STAR Correlations and Fluctuations PWG

[Anna Kraeva <annakraeva555 AT gmail.com>]

Dear Hanna and Toshihiro,

Thank you for your comments! I have uploaded a new version of the presentation. Please have a look:  https://drupal.star.bnl.gov/STAR/node/64541

Best regards,
Anna

ср, 16 авг. 2023 г. в 04:15, 野中俊宏 <nonaka.toshihiro.ge AT u.tsukuba.ac.jp>:

Dear Anna,

I sign off your nice slides with one minor comment below:

Title page: Add space before/after the "="

Best regards,

Toshihiro

---

差出人: Star-cf-l <star-cf-l-bounces AT lists.bnl.gov> が Hanna Paulina Zbroszczyk via Star-cf-l <star-cf-l AT lists.bnl.gov> の代理で送信
送信日時: 2023年8月16日 0:03
宛先: Anna Kraeva <annakraeva555 AT gmail.com>
CC: Hanna Paulina Zbroszczyk <hanna.zbroszczyk AT pw.edu.pl>; star-cf-l AT lists.bnl.gov <star-cf-l AT lists.bnl.gov>
件名: Re: [Star-cf-l] STAR presentation by Anna Kraeva for ISMD 2023 submitted for review

 

Dear Anna,

Thank you for implementing my comments.

I have the only one: slide 5, you actually define q_inv there, instead of q (the formula).

With this implemented, 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 Anna Kraeva <annakraeva555 AT gmail.com> w dniu 14.08.2023, o godz. 12:39:

Dear Hanna, 

Thank you for your comments! 

I took into account all your comments and updated the presentation. Please have a look: https://drupal.star.bnl.gov/STAR/presentations/ISMD-2023/Two-pion-Bose-Einstein-correlations-AuAu-collisions-3-GeV-STAR-experiment-0

Best regards,
Anna

сб, 12 авг. 2023 г. в 13:56, Hanna Paulina Zbroszczyk via Star-cf-l <star-cf-l AT lists.bnl.gov>:

Dear Anna,

Please find my comments on your nice ISMD presentation:

Slide 2: 

Femtoscopy helps to determine EoS not only in the case of QGP but might help look for signatures of the phase transition as well, so regarding the first bullet, please specify whether you mean the QGP properties (higher energies) or determination of the EoS (not only QGP should be mentioned then). 

A similar comment comes regarding the second bullet. The structure of the source is studied for higher energies as well. 

Instead of these two bullets stating higher and lower energies, you could mention: 1. EoS; 2. Geometry/shape/structure of the source.

Slide 5: 

It is contains quantum-statistical correlations (QS) and final state interactions -> It contains correlations due to quantum-statistics (QS) and final state interactions (FSI, Coulomb dominated).

Are from -> come/originate from (twice)

Physics correlations -> femtoscopic correlations

Please visualize/discuss out-long (ol) component.

These 2 figures are really small. Try to enlarge them.

q_inv is not defined (define or use q instead)

It would help if you briefly discuss the reference frame (LCMS).

You may split this slide into two separate ones. It helps to clarify the content of your presentation.

Slide 9:

More discussion about the out-long component will be appreciated.

More when other preliminary labels will be 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 09.08.2023, o godz. 18:55:

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

Anna Kraeva (annakraeva555 AT gmail.com) has submitted a material for a review,  
please have a look:
https://drupal.star.bnl.gov/STAR/node/64541

Deadline: 2023-08-21
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