STAR Flow, Chirality and Vorticity PWG

[webmaster AT star.bnl.gov]

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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