STAR Correlations and Fluctuations PWG

["Hu, Yu" <yuhu AT bnl.gov>]

Dear Hanna,

Thanks for your comments! Please fine my updated slides from the link below:

https://drupal.star.bnl.gov/STAR/system/files/CPOD24_20240522_YuHu_dL_v2.pdf

In addition, I would prefer to keep some of the major technical words there (like Smoothness approximation, and the Effective range expansion...) to give people an idea about how the equation models into S and Psi. But I don't think in the talk I will give too much time to explain it, like how smoothness approximation to evaluate the off-shell non-zero q for non-identical particles in the analytical equation, this would be too detailed. In case people ask, I will try to explain it in detail

Thank you.

Best,

Yu

---

From: Star-cf-l <star-cf-l-bounces AT lists.bnl.gov> on behalf of Hanna Paulina Zbroszczyk via Star-cf-l <star-cf-l AT lists.bnl.gov>
Sent: Wednesday, May 8, 2024 16:03
To: star-cf-l AT lists.bnl.gov <star-cf-l AT lists.bnl.gov>
Cc: Zbroszczyk Hanna <hanna.zbroszczyk AT pw.edu.pl>
Subject: Re: [Star-cf-l] STAR presentation by Yu Hu for CPOD 2024 submitted for review

 

Dear Yu,

Slide 4:

Please mention more about smoothness approximation and effective range of expansion in your talk.

Mentioning just bullets does not help to understand physics assumptions (mostly known for femtoscopic experts).

Slide 6:

3 GeV -> \sqrt{s_{NN}}

Slide 9:

Be consistent while you mention units:

p = 20 MeV -> p=20 MeV/c

k* \simeq 20 MeV -> k* \simeq 20 MeV/c

Kind regards,

Hanna

prof. dr hab. inż. Hanna Zbroszczyk
E-mail: hanna.zbroszczyk AT pw.edu.pl
Tel: +48 22 234 5851 (biuro)

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Wiadomo¶ć napisana przez webmaster--- via Star-cf-l <star-cf-l AT lists.bnl.gov> w dniu 08.05.2024, o godz. 17:46:

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

Yu Hu (yuhu AT bnl.gov) has submitted a material for a review, please have a  
look:
https://drupal.star.bnl.gov/STAR/node/67710

Deadline: 2024-05-20
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