STAR Correlations and Fluctuations PWG

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

Nu Xu ( nxu AT lbl.gov ) has commented on a material originally submitted by  
Boyang Fu ( boyangfu AT mails.ccnu.edu.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/SQM-2024/Measurements-pXi-Correlation-Function-200-GeV-Isobar-and-AuAu-collisions-STAR

Comment:
Hi Boyang, Here are my comments and suggestions on this presentation:
(1) Everywhere replace 'isobar' by "isobar (Zr+Zr and Ru+Ru)";
(2) Outline: Replace 'L-L Model' by "Data Analysis and L-L Fits";
(3) page 5: add a reference for "helix swimming method";
(4) page 7: (i) Mis-ID correction should be "Background Correction"; (ii) If  
possible, please list the relative contributions to the correlation functions 
 
from the four corrections;
(5) page 13: What do we mean by 'The effect of strong interaction is more  
significant in peripheral collisions'? I would suggest remove this bullet;
(6) page 13: What is the output parameters of R_G, f0, d0 from the UrQMD+HAL  
simulations? I believe we have asked the question few weeks back;
(7) page 14 - last bullet: Replace it by "R_G increase as charged  
multiplicity from these collisions". The same for page 16 - 2nd bullet


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