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Subject: STAR Flow, Chirality and Vorticity PWG
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Re: [[Star-fcv-l] ] FCV PWG meeting on 31/July/2024 Wed. 9:30 AM EDT
- From: Sooraj Radhakrishnan <skradhakrishnan AT lbl.gov>
- To: star-fcv-l AT lists.bnl.gov
- Cc: star-fcv-l-request AT lists.b… <star-fcv-l-request AT lists.bnl.gov>
- Subject: Re: [[Star-fcv-l] ] FCV PWG meeting on 31/July/2024 Wed. 9:30 AM EDT
- Date: Fri, 2 Aug 2024 17:57:14 -0700
Hi Xionghong, Minmin,
Thanks for this nice study and the presentation. If you use the two component model that we had for proton directed flow, I think it will give a natural explanation for the deuteron v1 being positive. I think currently no models explain the deuteron v1. But if you look at the two components separately, the anti-deuteron v1 and (to be scaled) difference, on your slides 12 and 13, they seem to follow the mass number scaling. It would be good if this can be checked
thanks,
Sooraj
On Wed, Jul 31, 2024 at 6:56 PM MMWang <minminwang12345 AT 163.com> wrote:
Dear convenors,My slides for the discussion can be found at https://drupal.star.bnl.gov/STAR/blog/hexh/anti-deuteron-v1-146-173-196-GeVBest regards,Minmin Wang---- Replied Message ----Dear convenors,
From <hexh AT impcas.ac.cn> Date 7/29/2024 23:44 To <star-fcv-l AT lists.bnl.gov>,
<star-fcv-l-request AT lists.bnl.gov>Cc <minminwang12345 AT 163.com> Subject RE: [[Star-fcv-l] ] FCV PWG meeting on 31/July/2024 Wed. 9:30 AM EDT
Minmin Wang would like to present the results for (anti-)deuteron v1 at
14.6, 17.3 and 19.6 GeV.
She couldn't receive the email from FCV group. Thanks.
Best regards,
Xionghong
-----Original Message-----
From: star-fcv-l-owner AT lists.bnl.gov <star-fcv-l-owner AT lists.bnl.gov> On
Behalf Of subhash
Sent: Monday, July 29, 2024 10:08 PM
To: star-fcv-l-request AT lists.bnl.gov; STAR Flow, Chirality and Vorticity PWG
<star-fcv-l AT lists.bnl.gov>
Subject: [[Star-fcv-l] ] FCV PWG meeting on 31/July/2024 Wed. 9:30 AM EDT
Dear All,
We shall have our weekly FCV PWG meeting this Wednesday (31/July/2024) at
9:30 AM EDT. If you wish to present please let us know. The agenda will be
collected at:
https://drupal.star.bnl.gov/STAR/blog/jjiastar/bulkcorr
Please send us your slides by Tuesday. Zoom details are copied below.
Thanks and regards,
Prithwish, Zhenyu and Subhash
ZOOM LINK FOR FCV MEETING:
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Sooraj Radhakrishnan
Research Scientist,
Department of Physics
Kent State University
Kent, OH 44242
Physicist Postdoctoral Affiliate
Lawrence Berkeley National Lab
MS70R0319, One Cyclotron Road
Email: skradhakrishnan AT lbl.gov
- Re: [[Star-fcv-l] ] FCV PWG meeting on 31/July/2024 Wed. 9:30 AM EDT, Sooraj Radhakrishnan, 08/02/2024
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