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Subject: STAR Flow, Chirality and Vorticity PWG
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Re: [Star-fcv-l] STAR presentation by Priyanshi Sinha for IS 2023 submitted for review
- 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 Priyanshi Sinha for IS 2023 submitted for review
- Date: Sun, 05 Mar 2023 08:45:32 +0530
Dear Priyanshi,
Nice abstract. I sign off with a few comments:
You can probably remove "It is essential to understand this difference .... to characterize them precisely." It looks redundant compared to previous line.
"Moreover, v2 measurements of the strange and multi-strange hadrons are excellent probes for understanding these initial state anisotropies of the medium produced in these collisions, owing to their smaller hadronic cross-section compared to light hadrons."
"System size dependence of v2 will also be ..." --> System size dependence of v2 will be
insight on --> insight into
Thanks and regards,
Subhash
On 2023-03-02 01:15 PM, webmaster--- via Star-fcv-l wrote:
Dear star-fcv-l AT lists.bnl.gov members,
Priyanshi Sinha (priyanshisinha AT students.iisertirupati.ac.in) has submitted a
material for a review, please have a look:
https://drupal.star.bnl.gov/STAR/node/62847
Deadline: 2023-03-10
---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
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[Star-fcv-l] STAR presentation by Priyanshi Sinha for IS 2023 submitted for review,
webmaster, 03/02/2023
- Re: [Star-fcv-l] STAR presentation by Priyanshi Sinha for IS 2023 submitted for review, subhash, 03/04/2023
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