STAR Flow, Chirality and Vorticity PWG

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

Dear Ding,

Nice poster. I have a few suggestions for your consideration:

Title: I suggest "Directed flow of ϕ-meson in fixed target Au+Au 
collisions at sNN = 3 and 7.2 GeV from STAR"

In abstract:
"anisotropic flows" --> directed flow
"compare our new results with STAR Beam Energy Scan I results" --> 
compare our new results with that from STAR Beam Energy Scan I.

In motivation:
You can probably try presenting them in separate small bullets.

In Datasets:
You didn't mention about 3 GeV data.

Analysis method:
Usually we fit phi meson with a Breit Wigner function. Could you remind 
me what is the reasoning behind Gaussian fit?

Summary:
"This may indicate a softest point of EoS for produced particles." --> 
This may be related to a change in EoS of the system.
I suggest "a change in EoS", because there is no evidence that this phi 
meson sign change is due to EoS softening.

"Results from fixed target and collider modes connect well. At same 
collision energy, combine FXT and COL modes can improve the flow 
measurements."
--> At similar collision energy, results from fixed target and collider 
modes are consistent within error. Upcoming measurements from FXT and 
COL data will improve the precision in \phi flow measurements.

I sign off with these addressed.

Thanks and regards,
Subhash

On 2022-07-11 10:31 PM, webmaster--- via Star-fcv-l wrote:
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Ding Chen (dchen087 AT ucr.edu) has submitted a material for a review, 
> please
> have a look:
> https://drupal.star.bnl.gov/STAR/node/60236
>
> ---
> If you have any problems with the review process, please contact
> webmaster AT www.star.bnl.gov
> _______________________________________________
> Star-fcv-l mailing list
> Star-fcv-l AT lists.bnl.gov
> https://lists.bnl.gov/mailman/listinfo/star-fcv-l