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Subject: STAR Flow, Chirality and Vorticity PWG
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Re: [Star-fcv-l] STAR presentation by Prabhupada Dixit for DAE HEP 2020 submitted for review
- From: Prithwish Tribedy <ptribedy AT rcf.rhic.bnl.gov>
- To: webmaster AT star.bnl.gov, "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
- Subject: Re: [Star-fcv-l] STAR presentation by Prabhupada Dixit for DAE HEP 2020 submitted for review
- Date: Tue, 15 Sep 2020 11:28:16 -0400
Hello Prabhupada,
The abstract is already in a good shape, please consider the following comments.
Comments on the abstract:
cross section for φ mesons are —> cross section for φ mesons is
φ mesons hadrons allows — > φ mesons allows
collective properties of early stages —> collective properties of the early stages
at a new centre-of-mass energies —> at the new centre-of-mass energies
Event Plane Detector (EPD) allows —> Event Plane Detectors (EPDs) allow
using event plane with large gaps —> using event planes with large gaps
and EPD (2.1<|η|<5.1) —> and EPDs (2.1<|η|<5.1)
High precision test —> A high precision test
constituent quark scaling of v2 (including other hadrons) —> constituent quark scaling of φ meson v2 (by including measurements for other hadrons)
such measurements at the other —> such measurements at the other collision energies
of beam energy scan phase II —> of the RHIC beam energy scan phase II
Comments on the analysis & preliminary approval:
I was looking at you studies:
https://drupal.star.bnl.gov/STAR/system/files/BullCorr_180820.pdf
https://drupal.star.bnl.gov/STAR/system/files/Bulkcorr_meeting2.pdf
1. In the abstract you mentioned “of 54.4 GeV (∼1.3 billion events) and 27 GeV (∼600 million events)”
but I see you only found 600 M for 54.4 and 350M for 27 GeV. Is this difference caused by some quality cuts or you are on your way to accumulate more events?
2. Did you consider the effect of pile-up and bad runs. If not, do you plan to include such in the future analysis?
3. I think the Nhits/hitmax > 0.52 cut can be removed to gain more statistics for this precision analysis.
4. For 27 GeV analysis, a while ago Risa presented Ψ2 event plane resolution for her study, can you please cross-check if your resolution numbers are consistent (at least in the same ballpark) with what she got:
https://drupal.star.bnl.gov/STAR/system/files/Risa_pwg0318_ver2.pdf
Regards,
Prithwish
On 2020-09-14 22:44, webmaster--- via Star-fcv-l wrote:
Dear star-fcv-l AT lists.bnl.gov members,
Prabhupada Dixit (prabhupadad AT iiserbpr.ac.in) has submitted a material for a
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/52051
---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
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-
Re: [Star-fcv-l] STAR presentation by Prabhupada Dixit for DAE HEP 2020 submitted for review,
Prithwish Tribedy, 09/15/2020
-
Re: [Star-fcv-l] STAR presentation by Prabhupada Dixit for DAE HEP 2020 submitted for review,
pdixit, 09/16/2020
- [Star-fcv-l] global polarization in smaller systems, Takafumi Niida, 09/16/2020
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Re: [Star-fcv-l] STAR presentation by Prabhupada Dixit for DAE HEP 2020 submitted for review,
pdixit, 09/16/2020
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