STAR Correlations and Fluctuations PWG

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

Hanna Zbroszczyk ( hanna.zbroszczyk AT pw.edu.pl ) has commented on a material  
originally submitted by Yu Zeng (  zengy AT mails.ccnu.edu.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2023/Proton-correlation-function-AuAu-collisions-sqrtsNN-32-GeV

Comment:
Dear Yu, please find my comments below:
Title, I propose to modify: Proton correlation function in Au+Au collisions  
at √sNN = 3.2 GeV -> Proton-proton  femstoscopy in Au+Au collisions at  
√sNN = 3.2 GeV
Line 1: Baryons -> baryons
Line 2: put the space: structure,the dynamical -> structure, the dynamical
Linę 5: BESII-> BES-II
Linę 8: as the title describes only one collision energy: \sqrt{s_NN} = 3.2  
GeV, what do you mean by the energy dependence? And moreover. do you expect  
to study the energy dependence of the parameters of interactions? What you  
can study is rather source size..

Thanks,
Hanna

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