STAR Flow, Chirality and Vorticity PWG

[Takafumi Niida <niida AT bnl.gov>]

Dear ShinIchi and Jiangyong,

Thank you for signing off on my slides. Please find my reply to ShinIchi’s 
comments below.

> * You have mentioned about the update on the alpha parameter in p4 between 
> old and new results, 
> but the update has been applied only for the p22-25, right? So it might be 
> easier for the audience 
> to follow, if you mention these changes when you show these a few figures. 
> But since the parameters 
> are printed only on these new figures, so it would already be clear enough… 

I will emphasize it during the talk.

> * on p2, I see some overlapping words on the left-bottom of the page, which 
> might be my viewer
> problem as well, though.  

This is because of animation.

> * It would be nice, if you can also discuss about your BW calculations in 
> your talk from the backup 
> slides p35-36. Have you also made your own calculation with your BW 
> assumption for the azimuthal 
> dependent gPh measurement on p18? 

Initially I was thinking the same thing therefore I keep them in the backup 
but it seems I don’t have much time for that. No calculation for global PH 
with BW.

Slides have been slightly modified as I mentioned before and the phi-meson 
spin alignment plot was replaced:
https://drupal.star.bnl.gov/STAR/presentations/aum-2020/global-polarization-hyperons-heavy-ion-collisions-star-experiment

Best regards,
Takafumi

> On Oct 13, 2020, at 12:44 AM, ShinIchi Esumi via Star-fcv-l 
> <star-fcv-l AT lists.bnl.gov> wrote:
> 
> Dear Takafumi
> Thanks for the nice presentation, I would approve with a few minor 
> comments. 
> 
> * You have mentioned about the update on the alpha parameter in p4 between 
> old and new results, 
> but the update has been applied only for the p22-25, right? So it might be 
> easier for the audience 
> to follow, if you mention these changes when you show these a few figures. 
> But since the parameters 
> are printed only on these new figures, so it would already be clear enough… 
> 
> * on p2, I see some overlapping words on the left-bottom of the page, which 
> might be my viewer
> problem as well, though.  
> 
> * It would be nice, if you can also discuss about your BW calculations in 
> your talk from the backup 
> slides p35-36. Have you also made your own calculation with your BW 
> assumption for the azimuthal 
> dependent gPh measurement on p18? 
> 
> Best regards, ShinIchi
> 
> PS : I do see overlapping posts for the same Petr’s ICPPA proceedings from 
> Grigory and Arkadiy, 
> so I wonder which one I should be reading. Do you know? Petr should be 
> posting to avoid this confusions.  
> 
>> On Oct 12, 2020, at 1:16, webmaster--- via Star-fcv-l 
>> <star-fcv-l AT lists.bnl.gov> wrote:
>> 
>> Dear star-fcv-l AT lists.bnl.gov members,
>> 
>> Takafumi Niida (taknda AT hotmail.co.jp) has submitted a material for a 
>> review,  
>> please have a look:
>> https://drupal.star.bnl.gov/STAR/node/52333
>> 
>> ---
>> If you have any problems with the review process, please contact  
>> webmaster AT www.star.bnl.gov
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