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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Prabhupada Dixit for CPOD 2022 submitted for review

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: subhash <subhash AT rcf.rhic.bnl.gov>
  • To: pdixit <pdixit AT rcf.rhic.bnl.gov>, "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] STAR presentation by Prabhupada Dixit for CPOD 2022 submitted for review
  • Date: Mon, 21 Nov 2022 23:48:34 +0530

Dear Prabhupada,

Thanks for addressing my comments.
I have one more related to KS0 v2, which you addressed in FCV list.
If the rise in KS0 v2 at 14.6 GeV is likely due to non-flow, why it is not observed at 19.6 GeV. Have you checked by playing with the eta-gaps if these points are sensitive to it or not? Have you estimated non-flow contribution?

Thanks and regards,
Subhash

On 2022-11-21 01:24 PM, pdixit via Star-fcv-l wrote:
Dear Subhash,
Thanks for the comments and suggestions. Below is the link to the
modified slide.
https://drupal.star.bnl.gov/STAR/system/files/CPOD_2022_slides_v2.pdf
s2: Last bullet, please also mention detector upgrades
I have mentioned that in the next slide (s3), where I am showing the
STAR detectors and PID.
Do you know why the phi-meson has a significantly different trend at
low pT, compared to others?
This is what we observed. We may need to look at other energies to
understand this trend.

Regards,
Prabhupada
On 2022-11-20 17:45, subhash via Star-fcv-l wrote:
Dear Prabhupada,

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

Check slide numbers. They are not consistent, sometimes missing.

s2: Last bullet, please also mention detector upgrades

s4: Check the X-axis level on top right hidden behind the text box.

s5: Mention detector name for resolution figure. Would be good if you
can enlarge the figure.

s5,7 ...: mention BES-II inside figures, rapidity range etc to be
consistent with other figures.

v_3/v_3^{3/2} ratio:
shows weak pT dependence above pT > 1.0 GeV/c. --> shows non-trivial
pT dependence.

Do you know why the phi-meson has a significantly different trend at
low pT, compared to others?

Thanks and regards,
Subhahs


On 2022-11-18 04:12 PM, webmaster--- via Star-fcv-l wrote:
Dear star-fcv-l AT lists.bnl.gov members,

Prabhupada Dixit (prabhupadad AT iiserbpr.ac.in) has submitted a material for a
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/61707

Deadline: 2022-11-28
---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
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