STAR Flow, Chirality and Vorticity PWG

[ShinIchi Esumi <esumi.shinichi.gn AT u.tsukuba.ac.jp>]

Dear Yicheng

After you prepare the preliminary summary page with all your preliminary plots to be linked 

at special drupal area for the preliminary location with necessary information at : 

https://drupal.star.bnl.gov/STAR/pwg/bulk-correlations/bulkcorr-preliminary-summary

then I would approve your talk. 

Best regards, ShinIchi

On Oct 18, 2020, at 11:50, ShinIchi Esumi via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:

Dear Yicheng
I would sign off your nice talk with a few comments.

You have chosen to say no signal for both 10-50% and 0-80%,
which we all agree, but I would say there is one “2-sigma” signal
deviation point at 50-60%...

For your future PWG presentation, could you also please show
us just with Lambda (or anti-Lambda) as well as just with a+ (or
a-) in stead of Delta_a (a+ and a- combined), the signal could
be there in any of these covariances.

Nobody have ever looked this in 200GeV AuAu, yet?  
Best regards, ShinIchi

On Oct 15, 2020, at 9:45, webmaster--- via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:

Dear star-fcv-l AT lists.bnl.gov members,

Yicheng Feng (feng216 AT purdue.edu) has submitted a material for a review,  
please have a look:
https://drupal.star.bnl.gov/STAR/node/52374

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