
signal, though.)
L42 : We could add "The particle phi and the event plane Psi are taken from
opposite eta region."
L48 : ... [4], but at pT above ...
L52 : ... does not, because ...
L68 : ... for v2, but ...

> On Jul 24, 2021, at 2:30, webmaster--- via Star-fcv-l
> <star-fcv-l AT lists.bnl.gov> wrote:
>
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Prabhupada Dixit (prabhupadad AT iiserbpr.ac.in) has submitted a material for
> a
> review, please have a look:
> https://drupal.star.bnl.gov/STAR/node/55702
>
> ---
> If you have any problems with the review process, please contact
> webmaster AT www.star.bnl.gov
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