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Subject: STAR Flow, Chirality and Vorticity PWG
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Re: [Star-fcv-l] STAR presentation by Xiaoyu Liu for ATHIC 2023 submitted for review
- From: subhash <subhash AT rcf.rhic.bnl.gov>
- To: star-fcv-l AT lists.bnl.gov, liu.6566 AT osu.edu
- Subject: Re: [Star-fcv-l] STAR presentation by Xiaoyu Liu for ATHIC 2023 submitted for review
- Date: Mon, 03 Apr 2023 16:25:39 +0800
Dear Xiaoyu,
Very nice slides. I sign off with a few minor comments:
s#7: Do you calculate resolution for different vz bins? I ma wondering how different are they for different vz selections?
s#14: You could indicate the Y-axis of lower panel, like you did in the subsequent slides.
s#22: 2nd bullet : "... at far forward and backward \eta (|\eta| > 1.0) using ....".
Because strictly speaking, we do have measurement within +/- 1.0
4th bullet: May be a better phrase, UrQMD fails to describe the measured v1(\eta) quantitatively.
5th bullet: I guess you mean \eta/S of the medium?
Thanks and regards,
Subhash
On 2023-04-01 03:40 PM, webmaster--- via Star-fcv-l wrote:
Dear star-fcv-l AT lists.bnl.gov members,
Xiaoyu Liu (liu.6566 AT osu.edu) has submitted a material for a review, please
have a look:
https://drupal.star.bnl.gov/STAR/node/63166
Deadline: 2023-04-24
---
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 Xiaoyu Liu for ATHIC 2023 submitted for review,
webmaster, 04/01/2023
- Re: [Star-fcv-l] STAR presentation by Xiaoyu Liu for ATHIC 2023 submitted for review, subhash, 04/03/2023
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