STAR Flow, Chirality and Vorticity PWG

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

Dear Sharang,

Nice proceedings. I have a few suggestions below for your consideration:

l#10: at s_NN  = 3.2, ...

l#11, 12: for identified hadrons (pi, K, p) and net-particles (net K and 
net p) ....

l#13, 14: The minimum in v1 slope for net-kaon is observed at lower 
collision energy than net-proton
--> I think we don't have sufficient data to comment about the minimum. 
You can probably say that the sign change occurred at different energy.

l#18: "The v3 slope for all particles decreases in magnitude with 
increasing collision energy, indicating the effect of the mean-field at 
the low energies."
--> How mean field connected to energy dependence, can you explain? 
There could be multiple effects folded in here mean-field, baryon 
stopping, geometry, ... right?

l#51, 55 and else where add a space X ~ GeV

l#59: remove bracket on \kappa

l#61,62: add a reference

l#66: The traditional v3, ...

l#77: In these proceedings,

l#88-93: You could mention the kinematics, pt, eta selections and track 
selection conditions before introducing particle identification.

l#93: I guess you are not using z-variable for all species, only for 
light nuclei. For other species you are using combination with Nsigma. 
So modify the discussions accordingly.

l#113: You could mention what is used as weight in Q reconstruction

l#130:  employed in the collider BES-I

l#141, 142: you can add model comparison or a reference for backing up 
the statement

l#155: linear term in a third-order polynomial, right?

l#160: Suggest to change the statement that we observe a sign change 
than observe a minima, as mentioned above. Also make a similar change in 
the conclusion.

l#172,  173: modify the statement that it is not solely from mean-field. 
Also make a similar change in the conclusion.

Thanks and regards,
Subhash




On 2023-11-20 01:44 PM, webmaster--- via Star-fcv-l wrote:
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> Sharang Rav Sharma (sharang.rav AT students.iisertirupati.ac.in) has 
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