STAR Flow, Chirality and Vorticity PWG

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

ps: I discarded the duplicate entry:
https://drupal.star.bnl.gov/STAR/node/60237


On 2022-07-15 09:01 AM, subhash wrote:
> Dear Ding,
>
> Nice poster. I have a few suggestions for your consideration:
>
> Title: I suggest "Directed flow of ϕ-meson in fixed target Au+Au
> collisions at sNN = 3 and 7.2 GeV from STAR"
>
> In abstract:
> "anisotropic flows" --> directed flow
> "compare our new results with STAR Beam Energy Scan I results" -->
> compare our new results with that from STAR Beam Energy Scan I.
>
> In motivation:
> You can probably try presenting them in separate small bullets.
>
> In Datasets:
> You didn't mention about 3 GeV data.
>
> Analysis method:
> Usually we fit phi meson with a Breit Wigner function. Could you
> remind me what is the reasoning behind Gaussian fit?
>
> Summary:
> "This may indicate a softest point of EoS for produced particles." -->
> This may be related to a change in EoS of the system.
> I suggest "a change in EoS", because there is no evidence that this
> phi meson sign change is due to EoS softening.
>
> "Results from fixed target and collider modes connect well. At same
> collision energy, combine FXT and COL modes can improve the flow
> measurements."
> --> At similar collision energy, results from fixed target and
> collider modes are consistent within error. Upcoming measurements from
> FXT and COL data will improve the precision in \phi flow measurements.
>
> I sign off with these addressed.
>
> Thanks and regards,
> Subhash
>
> On 2022-07-11 10:31 PM, webmaster--- via Star-fcv-l wrote:
> > Dear star-fcv-l AT lists.bnl.gov members,
> >
> > Ding Chen (dchen087 AT ucr.edu) has submitted a material for a review, 
> > please
> > have a look:
> > https://drupal.star.bnl.gov/STAR/node/60236
> >
> > ---
> > If you have any problems with the review process, please contact
> > webmaster AT www.star.bnl.gov
> > _______________________________________________
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