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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Chenlu Hu for CPOD March Meeting 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 Chenlu Hu for CPOD March Meeting 2021 submitted for review
  • Date: Thu, 4 Feb 2021 13:17:11 +0900

Dear Chenlu
I would sign off your nice abstract with a few questions.
Do you know why the yield reduces in central again even
considering smaller (5% or less?) centrality steps for the
last 2 bins compared to other 10% bins? I understood the
S/N would be worse in central, while the centrality dependence
of the yields, that you have attached in one of the previous E-mail,
can be explained by the efficiency? For the numbers you wrote in
your abstract, 4LHe is mostly unchanged, but 3LHe numbers are
quite reduced from your presentation slide in the PWG
(September 16, 2020), why?
Best regards, ShinIchi

> 2021/02/04 0:05、胡晨露 via Star-fcv-l <star-fcv-l AT lists.bnl.gov>のメール:
>
> Dear Jiangyong,
>
> Thank you very much for your comments.
>
> The CPOD abstract is updated accordingly. Updated abstract has been
> uploaded to below drupal link.
>
> https://drupal.star.bnl.gov/STAR/node/53562
>
> Thanks and best regards
>
> Chenlu
>
>





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