STAR Flow, Chirality and Vorticity PWG

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

Dear Xing,

Thanks for your answer. BTW, are the beam energy same here between STAR 
and E895? If you mean there is a discrepancy at a same energy, I would 
suggest removing that sentence in the abstract, meanwhile make sure we 
have similar centrality, acceptance etc for an apple to apple 
comparison.

Thanks and regards,
Subhash

On 2024-12-11 03:08 PM, "Xing Wu" wrote:
> 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?
>
> ---
> If you have any problems with the review process, please contact
> webmaster AT www.star.bnl.gov

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