STAR Correlations and Fluctuations PWG

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

Dear Ashutosh,

Please find my comments below.

It would be nice to explain why among of many STAR energies you chose \sqrt{s_{NN}} = 27 GeV.

Please consider some general one or two sentences about femtoscopy, to explain what can be studies with this technique. 

Explain also why you consider different pseudorapidity, transverse pair momentum and pair azimuthal angle. 

Explain please what is the tilt angle. 

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 webmaster--- via Star-cf-l <star-cf-l AT lists.bnl.gov> w dniu 12.07.2022, o godz. 08:14:

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

Ashutosh Pandey (ashutosh.iitb007 AT gmail.com) has submitted a material for a  
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/60249

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