STAR Flow, Chirality and Vorticity PWG

["Xing Wu" <wuxing6218 AT mails.ccnu.edu.cn>]

Hi Subhash,

Thank you for your nice comments and I have updated the version, please find in the link:

https://drupal.star.bnl.gov/STAR/presentations/Hot-Quarks-2025/Anisotropic-Flow-Identified-Particles-AuAu-Collisions-sqrtsNN-30-45--0

Question: l#14: "The anti-flow of K0S measured by STAR is a factor of eight lower ... "  --> It is not clear what do you mean? Is it v1 or v2? Why a factor of eight lower at similar energies?

Answer: Please take a look at the picture below.

Best regards，

Xing Wu

 

 

------------------ Original ------------------

From:  "webmaster"<webmaster AT star.bnl.gov>;

Date:  Wed, Dec 11, 2024 11:53 AM

To:  "star-fcv-l"<star-fcv-l AT lists.bnl.gov>;

Subject:  [[Star-fcv-l] ] STAR presentation by Xing Wu for Hot Quarks 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 Xing Wu ( wuxing6218 AT mails.ccnu.edu.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/Hot-Quarks-2025/Anisotropic-Flow-Identified-Particles-AuAu-Collisions-sqrtsNN-30-45--0

Comment:
Dear Xing, Nice abstract. I sign off with a few suggestions for your 
consideration:

l#9 and in title: please spell out beam energies between 3.0 - 4.5 GeV
l#10: spell out NCQ
l#14: "The anti-flow of K0S measured by STAR is a factor of eight lower ... " 
--> It is not clear what do you mean? Is it v1 or v2? Why a factor of eight 
lower at similar energies?


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