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Subject: STAR Flow, Chirality and Vorticity PWG
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Re: [Star-fcv-l] STAR presentation by Sharang Rav Sharma for Quark Matter 2023 got commented by Fuqiang Wang
- From: sharangrav <sharangrav AT rcf.rhic.bnl.gov>
- To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
- Cc: webmaster AT star.bnl.gov, sharang.rav AT students.iisertirupati.ac.in, fqwang AT purdue.edu
- Subject: Re: [Star-fcv-l] STAR presentation by Sharang Rav Sharma for Quark Matter 2023 got commented by Fuqiang Wang
- Date: Sat, 26 Aug 2023 09:51:07 +0200
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.
---
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[Star-fcv-l] STAR presentation by Sharang Rav Sharma for Quark Matter 2023 got commented by Fuqiang Wang,
webmaster, 08/25/2023
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Re: [Star-fcv-l] STAR presentation by Sharang Rav Sharma for Quark Matter 2023 got commented by Fuqiang Wang,
sharangrav, 08/26/2023
-
Re: [Star-fcv-l] STAR presentation by Sharang Rav Sharma for Quark Matter 2023 got commented by Fuqiang Wang,
sharangrav, 08/28/2023
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Re: [Star-fcv-l] STAR presentation by Sharang Rav Sharma for Quark Matter 2023 got commented by Fuqiang Wang,
sharangrav, 08/28/2023
-
Re: [Star-fcv-l] STAR presentation by Sharang Rav Sharma for Quark Matter 2023 got commented by Fuqiang Wang,
sharangrav, 08/26/2023
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