Skip to Content.
Sympa Menu

star-fcv-l - Re: [Star-fcv-l] STAR presentation by Ashik Ikbal Sheikh for EESM 2022 submitted for review

star-fcv-l AT lists.bnl.gov

Subject: STAR Flow, Chirality and Vorticity PWG

List archive

Chronological Thread  
  • From: subhash <subhash AT rcf.rhic.bnl.gov>
  • To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] STAR presentation by Ashik Ikbal Sheikh for EESM 2022 submitted for review
  • Date: Wed, 30 Mar 2022 16:10:32 +0800

Dear Ashik,

Nice abstract. I have the following comments:

"...complicated by the low magnitude of directed flow..." --> It is true for mid-rapidity or higher beam energy, right? Can you be specific in the abstract.

" e.g., v1(Ω−(sss)) − v1(Ω¯ +(¯ss¯s¯))," --> This is under the assumption s and s-bar have same v1, right?

"We measure v1 as a function of rapidity; and then ∆q and ∆S dependence of v1..." --> First, we measure v1 as a function of rapidity; and then we estimate ∆q and ∆S dependence of v1...

" Parton-Hadron String Dynamics (PHSD) model + EM-field" --> Parton-Hadron String Dynamics (PHSD) model calculations including EM-field

I sign off once you address them.

Thanks and regards,
Subhash

On 2022-03-15 02:23 AM, webmaster--- via Star-fcv-l wrote:
Dear star-fcv-l AT lists.bnl.gov members,

Ashik Ikbal Sheikh (ashikhep AT gmail.com) has submitted a material for a
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/58864

---
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




Archive powered by MHonArc 2.6.24.

Top of Page