STAR Correlations and Fluctuations PWG

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

Dear Chuan,

Please find below my comments to your nice slides:

General comment: if you don’t use plots from your own resources, please add references to all plots that are not yours (e.g, slide 5).

Slide 3: Since you mention all BES program, including COLL and FXT mode, I suggest to replace the plot with QCD phase diagram with one introducing all BES energies too. It is good to pay more attention to 3 GeV as you concentrate on it.

Slide 4: I suggest to underline that with at HBT method in astronomy we study angular sizes of stars while in heavy-ion we problem properties of the source.

Slide 5: please define all quantities from the formula of k*.

Make uniform Qinv or qinv

k* = qinv/2 (but only for particles with identical masses) - make it clear on your slide

Slide 10: is it labelled as preliminary?

I don’t see the plot there:

https://drupal.star.bnl.gov/STAR/blog/fuchuan/ppcfqpt2021

I also don’t remember we granted preliminary labels for this plot

Slide 12: The same comment as for slide 10, I don’t remember preliminary granted..

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 22.07.2022, o godz. 06:24:

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

Chuan Fu (fuchuan AT mails.ccnu.edu.cn) has submitted a material for a review,  
please have a look:
https://drupal.star.bnl.gov/STAR/node/60372

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