STAR Flow, Chirality and Vorticity PWG

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

Dear Subhash,

Thanks for your suggestions. I have modified the abstract based on your 
suggestion.

best regards,
Guangyu


> -----原始邮件-----
> 发件人: webmaster AT star.bnl.gov
> 发送时间: 2024-10-30 17:08:03 (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 Subhash Singha
> 
> Dear star-fcv-l AT lists.bnl.gov members,
> 
> Subhash Singha ( connectsubhash AT gmail.com ) 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:
> Dear Guangyu,
> 
> Nice abstract. I have a few suggestions:
> If your poster is focussed on directed flow, then I would suggest: "ϕ 
meson  
> flow" --> ϕ meson directed flow;
> 
> l#6: The ϕ meson is an excellent probe of the partonic phase due to its  
> small hadronic cross-section, making it less influenced by late-stage  
> interactions compared to other hadrons.
> 
> l#10, 10: nucleon --> proton
> 
> l#14, 15:The rapidity dependence of directed flow and its slope for the 
ϕ  
> meson will be presented as a function of beam energy and compared with  
> predictions from the AMPT-HC and JAM models.
> 
> l#16, 17: I don't know how we can connect it to "QCD phase structure". A 
 
> rephrase could be: Furthermore, the \phi meson will help understand  
> baryon/meson versus mass dependence in directed flow.
> 
> 
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