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Subject: STAR Flow, Chirality and Vorticity PWG
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[Star-fcv-l] Comments for Shengli Huang for QM22 talk from FCV conveners
- From: ShinIchi Esumi <esumi.shinichi.gn AT u.tsukuba.ac.jp>
- To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
- Subject: [Star-fcv-l] Comments for Shengli Huang for QM22 talk from FCV conveners
- Date: Mon, 22 Nov 2021 15:36:41 +0900
Dear Shengli (and Prithwish)
The followings are comments on your merged talk abstract from conveners.
Best regards, Jiangyong, Prithwish and ShinIchi
---------------------------------------
Jiangyong
Title-->remove "in varying system sizes"
L2 in the community of relativistic collisions --> in the heavy ion community.
L15 We exploit the advantage of wide mid-rapidity acceptance of Time Projection Chamber
(-1< η <1) of STAR to facilitate apples-to-apples comparison with boost-invariant model predictions. In addition, we make... --> In addition to the results obtained from the mid-rapidity acceptance (|eta|<1), we also use the Event Plane detector over 2.1<|eta|<5.1 to investigate
L21-24. How about: The photo-nuclear gamma+Au candidate events in Au+Au collisions were selected by requiring a single neutron hit on one side of the Zero-degree calorimeter.
L27 how about "to further improve the purity of gamma+Au events.
L29 harmonic anisotropy coefficients...--> v_n coefficients in gamma+Au events.
Prithwish:
The abstract is a bit long.
Combine 1st and 2nd sentence:
“The origin of collectivity in small collision systems is one of the most debated topics in the community of relativistic collisions. A satisfactory microscopic explanation of how collectivity originates and evolves with collision system size is still outstanding”
→
“A satisfactory explanation of how collectivity originates and evolves with collision system size is a highly debated topic in the community of relativistic collisions.”
“To address this problem” → “To address this topic”
“The pseudorapidity distribution of particles is strongly asymmetric in these interactions and the wide acceptance coverage of the STAR detector using TPC, Beam-Beam Counter and Vertex 27 Position Detector is exploited to improve the purity of the γ+Au-rich samples.”
→
“We further exploit the combination of STAR forward detectors to trigger on pseudorapidity asymmetry to improve the purity of the γ+Au-rich samples.”
ShinIchi
L1-15: Can you make it short at least about a half of this first part.
L17: “apples-to-apples comparison with boost…” part is not clear... compared to what? Phenix?
Use of EPD for isobar data (including wide TPC acceptance part), or at least, photo-nuclear part would be separated as a new paragraph.
---------------------------------------
On Nov 17, 2021, at 4:49, webmaster--- via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:Dear star-fcv-l AT lists.bnl.gov members,
Shengli Huang (shengli.huang AT stonybrook.edu) has submitted a material for a
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/57268
---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
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-
[Star-fcv-l] STAR presentation by Shengli Huang for Quark Matter 2022 submitted for review,
webmaster, 11/01/2021
- <Possible follow-up(s)>
-
[Star-fcv-l] STAR presentation by Shengli Huang for Quark Matter 2022 submitted for review,
webmaster, 11/16/2021
-
[Star-fcv-l] Comments for Shengli Huang for QM22 talk from FCV conveners,
ShinIchi Esumi, 11/22/2021
- Re: [Star-fcv-l] Comments for Shengli Huang for QM22 talk from FCV conveners, Shengli Huang, 11/23/2021
-
[Star-fcv-l] Comments for Shengli Huang for QM22 talk from FCV conveners,
ShinIchi Esumi, 11/22/2021
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