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star-fcv-l - Re: [[Star-fcv-l] ] STAR presentation by Sharang Rav Sharma for 68th DAE SYMPOSIUM ON NUCLEA... got commented by Subhash Singha

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: Richard Seto <seto AT ucr.edu>
  • To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Cc: subhash <subhash AT rcf.rhic.bnl.gov>, webmaster AT star.bnl.gov, SHARANG RAV SHARMA <sharang.rav AT students.iisertirupati.ac.in>
  • Subject: Re: [[Star-fcv-l] ] STAR presentation by Sharang Rav Sharma for 68th DAE SYMPOSIUM ON NUCLEA... got commented by Subhash Singha
  • Date: Tue, 10 Sep 2024 12:36:20 -0700

Hi Sharang
Minor gramatical stuff except last question.
Page 1 2nd column

Par 0 L1- TPC -> The TPC
L5 TOF -> the TOF
L6 delete “by putting an appropriate restriction on its value”

Par 1
L1 “Net particle represents” -> “Net particle refers to “
L20 kill “trend”
L21 kill “which happens”

In the last sentence - You talk about a comparison with JAM. Is it on the
figures?
It not you will have to say (not shown) after “Jam model”

Are there systematic errors on the points, and are they smaller than the
points. If so, you should stay that.

-Rich



Richard Seto
richard.seto AT ucr.edu
Department of Physics and Astronomy
University of California, Riverside
Riverside, CA 92521



> On Sep 9, 2024, at 9:34 PM, sharangrav <sharangrav AT rcf.rhic.bnl.gov> wrote:
>
> Dear Subhash,
>
> I have updated my abstract. If there are no further comments can we proceed
> further for the approval.
> Link to updated abstract:
> https://drupal.star.bnl.gov/STAR/presentations/68th-DAE-SYMPOSIUM-NUCLEAR-PHYSICS/Measurement-directed-flow-high-baryon-density-regio
>
> Thanks and regards,
> Sharang
>
> On 2024-09-06 16:50, sharangrav wrote:
>> Dear Subhash,
>> Thank you for your valuable comments. I have incorporated the comments
>> in the abstract and hereby sharing the link to the updated version.
>> https://drupal.star.bnl.gov/STAR/presentations/68th-DAE-SYMPOSIUM-NUCLEAR-PHYSICS/Measurement-directed-flow-high-baryon-density-regio
>> There was a page restriction so I have tried to keep everything under
>> 2 page. Please let me know if you have further comments.
>> Thanks and regards,
>> Sharang
>> On 2024-09-06 13:39, webmaster AT star.bnl.gov wrote:
>>> Dear star-fcv-l AT lists.bnl.gov members,
>>> Subhash Singha ( connectsubhash AT gmail.com ) has commented on a material
>>> originally submitted by Sharang Rav Sharma (
>>> sharang.rav AT students.iisertirupati.ac.in ) at
>>> https://drupal.star.bnl.gov/STAR/presentations/68th-DAE-SYMPOSIUM-NUCLEAR-PHYSICS/Measurement-directed-flow-high-baryon-density-regio
>>> Comment:
>>> Dear Sharang,
>>> Nice proceedings. I have a few suggestions below.
>>> Please include line numbers.
>>> Introduction:
>>> "At these energies, --> "At these lower energies,
>>> "This leads to a significant influence .... flow harmonics" --> This
>>> results
>>> in a significant influence of the shadowing effect, where passing
>>> spectator
>>> nucleons obstruct the interaction region, thereby affecting the measured
>>> flow
>>> observables.
>>> net-kaon, net-proton --> you could add definition for net-kaon and
>>> net-proton, either here or in next section. It is not a particle itself,
>>> but
>>> constructed from particle and antiparticle's v1.
>>> = 3.2 – 4.5 GeV --> Specify each beam energies reported
>>> Analysis Details:
>>> "Mass-squared (m2)" --> Moreover, mass-squared (m2) information from TOF
>>> "The reaction plane angle is estimated by the event plane method using
>>> Event
>>> Plane Detector (EPD) within" --> The event plane angle, a proxy for the
>>> reaction plane angle, is reconstructed using the Event Plane Detector
>>> (EPD),
>>> which has coverage ...
>>> "3 eta sub-events" --> 3 η-sub events, (also indicate the sub-event
>>> ranges)
>>> Results:
>>> "with increasing rapidity for all particle" --> with increasing rapidity
>>> for
>>> all particles
>>> "is attributed" --> can be attributed
>>> "The net-kaon dv1/dy .... 19.6 GeV" --> The net-kaon dv1dy trend shows a
>>> minimum between sqrt{s_{NN}} = 4.5 and 7.7 GeV, which happens at lower
>>> collision energies than for net-protons, where the minimum is found
>>> between
>>> sqrt{s_{NN}} = 11.5 and 19.6 GeV [7].
>>> Reference [7] and [1] is same, please correct it
>>> I sign off with these addressed.
>>> ---
>>> If you have any problems with the review process, please contact
>>> webmaster AT www.star.bnl.gov




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