STAR Correlations and Fluctuations PWG

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

Hi Ashish,

    Nice presentation.
    I have few minor suggestions :

    1. In summary :  indicates CP exists at sqrt(s )> 3 GeV.
        Please change to "If CP region created in HIC, it should exist 
at sqrt(s )> 3 GeV".

    2. In summary :  ~10 times of current statistics -> ~10-20 times of 
current statistics

    3. Slide 17 : In slide and table,  720 MeV -> 750 MeV.

    4. Slide 13, Legend, FRG paper has been published in PRD. Please 
update with journal #.


    With those implemented, I sign off.

Best Regards,
Xiaofeng

On 2022/5/30 10:13 PM, apandav via Star-cf-l wrote:
> Dear conveners and all,
>
> I was invited to give a talk on High Order Cumulants from STAR BES in 
> the RHIC/AGS AUM 2022 meeting.
>
> I have prepared a few slides with published and preliminary results. 
> The link to the slides can be found below.
> https://drupal.star.bnl.gov/STAR/node/59773
>
> Please let me know your comments and suggestions.
>
> Best regards,
> Ashish
>
> On 2022-05-30 19:37, webmaster--- via Star-cf-l wrote:
> > Dear star-cf-l AT lists.bnl.gov members,
> >
> > Ashish Pandav (apandav10 AT gmail.com) has submitted a material for a 
> > review,
> > please have a look:
> > https://drupal.star.bnl.gov/STAR/node/59773
> >
> > ---
> > If you have any problems with the review process, please contact
> > webmaster AT www.star.bnl.gov
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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