STAR Flow, Chirality and Vorticity PWG

[Gavin Wilks <gwilks3 AT uic.edu>]

Hello Subhash, 

Thank you for the comments.

Regarding the BES-I data, I thought there were only data sets for 
7.7,11.5,19.6,27,39, and 62.4 GeV. This is why I specify 14.6 GeV as a new 
set.

Best,
Gavin 

> On Mar 3, 2022, at 02:28, subhash via Star-fcv-l <star-fcv-l AT lists.bnl.gov> 
> wrote:
> 
> Dear Gavin,
> 
> I have a few suggestions for your consideration.
> 
> Rephrase this line "In heavy-ion collisions, global spin alignment is a 
> preferential alignment of particles’ spin with the large orbital angular 
> momentum produced at the center of these systems".
> 
> I feel we don't need these parts in the abstract "Finite elliptic flow (v2) 
> could affect global spin alignment by pushing more particles toward the 
> in-plane direction...will help to remove any potential bias in the 
> measurements.".
> 
> Suggest remove "provides a new data set for Au+Au collisions at √ sNN=14.6 
> GeV" --> We already have 14.5 from BES-I. You can simply mention both 14.6 
> and 19.6 BES-II data would provide better precision.
> 
> I don't understand what do you mean by "helping to clarify the behavior of 
> this
> quantity"? You can mention precision measurement will allow more 
> differential studies, e.g. centrality dependence which is not possible for 
> BES-I
> 
> "Additionally, the elliptic and triangular flow (v3) of ϕ and K∗0 can be 
> determined with higher precision and for a new collision energy." --> I 
> would suggest saying we will report high precision v3 for ϕ and K∗0 ...
> 
> One suggestion, you can probably mention that the comparison of ϕ and K∗0 
> is interesting because their lifetime differ by factor of ten and the 
> former is less affected by hadronic re-scattering.
> 
> Thanks and regards,
> Subhash
> 
> On 2022-03-03 02:46 AM, webmaster--- via Star-fcv-l wrote:
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>> Gavin Wilks (gwilks3 AT uic.edu) has submitted a material for a review, please
>> have a look:
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