STAR Flow, Chirality and Vorticity PWG

[vipul <vipul AT rcf.rhic.bnl.gov>]

Dear Conveners,

Please let me know if you have comments and suggestions on the 
proceedings.
If not, please sign off the proceedings.

Thanks,
With Regards,
Vipul

On 2024-09-27 12:36, vipul wrote:
> Dear Richard,
>
> Please let me know if there is more comments and suggestions on the 
> proceedings.
>
> Thanks,
> With Regards,
> Vipul
>
> On 2024-09-25 20:18, vipul wrote:
> > Dear Richard,
> >
> > Thank you very much for your comments and nice suggestions.
> > I have modified the proceedings with these.
> >
> > Please find updated version in the following link:
> > https://drupal.star.bnl.gov/STAR/system/files/Proceedings_STARflowHighlights_v1.pdf
> >
> > Yes, there is a limit on pages (between 3-10) but not exactly 6,
> > therefore I have added all the required references.
> >
> > Thanks,
> > With Regards,
> > Vipul
> >
> > On 2024-09-25 03:10, Richard Seto wrote:
> > > Vipuli,
> > > Nice comprehensinve proceedings.
> > > Most of the correction are grammar and wording, expect for an
> > > important change in the v_3 physics (indicated below)
> > >
> > > P1 column 2. "The observed phase transistion...." ->
> > > "Lattice QCD calculations indicate that the phase transition in the
> > > low mu_B region is a smooth crossover at Tc of about 150 MeV [give 
> > > the
> > > reference]. In the high mu_B region of the QCD phase diagram, the
> > > transition is expected to be first order ending at a critical end
> > > point as one progresses to lower mu_B [give a reference]. An
> > > expected...."
> > >
> > > Maybe you can get away with not referencing the Lattice(low mu_B) and
> > > analytical (high mu_B) calculations if reference 2 gives those
> > > references. Are you limitted to 6 pages. I will assume that you are.
> > >
> > > P2
> > > "the" after "explore" so it says "explore the QCD...."
> > >
> > > Even though you are low on space, you need to give a reference for
> > > BESII. You can probablty get away with nor referencing BES I, if your
> > > reference to BES II references BES I. You showd reference NA61 etc -
> > > but you don't have room. Hopefullyreference 2 has those and you can
> > > get away with it.
> > >
> > > Section 2.
> > > You can shorten the first paragraph to save space, if that helps. 
> > > Here
> > > is a suggestion:
> > >
> > > "RICH is a highly versatile collider, capable of colliding various
> > > nuclear species (U, Au, Ru, Zr, Cu, Al, O, He3 and d) and protons, at
> > > energies between 7.7 GeV and 200 GeV center of mass, and from 3.0 to
> > > 7.7 GeV in fixed-target mode."
> > >
> > > Bottom of column 1
> > > "Following a major upgrade, STAR provides full azimulthal coverage
> > > over a wide range in rapidity as depicted in Fugure 2. Large...."
> > >
> > > secction 3
> > > par 1, line 7, "as [5]" -> "[5]"
> > >
> > > P4
> > > For the faraday effect use [11]. For the transported quark effect you
> > > should probably reference the arXiv: https://arxiv.org/abs/2304.02831
> > > [1] since it has not been published yet.
> > >
> > > 4.3
> > > This is a very important major correction to correct the physics
> > > message:
> > >
> > > "An initial triangular shape in the initial geometry will result in a
> > > triangular flow v_3. This triangular shape, at higher energies, is
> > > attributed to even-by-event fluctuations in the positions of the
> > > participating nucleons, and is uncorrelated to the initial reaction
> > > plane PSI_1. At lower energies (sqrt_sNN=3 GeV) a triagular flow
> > > correlated to the reaction plane is clearly seen as shown in figure 
> > > 4,
> > > indicating that the triagular shape arises from dynamical effects due
> > > to stopping, the passing time of the spectators and the expansion of
> > > the fireball. The values of....."
> > >
> > > -Rich
> > >
> > > Richard Seto
> > > richard.seto AT ucr.edu
> > > Department of Physics and Astronomy
> > > University of California, Riverside
> > > Riverside, CA 92521
> > >
> > > > On Sep 22, 2024, at 9:33 AM, webmaster AT star.bnl.gov wrote:
> > > >
> > > > Dear star-fcv-l AT lists.bnl.gov members,
> > > >
> > > > Vipul Bairathi (vipul.bairathi AT gmail.com) has submitted a material
> > > > for a
> > > > review, please have a look:
> > > > https://drupal.star.bnl.gov/STAR/node/68996
> > > >
> > > > ---
> > > > If you have any problems with the review process, please contact
> > > > webmaster AT www.star.bnl.gov
> > >
> > >
> > >
> > > Links:
> > > ------
> > > [1] 
> > > https://urldefense.com/v3/__https://arxiv.org/abs/2304.02831__;!!P4SdNyxKAPE!HZta5FTGNjHRavwOBdHydT7XsYqO3osW1puyL8EawbZltrrr-W8q8EtI9s4L53zCjdgYiv8jyUUvZB-F8nO6$