STAR Correlations and Fluctuations PWG

[Xiaofeng Luo <xfluo.star AT hotmail.com>]

Hi Ke,

    Nice presentation.
    Please find my comments/suggestions below :

    1. slide 3, you may add some reference for this slide.
    2. slide 7, please put the text TPC PID and TOF PID to the empty 
place in this page, not covering the figures.

    3. slide 11, please make sure the results shown here is consistent 
with Yingjie's final p-Xi results.

    4. slide 2,  please modify the 3rd part to :
                Two-particle femtoscopy :
                     1) Meson-Meson (ks-ks)
                     2) Baryon-Baryon (p-p, p-Xi)
                     3) Light Nuclei (p-d, d-d)

    5. slide 6, the resolution of right figure is not good, please use 
the one in Yu Zhang's talk with better resolution.

    6. In slide 13 and 14, the legend L-L model is confusion if people 
only see the Figure, please spell it out as : Lednicky Model

    7. In the bottom of slide 16, add "Stay tuned for the RHIC BES-II"

    8. Summary:  d-d has larger source size -> d-d has larger emission 
source size

    With those implemented, I sign off.

Thank you,
Best Regards,
Xiaofeng

On 2022/3/21 5:32 PM, webmaster--- via Star-cf-l wrote:
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> Ke Mi (mike1996 AT mails.ccnu.edu.cn) has submitted a material for a review,
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--
Xiaofeng Luo
Professor of Physics
College of Physical Science and Technology
Central China Normal University
Luoyu Road 152, Wuhan China
Office Phone #: +86-27-67867500