STAR Correlations and Fluctuations PWG

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

Dear Paweł,

Many thanks for implementing the comments. 

What will be the size of your poster? If It will be A0, then you should be able to decrease some windows little bit and add new elements.

Regarding interpretation of the asymmetry, you can mention that asymmetry is determined with the help of model predictions. I would consider adding little plot showing model predictions in terms of shifter emission positions of the particle.

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 Paweł Szymański via Star-cf-l <star-cf-l AT lists.bnl.gov> w dniu 18.06.2022, o godz. 14:42:

Dear Hanna,

Thank you for your comments.
The new version of the poster is under the following link:

https://drupal.star.bnl.gov/STAR/system/files/HYP2022_Poster_PSzymanski_v2.pdf 

Best regards,

Pawel

sob., 18 cze 2022 o 04:52 Hanna Paulina Zbroszczyk via Star-cf-l <star-cf-l AT lists.bnl.gov> napisał(a):

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)

I don't have enough space to add this.

 

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, 

I added information that negative values of mu indicate this.

 

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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