STAR Correlations and Fluctuations PWG

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

Dear Hanna and Xiaofeng,

Thank you very much for your valuable comments.

I have implemented all your suggestions. 

The revised draft can be found below:

https://drupal.star.bnl.gov/STAR/system/files/tnonaka_ICNFP2021.pdf

Best regards,

Toshihiro

On Aug 19, 2021, at 22:36, Hanna Zbroszczyk via Star-cf-l <star-cf-l AT lists.bnl.gov> wrote:

Dear Toshihiro,

I have 2 comments to your nice slides:
As you mention later FXT program too, please extend your table describing
BES II program and mention energies, muB and other quantities too regarding
FXT (down to 3 GeV).

I also think you should mention results related to net-kaon and net-charge
too.

With these implemented, I sign off.

Thanks,
Hanna

Wysłane z iPhone'a

Wiadomość napisana przez Xiaofeng Luo via Star-cf-l
<star-cf-l AT lists.bnl.gov> w dniu 19.08.2021, o godz. 14:56:

Hi Toshihiro,

   Nice presentation.
   Please find my comments and suggestions below :
   1. Slide 5 , 54.4 GeV is taken in 2017.
   2. Slide 6 : May specify that X, Y should be independent variable for
additivity.
                S and κ are non-gaussian fluctuations. -> S and κ are
sensitive to non-gaussian fluctuations.
               Moment -> Central Moment

3. Slide 9, also put reference of STAR net-proton long paper.
   4. Slide 10, B. X. Luo  -> X. Luo
   5. Slide 13:  3 sigma -> 3.1 sigma

   6. Slide 18: long paper : replace arXiv number with Journal number.

   7. Slide 19: Huge datasets -> 10-20 times or you may specific the
number of events collected.

   8. Slide 20: FXT  -> Fixed-target (FXT）: Need to explain what does
FXT mean.  Add : Extend muB up to 720 MeV.

   9. Slide 22 : Non-binomial efficiencies -> Non-binomial eff. corr.
                       if the efficiency distributions deviate from
binomial distribution -> If the response function of detector deviated
from binomial distribution.
                       Efficiency distributions ->Detector response
function

   10. Slide 24: The last two bullets can be merged into one : Detector
efficiencies and volume fluctuations need to be carefully studied for each
experiment.
                       The last sentence of first bullet and third bullet
can be merged into  : Stay tuned for precise measurement from BES-II and
FXT energies (3.3 - 19.6 GeV) to have more definitive message.

   11. You may add one slide to discuss the results of net-charge and
net-kaon fluctuations, as your talk title is high moments analysis.

   With those implemented, I sign off.

Thank you,
Best Regards,
Xiaofeng

On 2021/8/18 10:23 AM, webmaster--- via Star-cf-l wrote:
Dear star-cf-l AT lists.bnl.gov members,

Toshihiro Nonaka (tnonaka AT rcf.rhic.bnl.gov) has submitted a material for
a
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/56040

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If you have any problems with the review process, please contact
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--
Xiaofeng Luo
Professor of Physics
College of Physical Science and Technology
Central China Normal University
Luoyu Road 152, Wuhan China
Office Phone #: +86-27-67867963

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