STAR Flow, Chirality and Vorticity PWG

[subhash <subhash AT rcf.rhic.bnl.gov>]

Dear Qiang,

Thanks for the updated poster. I have a few more suggestions for you to 
consider.

slide#1: Lower left Lambda --> p pi, "p" is missing.
slide#2: It is kind of busy to follow the ordering of the plots. You can 
probably remove the top two middle plots (related to SIP) and make a few 
additional bullets, e.g,
. Predicted Spin Hall effect in HIC driven by baryon density gradient
. Can be accessed by net local Polarization (Pz) of P_{L} - P_{aL}

slide#3: Check the lower left box, EPD is missing before the arrow.
slide#4: You don't need STAR preliminary for the inset plots. They are 
part of the main plot. Mention XX.X GeV (BES-II).
No significant centrality dependence ...

Please also send us your updated slides with systematic uncertainty to 
the FCV list.

I have deleted the duplicate entry: 
https://drupal.star.bnl.gov/STAR/node/59920

Thanks and regards,
Subhash


On 2022-06-10 10:44 AM, 胡强 wrote:
> Dear Subhash,
>
> Many thanks for your comments and suggestion.
>
> I have update the poster and upload to the STAR drupal site. Please
> find the link as follow:
>
> https://drupal.star.bnl.gov/STAR/presentations/SQM-2022/Probing-novel-baryonic-spin-Hall-effect-using-lambda-polarization-STAR-0
>
> With best regards,
>
> Qiang
>
>
> > -----原始邮件-----
> &gt; 发件人: subhash <subhash AT rcf.rhic.bnl.gov>
> &gt; 发送时间: 2022-06-08 09:27:41 (星期三)
> &gt; 收件人: "STAR Flow, Chirality and Vorticity PWG" 
> <star-fcv-l AT lists.bnl.gov>
> &gt; 抄送: qianghu AT impcas.ac.cn
> &gt; 主题: Re: [Star-fcv-l] STAR presentation by Qiang Hu for SQM 2022
> submitted for review
> &gt;
> &gt; Dear Qiang,
> &gt;
> &gt; Nice poster. Here are a few suggestions for your consideration.
> &gt;
> &gt; Please elaborate a little more on the baryonic Spin Hall effect. 
> Mention
> &gt; that Spin Hall type effect in lambda polarization is predicted to 
> be
> &gt; driven by baryon density gradient. You can even expand it more 
> with one
> &gt; additional slide. You can combine current slide#4 and #5 into one 
> slide
> &gt; that could provide you an extra space.
> &gt;
> &gt; slide#2: Mention the data taking year or BES-II in the legend
> &gt; Lower left: fix "EPD: Zero Degree Calorimeters"
> &gt;
> &gt; slide#3: Add systematic uncertainty on these points. Can you also 
> draw
> &gt; it on a smaller Y-axis range so that we can see the centrality 
> dependent
> &gt; pattern.
> &gt; Can you add a statement about the centrality dependent of Pz?
> &gt;
> &gt; slide#5: Here and elsewhere use "baryonic" Spin Hall Effect.
> &gt; You can add another bullet: Analysis on other BES energies are 
> underway.
> &gt;
> &gt; Thanks and regards,
> &gt; Subhash
> &gt;
> &gt;
> &gt; On 2022-05-31 05:11 PM, webmaster--- via Star-fcv-l wrote:
> &gt; &gt; Dear star-fcv-l AT lists.bnl.gov members,
> &gt; &gt;
> &gt; &gt; Qiang Hu (qianghu AT impcas.ac.cn) has submitted a material for
> a review,
> &gt; &gt; please
> &gt; &gt; have a look:
> &gt; &gt; https://drupal.star.bnl.gov/STAR/node/59786
> &gt; &gt;
> &gt; &gt; ---
> &gt; &gt; If you have any problems with the review process, please 
> contact
> &gt; &gt; webmaster AT www.star.bnl.gov
> &gt; &gt; _______________________________________________
> &gt; &gt; Star-fcv-l mailing list
> &gt; &gt; Star-fcv-l AT lists.bnl.gov
> &gt; &gt; https://lists.bnl.gov/mailman/listinfo/star-fcv-l
> </star-fcv-l AT lists.bnl.gov></subhash AT rcf.rhic.bnl.gov>