STAR Flow, Chirality and Vorticity PWG

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

Hi Subhash,

Yes, we have ensured consistency among these cuts during our work. I have removed this sentence from the abstract.

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

Best regards，

Xing Wu  

 

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

From:  "subhash"<subhash AT rcf.rhic.bnl.gov>;

Date:  Wed, Dec 11, 2024 03:21 PM

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

Subject:  Re: [[Star-fcv-l] ] STAR presentation by Xing Wu for Hot Quarks 2025 got commented by Subhash Singha

 

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