STAR Correlations and Fluctuations PWG

[misshiki <misshiki AT rcf.rhic.bnl.gov>]

Dear Hanna,


Thank you for your comments.
I modified my presentation.
https://drupal.star.bnl.gov/STAR/system/files/JPS2021_Spring_MoeIsshiki__v3.pdf

Best  regards,
Moe



On 2021-03-10 17:37, Hanna Paulina Zbroszczyk via Star-cf-l wrote:
> Dear Moe,
>
> Please find below my comments to your nice presentation:
>
> Slide 3: remove one question mark from the title
>
> The HBT method from astronomy was an inspiration to use a different
> method for two-particle correlations.
> It would be good to underline these methods are different (different
> scales, different measured quantities, different determined
> quantities).
>
> I don’t understand the plot here: do you refer to astronomy or
> (heavy) ion collisions?
> It would be better to concentrate on case you study: you have a source
> that emits particles.
> Detector registers particles momenta (having just two: p1 and p2 would
> be enough).
> Regarding the plot: R is a radius, you plotted as diameter.
>
> Instead you third bullet you can add that femtoscopic correlations
> arise due to quantum statistics effects and Final State Interactions
> (if present).
>
> Slide 4: Many hyperon -> may hyperon
>
> Slide 5: dE/dx ,Reconstruct -> dE/dx, reconstruct
>
> Slide 6: 2014(1 billion..) -> 2014 (1 billion..) (add space)
> Mass(from.. -> Mass (from.. (add space)
>
> Slide 7: Theory equation: q -> q_{inv} (as you mention C_2(q_{inv}))
> It would be good to add that usually this equation is used to
> parametrize correlation function including quantum statistics (only)
>
> Slide 8: in previous slide you use q, here you use Q, please make them
> consistent
>
> Slide 10: define \Delta \Eta
>
> Slide 14: Separate title: \Delta\phi vs \delta\Eta (add two spaces:
> before and after vs)
>
> Best regards,
> Hanna
>
> Hanna Paulina Zbroszczyk
> PhD DSc Eng, Professor WUT
>
> E-mail: hanna.zbroszczyk AT pw.edu.pl
> Tel: +48 22 234 5851 (office)
>
> Address:
> Warsaw University of Technology
> Faculty of Physics
> Nuclear Physics Division
> Koszykowa 75
> Office: 117b (via 115)
> 00-662 Warsaw, Poland
>
> > Wiadomość napisana przez Xiaofeng Luo via Star-cf-l
> > <star-cf-l AT lists.bnl.gov> w dniu 09.03.2021, o godz. 17:27:
> >
> > Hi Moe,
> >
> > Very nice presentation.
> > Please add "for the STAR Collaboration" in the first page.
> > I sign off.
> >
> > Thank you,
> > Best Regards,
> > Xiaofeng
> >
> > On 2021/3/8 1:44 AM, webmaster--- via Star-cf-l wrote:
> >
> > > Dear star-cf-l AT lists.bnl.gov members,
> > >
> > > Moe Isshiki (k0nchar0127 AT gmail.com) has submitted a material for a
> > > review,
> > > please have a look:
> > > https://drupal.star.bnl.gov/STAR/node/54113
> > >
> > > ---
> > > If you have any problems with the review process, please contact
> > > webmaster AT www.star.bnl.gov
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