STAR Flow, Chirality and Vorticity PWG

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

Dear convenors,

Since the deadline to submit the poster is approaching and if there are 
no further comments can we proceed further for the approval of the 
poster.

Thanks and regards,
Sharang

On 2023-08-28 21:27, sharangrav via Star-fcv-l wrote:
> Dear Fuqiang and FCV convenors,
>
> Thank you very much for signing off. Can we proceed further for the
> approval of the poster.
> https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2023/Directed-and-triangular-flow-identified-hadrons-and-light-nuclei-f-0
>
> Thanks and regards,
> Sharang
>
> On 2023-08-28 20:05, Wang, Fuqiang wrote:
> > I have no further comments. Thank you.
> >
> > Best regards,
> > Fuqiang
> >
> > > On Aug 28, 2023, at 8:36 AM, sharangrav <sharangrav AT rcf.rhic.bnl.gov> 
> > > wrote:
> > >
> > > [You don't often get email from sharangrav AT rcf.rhic.bnl.gov. Learn 
> > > why this is important at 
> > > https://urldefense.com/v3/__https://aka.ms/LearnAboutSenderIdentification__;!!P4SdNyxKAPE!HvtjkW8TxH7CpcX1Mt9SF2Yk_xPgHdQEW_AnrDO0WrsgGrGXgT3hfltAJLjraj-Km1WnBsjkzpaGXadU9_OWe9gNQ-Y$ 
> > >  ]
> > >
> > > ---- External Email: Use caution with attachments, links, or sharing 
> > > data ----
> > >
> > >
> > > Dear Fuqiang,
> > >
> > > A gentle reminder. If there are no further comments on my poster can 
> > > we
> > > proceed further.
> > > I have incorporated your previous comments and here is the link to my
> > > updated poster:
> > > https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2023/Directed-and-triangular-flow-identified-hadrons-and-light-nuclei-f-0
> > >
> > > Thanks and regards,
> > > Sharang
> > >
> > >
> > >
> > > > On 2023-08-26 13:21, sharangrav via Star-fcv-l wrote:
> > > > Dear Fuqiang,
> > > >
> > > > Thank you very much for your very valuable comments.
> > > >
> > > > Here is the link to my updated poster:
> > > > https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2023/Directed-and-triangular-flow-identified-hadrons-and-light-nuclei-f-0
> > > >
> > > > Here are some of the explanations:
> > > > The magnitude of pion also shows and increasing trend with rapidity
> > > > (as shown in the figure 4: left side in red marker) but its is
> > > > opposite direction because of shadowing effects at lower collision
> > > > energies.
> > > >
> > > > The proton v1 is measured over the range of 0.4 < pT < 2.0 GeV/c. In
> > > > this measurement, the lower cutoffs of light nucleus pT are 
> > > > restricted
> > > > to the same value in terms of pT/A (> 0.4 GeV/c). The pT upper 
> > > > limits
> > > > are determined based on the pT versus y acceptances. We have tried 
> > > > to
> > > > incorporate the maximum without compromising with the signal purity.
> > > >
> > > > In order to extract the slope parameter(a) for every particle of
> > > > interest we have used the 3rd order polynomial of form (ax+bx^3) and
> > > > considered the other order functions in systematics. Fitting is done
> > > > in range [y: 0,-1].
> > > >
> > > >
> > > > Please let me know if you have any further comments.
> > > >
> > > > Thanks and regards,
> > > > Sharang
> > > >
> > > >
> > > >
> > > >
> > > >
> > > >
> > > > > On 2023-08-25 16:40, webmaster--- via Star-fcv-l wrote:
> > > > > Dear star-fcv-l AT lists.bnl.gov members,
> > > > >
> > > > > Fuqiang Wang ( fqwang AT purdue.edu ) has commented on a material
> > > > > originally
> > > > > submitted by Sharang Rav Sharma (
> > > > > sharang.rav AT students.iisertirupati.ac.in )
> > > > > at
> > > > > https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2023/Directed-and-triangular-flow-identified-hadrons-and-light-nuclei-f-0
> > > > >
> > > > > Comment:
> > > > > Sharang,
> > > > >
> > > > > I was asked to review a few posters including yours. Please find my
> > > > > comments
> > > > > below.
> > > > >
> > > > > I would keep the section numbering and section title in the same
> > > > > color.
> > > > >
> > > > > Motivation:
> > > > > Just below Eq.1: reaction plane -> nth harmonic plane
> > > > > First bullet: delete one 'slope'
> > > > > Second bullet: shape -> shape fluctuations
> > > > >
> > > > > Methodology
> > > > > Add a note on the weight w_i
> > > > > Fig.2: add preliminary onto plots
> > > > >
> > > > > Results:
> > > > > Magnitude of í‘£1 increases with increasing rapidity for all the
> > > > > particles.
> > > > > -> but it's not the case for pion+
> > > > >
> > > > > It would be interesting to add the antiparticle results onto the 
> > > > > left
> > > > > plot.
> > > > >
> > > > > Fig.3 right plot: the pt ranges are not exactly according to A, 
> > > > > which
> > > > > makes
> > > > > the mass number scaling conclusion a bit loose. Would it be 
> > > > > possible
> > > > > to use
> > > > > the A-scaled pt range?
> > > > >
> > > > > Fig.4: would be useful to have the same horizontal range for all 
> > > > > three
> > > > > plots.
> > > > >
> > > > > Fig.4 right plot: the proton data point is inconsistent with the 
> > > > > fit
> > > > > curve in
> > > > > Fig.3 at the first glance. The fit is 3rd order polynomial so slope
> > > > > may not
> > > > > be readily obtained from the curve (but it does look very linear). 
> > > > > How
> > > > > do you
> > > > > actually obtain dv1/dy|y=0? Would be helpful to state that 
> > > > > explicitly.
> > > > >
> > > > > Fig.5 caption third line: delete one 'and'
> > > > >
> > > > > Summary:
> > > > > Add a bullet on mass scaling.
> > > > >
> > > > >
> > > > > ---
> > > > > If you have any problems with the review process, please contact
> > > > > webmaster@http://www.star.bnl.gov/
> > > > >
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