STAR Flow, Chirality and Vorticity PWG

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

Dear Subhash,

Please let me know if you have any further comments.

Thanks and regards,
Sharang


On 2023-08-17 16:26, sharangrav via Star-fcv-l wrote:
> Dear Subhash,
>
> Thanks for the valuable suggestions. I have updated the slides and
> here is the link to the same:
> https://drupal.star.bnl.gov/STAR/node/64502
>
> You are right about v3^odd of deuteron. It is not the part of current
> 3 GeV paper. This is first time we are observing it in our analysis.
>
> Thanks and regards,
> Sharang Rav Sharma
>
>
> On 2023-08-17 12:39, subhash wrote:
> > Dear Sharang,
> >
> > Thanks for considering my suggestions.
> >
> > I would suggest to mention in respective slides if v1 fit functions
> > and/or pt-acceptance are different between different data sets,
> > especially for published vs. preliminary slides s#15, 17, 19, 22, 24.
> >
> > s#23: I already asked this. Do you know why the sign of p and d are
> > different for 3.9 GeV?
> > My recollection is that we never presented v3^odd of deuteron outside
> > (and also not part of current 3 GeV v3^odd paper) because we don't
> > understand the difference between them.
> >
> > A few minor edits:
> > s#15: title you could add (pi, K, p)
> > s#17: similarly net p and net K in title
> > s#19: title (p, d, t)
> >
> > Thanks and regards,
> > Subhash
> >
> >
> >
> > On 2023-08-16 02:13 AM, sharangrav wrote:
> > > Dear Subhash,
> > >
> > > Thank you for your nice comments and suggestions. I have incorporated
> > > your suggestion in my presentation slides and here is the link to my
> > > updated slides:
> > >
> > > https://drupal.star.bnl.gov/STAR/node/64502
> > >
> > > Here are some of the explanations to your comments:
> > > s#15: Are the pt-acceptance and v1 fit function same for published 
> > > and
> > > this analysis?
> > > The pT acceptance is the same. The fit function for collider energies
> > > was 1st order polynomial. In published 3 GeV (FXT) and my analysis 
> > > 3rd
> > > order polynomial is implemented (1st order polynomials is 
> > > incorporated
> > > in systematics)
> > >
> > > s#17: same question as above, is the pt-acceptance same? Visually,
> > > your net-p points doesn't seem to be smooth as function sNN!
> > > The pT acceptance is the same. The fit function for collider energies
> > > was 1st order polynomial. In my analysis 3rd order polynomial is
> > > implemented (1st order polynomials is incorporated in systematics)
> > >
> > > s#22: What is the pt-acceptance of HADES?
> > > pT for HADES: [1 - 1.5 GeV/c]
> > >
> > > s#23: On the coalescence point of view, how do we understand 
> > > different
> > > sign of v3^odd for p and d?
> > > Within systematics the slope for scaled v3 (d(v3/A)/dy) for both
> > > proton and deuteron seems consistent with each other
> > >
> > > Please let me know if you have any further comments.
> > >
> > > Thanks and regards,
> > > Sharang Rav Sharma
> > >
> > >
> > > On 2023-08-14 16:16, subhash via Star-fcv-l wrote:
> > > > Dear Sharang,
> > > >
> > > > Nice presentation. I have a few question and suggestions for your 
> > > > consideration:
> > > >
> > > > In general: when presenting dvn/dy and comparing different data, it
> > > > would be good to indicate whether the pt-acceptance is same or not. 
> > > > I
> > > > have indicated specific slide numbers below.
> > > >
> > > > s#4:  minimum in v1 --> minimum in baryon's dv1/dy sensitive to 
> > > > softening of EoS
> > > > s#5: Correct the typo:  3.2,
> > > >
> > > > s#7 or 8: you could indicate the sub-events eta ranges used for
> > > > resolution calculation
> > > >
> > > > s#9: You could indicate the beam energy in figure panel
> > > > Although you have mentioned, a line/box in the 2D plots indicating 
> > > > the
> > > > acceptance used would be helpful.
> > > >
> > > > s#15: Are the pt-acceptance and v1 fit function same for published 
> > > > and
> > > > this analysis?
> > > >
> > > > s#17: same question as above, is the pt-acceptance same? Visually,
> > > > your net-p points doesn't seem to be smooth as function sNN!
> > > >
> > > > I would suggest to remove bullet "signature of first-order phase
> > > > transition" here. Also I would not say "Similar trend is observed 
> > > > for
> > > > net-kaon". Important observation is that the turn-over of net-p and
> > > > net-K seems to be at different energy. BTW, do you have any
> > > > explanation for this observation?
> > > >
> > > > s#21: Weak rapidity dependence is not true for protons especially at
> > > > 3.2 GeV. Please rephrase bullets according to particle species.
> > > >
> > > > s#22: What is the pt-acceptance of HADES?
> > > >
> > > > s#23: On the coalescence point of view, how do we understand 
> > > > different
> > > > sign of v3^odd for p and d?
> > > >
> > > > s#24: Is it possible to add the EoS model lines on s#4 rightmost 
> > > > plot
> > > > here in this plot?
> > > >
> > > > s#25: Since you are doing A-scaling for p and d with both v1^odd and
> > > > v3^odd, can you make a statement on coalescence mechanism?
> > > >
> > > > Thanks and regards,
> > > > Subhash
> > > >
> > > > On 2023-08-07 06:46 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/64502
> > > > >
> > > > > Deadline: 2023-08-21
> > > > > ---
> > > > > If you have any problems with the review process, please contact
> > > > > webmaster AT www.star.bnl.gov
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