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SUMMARY:Astrophysical gravitational wave background: from theoretical mode
 lling to detection prospects - Giulia Cusin (Institut d'Astrophysique de P
 aris)
DTSTART:20250317T130000Z
DTEND:20250317T140000Z
UID:TALK226549@talks.cam.ac.uk
CONTACT:Louis Legrand
DESCRIPTION:When looking at a population of astrophysical gravitational wa
 ve sources we can either decide to focus on those sources that are particu
 larly bright\, and build a catalogue\, or characterise collectively the su
 perposition of all signals from all sources from the onset of stellar acti
 vity until today. This stochastic background of gravitational radiation is
  an interesting observable as it can allow us to extract astrophysical inf
 ormation that cannot be extracted from the study of individual events. In 
 this talk\, I will give an overview of different astrophysical populations
  expected to generate a stochastic background in the frequency band of cur
 rent and future gravitational wave detectors. I will then review the state
  of the art of background modeling and illustrate future detection prospec
 ts.\n
LOCATION:CMS\, Pav. B\, CTC Common Room (B1.19) [Potter Room]
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