Dear Hanna,
Thank you for your comments, I have implemented your suggestions.
Regarding your last point, the suppression shown at 3GeV is mainly from the contribution of Strangeness conservation and when comparing with the statistical hadronization model using the QvdW interactions we observe that interactions between baryons also show
suppression at this energy, implying that hadronic interactions play a role in the suppression of the cumulant ratios.
Find the updated version in the same link as before:
https://drupal.star.bnl.gov/STAR/presentations/SQM-2022/Fluctuations-Lambda-Multiplicity-Distribution-AuAu-collisions-sqrtsNN30-GeV-S
Best regards,
Jonathan Ball
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Today's Topics:
1. Re: STAR presentation by Jonathan Gonzalo Ball Cap for SQM
2022 submitted for review (Hanna Paulina Zbroszczyk)
2. Re: STAR presentation by Ashish Pandav for SQM 2022 submitted
for review (Hanna Paulina Zbroszczyk)
----------------------------------------------------------------------
Message: 1
Date: Mon, 6 Jun 2022 10:53:34 +0200
From: Hanna Paulina Zbroszczyk <hanna.zbroszczyk AT pw.edu.pl>
To: "star-cf-l AT lists.bnl.gov" <star-cf-l AT lists.bnl.gov>
Subject: Re: [Star-cf-l] STAR presentation by Jonathan Gonzalo Ball
Cap for SQM 2022 submitted for review
Message-ID: <AE25A070-CB7D-411C-A8F1-812C364D15F9 AT pw.edu.pl>
Content-Type: text/plain; charset="utf-8"
Hi Jonathan,
Please find below comments to your nice slides:
Slide 2: Add definitions of cumulants (more formulas)
Figure does not contain description on Y axis (title).
Name / describe freeze-out parameters you intend to investigate
Slide 3: Add a reference /any link to KF-Package (describe how it works)
Slide 4: second bullet, add a space: cumulants( -> cumulants (
Add a Poissin baseline (name it), you mention in but never show it
Slide 5: you mention strong suppression for lambda cumulants, add also interpretation of it
In genera?, I would add more physics discussion / explanation.
Thanks,
Hanna
Hanna Paulina Zbroszczyk
PhD DSc Eng, Professor WUT
E-mail: hanna.zbroszczyk AT pw.edu.pl
Tel: +48 22 234 5851 (office)
Address:
Warsaw University of Technology
Faculty of Physics
Nuclear Physics Division
Koszykowa 75
Office: 117b (via 115)
00-662 Warsaw, Poland
> Wiadomo?? napisana przez webmaster--- via Star-cf-l <star-cf-l AT lists.bnl.gov> w dniu 31.05.2022, o godz. 17:18:
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> Dear star-cf-l AT lists.bnl.gov members,
>
> Jonathan Gonzalo Ball Cap (jballcap AT central.uh.edu) has submitted a material
> for a review, please have a look:
>
https://urldefense.com/v3/__https://drupal.star.bnl.gov/STAR/node/59788__;!!LkSTlj0I!FAybFf0mGH0n8ye1QJ2WVJ4sBiid9Qx4p6XP861i4Cz0Lpof09NZJ8DryIeh55RuoSEoNhETTiQ8FT7_SWILH0yX16Ga0QZp0fmMWSg$
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Message: 2
Date: Mon, 6 Jun 2022 11:11:54 +0200
From: Hanna Paulina Zbroszczyk <hanna.zbroszczyk AT pw.edu.pl>
To: "star-cf-l AT lists.bnl.gov" <star-cf-l AT lists.bnl.gov>
Subject: Re: [Star-cf-l] STAR presentation by Ashish Pandav for SQM
2022 submitted for review
Message-ID: <CC01A3B1-55CF-4ECB-96A1-E214A391A74D AT pw.edu.pl>
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Dear Ashish,
Please find below my comments to your nice slides:
Slide 2: add a reference to the second plot
Slide 3: add a reference to the plot
Slide 4: add references to the plots
Genera? comments: add more physics discussion about possible interpretation about C7/C1 and C8/C2 measurements.
With those implemented, I sign off.
Thanks,
Hanna
Hanna Paulina Zbroszczyk
PhD DSc Eng, Professor WUT
E-mail: hanna.zbroszczyk AT pw.edu.pl
Tel: +48 22 234 5851 (office)
Address:
Warsaw University of Technology
Faculty of Physics
Nuclear Physics Division
Koszykowa 75
Office: 117b (via 115)
00-662 Warsaw, Poland
> Wiadomo?? napisana przez webmaster--- via Star-cf-l <star-cf-l AT lists.bnl.gov> w dniu 02.06.2022, o godz. 12:56:
>
> Dear star-cf-l AT lists.bnl.gov members,
>
> Ashish Pandav (apandav10 AT gmail.com) has submitted a material for a review,
> please have a look:
>
https://urldefense.com/v3/__https://drupal.star.bnl.gov/STAR/node/59832__;!!LkSTlj0I!FAybFf0mGH0n8ye1QJ2WVJ4sBiid9Qx4p6XP861i4Cz0Lpof09NZJ8DryIeh55RuoSEoNhETTiQ8FT7_SWILH0yX16Ga0QZpeEaSq4g$
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