STAR Flow, Chirality and Vorticity PWG

[Prithwish Tribedy <ptribedy AT rcf.rhic.bnl.gov>]

Dear Cameron,
  Very nice slides. I have a few comments. With these included I sign 
off your talk.

slide#2: "at high energies; ~200 GeV" (this is not exactly true, we have 
BES analyses, arXiv:1601.01999).

How about something like:
 "at high energies; ~200 GeV" --> "using collider mode data (√s_{NN}= 
7.7-200 GeV) with a focus on the rapidity-even v_3 studies" ?

"no correlation" --> "no direct correlation" (This is better as \Psi1, 
\Psi2 & \Psi3 correlations have been studied before and nonzero 
correlations have been observed, arXiv:1701.06497)

"; must use \Psi_3" --> "& only to \Psi_3"

"HEDES shows" --> "Recent HEDES results show"

Somewhere on this slide it would be good to say "STAR fixed target mode 
provides unique opportunity to go to energies down to √s_{NN}=3 GeV"

slide#3: Title "Experimental Setup" --> "STAR fixed target experimental 
setup" (It's better to explicitly mention "Fixed target mode" somewhere 
in the beginning of your talk)

slide#8: "clear signal for protons" --> "significant non-zero v_3 for 
protons"
"made on " --> "made about"

slide#9: "opposite sign to v_1 at 3 GeV" --> Needs a reference

slide#10: Define what is "A".
"A-scaling" --> "Nuclear mass number scaling (A)"

"v_3{\Psi_1} is also present" --> "Non-zero significant v_3{\Psi_1} 
observed"


"Tritons are currently under investigation for anything influencing the 
results." --> "Triton results are currently under investigation for the 
following effects:"


slide#10: "Tritons may have" --> "Tritons show"


Best,
Prithwish


On 2022-10-13 15:51, webmaster--- via Star-fcv-l wrote:
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Cameron Racz (cracz001 AT ucr.edu) has submitted a material for a review, 
> please
> have a look:
> https://drupal.star.bnl.gov/STAR/node/61320
>
> Deadline: 2022-10-27
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