STAR Flow, Chirality and Vorticity PWG

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

Dear Yicheng,

Nice abstract. I sign off with the following wording suggestions for 
your consideration:

l#11-13: "The background baseline for the isobar ratio Y = 
(∆γ/v2)Ru(∆γ/v2)Zr is naively expected to be (1/N)Ru(1/N)Zr, however, 
genuine two- and three-particle correlations are expected to alter it."
--> The background baseline of the isobar ratio Y (=(∆γ/v2)Ru / 
(∆γ/v2)Zr) is naively anticipated to be (1/N)Ru / (1/N)Zr. However, 
genuine two- and three-particle correlations have the potential to alter 
this baseline.

l#13-15: "We estimate the contributions from those correlations to Y , 
utilizing the STAR isobar data as well as HIJING simulations. Including 
those contributions, we arrive at a final background baseline for Y."
--> We calculate the influence of these correlations on Y by 
incorporating data from STAR isobar experiments and HIJING simulations. 
By accounting for these contributions, we establish a comprehensive 
background reference for Y.

Thanks and regards,
Subhash

On 2023-09-20 09:20 PM, webmaster--- via Star-fcv-l wrote:
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Yicheng Feng (feng216 AT purdue.edu) has submitted a material for a 
> review,
> please have a look:
> https://drupal.star.bnl.gov/STAR/node/65199
>
> Deadline: 2023-10-10
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