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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Qiang Hu for SQM 2022 submitted for review

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: subhash <subhash AT rcf.rhic.bnl.gov>
  • To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Cc: qianghu AT impcas.ac.cn
  • Subject: Re: [Star-fcv-l] STAR presentation by Qiang Hu for SQM 2022 submitted for review
  • Date: Wed, 08 Jun 2022 09:27:41 +0800

Dear Qiang,

Nice poster. Here are a few suggestions for your consideration.

Please elaborate a little more on the baryonic Spin Hall effect. Mention that Spin Hall type effect in lambda polarization is predicted to be driven by baryon density gradient. You can even expand it more with one additional slide. You can combine current slide#4 and #5 into one slide that could provide you an extra space.

slide#2: Mention the data taking year or BES-II in the legend
Lower left: fix "EPD: Zero Degree Calorimeters"

slide#3: Add systematic uncertainty on these points. Can you also draw it on a smaller Y-axis range so that we can see the centrality dependent pattern.
Can you add a statement about the centrality dependent of Pz?

slide#5: Here and elsewhere use "baryonic" Spin Hall Effect.
You can add another bullet: Analysis on other BES energies are underway.

Thanks and regards,
Subhash


On 2022-05-31 05:11 PM, webmaster--- via Star-fcv-l wrote:
Dear star-fcv-l AT lists.bnl.gov members,

Qiang Hu (qianghu AT impcas.ac.cn) has submitted a material for a review, please
have a look:
https://drupal.star.bnl.gov/STAR/node/59786

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