STAR Flow, Chirality and Vorticity PWG

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

Dear Subhash,

Thank you very for your nice comments and suggestions. I have submitted 
the updated slides on Drupal page and also sharing the link to the same
https://drupal.star.bnl.gov/STAR/presentations/68th-DAE-SYMPOSIUM-NUCLEAR-PHYSICS/Measurement-directed-flow-high-baryon-density-reg-0

In this presentation, we are only showing results that have already been 
preliminarily approved.
Regarding the net-kaon minimum, we are still working on some theoretical 
model calculations to finalise the physics interpretation.
For the light nuclei (p and d) v1 slope, it generally follows 
approximate mass number scaling at lower energies. However, as you 
correctly pointed out, particularly for tritons, we observe a deviation 
from the mass number scaling behaviour as we move from 3.2 GeV to 
comparatively higher energies like 4.5 GeV.

Thanks and regards,
Sharang

On 2024-11-25 18:47, subhash wrote:
> Dear Sharang,
>
> Nice slides. I have a few questions and suggestions:
>
> Could you point to me if you have any new candidate of preliminary,
> that will be shown for the first time?
>
> s#3: suggest to remove "Predicted" from first bullet, because I
> believe it is common for all the bullets? and they will probed using
> BES data.
>
> s#4:You can also mention the mu_B corresponding to beam energy of 
> interest.
>
> s#5: left figure, can you make the labels for individual particles
> prominent like you did for the rhs figure.
>
> s#7: "Signature of 1st order phase transition" --> I don't think we
> should say, this is the signature of 1st order PT. You can rephrase it
> as, predicted signature for softening of EoS near 1st order phase
> transition. Then also add a reference of the study (Stoeker et al ?)
> "No minima for net-K" --> not sufficient data to locate possible
> minima for net-K using BES-I data or no minima observed for net-K with
> BES-I data
> BTW, do you know what do we learn with minimum of net-kaon, any theory
> predictions?
> "Approximate mass no. scaling" --> perform mass number scaling with
> precise BES-II data (because for BES-I uncertainties are quite large,
> central values for p and d are opposite)
> you can probably rephrase suggested wordings accordingly
>
> "Nucleon coalescence" --> test of Nucleon coalescence, because it
> seems the triton is clearly not scaling with A, right?
>
> s#9: add a reference for JAM model,
> the legends for JAM seems blurred in my screen.
> when you say "JAM with mean-field gives better description to the
> experimental data", can you point out which scenario is favored than
> the other, NS2 vs MD2?
>
>
> s#11: "No requirement of Kaon potential" --> I think better to say,
> kaon potential is not necessary or not a necessary condition
>
>
> #12: "Might be a signature of 1st order phase transition" --> May be
> we can rephrase it as "the connection with changes in the Equation of
> State (EoS) is to be explored"
> "JAM mean-field gives a better description ..." --> can we say
> anything on preferred compressibility parameter?
>
> ps: I believe Drupal is back, and you can upload your updated 
> presentation.
>
> Thanks and regards,
> Subhash
>
> On 2024-11-25 11:28 AM, sharangrav wrote:
> > Dear convenors,
> >
> > I hope this email finds you well. I am experiencing difficulty
> > connecting to the server to upload my presentation for the conference,
> > as it has been offline for the past two days. Therefore, I am sharing
> > my presentation slides here in this email thread for your kind review
> > and valuable comments.
> > I would greatly appreciate it if you could let me know of any comments
> > or suggestions. Once the server is back online, I will promptly submit
> > my slides there as well.
> > Thank you very much for your time and kind consideration.
> >
> > Thanks and regards,
> > Sharang Rav Sharma
> >
> >
> > On 2024-09-04 17:36, webmaster AT star.bnl.gov 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/68805
> > >
> > > Deadline: 2024-09-15
> > > ---
> > > If you have any problems with the review process, please contact
> > > webmaster AT www.star.bnl.gov