STAR Flow, Chirality and Vorticity PWG

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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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