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Subject: STAR Flow, Chirality and Vorticity PWG
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Re: [Star-fcv-l] FCV PWG meeting on 01/November/2023 Wed. 9:30 AM EDT
- From: Sooraj Radhakrishnan <skradhakrishnan AT lbl.gov>
- To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
- Subject: Re: [Star-fcv-l] FCV PWG meeting on 01/November/2023 Wed. 9:30 AM EDT
- Date: Mon, 6 Nov 2023 15:39:54 -0800
Hi Gavin,
Thanks for the nice presentation with many details. Sorry, I could not attend your talk at the PWG meeting last week. Could please answer a few questions I have on your slides?
S8: Why is the input phi distribution flat in rapidity? Is this a reasonable choice at these low energies? Did you have any evaluation of systematic uncertainty if you input a rapidity dependent distribution? I had asked this before, but did not get a response from you
S8: Do you have an acceptance plot in pT - rapidity for the reconstructed phi mesons?
S15: From what I understand from your back up slide (S.25), the error band on the theory curve is from the uncertainties on rho_00 measurements in the data. In that case, the band can be misleading, particularly as the BES-I uncertainties were large. Do you know if the lower end of the error band corresponds to the lower end of variation in data? Can we get a set of values for the curve from the theorists for +-2 sigma range from BES-I of rho_00s (at least of rho_00^y), so that we can update the curve with the uncertainties and values corresponding to BES-II measurements? (My point is we should get the calculations without telling the theorists what our BES-II measurements are, and I know the data points are different from our Preliminary for BES-II)
S13: With the BES-II data, can we extend the measurements to lower pT? At LHC, rho_00 < 1/3 was observed for low pT, do we also see similar trend at lower energies at RHIC? What is the reason for stopping at 1.5 GeV/c?
thanks
Sooraj
On Wed, Nov 1, 2023 at 4:54 PM Sergei Voloshin via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:
Dear Gavin,Unfortunately I was not able to attend the meeting. I looked through your slides but could not find answers to several important (from my point of view) questions:- Did you try to get an efficiency for phi reconstruction as a function of the relative angle of one of the daughters to the phi momentum?(see for example slide 6 in my presentation https://drupal.star.bnl.gov/STAR/system/files/voloshin_SpinAlgnAcceptance-4.pdf )- What values of phi v2(pt) were used?- How large is the effect of elliptic flow "entanglement" with the efficiency to rho00 calculations? (again you can see my presentation, if it is not clear what I mean here).best regards,SergeiOn Tue, Oct 31, 2023 at 12:26 PM Gavin Wilks via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:Dear Conveners,
I would like to present some slides at this week’s meeting regarding a paper proposal titled: “Differential measurements of φ-meson global spin alignment in Au+Au collisions at RHIC”.
Best,
Gavin
> On Oct 29, 2023, at 21:58, subhash via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:
>
> Dear All,
>
> We shall have our weekly FCV PWG meeting this Wednesday (01/Nov/2023) at 9:30 AM EDT. If you would like to present please let us know. Please try posting your slides by Tuesday. The agenda will be collected at: https://urldefense.com/v3/__https://nam04.safelinks.protection.outlook.com/?url="https*3A*2F*2Fdrupal.star.bnl.gov*2FSTAR*2Fblog*2Fjjiastar*2Fbulkcorr&data=05*7C01*7Cgwilks3*40groute.uic.edu*7C2cf353dcaea34799102808dbd8f42c46*7Ce202cd477a564baa99e3e3b71a7c77dd*7C0*7C0*7C638342315463237743*7CUnknown*7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0*3D*7C3000*7C*7C*7C&sdata=7TaVBSaFStsQSg8WcaUNdHwJB1bBjhS3obMNIlK5DnI*3D&reserved=0__;JSUlJSUlJSUlJSUlJSUlJSUlJSUlJSU!!P4SdNyxKAPE!Bqgg_Pbnmg8IXawxhk0poc0O3PTc3VNZldVfbvf84Xi0NyZciPXxDur7C4k9KCFUnW3U6T6l_Kf8Vl2dL5OuzvkI$
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--_______________________________________________======================================
Sergei A. VoloshinDistinguished Professor,Department of Physics and Astronomy,Wayne State University,
666 W. Hancock, Detroit, Michigan, 48201
e-mail: sergei.voloshin AT wayne.edu
======================================
Star-fcv-l mailing list
Star-fcv-l AT lists.bnl.gov
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Sooraj Radhakrishnan
Research Scientist,
Department of Physics
Kent State University
Kent, OH 44243
Physicist Postdoctoral Affiliate
Lawrence Berkeley National Lab
MS70R0319, One Cyclotron Road
Email: skradhakrishnan AT lbl.gov
-
Re: [Star-fcv-l] FCV PWG meeting on 01/November/2023 Wed. 9:30 AM EDT,
sharangrav, 11/01/2023
- Re: [Star-fcv-l] FCV PWG meeting on 01/November/2023 Wed. 9:30 AM EDT, sharangrav, 11/01/2023
- <Possible follow-up(s)>
- Re: [Star-fcv-l] FCV PWG meeting on 01/November/2023 Wed. 9:30 AM EDT, Gavin Wilks, 11/01/2023
- Re: [Star-fcv-l] FCV PWG meeting on 01/November/2023 Wed. 9:30 AM EDT, Zuowen Liu, 11/01/2023
- Re: [Star-fcv-l] FCV PWG meeting on 01/November/2023 Wed. 9:30 AM EDT, Junyi Han, 11/01/2023
-
Re: [Star-fcv-l] FCV PWG meeting on 01/November/2023 Wed. 9:30 AM EDT,
Sergei Voloshin, 11/01/2023
- Re: [Star-fcv-l] FCV PWG meeting on 01/November/2023 Wed. 9:30 AM EDT, Sooraj Radhakrishnan, 11/06/2023
- Re: [Star-fcv-l] FCV PWG meeting on 01/November/2023 Wed. 9:30 AM EDT, Sooraj Radhakrishnan, 11/06/2023
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