STAR Correlations and Fluctuations PWG

[Mate Csanad <csanad AT bnl.gov>]

Hi Nu,

Thanks for the quick response. Let me send some replies:

1) Yes, there were several talks, I also showed the status at the last collab meeting (from slide 11)

https://drupal.star.bnl.gov/STAR/system/files/csanad_collabmeeting2024_levyhbt_0.pdf 

but here is a PWG talk as well:

https://drupal.star.bnl.gov/STAR/system/files/sbhosale_STAR_pdg_16112023.pdf_0.pdf 

2) Yes, and thanks for the suggestion. 

3) The main advantage is that it provides a better description (well beyond the limit of statistical significance), and thus allows for a better characterozation of the source shape and size. 

Best regards, 

Mate

Nu Xu <nxu AT lbl.gov> ezt írta (időpont: 2024. szept. 5., Csü 18:30):

Dear Sneha and All,

Thank you for preparing this abstract.
Here are my comments/suggestions:

1) I may have missed this, but I do not remember when we had the discussion about this new analysis before. If this has been discussed in the PWG, please send me the link. Otherwise, I think we should have the discussion first before going to outside the collaboration;

2) About the abstract: Is this about 3D analysis of pion HBT? If so, I suggest mention it in the abstract.

3) For pion HBT, 3D analysis has been done previously. What is the advantage for the approach with Levy function?

Regards,
Nu

> On Sep 5, 2024, at 8:55 AM, Bhosale Sneha <bhosales AT staff.elte.hu> wrote:
>
> P {margin-top:0;margin-bottom:0;} Dear Hanna, Nu, and All,
>  I have prepared the abstract for the WPCF. In the upcoming days, I will be presenting the latest 3D results in PWD meeting. Meanwhile please have a look at the abstract and let me know your feedback.
> https://drupal.star.bnl.gov/STAR/node/68840
> There is something strange with the system, the author, format and meeting do not look correct, not sure what happened, but I hope it still can be seen.
> Thank you all, best regards,
> Sneha