STAR Flow, Chirality and Vorticity PWG

[pdixit <pdixit AT rcf.rhic.bnl.gov>]

Dear Subhash,
Thanks for the nice comments and suggestions. I have updated the 
abstract.
Link to the new version: 
https://drupal.star.bnl.gov/STAR/system/files/ATHIC_abstract_v2_0.pdf

Regards,
Prabhupada

On 2024-11-08 12:19, webmaster AT star.bnl.gov wrote:
> 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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