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Subject: STAR Flow, Chirality and Vorticity PWG
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[Star-fcv-l] Comments for Takafumi Niida for QM22 poster from FCV conveners
- From: ShinIchi Esumi <esumi.shinichi.gn AT u.tsukuba.ac.jp>
- To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
- Subject: [Star-fcv-l] Comments for Takafumi Niida for QM22 poster from FCV conveners
- Date: Tue, 23 Nov 2021 13:00:01 +0900
Dear Takafumi
The followings are comments for your QM22 poster from conveners.
We are ready to sign off.
Best regards, Jiangyong, Prithwish and ShinIchi
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Prithwish
L7: “can clarify the problem” → “may shed light on this problem”
L7: “One can also expect similar local polarization” → Please specify “similar” to what ?
L8: “higher harmonic flow” → Please specify “higher” than what?
L9: Remove: “if it exists”
L11: Specify the energy of Au+Au collisions or say at same energy as isobar.
Jiangyong
The abstract is well written just a minor comment
L11 isobar collisions→ make clear that this is Ru+Ru and Zr+Zr collisions.
ShinIchi
I’m fine to sign off, it would be nice, if you can compare with your blast wave calculations which you have done for the 2nd order…
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On Nov 16, 2021, at 11:23, webmaster--- via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:Dear star-fcv-l AT lists.bnl.gov members,
Takafumi Niida (niida.takafumi.fw AT u.tsukuba.ac.jp) has submitted a material
for a review, please have a look:
https://drupal.star.bnl.gov/STAR/node/57246
---
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 Takafumi Niida for Quark Matter 2022 submitted for review,
webmaster, 11/15/2021
-
[Star-fcv-l] Comments for Takafumi Niida for QM22 poster from FCV conveners,
ShinIchi Esumi, 11/22/2021
- Re: [Star-fcv-l] Comments for Takafumi Niida for QM22 poster from FCV conveners, Takafumi Niida, 11/23/2021
-
[Star-fcv-l] Comments for Takafumi Niida for QM22 poster from FCV conveners,
ShinIchi Esumi, 11/22/2021
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