STAR Flow, Chirality and Vorticity PWG

["Zuowen Liu" <liuzw AT mails.ccnu.edu.cn>]

Dear Subhash,

I understood the decision made by conveners.

I would delete v1 results at 14.6 GeV in my slides.

Thank you for your other comments. I have implemented them into the slides.

Kindly find the modified slides by the link:

https://drupal.star.bnl.gov/STAR/system/files/ISMD_presentation.pdf

Thanks and Best regards,

Zuowen

 

 

------------------ Original ------------------

From:  "subhash"<subhash AT rcf.rhic.bnl.gov>;

Date:  Tue, Jul 26, 2022 09:50 AM

To:  "star-fcv-l"<star-fcv-l AT lists.bnl.gov>;

Cc:  "liuzw"<liuzw AT mails.ccnu.edu.cn>;

Subject:  Re: [Star-fcv-l] STAR presentation by Zuowen Liu for ISMD2022 submitted for review

 

Dear Zuowen,

Nice slides. Here are my comments:

General:
For 14.6 GeV results in finer centrality bins, we have discussed at the
conveners meeting. It is decided that no centrality results will be
released until the official announcement by the centrality group. This
is to make sure all corrections in centrality (vz corrections, pile up
etc) are in place and finalized. Sorry about that. We believe you still
have enough materials to present at ISMD.

s#7: Mention on the right panel 2019 or BES-II

s#8: Top resolution plot: mention Psi1 resolution
Mention the errors are statistical inside the bottom panels.

Summary slide:
"more precise measurement" --> You could specify example from 19.6 GeV
(factor of 8 reduction)

"Centrality dependence of net-particle dv1/dy" --> Mention the sign
change and the behavior. Then say offer more constraint.

You could stress on observation. e.g. "UrQMD shows oppositive trend of
proton and lambda" --> Say what we observe in data, then mention UrQMD
trend and/or say it does not describe data.


Thanks and regards,
Subhash



On 2022-07-20 04:46 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/60349
>
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