Post-ISCO Ringdown Amplitudes in Extreme Mass Ratio Inspiral
نویسندگان
چکیده
منابع مشابه
Astrophysics of extreme mass ratio inspiral sources
Compact remnants on orbits with peri-apses close to the Schwarzschild radius of a massive black hole (MBH) lose orbital energy by emitting gravitational waves (GWs) and spiral in. Scattering with other stars allows successful inspiral of such extreme mass ratio inspiral sources (EMRIs) only within small distances, a < few× 0.01pc from the MBH. The event rate of EMRIs is therefore dominated by t...
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ژورنال
عنوان ژورنال: Nuclear Physics B - Proceedings Supplements
سال: 2011
ISSN: 0920-5632
DOI: 10.1016/j.nuclphysbps.2011.04.164