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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: 胡强 <qianghu AT impcas.ac.cn>
  • Cc: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] STAR presentation by Qiang Hu for SQM 2022 submitted for review
  • Date: Fri, 10 Jun 2022 14:18:50 +0800

Dear Qiang,

Thanks for this updated poster. I sign off with two minor comments:

slide#2: 3rd bullet: You can rephrase "RHIC BES offer ideal conditions to probe baryonic SHE: large baryon density and abundant Λ/anti-Λ production"

You can post your systematic studies in your personal Drupal blog and send to FCV list.

Thanks and regards,
Subhash

On 2022-06-10 01:33 PM, 胡强 wrote:
Dear Subhash,

Thanks for the comments. I have updated the poster and upload it as
well as the systematic study plots to STAR drupal. Please find the
following link:

https://drupal.star.bnl.gov/STAR/presentations/SQM-2022/Probing-novel-baryonic-spin-Hall-effect-using-lambda-polarization-STAR

Best regards,

Qiang


&gt; -----原始邮件-----
&gt; 发件人: subhash <subhash AT rcf.rhic.bnl.gov>
&gt; 发送时间: 2022-06-10 11:10:12 (星期五)
&gt; 收件人: "胡强" <qianghu AT impcas.ac.cn>
&gt; 抄送: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
&gt; 主题: Re: [Star-fcv-l] STAR presentation by Qiang Hu for SQM 2022
submitted for review
&gt;
&gt; Dear Qiang,
&gt;
&gt; Thanks for the updated poster. I have a few more suggestions for you to
&gt; consider.
&gt;
&gt; slide#1: Lower left Lambda --&gt; p pi, "p" is missing.
&gt; slide#2: It is kind of busy to follow the ordering of the plots. You can
&gt; probably remove the top two middle plots (related to SIP) and make a few
&gt; additional bullets, e.g,
&gt; . Predicted Spin Hall effect in HIC driven by baryon density gradient
&gt; . Can be accessed by net local Polarization (Pz) of P_{L} - P_{aL}
&gt;
&gt; slide#3: Check the lower left box, EPD is missing before the arrow.
&gt; slide#4: You don't need STAR preliminary for the inset plots. They are
&gt; part of the main plot. Mention XX.X GeV (BES-II).
&gt; No significant centrality dependence ...
&gt;
&gt; Please also send us your updated slides with systematic uncertainty to
&gt; the FCV list.
&gt;
&gt; I have deleted the duplicate entry:
&gt; https://drupal.star.bnl.gov/STAR/node/59920
&gt;
&gt; Thanks and regards,
&gt; Subhash
&gt;
&gt;
&gt; On 2022-06-10 10:44 AM, 胡强 wrote:
&gt; &gt; Dear Subhash,
&gt; &gt;
&gt; &gt; Many thanks for your comments and suggestion.
&gt; &gt;
&gt; &gt; I have update the poster and upload to the STAR drupal site. Please
&gt; &gt; find the link as follow:
&gt; &gt;
&gt; &gt;
https://drupal.star.bnl.gov/STAR/presentations/SQM-2022/Probing-novel-baryonic-spin-Hall-effect-using-lambda-polarization-STAR-0
&gt; &gt;
&gt; &gt; With best regards,
&gt; &gt;
&gt; &gt; Qiang
&gt; &gt;
&gt; &gt;
&gt; &gt; &gt; -----原始邮件-----
&gt; &gt; &gt; 发件人: subhash <subhash AT rcf.rhic.bnl.gov>
&gt; &gt; &gt; 发送时间: 2022-06-08 09:27:41 (星期三)
&gt; &gt; &gt; 收件人: "STAR Flow, Chirality and Vorticity PWG"
&gt; &gt; <star-fcv-l AT lists.bnl.gov>
&gt; &gt; &gt; 抄送: qianghu AT impcas.ac.cn
&gt; &gt; &gt; 主题: Re: [Star-fcv-l] STAR presentation by Qiang Hu for SQM 2022
&gt; &gt; submitted for review
&gt; &gt; &gt;
&gt; &gt; &gt; Dear Qiang,
&gt; &gt; &gt;
&gt; &gt; &gt; Nice poster. Here are a few suggestions for your consideration.
&gt; &gt; &gt;
&gt; &gt; &gt; Please elaborate a little more on the baryonic Spin Hall effect.
&gt; &gt; Mention
&gt; &gt; &gt; that Spin Hall type effect in lambda polarization is
predicted to
&gt; &gt; be
&gt; &gt; &gt; driven by baryon density gradient. You can even expand it more
&gt; &gt; with one
&gt; &gt; &gt; additional slide. You can combine current slide#4 and
#5 into one
&gt; &gt; slide
&gt; &gt; &gt; that could provide you an extra space.
&gt; &gt; &gt;
&gt; &gt; &gt; slide#2: Mention the data taking year or BES-II in the legend
&gt; &gt; &gt; Lower left: fix "EPD: Zero Degree Calorimeters"
&gt; &gt; &gt;
&gt; &gt; &gt; slide#3: Add systematic uncertainty on these points.
Can you also
&gt; &gt; draw
&gt; &gt; &gt; it on a smaller Y-axis range so that we can see the centrality
&gt; &gt; dependent
&gt; &gt; &gt; pattern.
&gt; &gt; &gt; Can you add a statement about the centrality dependent of Pz?
&gt; &gt; &gt;
&gt; &gt; &gt; slide#5: Here and elsewhere use "baryonic" Spin Hall Effect.
&gt; &gt; &gt; You can add another bullet: Analysis on other BES energies are
&gt; &gt; underway.
&gt; &gt; &gt;
&gt; &gt; &gt; Thanks and regards,
&gt; &gt; &gt; Subhash
&gt; &gt; &gt;
&gt; &gt; &gt;
&gt; &gt; &gt; On 2022-05-31 05:11 PM, webmaster--- via Star-fcv-l wrote:
&gt; &gt; &gt; &gt; Dear star-fcv-l AT lists.bnl.gov members,
&gt; &gt; &gt; &gt;
&gt; &gt; &gt; &gt; Qiang Hu (qianghu AT impcas.ac.cn) has submitted a material for
&gt; &gt; a review,
&gt; &gt; &gt; &gt; please
&gt; &gt; &gt; &gt; have a look:
&gt; &gt; &gt; &gt; https://drupal.star.bnl.gov/STAR/node/59786
&gt; &gt; &gt; &gt;
&gt; &gt; &gt; &gt; ---
&gt; &gt; &gt; &gt; If you have any problems with the review process, please
&gt; &gt; contact
&gt; &gt; &gt; &gt; webmaster AT www.star.bnl.gov
&gt; &gt; &gt; &gt; _______________________________________________
&gt; &gt; &gt; &gt; Star-fcv-l mailing list
&gt; &gt; &gt; &gt; Star-fcv-l AT lists.bnl.gov
&gt; &gt; &gt; &gt; https://lists.bnl.gov/mailman/listinfo/star-fcv-l
&gt; &gt; </star-fcv-l AT lists.bnl.gov></subhash AT rcf.rhic.bnl.gov>
</star-fcv-l AT lists.bnl.gov></qianghu AT impcas.ac.cn></subhash AT rcf.rhic.bnl.gov>




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