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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 68th DAE SYMPOSIUM ON NUCLEA... got commented by Subhash Singha
- From: sharangrav <sharangrav AT rcf.rhic.bnl.gov>
- To: star-fcv-l AT lists.bnl.gov
- Cc: webmaster AT star.bnl.gov, sharang.rav AT students.iisertirupati.ac.in
- Subject: Re: [[Star-fcv-l] ] STAR presentation by Sharang Rav Sharma for 68th DAE SYMPOSIUM ON NUCLEA... got commented by Subhash Singha
- Date: Fri, 06 Sep 2024 16:50:28 +0530
Dear Subhash,
Thank you for your valuable comments. I have incorporated the comments in the abstract and hereby sharing the link to the updated version.
https://drupal.star.bnl.gov/STAR/presentations/68th-DAE-SYMPOSIUM-NUCLEAR-PHYSICS/Measurement-directed-flow-high-baryon-density-regio
There was a page restriction so I have tried to keep everything under 2 page. Please let me know if you have further comments.
Thanks and regards,
Sharang
On 2024-09-06 13:39, webmaster AT star.bnl.gov wrote:
Dear star-fcv-l AT lists.bnl.gov members,
Subhash Singha ( connectsubhash AT gmail.com ) 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/68th-DAE-SYMPOSIUM-NUCLEAR-PHYSICS/Measurement-directed-flow-high-baryon-density-regio
Comment:
Dear Sharang,
Nice proceedings. I have a few suggestions below.
Please include line numbers.
Introduction:
"At these energies, --> "At these lower energies,
"This leads to a significant influence .... flow harmonics" --> This results
in a significant influence of the shadowing effect, where passing spectator
nucleons obstruct the interaction region, thereby affecting the measured flow
observables.
net-kaon, net-proton --> you could add definition for net-kaon and
net-proton, either here or in next section. It is not a particle itself, but
constructed from particle and antiparticle's v1.
= 3.2 – 4.5 GeV --> Specify each beam energies reported
Analysis Details:
"Mass-squared (m2)" --> Moreover, mass-squared (m2) information from TOF
"The reaction plane angle is estimated by the event plane method using Event
Plane Detector (EPD) within" --> The event plane angle, a proxy for the
reaction plane angle, is reconstructed using the Event Plane Detector (EPD),
which has coverage ...
"3 eta sub-events" --> 3 η-sub events, (also indicate the sub-event ranges)
Results:
"with increasing rapidity for all particle" --> with increasing rapidity for
all particles
"is attributed" --> can be attributed
"The net-kaon dv1/dy .... 19.6 GeV" --> The net-kaon dv1dy trend shows a
minimum between sqrt{s_{NN}} = 4.5 and 7.7 GeV, which happens at lower
collision energies than for net-protons, where the minimum is found between
sqrt{s_{NN}} = 11.5 and 19.6 GeV [7].
Reference [7] and [1] is same, please correct it
I sign off with these addressed.
---
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-
[[Star-fcv-l] ] STAR presentation by Sharang Rav Sharma for 68th DAE SYMPOSIUM ON NUCLEA... got commented by Subhash Singha,
webmaster, 09/06/2024
-
Re: [[Star-fcv-l] ] STAR presentation by Sharang Rav Sharma for 68th DAE SYMPOSIUM ON NUCLEA... got commented by Subhash Singha,
sharangrav, 09/06/2024
-
Re: [[Star-fcv-l] ] STAR presentation by Sharang Rav Sharma for 68th DAE SYMPOSIUM ON NUCLEA... got commented by Subhash Singha,
sharangrav, 09/10/2024
- Re: [[Star-fcv-l] ] STAR presentation by Sharang Rav Sharma for 68th DAE SYMPOSIUM ON NUCLEA... got commented by Subhash Singha, Richard Seto, 09/10/2024
-
Re: [[Star-fcv-l] ] STAR presentation by Sharang Rav Sharma for 68th DAE SYMPOSIUM ON NUCLEA... got commented by Subhash Singha,
sharangrav, 09/10/2024
-
Re: [[Star-fcv-l] ] STAR presentation by Sharang Rav Sharma for 68th DAE SYMPOSIUM ON NUCLEA... got commented by Subhash Singha,
sharangrav, 09/06/2024
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