STAR Correlations and Fluctuations PWG

[Mate Csanad <csanad AT bnl.gov>]

Hi Nu,

Thank you for the response and comments!

Please find the updated version at
https://drupal.star.bnl.gov/STAR/system/files/STAR_LevyHBT_abstract_0.pdf
but let me respond here as well:

1) The energies are 3.2, 3.9, 7.7, 14.5, 19.6, 27, 54.5, and 200 GeV, now 
mentioned in the abstract (too long for the title, hence I removed the energy 
range from there, and it is only given in the text).

2) Indeed this was missing, now it is mentioned.

3) Such a detailed description is not really possible in the abstract, and I 
guess this should anyway happen in various meetings in the subsequent 
weeks/months; thus I modified the text,
from ->
"also sheds light on the physical explanation behind the appearance of these 
source shapes"
to ->
"is also discussd"

Best regards,
Mate

2024. 10. 17. 17:42 keltezéssel, Nu Xu írta:
> Hi Mate and All,
>
> Thank you for the QM25 abstract!
>
> I have the following requests:
> 1) Let us specify collision energies. 3-200 GeV is too vague to me;
> 2) No centrality nor mt dependence is mentioned, why? I suggest to mention 
> these dependences in the abstract.
> 3) I would like to see a clear description of data analysis before jumping to 
> some physics conclusions such as ‘te appearance of these source shapes’.
>
> Please update the abstract and send to the PWG asap.
>
> Many thanks,
>
> Nu