The multi-messenger picture of compact binary mergers
by
S. Rosswog(OKC)
→
Europe/Stockholm
FA 32
FA 32
Description
Mergers of compact stellar objects are fascinating multi-physics
problems. To date, several double neutron star systems are known
and binary systems with a neutron star and a stellar mass black hole
are believed to exist. Such binary systems are excellent laboratories for
strong gravity and they are the most promising sources for a direct
detection of gravitational waves in the kHz range. Their final merger
most likely powers (about one third) the observed gamma-ray bursts,
the most luminous explosions in the universe since the Big Bang.
Moreover, recent research indicates that compact binary mergers may
be a major source for those heavy elements that form via the rapid neutron
capture process. I will give an overview over the various facets of what
happens in the last moments in the life of a compact binary system.
