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SUMMARY:Primordial Black Holes and Gravitational Wave Observations
DTSTART:20211115T140000
DTEND:20211115T153000
DTSTAMP:20260427T212751Z
UID:86c4a369d1a46cb034abe13ef6efa7ce51174bf4db05a1cd716137ad
CATEGORIES:Conferences - Seminars
DESCRIPTION:Gabriele Franciolini\nPrimordial Black Holes might comprise a 
 significant fraction of dark matter in the Universe and can give rise to o
 bservable signatures at current and future gravitational wave experiments.
  First\, we review the PBH model and discuss how accretion and clustering 
 may affect the properties of PBH binaries. Second\, we confront the PBH mo
 del with LIGO/Virgo data showing its upsides and shortcomings\, by also in
 cluding state-of-the-art astrophysical models in a multi-population infere
 nce. Finally\, we discuss how 3G detectors\, such as Einstein Telescope an
 d Cosmic Explorer\, may be able to discover a PBH population by searching 
 for high redshift merger events.
LOCATION:https://epfl.zoom.us/j/61161964077?pwd=cTVNd3luOVhXWi9KbFhMNWordj
 NvQT09
STATUS:CONFIRMED
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