STAR Flow, Chirality and Vorticity PWG

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

Hello Brian,
  Please find my comments on your nice slides. With these included I 
sign off.

General:
Just to clarify, you are not going to show any new STAR data in this 
talk, right. You only have either AMPT results (or comparison of 
published STAR data to AMPT) to establish the methodology. It is 
perfectly ok. But in that case maybe I would change the title a bit to 
something like:
"Methods for studying Λ-p azimuthal correlation..."

Also, in your content slides you should make it clear that this is a 
feasibility study and similar analysis with STAR data is ongoing.

Title:
"w.r.t" --> "with respect to"

Slide#3:
"Magnetic field + Chirality"
-->
"Magnetic field + Chirality imbalance"
or
"Magnetic field + net-Chirality"

Slide#4:
I would replace "Fancy Effects" with something like "Exotic Effects" or 
"Novel Phenomena"

Slide#7:
You need to mention which detectors you plan to use for: identifying 
tracks, centrality selection, pile-up rejection and one for event plane 
measurement.

Slide#8:
"Centrality-Dependent"
-->
"We apply centrality dependent quality cuts"

Slide#9:
Is this invariant mass distribution obtained from data? If yes, please 
add STAR preliminary.

Slide#11-13: You need to add at least one comment on these slides

Summary:
I would bring the line "Methodology has been tested with AMPT" above and 
as a separate bullet.

Best,
Prithwish



On 2020-10-14 14:45, webmaster--- via Star-fcv-l wrote:
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Brian Chan (brianchan40 AT physics.ucla.edu) has submitted a material for 
> a
> review, please have a look:
> https://drupal.star.bnl.gov/STAR/node/52370
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