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Subject: STAR Flow, Chirality and Vorticity PWG
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Re: [Star-fcv-l] STAR presentation by Charles Robertson for Quark Matter 2023 submitted for review
- From: subhash <subhash AT rcf.rhic.bnl.gov>
- To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
- Subject: Re: [Star-fcv-l] STAR presentation by Charles Robertson for Quark Matter 2023 submitted for review
- Date: Thu, 27 Apr 2023 18:03:48 +0900
Dear CWR,
Nice abstract. I have a few suggestions for your consideration:
"In heavy ion collisions that are not exactly head-on, a large Orbital Angular Momentum (OAM) is produced that can affect the polarization of the quarks inside the quark-gluon plasma."
-->
In non-central heavy ion collisions, a large Orbital Angular Momentum (OAM) is produced.
"This polarization influences the production of vector mesons and can cause global spin alignment." --> A part of OAM can induce polarization of the quarks and anti-quarks, hence the vector mesons, inside the medium.
l#10-11: from the first phase of the RHIC Beam Energy Scan (BES-I) Au+Au collisions.
Suggest to remove: "and found energy dependence."
"The analysis method employed resonance yield in the angle (θ∗) between the decay daughter’s momentum and the OAM and relied on acceptance and efficiency corrections that are also dependent of θ∗."
-->
The global spin alignment, quantified by the 00th coefficient of the spin density matrix rho_00, is measured by a fit to the acceptance and efficiency corrected \phi meson yield versus polar angle (\theta*) between the daughter kaon in parent's rest frame and OAM direction.
"In this poster, we present an alternative method to extract the spin alignment without analyzing the yield vs. θ∗, but the ⟨cos2θ∗⟩ as a function of pair invariant mass."
-->
In this poster, we present an alternative approach to extract the \rho_00 by utilizing ⟨cos2 θ∗⟩ distribution as a function of pair-invariant mass instead of analyzing the \phi meson yields in cos θ∗ bins.
I would suggest to be conservative and suggest to remove the last part, ie, "We report preliminary results for this method and discuss our results in the context of the energy dependence previously measured by STAR." Instead you can simply mention we will compare measurements using both these methods.
Thanks and regards,
Subhash
On 2023-04-22 04:16 AM, webmaster--- via Star-fcv-l wrote:
Dear star-fcv-l AT lists.bnl.gov members,
Charles Robertson (rober558 AT purdue.edu) has submitted a material for a
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/63531
Deadline: 2023-05-01
---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
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[Star-fcv-l] STAR presentation by Charles Robertson for Quark Matter 2023 submitted for review,
webmaster, 04/21/2023
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Re: [Star-fcv-l] STAR presentation by Charles Robertson for Quark Matter 2023 submitted for review,
subhash, 04/27/2023
- Re: [Star-fcv-l] STAR presentation by Charles Robertson for Quark Matter 2023 submitted for review, Robertson, Charles William, 04/27/2023
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- [Star-fcv-l] STAR presentation by Charles Robertson for Quark Matter 2023 submitted for review, webmaster, 04/21/2023
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Re: [Star-fcv-l] STAR presentation by Charles Robertson for Quark Matter 2023 submitted for review,
subhash, 04/27/2023
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