STAR Flow, Chirality and Vorticity PWG

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

Dear Aditya,

Nicely written proceedings. I have a few suggestions for your 
consideration:


title: BES-II

l#7-10: you can probably split it into two/three sentences. e.g.
In this work, we report measurements of two types of observables: (i) 
charge-dependent directed flow (∆v1), which is sensitive to the initial 
ultra-strong electromagnetic fields, and (ii) flow correlation, such as 
rn(η), which is sensitive to the initial longitudinal de-correlation and 
correlations among flow harmonics. These measurements contribute to 
constraining the initial state of the collisions.

l#15-16: of heavy-ion collisions at RHIC energies.

l#19: the medium properties (such as electrical conductivity) and on the 
formation time

l#20: "is essential to understanding the evolution" --> is essential for 
understanding the evolution

l#40: should contribute --> could contribute to a

l#46: "Data at √sNN = 200 GeV..." --> to be more specific you can 
mention, the negative splitting in peripheral collisions at 200 GeV 
right?

l#48: "The larger magnitudes of ∆dv1/dy in peripheral collisions at 
lower energies" ---> How about: An increase in magnitude of ∆dv1/dy in 
peripheral collisions with decrease in beam energies. Along this lines, 
you could mention we observed a similar pattern in data. It is not 
evident from the text.

l#62-63: "r3(η) shows hints of larger deviation at lower beam energies"
--> I am not sure we can make conclusion on energy dependence based on 
uncertainties. You can rephrase it with keeping only AMPT comparison.

l#77: "We have presented STAR preliminary measurements" --> We have 
presented measurements ... in the Beam Energy Scan program by STAR 
experiment.


Thanks and regards,
Subhash


On 2023-11-25 06:14 AM, webmaster--- via Star-fcv-l wrote:
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> Aditya Prasad Dash (adityaprasaddash55 AT gmail.com) has submitted a 
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