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About: Extreme mass ratio inspiral     Goto   Sponge   NotDistinct   Permalink

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Type: yago:WikicatBinarySystemsyago:Abstraction100002137yago:BinaryNumerationSystem106810020yago:Communication100033020yago:Event100029378yago:Happening107283608yago:MathematicalNotation106808720yago:Movement107309781yago:Notation106808493yago:NumerationSystem106809074yago:PositionalNotation106809421yago:PsychologicalFeature100023100yago:WikicatGravitationalWavesyago:Writing106359877yago:WrittenCommunication106349220yago:YagoPermanentlyLocatedEntityyago:Wave107352190ArtificialSatellite New Facet based on Instances of this Class

In astrophysics, an extreme mass ratio inspiral (EMRI) is the orbit of a relatively light object around a much heavier (by a factor 10,000 or more) object, that gradually spirals in due to the emission of gravitational waves. Such systems are likely to be found in the centers of galaxies, where stellar mass compact objects, such as stellar black holes and neutron stars, may be found orbiting a supermassive black hole. In the case of a black hole in orbit around another black hole this is an extreme mass ratio binary black hole. The term EMRI is sometimes used as a shorthand to denote the emitted gravitational waveform as well as the orbit itself.