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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Subhash Singha for Quark Matter 2022 submitted for review

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: subhash <subhash AT rcf.rhic.bnl.gov>
  • To: Jiangyong Jia <jiangyong.jia AT stonybrook.edu>, "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] STAR presentation by Subhash Singha for Quark Matter 2022 submitted for review
  • Date: Tue, 26 Jul 2022 09:41:32 +0800

Dear Jiangyong,

Thanks for your nice comments. I have incorporated them and the updated version is uploaded in the same link.

Thanks and regards,
Subhash

On 2022-07-25 11:14 PM, Jiangyong Jia via Star-fcv-l wrote:
Hi, Subash,

A few comments on your nice proceedings.
Jiangyong

Latex type setting should be used N_{\mathrm{part}}, p_{\mathrm{T}},
R_{2,\mathrm{TPC}} etc...

L1 We report the measurements of spin alignment (rho_00) for K... add
comma before K*+.

L28 The spin alignment is quantified... density matrix, rho_00, and

L35/36 and many other places (1/3) -->\frac{1}{3}

L43. a positive contribution to rho_00, rho_00-1/3 ~ 10^-4
L45 with a negative contribution to rho_00, rho_00-1/3~-10^-5

L87 remove (1/beta) since you never used it later
L92 originate-->originating
L100. (m0 ± 3Γ) ->m0 ± 3Γ

On 7/16/22 12:11 AM, webmaster--- via Star-fcv-l wrote:

Dear star-fcv-l AT lists.bnl.gov members,

Subhash Singha (connectsubhash AT gmail.com) has submitted a material
for a
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/60302

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