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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Niseem Magdy Abdelwahab Abdelrahman for DNP 2022 submitted for review

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: Prithwish Tribedy <ptribedy 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 Niseem Magdy Abdelwahab Abdelrahman for DNP 2022 submitted for review
  • Date: Sun, 23 Oct 2022 19:00:20 -0400

Dear Niseem,
Your slides are very similar to what you have presented before. I sign off with a few minor comments.

General comment: Since this is an in-person talk, I think some of the fonts you've used are too small for the audience.

Slide#2: "more susceptible" than what? Individual v_ns ?

Slide#3: Please provide some details about the STAR datasets, detectors & acceptance used in this analysis.

Slide#4: Please provide the details of the hydro model used here. Also what is the initial state model?

Slide#10: "as a function centrality" --> "as a function of centrality"

Are we implying here that the initial state does not change with energy ?



Best,
Prithwish


On 2022-10-17 11:10, webmaster--- via Star-fcv-l wrote:
Dear star-fcv-l AT lists.bnl.gov members,

Niseem Magdy Abdelwahab Abdelrahman (niseemmagdy AT yahoo.com) has submitted a
material for a review, please have a look:
https://drupal.star.bnl.gov/STAR/node/61385

Deadline: 2022-10-27
---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
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