STAR Correlations and Fluctuations PWG

[Hanna Zbroszczyk <hanna.zbroszczyk AT pw.edu.pl>]

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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> 
> -- 
> 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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