Skip to Content.
Sympa Menu

star-fcv-l - Re: [Star-fcv-l] STAR presentation by Cameron Racz for AUM 2023 submitted for review

star-fcv-l AT lists.bnl.gov

Subject: STAR Flow, Chirality and Vorticity PWG

List archive

Chronological Thread  
  • From: Cameron Racz <cracz001 AT ucr.edu>
  • To: subhash <subhash 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 Cameron Racz for AUM 2023 submitted for review
  • Date: Mon, 31 Jul 2023 12:29:26 -0500

Hi Subhash,

Thank you for the great comments, I have made the changes and uploaded the
new version 2 of my slides.

Cameron Racz
Ph.D. Candidate
Heavy-ion Physics Group
University of California, Riverside






> On Jul 31, 2023, at 12:04 AM, subhash <subhash AT rcf.rhic.bnl.gov> wrote:
>
> Dear Cameron,
>
> Very nice and comprehensive slides. I have a few comments below for your
> consideration:
>
> s#2: "Sign change in dv1/dy is a signal for 1st-order phase transition.".
> It is a strong statement and model dependent, you can soften it, e.g Sign
> of dv1/dy is sensitive to 1st-order phase transition
>
> s#3: "Opportunity to get a complete picture of flow observables across the
> phase transition." --> I would suggest, Opportunity to probe the QCD phase
> diagram through flow observables.
> or, you can rephrase accordingly.
> You can probably remove "Many energies to be used to"
>
> s#4: I think this slide is not necessary. You can consider removing it.
>
> s#9: You are comparing two different beam energies and you want to say the
> v2, v3 ordering is same, which is fine.
> "v3 < 0.1 up to pT ∼ 3 GeV/c" --> I am not sure I understand what do you
> want mean here?
>
> s#14,15: In the title you can mention beam energy, like you are doing for
> all other slides.
>
> s#15: You are focussing on light nuclei. May be you can mention "light
> nuclei" in the title
>
> s#16: 27 GeV (2019) is also part of BES-II
>
> s#18: Replace the figure with the version from arXiv. In this paper the v1
> splitting also increases with _Delta_S_. You should mention this important
> feature.
>
> ps: For completeness, you could also mention there is companion paper
> 2304.03430 observed v1 splitting for light hadrons.
>
>
> Thanks and regards,
> Subhash
>
>
>
> On 2023-07-31 05:26 AM, webmaster--- via Star-fcv-l wrote:
>> Dear star-fcv-l AT lists.bnl.gov members,
>> Cameron Racz (cracz001 AT ucr.edu) has submitted a material for a review,
>> please
>> have a look:
>> https://drupal.star.bnl.gov/STAR/node/64457
>> Deadline: 2023-08-01
>> ---
>> 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





Archive powered by MHonArc 2.6.24.

Top of Page