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star-fcv-l - [[Star-fcv-l] ] 回复: STAR presentation by Ze Qiu for Quark Matter 2025 got commented by Richard Seto

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: "仇泽" <zeqiu AT mails.ccnu.edu.cn>
  • To: "star-fcv-l" <star-fcv-l AT lists.bnl.gov>
  • Subject: [[Star-fcv-l] ] 回复: STAR presentation by Ze Qiu for Quark Matter 2025 got commented by Richard Seto
  • Date: Fri, 1 Nov 2024 00:04:06 +0800

Dear Richard,

Thank you for your suggestion. I have updated my abstract. Please find in the below link:
https://drupal.star.bnl.gov/STAR/node/69785

Best regards,
Ze


webmaster<webmaster AT star.bnl.gov> 在 2024年10月30日 周三 4:47 写道:
Dear star-fcv-l AT lists.bnl.gov members,

Richard  Seto ( richard.seto AT ucr.edu ) has commented on a material originally 
submitted by Ze Qiu ( zeqiu AT mails.ccnu.edu.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2025/Directed-flow-pions-kaons-and-protons-AuAu-collisions-%E2%88%9AsNN-173-GeV-0

Comment:
Here is a rewrite
Quantum Chromodynamics (QCD) predicts that hadronic matter transitions to a 
deconfined state called the Quark-Gluon Plasma (QGP) at extremely high 
temperatures and densities. Heavy-ion collisions create these extreme 
conditions, enabling studies of the nuclear matter phase diagram, QGP 
properties, and the QCD phase transition. The directed flow (v1), which is 
the first harmonic coefficient in the Fourier expansion of the azimuthal 
distribution relative to the collision reaction plane, is sensitive to the 
equation of state of the produced matter and may provide information about 
the QGP phase transition.

The 2nd paragraph is fine



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  • [[Star-fcv-l] ] 回复: STAR presentation by Ze Qiu for Quark Matter 2025 got commented by Richard Seto, 仇泽, 10/31/2024

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