STAR Flow, Chirality and Vorticity PWG

["Wang, Fuqiang" <fqwang AT purdue.edu>]

Hi, Shengli,

I don't follow the difference between the c1 method and the template method. 
It seems to me that the template method assumes c1 to be zero, so isn't it 
identical to the c1 method? You recently presented the near-side jet scaling 
method, but it's not mentioned in the talk at all. I think that would be a 
viable third method. 

I would remove the mentioning of isobar data.

Best regards,
Fuqiang


> -----Original Message-----
> From: Star-fcv-l <star-fcv-l-bounces AT lists.bnl.gov> On Behalf Of 
> webmaster---
> via Star-fcv-l
> Sent: Monday, January 4, 2021 11:21 PM
> To: star-fcv-l AT lists.bnl.gov
> Subject: [Star-fcv-l] STAR presentation by Shengli Huang for Initial Stages 
> 2021
> submitted for review
> 
> Dear star-fcv-l AT lists.bnl.gov members,
> 
> Shengli Huang (shengli.huang AT stonybrook.edu) has submitted a material for a
> review, please have a look:
> https://drupal.star.bnl.gov/STAR/node/53200
> 
> ---
> If you have any problems with the review process, please contact
> webmaster AT www.star.bnl.gov
> _______________________________________________
> Star-fcv-l mailing list
> Star-fcv-l AT lists.bnl.gov
> https://lists.bnl.gov/mailman/listinfo/star-fcv-l