STAR Flow, Chirality and Vorticity PWG

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

Hi Subhash,

Thanks for your signing off. I will add your cosmetic comments in my 
next version.

Best,
Gaoguo



在 2022-07-27 08:59，subhash 写道：
> Dear Gaoguo,
>
> Thanks for updating the proceedings. I am sending it to star-talks
> with a few cosmetic comments for your consideration:
>
> please use "\mathrm" for s_{\mathrm NN}, p_{\mathrm T} etc 
> consistently.
> Equation 1 angular brakets \langle .... \rangle
>
> Thanks and regards,
> Subhash
>
> On 2022-07-25 03:49 PM, gyan wrote:
> > Dear Subhash,
> >
> > Thanks for your further suggestions, please find a newer version from
> > the link below:
> > https://drupal.star.bnl.gov/STAR/system/files/v5_1.pdf
> >
> > Best,
> > Gaoguo
> >
> > 在 2022-07-25 13:07，subhash 写道：
> > > Dear Gaoguo,
> > >
> > > Thanks a lot for the updated proceedings. I have a few additional
> > > suggestions for your consideration:
> > >
> > > line 31: charge distributions. (?)
> > > line 39: backward rapidities
> > > line 43: GeV/c
> > > line 44: except for
> > > line 45: by using separately negative and positive tracks, and by
> > > varying track selections.
> > > line 47: remove "in addition". You can say something like, The shape
> > > and size of initial state fluctuations can contribute to the higher
> > > harmonics (vn 48 for n=3,4,...) and to the fluctuation of mean
> > > transverse momentum of final state particles, respectively.
> > > line 56: we also present
> > > line 58: to probe it's beam energies dependence.
> > > line 64: implying a stronger flow decorrelation
> > > line 65-66: The second order decorrelation becomes stronger as we 
> > > move
> > > from central to peripheral collisions. Such a dependence is the 
> > > result
> > > of ....
> > > line 67: which is dominated by the initial ...
> > > line 69: no obvious centrality dependence since the third order flow 
> > > is ...
> > > line 74: which same as observed in isobar ...
> > > line 75: "The decreasing trend" --> Can you call it slope of r{eta}
> > > line 76: lower energy collisions has large decorrelation
> > > line 78: along the longitudinal direction
> > > line 85: and shows a hint of
> > > line 90: similar initial fluctuations
> > >
> > > I sign off with these are addressed.
> > >
> > > Thanks and regards,
> > > Subhash
> > >
> > >
> > > On 2022-07-25 11:26 AM, gyan wrote:
> > > > Dear Subhash,
> > > >
> > > > Thanks for your suggestions. Please find a new version from the link 
> > > > below:
> > > > https://drupal.star.bnl.gov/STAR/system/files/v4_1.pdf
> > > >
> > > > Best,
> > > > Gaoguo Yan
> > > >
> > > > 在 2022-07-22 17:52，subhash via Star-fcv-l 写道：
> > > > > Dear Gaoguo,
> > > > >
> > > > > Thanks for writing the proceedings. I have embedded my suggestions
> > > > > into the following pdf file at:
> > > > > https://drupal.star.bnl.gov/STAR/system/files/v3_1_SS.pdf
> > > > > In the next iteration, please do a latex spell check and get it 
> > > > > read
> > > > > by someone from your institute. It probably need to be sharpened a
> > > > > bit.
> > > > >
> > > > > Thanks and regards,
> > > > > Subhash
> > > > >
> > > > > On 2022-07-19 04:51 PM, webmaster--- via Star-fcv-l wrote:
> > > > > > Dear star-fcv-l AT lists.bnl.gov members,
> > > > > >
> > > > > > Gaoguo Yan (gaoguo.yan AT Outlook.com) has submitted a material for a 
> > > > > > review,
> > > > > > please have a look:
> > > > > > https://drupal.star.bnl.gov/STAR/node/60322
> > > > > >
> > > > > > ---
> > > > > > If you have any problems with the review process, please contact
> > > > > > webmaster AT www.star.bnl.gov
> > > > > > _______________________________________________
> > > > > > Star-fcv-l mailing list
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