STAR Flow, Chirality and Vorticity PWG

[subhash <subhash AT rcf.rhic.bnl.gov>]

Dear Zuowen,

Nice poster.
As decided by the management, we will only release 0-80% centrality for 
14.6 GeV. So please remove results of v1 figures for 14.6 GeV at 10-40% 
centrality (slide 4 and 5).

slide#2: "v1 is sensitive to the 1st order phase transition." --> v1 is 
sensitive to the QCD order phase transition. Because depending on 
cross-ver or 1st order PT the v1 can be different.
Can you add a reference for data and model here?

slide#3: Inside figure indicate run year or BES-II.
Can you indicate the improved 1st order EP resolution in BES-II compared 
to BES-I?

slide#5: Modify the summary accordingly, since 14.6 GeV is removed.

Thanks and regards,
Subhash


On 2022-05-30 07:57 PM, webmaster--- via Star-fcv-l wrote:
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Zuowen Liu (liuzw AT mails.ccnu.edu.cn) has submitted a material for a 
> review,
> please have a look:
> https://drupal.star.bnl.gov/STAR/node/59770
>
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