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star-fcv-l - [Star-fcv-l] STAR presentation by Zuowen Liu for Quark Matter 2023 got commented by Prithwish Tribedy

star-fcv-l AT lists.bnl.gov

Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: webmaster AT star.bnl.gov
  • To: star-fcv-l AT lists.bnl.gov
  • Subject: [Star-fcv-l] STAR presentation by Zuowen Liu for Quark Matter 2023 got commented by Prithwish Tribedy
  • Date: Sat, 22 Apr 2023 15:19:53 -0400

Dear star-fcv-l AT lists.bnl.gov members,

Prithwish Tribedy ( ptribedy AT bnl.gov ) has commented on a material originally

submitted by Zuowen Liu ( liuzw AT mails.ccnu.edu.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2023/Anisotropic-flow-identifed-particles-Au-Au-Collisions-sqrtsNN-30-196

Comment:
Very nice abstract! The version 1 is already in a very good shape. The first
para can be made a bit more cohesive but the current version is still
effective.,,,

Here are some minor comments:,,,

"Equation of State (EoS)"-->"equation of state (EoS)" (I think),,,

"complementary information" --> "valuable information",,,


After this line add a line as follows:,,,
"Studying these flow harmonics for various identified particles at different
energies provides insights on a medium going through QCD phase transition."

"early stage" -->"early stages",,,

"may provide" --> "making them cleaner probe to provide",,,


Basically you can change this sentence:
"(Multi-)strange hadrons with small hadronic cross-sections may provide
information primarily from the early stage of the heavy-ion collisions and
are
important for the study of the QCD phase diagram at RHIC."
-->
"In particular, multi-strange hadrons with small hadronic cross-sections are
cleaner probes of the early stages of heavy-ion collisions",,,

And the following as the last sentence of the first paragraph:
"A comparative study of light and multi-strange hadrons provides valuable
insights into the subsequent stages of the medium evolution.",,,

For line 10-13, revise the sentence as follows:
In this talk, the measurements of v1,v2 and v3 for both light and
(multi-)strange hadrons at √sNN = 3.0, 3.2, 3.5, 3.9, 7.7, 9.2, 11.5, 14.6,

and 19.6 GeV , utilizing the enhanced capabilities of the STAR detector and
enhanced statistics datasets from the second phase of the RHIC beam energy
scan (BES-II) program, will be presented.






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