STAR Correlations and Fluctuations PWG

[Kincses Dániel <kincses AT ttk.elte.hu>]

Dear Hanna,

Thank you for your comments, I implemented all your suggestions.
I included one more slide about the motivation at the top rhic energy, and also extended the core-halo slide:
https://drupal.star.bnl.gov/STAR/system/files/kincsesd_WPCF2023_talk_v3.pdf

Thanks,
Daniel

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Feladó: Star-cf-l <star-cf-l-bounces AT lists.bnl.gov>, meghatalmazó: Hanna Paulina Zbroszczyk via Star-cf-l <star-cf-l AT lists.bnl.gov>
Elküldve: 2023. október 31., kedd 9:10
Címzett: star-cf-l AT lists.bnl.gov <star-cf-l AT lists.bnl.gov>
Másolatot kap: Hanna Paulina Zbroszczyk <hanna.zbroszczyk AT pw.edu.pl>
Tárgy: Re: [Star-cf-l] STAR presentation by Daniel Kincses for WPCF 2023 submitted for review

 

Dear Daniel,

Thank you for your slides.

Please find my comments below.

Slide 1: Add information that your work is partially funded by DOE, add logo of DOE.

Slide 4/5: I find useful listing of all approaches, however it would be nice to spend more time on what is the advantages of Levy parametrization at top RHIC energies (as we do not observe spherical source, and as we are far away from CP, etc..).

Please extend the motivation of your studies

Slide 14: please give more introduction to the Core-halo picture, what is the motivation, why it is proposed, how it may change with different contributions, how (RHIC?) meauremets can be sensitive to these different fractions, etc..

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

Wiadomość napisana przez EsumiShinIchi via Star-cf-l <star-cf-l AT lists.bnl.gov> w dniu 31.10.2023, o godz. 08:33:

Dear Daniel

Thank you very much for the very nice presentation. I here send you some minor 

comments, that I find your instruction in your earlier pages are quite nice, especially 

how this alpha parameter acts as non-gaussian source shape etc in p5. While I also 

think it would be very good, if you could tell what would be the merit of this 1D Levy 

fitting compared to the usual 3D gaussian source analysis, if you can at least say 

this non-gaussian shape is not just coming from the 3D to 1D conversion/averaging, 

that would have different source sizes depending on the 3 directions. Therefore you 

might like to go to the 3D-Levy as your next step, though… Thanks again. 

Best regards, ShinIchi

2023/10/31 16:04、Kincses Dániel via Star-cf-l <star-cf-l AT lists.bnl.gov>のメール:

Dear Conveners,

My talk is currently scheduled for the first day of the conference (November 6). I would appreciate any comments or suggestions!

Thanks,
Daniel

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Elküldve: 2023. október 26., csütörtök 10:47
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Tárgy: [Star-cf-l] STAR presentation by Daniel Kincses for WPCF 2023 submitted for review

 

Dear star-cf-l AT lists.bnl.gov members,

Daniel Kincses (kincses AT ttk.elte.hu) has submitted a material for a review,  
please have a look:
https://drupal.star.bnl.gov/STAR/node/65727

Deadline: 2023-11-06
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webmaster AT www.star.bnl.gov
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