STAR Flow, Chirality and Vorticity PWG

[webmaster AT star.bnl.gov]

Dear star-fcv-l AT lists.bnl.gov members,

Subhash Singha ( connectsubhash AT gmail.com ) has commented on a material  
originally submitted by Prabhupada Dixit ( prabhupadad AT iiserbpr.ac.in ) at
https://drupal.star.bnl.gov/STAR/presentations/10th-Asian-Triangle-Heavy-Ion-Conference-ATHIC-2025/Azimuthal-anisotropic-flow-measure

Comment:
Dear Prabhupada, Nice abstract. I have a few suggestions for your  
consideration:

"One of the primary objectives of the STAR experiment is to identify the  
”turnoff” signature of the Quark-Gluon Plasma (QGP). This can be  
investigated through measurements of the collective flow of particles  
produced in heavy-ion collisions"
--> One of the primary objectives of the STAR experiment is to identify the  
disappearance of the Quark-Gluon Plasma (QGP). This can be investigated by  
studying the collective flow of various particle types produced in heavy-ion  
collisions, particularly by testing whether the number of constituent quark  
(NCQ) scaling holds or breaks across different energies.

"hadrons—including .... —from" --> hadrons, including ..... , from

"at center-of-mass energies √ sNN ranging from 3.0 to 19.6 GeV" --> at √  
sNN - 3.0 - 19.6 GeV.

as well as the NCQ scaling of v_n


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