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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: Jiangyong Jia <jiangyong.jia AT stonybrook.edu>
  • To: 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: Mon, 25 Jul 2022 11:14:01 -0400

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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