STAR Correlations and Fluctuations PWG

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

Hi Chuan,

    Nice presentation.
    Please find my suggestions below :

    1. Please add PID plots and PID cuts in your presentation.

    2. In slide 5, why k* is written as q_inv ? I think if k* is 
usually used, to avoid confusion, we should directly use k* instead of 
using
        q_inv. because by convention, the k* and q_inv have different 
expression.

    3. Slide 8, should mention, those are "proton" phase space.

    4. Slide 11, you may add some references about this study.

    5. Slide 18, Based on crab and In the legend of plots, You already 
obtain some source size information at 3 GeV and 7.7 GeV.
                       You may want to mention those in your slides and 
what we can learn from the extracted source size information.


    With those implemented, I sign off.

Thank you,
Best Regards,
Xiaofeng

On 2022/7/22 6:24 PM, webmaster--- via Star-cf-l wrote:
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> Chuan Fu (fuchuan AT mails.ccnu.edu.cn) has submitted a material for a review,
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> https://drupal.star.bnl.gov/STAR/node/60372
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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