STAR Flow, Chirality and Vorticity PWG

[Yufu <yufulin AT mails.ccnu.edu.cn>]

Dear Shinlchi,

Thanks a lot for your sign off.

The signal in AVFD are represented with the fermion axial charge density 
(n_5/s) in initial conditions (event-by-event fluctuations),  and the listed 
a1 in the table(slides 9) is the final particles, so the a1 value is 
fluctuate event-by-event in each event for each case.

Please feel free to emails me if you have any questions/suggestions.

Cheers,
Yufu Lin

Besides, this is Yufu Lin  from CCNU&GXNU


> On Oct 30, 2021, at 21:35, ShinIchi Esumi via Star-fcv-l 
> <star-fcv-l AT lists.bnl.gov> wrote:
> 
> Dear Yu
> I would also sign off your nice talk in ATHIC. 
> Could you remind me the assumption of the a1 signal in AVFD? 
> Does it fluctuate event-by-event at the given fraction for each case 
> at about 0, ~1, and ~2%?
> Best regards, ShinIchi
> 
>> 2021/10/29 20:44、webmaster--- via Star-fcv-l 
>> <star-fcv-l AT lists.bnl.gov>のメール:
>> 
>> Dear star-fcv-l AT lists.bnl.gov members,
>> 
>> Jiangyong Jia ( jjia AT bnl.gov ) has commented on a material originally  
>> submitted by Yufu Lin ( yufulin AT mails.ccnu.edu.cn ) at
>> https://drupal.star.bnl.gov/STAR/presentations/athic-2021/investigation-sensitivities-observables-cme-search-star-experiment-using--0
>> 
>> Comment:
>> The slides look very nice. I sign off.
>> 
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