STAR Correlations and Fluctuations PWG

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

Dear Diana,

I have just one comment regarding your figure 1. 

What is the reference of this plot?  I would expect that pion’s source should be bigger and the kaon source (due to bigger mass) should be smaller, but I would expect that the collective behavior would cause that particles would be emitted in the same direction (this is what we usually consider in nonidentical particles, taking into account both components of the particles’ velocity: \beta_f and \beta_t). Usually this is how we use such plot for correlations. So, I understand that pion’s source should be bigger, and the kaon’s course should be drawn inside pion’s one (but smaller), then you could see a shift of their mean values of their emission points.

With those explained, I sign off.

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 18.08.2022, o godz. 09:59:

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

Diana Pawlowska (diapaw93 AT gmail.com) has submitted a material for a review,  
please have a look:
https://drupal.star.bnl.gov/STAR/node/60558

---
If you have any problems with the review process, please contact  
webmaster AT www.star.bnl.gov
_______________________________________________
Star-cf-l mailing list
Star-cf-l AT lists.bnl.gov
https://lists.bnl.gov/mailman/listinfo/star-cf-l