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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Prabhupada Dixit for SQM 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>
  • Cc: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] STAR presentation by Prabhupada Dixit for SQM 2022 submitted for review
  • Date: Wed, 08 Jun 2022 16:13:24 +0800

Dear Prabhupada,

Thanks for incorporating my comments.
I am fine with your poster once the following suggestions are addressed.

Can you add either data taking year (2019) or BES-II in all the relevant figures?
Can you draw add a horizontal straight line at 1, on the right hand side ratio plots?
Can you add the conclusion in your slides based on your v_n ratios, e.g. ratios are sensitive to initial fluctuations and transport properties; can be used constrain hydrodynamic models.

Thanks and regards,
Subhash

On 2022-06-08 02:59 PM, pdixit wrote:
Dear Subhash,
Thank you for the comments and the suggestions. I have modified the
poster accordingly. Please find the new version of the poster in the
link below.
https://drupal.star.bnl.gov/STAR/system/files/SQM22_poster_v3.pdf
What do we learn from the ratio v3/v2^3/2?
This ratio is a prediction from hydrodynamics. It's sensitive to the
magnitude of the transport properties (viscosity) and the fluctuations
present in the initial stage of the system and is useful to filter
various models.
Reference: PRL 105, 062301 (2010), Phys. Rev. Lett. 92, 062301

Regards,
Prabhupada


On 2022-06-07 16:28, subhash wrote:
Dear Prabhupada,

Nice poster. I have a few suggestions for your consideration.
slide#1: Top right, the x-arrow coincide with event-by-event. Please fix it.
Can you add reference for Early freeze-out and small hadronic
interaction cross section?
2nd bullet mention improved detector.

slide#2: Add bema energy and data taking year in both the figures.

slide#3: Can you indicate the improvement in resolution relative to BES-I?

slide#4:
The NCQ scaling holds within 30% for particles and within 15% for
anti-particles which indicates the contribution from transported
quarks in particles.

What do we learn from the ratio v3/v2^3/2?

Thanks and regards,
Subhash

On 2022-06-05 03:23 PM, pdixit via Star-fcv-l wrote:
Dear convenors,
I have updated my poster with the suggestions from the last FCV
meeting. Please have a look at the link below.
https://drupal.star.bnl.gov/STAR/system/files/SQM22_poster_v2.pdf

Regards,
Prabhupada
On 2022-05-30 20:28, 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/59774

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