Skip to Content.
Sympa Menu

star-cf-l - Re: [Star-cf-l] CF PWG meeting March 30th (Thursday) 9:30am (BNL time)

star-cf-l AT lists.bnl.gov

Subject: STAR Correlations and Fluctuations PWG

List archive

Chronological Thread  
  • From: "Yu Zhang" <yuz AT ccnu.edu.cn>
  • To: "江角晋一" <esumi.shinichi.gn AT u.tsukuba.ac.jp>, "star-cf-l AT lists.bnl.gov" <star-cf-l AT lists.bnl.gov>
  • Subject: Re: [Star-cf-l] CF PWG meeting March 30th (Thursday) 9:30am (BNL time)
  • Date: Fri, 31 Mar 2023 09:50:53 +0800

Dear ShinIchi,
Thank you very much for your comments.
I agree with that. I will keep the current result and 
calculate the cumulants from the real pairs.
Best regards,
Yu
 
 
------------------ Original ------------------
From:  "江角晋一"<esumi.shinichi.gn AT u.tsukuba.ac.jp>;
Date:  Fri, Mar 31, 2023 01:20 AM
To:  "张宇"<yuz AT ccnu.edu.cn>; "star-cf-l AT lists.bnl.gov"<star-cf-l AT lists.bnl.gov>;
Subject:  Re: [Star-cf-l] CF PWG meeting March 30th (Thursday) 9:30am (BNL time)
 
Dear Yu
As we discussed in the PWG, we would like you to plot cumulants from
the real pair in stead of the rotated BG pair for the right plot of page 11
in your slide. But I would just like to remind you the comparison of real
and rotated pair is also meaningful as well. As we do see slight slope
especially on the blue points in the right plot, that might be related to
the kinematics coming from the minv, although the black and the red
points (at least black) are expected to be flat by definition, if your original
bin width is small enough. So please keep in mind to compare the current
ones from the rotated pairs with the other ones from the true pairs, not
just to replace them. I hope you agree with that. Thank you very much.
Best regards, ShinIchi

2023/03/30 20:20、Yu Zhang via Star-cf-l <star-cf-l AT lists.bnl.gov>のメール:

Dear All,

Please find my slides for today's discussion.

Thank you!
Yu
 
------------------ Original ------------------
Date:  Wed, Mar 29, 2023 04:44 PM
Subject:  Re: [Star-cf-l] CF PWG meeting March 30th (Thursday) 9:30am (BNL time)
 
Dear Conveners,

If time permits, I would like to give an update on the baryon-strangeness correlation
in 3GeV Au+Au collision. I will post my slides soon.
Thank you,
Best regards,
Yu
 
------------------ Original ------------------
From:  "Hanna Paulina Zbroszczyk via Star-cf-l"<star-cf-l AT lists.bnl.gov>;
Date:  Tue, Mar 28, 2023 01:07 AM
Subject:  [Star-cf-l] CF PWG meeting March 30th (Thursday) 9:30am (BNL time)
 
Dear CF Activists,

We will have our weekly CF PWG meeting on Thursday, March 30th, 9:30 AM
(BNL time).
If you would like to contribute, please let us know.

Please try to post your slides at your earliest convenient.
We will connect via Zoom. Please find the connection details under the
meeting webpage.

Thank you,
Best regards,
Toshihiro and Hanna

https://drupal.star.bnl.gov/STAR/blog/luoxf/correlations-and-fluctuations
https://drupal.star.bnl.gov/STAR/blog/gos/correlations-and-fluctuations-preliminary-plots 



Hanna Paulina Zbroszczyk
PhD DSc Eng, Professor WUT

Tel: +48 22 234 5851 (office)

Address:
Warsaw University of Technology
Faculty of Physics
Nuclear Physics Division
Koszykowa 75
Office: 117b (via 115)
00-662 Warsaw, Poland















_______________________________________________
Star-cf-l mailing list
Star-cf-l AT lists.bnl.gov
https://lists.bnl.gov/mailman/listinfo/star-cf-l




Archive powered by MHonArc 2.6.24.

Top of Page