STAR Flow, Chirality and Vorticity PWG

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

Dear Subhash,
Thank you for the comments. I have modified the poster accordingly.
https://drupal.star.bnl.gov/STAR/system/files/SQM22_poster_v4.pdf

Regards,
Prabhupada

On 2022-06-08 13:43, subhash wrote:
> Dear Prabhupada,
>
> Thanks for incorporating my comments.
> I am fine with your poster once the following suggestions are 
> addressed.
>
> Can you add either data taking year (2019) or BES-II in all the
> relevant figures?
> Can you draw add a horizontal straight line at 1, on the right hand
> side ratio plots?
> Can you add the conclusion in your slides based on your v_n ratios,
> e.g. ratios are sensitive to initial fluctuations and transport
> properties; can be used constrain hydrodynamic models.
>
> Thanks and regards,
> Subhash
>
> On 2022-06-08 02:59 PM, pdixit wrote:
> > Dear Subhash,
> > Thank you for the comments and the suggestions. I have modified the
> > poster accordingly. Please find the new version of the poster in the
> > link below.
> > https://drupal.star.bnl.gov/STAR/system/files/SQM22_poster_v3.pdf
> > > > What do we learn from the ratio v3/v2^3/2?
> > This ratio is a prediction from hydrodynamics. It's sensitive to the
> > magnitude of the transport properties (viscosity) and the fluctuations
> > present in the initial stage of the system and is useful to filter
> > various models.
> > Reference: PRL 105, 062301 (2010), Phys. Rev. Lett. 92, 062301
> >
> > Regards,
> > Prabhupada
> >
> >
> > On 2022-06-07 16:28, subhash wrote:
> > > Dear Prabhupada,
> > >
> > > Nice poster. I have a few suggestions for your consideration.
> > > slide#1: Top right, the x-arrow coincide with event-by-event. Please 
> > > fix it.
> > > Can you add reference for Early freeze-out and small hadronic
> > > interaction cross section?
> > > 2nd bullet mention improved detector.
> > >
> > > slide#2: Add bema energy and data taking year in both the figures.
> > >
> > > slide#3: Can you indicate the improvement in resolution relative to 
> > > BES-I?
> > >
> > > slide#4:
> > > The NCQ scaling holds within 30% for particles and within 15% for
> > > anti-particles which indicates the contribution from transported
> > > quarks in particles.
> > >
> > > What do we learn from the ratio v3/v2^3/2?
> > >
> > > Thanks and regards,
> > > Subhash
> > >
> > > On 2022-06-05 03:23 PM, pdixit via Star-fcv-l wrote:
> > > > Dear convenors,
> > > > I have updated my poster with the suggestions from the last FCV
> > > > meeting. Please have a look at the link below.
> > > > https://drupal.star.bnl.gov/STAR/system/files/SQM22_poster_v2.pdf
> > > >
> > > > Regards,
> > > > Prabhupada
> > > > On 2022-05-30 20:28, webmaster--- via Star-fcv-l wrote:
> > > > > Dear star-fcv-l AT lists.bnl.gov members,
> > > > >
> > > > > Prabhupada Dixit (prabhupadad AT iiserbpr.ac.in) has submitted a 
> > > > > material for a
> > > > > review, please have a look:
> > > > > https://drupal.star.bnl.gov/STAR/node/59774
> > > > >
> > > > > ---
> > > > > If you have any problems with the review process, please contact
> > > > > webmaster AT www.star.bnl.gov
> > > > > _______________________________________________
> > > > > Star-fcv-l mailing list
> > > > > Star-fcv-l AT lists.bnl.gov
> > > > > https://lists.bnl.gov/mailman/listinfo/star-fcv-l
> > > > _______________________________________________
> > > > Star-fcv-l mailing list
> > > > Star-fcv-l AT lists.bnl.gov
> > > > https://lists.bnl.gov/mailman/listinfo/star-fcv-l