Skip to Content.
Sympa Menu

star-fcv-l - Re: [Star-fcv-l] STAR presentation by Dhananjaya Thakur for Hot QCD Matter 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>
  • Cc: thakurdhana AT gmail.com
  • Subject: Re: [Star-fcv-l] STAR presentation by Dhananjaya Thakur for Hot QCD Matter 2022 submitted for review
  • Date: Tue, 12 Apr 2022 13:26:11 +0800

Dear Dhananjaya,

Nice abstract. I am fine with it once you address the following suggestions.

magnetic filed --> magnetic field

The difference v1 slope --> The difference of v1 slope

Replace Delta v1/dy with Delta dv1/dy at several places

"Contribution from transported quark ... predicted to give negative ..." --> While the contribution from transported quark can give positive .., the electromagnetic field is predicted ..."

"...proton in peripheral collisions consistent with the theoretical prediction, and favours the presence of initial strong electromagnetic field in heavy-ion collisions." --> ..proton in peripheral collisions is consistent with the prediction from initial strong electromagnetic field in heavy-ion collisions.

Thanks and regards,
Subhash

On 2022-04-12 12:57 PM, webmaster--- via Star-fcv-l wrote:
Dear star-fcv-l AT lists.bnl.gov members,

Dhananjaya Thakur (thakurdhana AT gmail.com) has submitted a material for a
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/59142

---
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