STAR Correlations and Fluctuations PWG

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

Dear Paweł,

Please find my comments to your nice poster:

Abstract: two kinds of particles -> two types of particles (or two particles’ species)

Asymmetry gives knowledge 0-> Asymmetry gives us knowledge

Please consider adding to the poster the STAR detector and short introduction to the detector’s subsystems you use (TPC and TOF)

Particle identification: explain what the momentum threshold is

Add example with the mass^2 as a function of particle’s momentum

Femtiscopy: k* and r are undefined, as well as r_out, r_side and r_long (BP parametrization should be described)

Explain definitions of directions: our, side and long

Correlation functions: lambda -> \Lambda (greek symbol)

Summary: it is unclear to me why you conclude that Lighter particles are emitted closer to the center and/or later, 

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 10.06.2022, o godz. 09:30:

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

Pawel Szymanski (pawszy91 AT gmail.com) has submitted a material for a review,  
please have a look:
https://drupal.star.bnl.gov/STAR/node/59924

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