STAR Flow, Chirality and Vorticity PWG

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

Hello Kishora,
  Your slides are already in good shapes. I sign-off with the following 
comments.

Slide#3: Add details on the sources of systematics and centrality 
determination (try to avoid STAR terminologies).

Slide#4: "Understanding initial fluctuations"
I am not sure how much we can learn about "initial fluctuations" from 
the odd v1 measurements. I would change it to:
"Understanding initial state" or "Understanding initial state in 
rapidity direction"

Slide#5: "Particle formation time are" --> "Particle formation time is"

Slide#7-10: Why did you choose to show 0.5<|y|<1.0 ?

Slide#7:
"Zero crossing for central (0-10%) collisions: pT~1-2 GeV/c"
-->
"Sign change for central (0-10%) collisions at high pT"

Slide#8&9: You put many details on the thermal model -- I think you 
should put a comment on the results. Even saying "It predicts positive 
v1 at all pT" or something like that would suffice.

Slide#10: "Shadowing (or absorption)" needs a reference.

Slide#10: "in all observed" --> "at all observed"

Slide#10: "Baryon-meson dependence" --> "Baryon-meson separation"

Slide#11: "(NCQ) scaling is observed at low pT" --> "(NCQ) scaling holds 
best at low mT"

Slide#12: "low-pT" --> "low-mT" I think.

Slide#13: I would add a concise version of bullet no. 3 on slide #8 & #9 
where you show the AMPT results.

Best,
Prithwish



On 2020-12-02 07:14, webmaster--- via Star-fcv-l wrote:
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Kishora Nayak (k.nayak1234 AT gmail.com) has submitted a material for a 
> review,
> please have a look:
> https://drupal.star.bnl.gov/STAR/node/52962
>
> ---
> 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