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Subject: STAR HardProbes PWG
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- From: Barbara Trzeciak <barbara.trzeciak AT gmail.com>
- To: 沈丹丹 <shendandan AT mail.sdu.edu.cn>, STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
- Subject: Re: [Star-hp-l] QM Abstract Letter of Intent
- Date: Mon, 3 Apr 2023 09:03:14 +0200
Dear Dandan,
Thank you for your interesting abstract.
I would like to however remind that in order to submit an abstract, we require that progress of the analysis has been presented at the PWG meetings.
We should see a first look at the data, e.g. signal extraction, and at least two presentations to the HP group.
Best regards,
Barbara
On Mon, Apr 3, 2023 at 3:52 AM 沈丹丹 via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:
Hello HP-working group,I intend to submit an abstract for QM 2023.The title is "Measurements of $J/\psi$ polarization in Ru+Ru and Zr+Zr collisions at $\sqrt{s_{NN}} = 200$ GeV from STAR experiment ".abstract:$J/\psi$ is an important probe to study the properties of the quark-gluon plasma (QGP) created in heavy-ion collisions. A strong suppression of $J/\psi$ and zero $J/\psi$ $v_{2}$ have been observed in the isobar collisions system at RHIC-STAR experiment, which indicates a strong coupling of $J/\psi$ and QGP and limited regeneration effect. Beside $J/\psi$ nulcear modification factor and $J/\psi$ azimuthal anisotropy observable, the $J/\psi$ polarization could be a new degree of studying QGP properties and $J/\psi$ production mechanism in heavy-ion collisions. Moreover, it has been hypothesized that $J/\psi$ can be polarized by different mechanism, such as the spin-orbit coupling of $J/\psi$ and QGP's large angular momentum produced in non-central heavy-ion collisions and the early production of $J/\psi$ could makes its polarization sensitive to the strong magnetic field produced in early stage.In this talk, we will present the first $J/\psi$ polarization measurement of in a heavy-ion collision in RHIC energy. The $J/\psi$ polarization results in the Helicity frame, Collins-Soper frame as well as the polarization with respect to the event-plane in Ru+Ru and Zr+Zr at $\sqrt{s_{NN}} = 200$ GeV will be present and its physics implications will also be discussed.PDF version can be find in this link: https://drupal.star.bnl.gov/STAR/system/files/QM2023_abs_DandanShen_0.pdfBest,Dandan
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-
[Star-hp-l] QM Abstract Letter of Intent,
沈丹丹, 04/02/2023
- Re: [Star-hp-l] QM Abstract Letter of Intent, Barbara Trzeciak, 04/03/2023
- <Possible follow-up(s)>
- Re: [Star-hp-l] QM Abstract Letter of Intent, Dandan Shen, 04/03/2023
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