STAR Flow, Chirality and Vorticity PWG

[Richard Seto <seto AT ucr.edu>]

Hi vipul
No more comments . you are free to submit
Rich
Richard Seto
richard.seto AT ucr.edu
Department of Physics and Astronomy
University of California, Riverside
Riverside, CA 92521
Sent from my iPhone

> On Sep 29, 2024, at 7:22 PM, vipul <vipul AT rcf.rhic.bnl.gov> wrote:
> 
> 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://urldefense.com/v3/__https://arxiv.org/abs/2304.02831__;!!P4SdNyxKAPE!Gzi_Btun-rzFf6k0xea2sKO0BmeAGw3fl8VA7hd9DFvW6G_sHdCdqLP7EB4qaiK3zMlfRhonyHtS89Gp_SSV$
>>>>  
>>>> [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$