STAR Flow, Chirality and Vorticity PWG

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

Dear Subhash,

Thank you for your nice comments. I have incorporated your suggestions 
into my presentation slides accordingly.
Here is the updated link:
https://drupal.star.bnl.gov/STAR/presentations/Dynamics-QCD-2023/First-order-event-plane-correlated-directed-and-triangular-flow-fi-0
Please let me know if there are any further comments.

Thanks and regards,
Sharang Rav Sharma

On 2023-09-28 11:30, webmaster--- via Star-fcv-l wrote:
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Subhash Singha ( connectsubhash AT gmail.com ) has commented on a material
> originally submitted by Sharang Rav Sharma (
> sharang.rav AT students.iisertirupati.ac.in ) at
> https://drupal.star.bnl.gov/STAR/presentations/Dynamics-QCD-2023/First-order-event-plane-correlated-directed-and-triangular-flow-fi-0
>
> Comment:
> Hi Sharang,
>
> Nice slides. I am signing off with a few comments:
>
> s#4:  Last bullet I would suggest a rephrase, like contrary to higher 
> energy
> v3 is correlated to RP at 3 GeV and below; Then you say you are 
> extending it
> to 3.2-3.9 GeV; Also our recent 3 GeV v3 paper 2309.12610 should be 
> cited;
>
> s#5: You can probably make a bold font for energies you will be 
> presenting,
> 3.2-3.9;
>
> s#25: last bullet: " for all particles and light nuclei" --> for pi, p 
> and d;
>
>
> ---
> If you have any problems with the review process, please contact
> webmaster AT www.star.bnl.gov
> _______________________________________________
> Star-fcv-l mailing list
> Star-fcv-l AT lists.bnl.gov
> https://lists.bnl.gov/mailman/listinfo/star-fcv-l