Skip to Content.
Sympa Menu

star-fcv-l - Re: [Star-fcv-l] STAR presentation by Zuowen Liu for ISMD2022 submitted for review

star-fcv-l AT lists.bnl.gov

Subject: STAR Flow, Chirality and Vorticity PWG

List archive

Chronological Thread  
  • From: subhash <subhash AT rcf.rhic.bnl.gov>
  • To: Zuowen Liu <liuzw AT mails.ccnu.edu.cn>
  • Cc: star-fcv-l <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] STAR presentation by Zuowen Liu for ISMD2022 submitted for review
  • Date: Wed, 27 Jul 2022 10:14:33 +0800

Dear Zuowen,

Thanks for the updated slides. I sign off with a few additional suggestions:

s#3: top left: COLLIDER

s#8-11: Mention BES-II somewhere in the slides.

s#9: mention whether uncertainties are only statistical or, systematic included.
Above the bullets, add "In mid-central collisions:"
1st bullet: Say Negative slope for kaons. Then say sign consistent with UrQMD, but underestimate the magnitude.
2nd bullet: There is an asymmetry in phi v1. Could you remind me what is the significance of v1 slope to be positive? If it is not significant, I would rephrase it as hints of positive v1 slope is observed. Then say consistent with UrQMD.
3rd butter: First mention the observation: Both proton and lambda show negative v1 slope. Then say UrQMD shows opposite trend.

s#10: Here also add the definition of net-particle v1

Thanks and regards,
Subhash

On 2022-07-26 06:07 PM, Zuowen Liu wrote:
Dear Subhash,

I understood the decision made by conveners.
I would delete v1 results at 14.6 GeV in my slides.

Thank you for your other comments. I have implemented them into the
slides.
Kindly find the modified slides by the link:
https://drupal.star.bnl.gov/STAR/system/files/ISMD_presentation.pdf

Thanks and Best regards,
Zuowen

------------------ Original ------------------

From: "subhash"<subhash AT rcf.rhic.bnl.gov>;
Date: Tue, Jul 26, 2022 09:50 AM
To: "star-fcv-l"<star-fcv-l AT lists.bnl.gov>;
Cc: "liuzw"<liuzw AT mails.ccnu.edu.cn>;
Subject: Re: [Star-fcv-l] STAR presentation by Zuowen Liu for
ISMD2022 submitted for review

Dear Zuowen,

Nice slides. Here are my comments:

General:
For 14.6 GeV results in finer centrality bins, we have discussed at
the
conveners meeting. It is decided that no centrality results will be
released until the official announcement by the centrality group. This

is to make sure all corrections in centrality (vz corrections, pile up

etc) are in place and finalized. Sorry about that. We believe you
still
have enough materials to present at ISMD.

s#7: Mention on the right panel 2019 or BES-II

s#8: Top resolution plot: mention Psi1 resolution
Mention the errors are statistical inside the bottom panels.

Summary slide:
"more precise measurement" --> You could specify example from 19.6 GeV

(factor of 8 reduction)

"Centrality dependence of net-particle dv1/dy" --> Mention the sign
change and the behavior. Then say offer more constraint.

You could stress on observation. e.g. "UrQMD shows oppositive trend of

proton and lambda" --> Say what we observe in data, then mention UrQMD

trend and/or say it does not describe data.

Thanks and regards,
Subhash

On 2022-07-20 04:46 PM, webmaster--- via Star-fcv-l wrote:
Dear star-fcv-l AT lists.bnl.gov members,

Zuowen Liu (liuzw AT mails.ccnu.edu.cn) has submitted a material for a
review,
please have a look:
https://drupal.star.bnl.gov/STAR/node/60349

---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
_______________________________________________
Star-fcv-l mailing list
Star-fcv-l AT lists.bnl.gov
https://lists.bnl.gov/mailman/listinfo/star-fcv-l




Archive powered by MHonArc 2.6.24.

Top of Page