STAR Flow, Chirality and Vorticity PWG

[郑光裕 <zhengguangyu23 AT mails.ucas.ac.cn>]

Dear Richard

Thanks for your suggestions,I have modified the abstract accordingly.
The updated version is at the same link.
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2025/phi-meson-directed-flow-3GeV-45GeV-AuAu-collisions-STAR

Best regrads
Guangyu


> -----原始邮件-----
> 发件人: webmaster AT star.bnl.gov
> 发送时间: 2024-11-06 06:41:54 (星期三)
> 收件人: star-fcv-l AT lists.bnl.gov
> 抄送: 
> 主题: [[Star-fcv-l] ] STAR presentation by Guangyu Zheng for Quark Matter 
2025 got commented by Richard  Seto
> 
> Dear star-fcv-l AT lists.bnl.gov members,
> 
> Richard  Seto ( richard.seto AT ucr.edu ) has commented on a material 
originally  
> submitted by Guangyu Zheng ( zhengguangyu23 AT mails.ucas.ac.cn ) at
> 
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2025/phi-meson-directed-flow-3GeV-45GeV-AuAu-collisions-STAR
> 
> Comment:
> rewriting the 2nd sentence:In the energy range of the STAR Beam Energy 
Scan  
> II (BES II), the directed flow (v₁) of net-baryons has been suggested as 
a  
> sensitive probe of the equation of state of hot and dense matter. The 
phi  
> meson, with its mass close to that of the proton but with strange (s̄s)  
> quark content, provides a unique test for understanding the differences  
> between net-baryon and net-meson directed flow.
> 
> 
> ---
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