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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Sharang Rav Sharma for EMMI Workshop Probing dense ... got commented by Prithwish Tribedy

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: sharangrav <sharangrav AT rcf.rhic.bnl.gov>
  • To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Cc: webmaster AT star.bnl.gov, sharang.rav AT students.iisertirupati.ac.in
  • Subject: Re: [Star-fcv-l] STAR presentation by Sharang Rav Sharma for EMMI Workshop Probing dense ... got commented by Prithwish Tribedy
  • Date: Tue, 13 Feb 2024 09:49:13 +0530

Dear Prithwish,

Thank you very much for your valuable comments. Here is the link to my updated presentaion slides.
https://drupal.star.bnl.gov/STAR/presentations/EMMI-Workshop-Probing-dense-baryonic-matter-hadrons-II-FAIR-Phase-0/Overview-fixed-tar
I have also included the references for the previous STAR talks on my slides.
Please let me know if you have any further comments.

Thanks and regards,
Sharang

On 2024-02-12 22:30, webmaster--- via Star-fcv-l wrote:
Dear star-fcv-l AT lists.bnl.gov members,

Prithwish Tribedy ( ptribedy AT bnl.gov ) 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/EMMI-Workshop-Probing-dense-baryonic-matter-hadrons-II-FAIR-Phase-0/Overview-fixed-tar

Comment:
Very nice slides. It seems you put a lot of efforts in making these results
to create this review talk -- good job. Some of your slides are heavy. I hope
you will have time to cover them all. A few of your slides lack references to
preliminary data (you have to cite previous STAR talks). Also, consider
adding a highlight sentence (in color) if you think a slide will take too
long. I leave it to you.

I sign off with a few comments.

Slide#4:
"Enlarged rapidity acceptance" --> "Extended pseudorapidity acceptance"
"Extends η coverage from 1.0 to 1.5" --> "Extends η coverage from ±1.0 to
±1.5"
Slide#6:
"Two main detectors" --> "Two detectors"
Slide#8:
"event-by-event fluctuations,"-->"event-by-event geometry and fluctuations,"
Slide#10:
"increases in magnitude with increasing rapidity" --> "increases in magnitude
with increasing rapidity for most particle species"
"Magnitude of v 1 increases with increasing mass of the particle" -->
"Magnitude of v1 has a strong particle species dependence"
Slide#11:
I don't understand this statement:
"v1 slope decreases in magnitude as collision energy increases --> Stronger
tilted expansion."
Do you mean v1 slope decrease is due to more boost invariant structure of 3D
geometry at higher energies ? This would not mean stronger tilt,
it would mean less tilt in a given slice of rapidity.

After this "Strong mean field at high baryon density region" add "(at lower
energies)"

Slide#12:
After the first bullet on about negative slope add "at low pT"
Slide#13:
The right plot needs a reference for the preliminary results

Slide#18:
Needs a reference. "Disappearance of partonic collectivity" --> "Possible
indication of the disappearance of partonic collectivity"

Slide#22:
"Geometry drives v3(\psi_1)" --> "strong geometric effect"
You should use this as your first bullet : "geometry drives v3(\psi_1)"
because non-zero v3(\psi_1) is already an indication of geometry driven
v3(\Psi_1)

Slide#24:
"from coalescence mechanism" --> "from coalescence of nucleons"

Slide#27:
Needs a reference to STAR results (Ben's QM 2022 talk maybe)

Slide#30:
"Larger v_3{\Psi_1} for peripheral than central collisions" --> "Nonzero
v_3{\Psi_1}, stronger in peripheral than central collisions"
"observed p T spectra" --> "observed for p_T spectra"
"indicating less baryon stopping" -->"indicating centrality-dependent baryon
stopping"








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