STAR Correlations and Fluctuations PWG

[Hanna Paulina Zbroszczyk <hanna.zbroszczyk AT pw.edu.pl>]

Hi Li’Ang,

Please find my comments on your nice poster.

Please remove the comma after your email.

Motivation:

Consider making the motivation part shorter. The content can remain the same but I suggest to make the statement shorter to give a space to some extra definitions.

Correct \bar{K^0} where appropriate,

Define S(\vec{r}), \vec{r}, \Psi.

k* usually denotes momentum of the first particle in PRF (if PRF is used, but at your measurements I see q_{inv} instead, which is also undefined). Instead of k* formalism I suggest to work with q, that you can define as relative momentum.

Define q_{inv}

Particle reconstruction:

Add please a reference [3] to KF where you describe the 3rd bullet.

Correlation function:

Can you add missing \bar at some K^0?

Please briefly define all symbols you use in the LL parametrization.

Define \epsilon

Particle emission source parameters:

Lednicky-Lyuboshitz Weight -> Lednicky-Lyuboshitz model.

Please add a reference to CRAB

With those implemented, I sign off.

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 webmaster--- via Star-cf-l <star-cf-l AT lists.bnl.gov> w dniu 25.08.2023, o godz. 08:25:

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

Liang Zhang (liangzhang AT mails.ccnu.edu.cn) has submitted a material for a  
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/64870

Deadline: 2023-09-03
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