STAR Correlations and Fluctuations PWG

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

Dear Hanna,

Thanks for your comments. I have uploaded the second version of the 
abstract which could be found at the same link ( 
https://drupal.star.bnl.gov/STAR/presentations/JPS-2022-Autumn/Femtoscopic-studies-identical-pions-AuAu-collisions-sqrtsNN-27-GeV-STA 
)

> It would be nice to explain why among of many STAR energies you chose
> \sqrt{s_{NN}} = 27 GeV.
The tilt angle is expected to decrease with increasing COM energy so the 
plan is to work at different COM energies. I chose 27 GeV as starting 
energies and will work in other lower energies too.

> Please consider some general one or two sentences about femtoscopy, to
> explain what can be studies with this technique.
> Explain please what is the tilt angle.
Done in second version of the abstract. I will explain more in the 
slides during presentation.

> Explain also why you consider different pseudorapidity, transverse
> pair momentum and pair azimuthal angle.
The idea is to construct the correlation functions for different bins of 
pair azimuthal angle relative to \Psi_1 for different centralities, 
pseudorapidity, transverse
pair momentum and extract various parameter (radii) by fitting it with 
cross term. And using these parameters, to calculate the tilt angle as a 
function of different centralities, pseudorapidity, transverse pair 
momentum etc. For time being I have removed pseudorapidity, transverse 
pair momentum dependence and will only show centralities dependence.

Best regards,
Ashutosh

On 2022-07-13 00:15, Hanna Paulina Zbroszczyk via Star-cf-l wrote:
> Dear Ashutosh,
>
> Please find my comments below.
>
> It would be nice to explain why among of many STAR energies you chose
> \sqrt{s_{NN}} = 27 GeV.
> Please consider some general one or two sentences about femtoscopy, to
> explain what can be studies with this technique.
> Explain also why you consider different pseudorapidity, transverse
> pair momentum and pair azimuthal angle.
> Explain please what is the tilt angle.
>
> Thanks,
> 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 webmaster--- via Star-cf-l
> > <star-cf-l AT lists.bnl.gov> w dniu 12.07.2022, o godz. 08:14:
> >
> > Dear star-cf-l AT lists.bnl.gov members,
> >
> > Ashutosh Pandey (ashutosh.iitb007 AT gmail.com) has submitted a
> > material for a
> > review, please have a look:
> > https://drupal.star.bnl.gov/STAR/node/60249
> >
> > ---
> > If you have any problems with the review process, please contact
> > webmaster AT www.star.bnl.gov
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