STAR Flow, Chirality and Vorticity PWG

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

Dear Subhash,

A gentle reminder for your further comments on my proceedings.
Here is the link to updated version: 
https://drupal.star.bnl.gov/STAR/node/66043
The deadline for the same is 30th November. Apologies for the 
inconvenience.

Thanks and regards,
Sharang

On 2023-11-23 23:20, sharangrav via Star-fcv-l wrote:
> Dear Subhash,
>
> Thanks for your nice comments. I have incorporated all of them in the
> updated version and here is the link to the same.
> https://drupal.star.bnl.gov/STAR/node/66043
> Please le me know if you have further comments.
>
> Thanks and regards,
> Sharang
>
> On 2023-11-22 18:47, subhash via Star-fcv-l wrote:
> > Dear Sharang,
> >
> > Nice proceedings. I have a few suggestions below for your 
> > consideration:
> >
> > l#10: at s_NN  = 3.2, ...
> >
> > l#11, 12: for identified hadrons (pi, K, p) and net-particles (net K
> > and net p) ....
> >
> > l#13, 14: The minimum in v1 slope for net-kaon is observed at lower
> > collision energy than net-proton
> > --> I think we don't have sufficient data to comment about the
> > minimum. You can probably say that the sign change occurred at
> > different energy.
> >
> > l#18: "The v3 slope for all particles decreases in magnitude with
> > increasing collision energy, indicating the effect of the mean-field
> > at the low energies."
> > --> How mean field connected to energy dependence, can you explain?
> > There could be multiple effects folded in here mean-field, baryon
> > stopping, geometry, ... right?
> >
> > l#51, 55 and else where add a space X ~ GeV
> >
> > l#59: remove bracket on \kappa
> >
> > l#61,62: add a reference
> >
> > l#66: The traditional v3, ...
> >
> > l#77: In these proceedings,
> >
> > l#88-93: You could mention the kinematics, pt, eta selections and
> > track selection conditions before introducing particle identification.
> >
> > l#93: I guess you are not using z-variable for all species, only for
> > light nuclei. For other species you are using combination with Nsigma.
> > So modify the discussions accordingly.
> >
> > l#113: You could mention what is used as weight in Q reconstruction
> >
> > l#130:  employed in the collider BES-I
> >
> > l#141, 142: you can add model comparison or a reference for backing up
> > the statement
> >
> > l#155: linear term in a third-order polynomial, right?
> >
> > l#160: Suggest to change the statement that we observe a sign change
> > than observe a minima, as mentioned above. Also make a similar change
> > in the conclusion.
> >
> > l#172,  173: modify the statement that it is not solely from
> > mean-field. Also make a similar change in the conclusion.
> >
> > Thanks and regards,
> > Subhash
> >
> >
> >
> >
> > On 2023-11-20 01:44 PM, webmaster--- via Star-fcv-l wrote:
> > > Dear star-fcv-l AT lists.bnl.gov members,
> > >
> > > Sharang Rav Sharma (sharang.rav AT students.iisertirupati.ac.in) has 
> > > submitted a
> > > material for a review, please have a look:
> > > https://drupal.star.bnl.gov/STAR/node/66043
> > >
> > > ---
> > > If you have any problems with the review process, please contact
> > > webmaster AT www.star.bnl.gov
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