STAR Correlations and Fluctuations PWG

[张宇 <zhang_yu AT mails.ccnu.edu.cn>]

Dear Xiaofeng,

Thank you very much for your comments.
I have implemented them accordingly.
https://drupal.star.bnl.gov/STAR/node/55686

Best regards,
Yu

On Jul 30, 2021, 9:40 AM -0700, Xiaofeng Luo via Star-cf-l <star-cf-l AT lists.bnl.gov>, wrote:

Hi Yu,

    Nice proceedings.
    I have few minor suggestions :

    1. Line 54 :  shows no non-monotonic energy dependence -> shows
monotonic energy dependence

    2. Line 55:   is not qualitatively described by HRG and UrQMD ->
can not be described by different variants (GCE, EV, CE) of HRG and
UrQMD model

    3. Line 59 : negative sign -> negative signs

    4. Line 62-63: Similar to C6/C2, It is better to quantify the
deviation for C5/C1 not just mention which is positive or negative . For
eg. what is the significance of deviation from zero. less than 2 sigma  
?   or consistent with zero ?

    5.  Line 76: s due to crossover phase transition -> due to smooth
crossover transition

    6. Summary: We may also mention : In 2023-2025, STAR plan to
collect 15-20 billion Au+Au 200 GeV high statistics data . This allows
us to perform
        precise measurement of higher-order cumulants, maybe even to
8th order.

    7： Line 25: net-baryon number -> net-baryon  ($B$); net-charge
number -> net-charge (Q) ; net-strangeness number -> net-strangeness ($S$)

    8 : Line 20:  suggests that the phase transition is a smooth
crossover -> suggests a smooth crossover transition.

    With those implemented, I sign off.

Thank you,
Best Regards,
Xiaofeng


On 2021/7/23 12:02, webmaster--- via Star-cf-l wrote:

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

Yu Zhang (zhang_yu AT mails.ccnu.edu.cn) has submitted a material for a review,
please have a look:
https://drupal.star.bnl.gov/STAR/node/55686

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If you have any problems with the review process, please contact
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