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star-fcv-l - Re: [Star-fcv-l] [Star-talks-l] STAR presentation by Sharang Rav Sharma for ISMD 2023 submitted for review

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: Sooraj Radhakrishnan <skradhakrishnan AT lbl.gov>
  • To: star-talks-l AT lists.bnl.gov, "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Cc: sharangrav <sharangrav AT rcf.rhic.bnl.gov>, webmaster AT star.bnl.gov
  • Subject: Re: [Star-fcv-l] [Star-talks-l] STAR presentation by Sharang Rav Sharma for ISMD 2023 submitted for review
  • Date: Sun, 20 Aug 2023 10:08:27 -0700

Hi Sharang,
   I see your Preliminary request for v3 of identified hadrons and light nuclei (https://drupal.star.bnl.gov/STAR/blog/sharangrav/Study-triangular-flow-identified-hadrons-and-light-nuclei-fixed-target-energies-RH-1). Did you also make a request for the v1 of identified hadrons at FXT energies? I couldnt find the request, and couldnt find the results in the list of approved Preliminaries. May be I missed. Could you clarify?

thanks
Sooraj

On Sun, Aug 20, 2023 at 9:49 AM Sooraj Radhakrishnan <skradhakrishnan AT lbl.gov> wrote:
Hi Sharang,
   Please find a few comments from me on your nicely prepared slides. 

You have 25 slides, how much time is there for your presentation? Please ensure you can go through the presentation in time. Else you could move some of the differential measurements to the backup

S3: Psi_RP --> Psi_n (you use Psi_1 in the next equations)
S3: Reaction plane correlated v3 is also driven by geometry, right? And not fluctuations.
S4: predicted to be sensitive 
S4: EoS. Signature of a .. -> EoS arising from a ...
S7: Please add some back up slide to inform why the default EP are chosen as in S8 and what systematics are included
S9: The x-axis in your acceptance plots are having opposite sign as for the results plots from next slide and the previous slides where you define the EP?
S11: Increasing with mass is true for the particles here, but is not a general trend for v1 of identified particles 
S12: Are we showing beyond 40% centrality results now? Do you include the systematic uncertainty from EP resolution? The systematic uncertainties are quite small compared to Cameron's or ther results. I dont think dividing by sqrt(12) is a sound approach here, as we are not exploring the full limits of variation, nor are we evaluating the distribution to quote a standard deviation. 
S15: This is true for the particles shown, but not in general, as protons have larger slope than pbar or phi for example. Better to list magnitude of v_1(p) > v_1(K) > v_1(pi)
S25: Approaches zero near?
S25: In the new measurements you present in this talk, there is no non-monotonic dependence 

Best,
Sooraj



On Sun, Aug 20, 2023 at 9:10 AM sharangrav via Star-talks-l <star-talks-l AT lists.bnl.gov> wrote:
Dear Sooraj,

A gentle reminder for the comments on my presentation slides. My
presentation is tomorrow on August 21 at 10:00 AM (GMT+2).
Here is the link to my FCV approved slides:
https://drupal.star.bnl.gov/STAR/presentations/ISMD-2023/First-order-event-plane-correlated-directed-and-triangular-flow-fixed-targ-0

Sorry for the inconvenience caused.
Thanks and regards,
Sharang Rav Sharma

On 2023-08-19 14:06, webmaster--- via Star-talks-l wrote:
> Dear star-talks-l AT lists.bnl.gov members,
>
> Sharang Rav Sharma (sharang.rav AT students.iisertirupati.ac.in) has
> submitted a
> material for a review, please have a look:
> https://drupal.star.bnl.gov/STAR/presentations/ISMD-2023/First-order-event-plane-correlated-directed-and-triangular-flow-fixed-targ-0
>
> ---
> If you have any problems with the review process, please contact
> webmaster AT www.star.bnl.gov
> _______________________________________________
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--
Sooraj Radhakrishnan
Research Scientist,
Department of Physics
Kent State University
Kent, OH 44243

Physicist Postdoctoral Affiliate
Nuclear Science Division
Lawrence Berkeley National Lab
MS70R0319, One Cyclotron Road
Berkeley, CA 94720
Ph: 510-495-2473


--
Sooraj Radhakrishnan
Research Scientist,
Department of Physics
Kent State University
Kent, OH 44243

Physicist Postdoctoral Affiliate
Nuclear Science Division
Lawrence Berkeley National Lab
MS70R0319, One Cyclotron Road
Berkeley, CA 94720
Ph: 510-495-2473


  • Re: [Star-fcv-l] [Star-talks-l] STAR presentation by Sharang Rav Sharma for ISMD 2023 submitted for review, Sooraj Radhakrishnan, 08/20/2023

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