STAR Flow, Chirality and Vorticity PWG

["Junyi Han" <jyhan AT mails.ccnu.edu.cn>]

Dear Subhash,

Thank you for your nice suggestions! I have update the abstract based on your suggestions, and it can be found in this link: https://drupal.star.bnl.gov/STAR/system/files/INPC_2025_abstract_v3.pdf.

For hyper-nuclei v2, we don't make sure if we have enough statistics in other FXT energies to measure them. But for v1, I think we can include other FXT energies results. Thanks!

Best regards,

Junyi

 

 

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

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

Date:  Wed, Dec 18, 2024 03:16 AM

To:  "STAR Flow, Chirality and Vortici"<star-fcv-l AT lists.bnl.gov>;

Subject:  [[Star-fcv-l] ] STAR presentation by Junyi Han for INPC 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 Junyi Han ( jyhan AT mails.ccnu.edu.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/INPC-2025/Flow-measurements-hyper-and-light-nuclei-AuAu-collisions-30-GeV-RHIC-1

Comment:
Dear Junyi, Nice abstract. I have following comments:

l#7: About 2 billion minimum bias ....
l#10: p, d, t, 3He and 4He

Why do you want to focus on only 3 GeV, do you plan to include flow results 
from other FXT energies as well?

---
If you have any problems with the review process, please contact 
webmaster AT www.star.bnl.gov