STAR Flow, Chirality and Vorticity PWG

[Maowu Nie <nie AT rcf.rhic.bnl.gov>]

Dear ShinIchi,

Thanks for the reply.
r2 results in Gaoguo's page 13 cannot directly compared with Au+Au 
results, since it still has large non-flow contribution for isobar.
The eta_ref dependence is in our to-do list with full isobar dataset.

I quote one plot of the comparison in Gaoguo's Collaboration Meeting 
slides.(https://drupal.star.bnl.gov/STAR/system/files/collaboration_meeting_20210303_GaoguoYan.pdf)

You can see a clear offset in Au+Au data, which makes it hard to 
compare. This is also another big reason we need run19 Au+Au 200GeV 
data.
To study the system size dependence of flow decorrelation needs precise 
measurements for both systems.

The above information are included in the slides with the same link:
https://drupal.star.bnl.gov/STAR/system/files/request_run19AuAu200GeV.pdf

Hope it helps.

Regards,
Maowu


在 2021-04-15 18:34，ShinIchi Esumi via Star-fcv-l 写道：
> Dear Maowu, Thank you very much.
> Please overlay your two plots in your first page with the plots at
> shown yesterday
> by Gaoguo in his page 13 or show them by side-by-side.
> Best regards, ShinIchi
>
> > On Apr 15, 2021, at 17:35, Maowu Nie <nie AT rcf.rhic.bnl.gov> wrote:
> >
> > Dear ShinIchi, Prithwish, Jiangyong and FCV enthusiasts,
> >
> > As we already discussed yesterday, we would like to request high 
> > priority of run19 Au+Au@200GeV data production.
> > You can find the request slides below:
> >
> > https://drupal.star.bnl.gov/STAR/system/files/request_run19AuAu200GeV.pdf
> >
> > Inputs from other related physics interests are also welcome.
> >
> > Regards,
> > Maowu
>
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