STAR Correlations and Fluctuations PWG

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

Hi Ashutosh,

    Nice abstract. I sign off.
    Please present the analysis update in coming PWG meeting asap.

Thank you,
Best Regards,
Xiaofeng

On 2022/7/16 14:48, apandey via Star-cf-l wrote:
> Dear Hanna and Xiaofeng,
>
> I am sorry for the rush but I request you to review my abstract since 
> last date is 19 July, 2022 (2:00 PM JST time). I will present my 
> progress in coming PWG meetings.
>
> Best regards,
> Ashutosh
>
> On 2022-07-14 13:05, apandey via Star-cf-l wrote:
> > 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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--
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