STAR Correlations and Fluctuations PWG

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

Hi Asish,

I agree with Xiaofeng that net-proton results need more investigation and should not be presented during this talk. Except this, I have found few minor parts to be improved:

nature of quark-hadron phase transition and freeze-out dynamics -> nature of quark-hadron phase transition, and freeze-out dynamics

The cumulants and their ratios are related to the correlation length of the system and the susceptibilities that are also calculable in various QCD-based models. -> The cumulants and their ratios related to the system's correlation length and the susceptibilities are also calculable in various QCD-based models. 

the STAR detector at RHIC in the year 2018.-> the STAR detector at RHIC in 2018.

Cumulants and ratios of cumulants of net-proton, net-kaon and net-charge distributions -> Cumulants and ratios of cumulants of net-kaon, and net-charge distributions.

Thank you,

With my best regards,

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 17.09.2020, o godz. 08:05:

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

Ashish Pandav (apandav10 AT gmail.com) has submitted a material for a review,  
please have a look:
https://drupal.star.bnl.gov/STAR/node/52110

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