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- W2895718133 abstract "We give here a brief review of the works studying the signatures of accretion disks on the gravitational wave signals generated by extreme mass ratio binary systems of compact objects. An example of such a system is a stellar mass compact star (typically a neutron star or a black hole) orbiting a central super-massive black hole embedded in a massive accretion disk. We particularly focus on the effects produced by hydrodynamic drag of the disk on the orbiting companion and find that the drag effects produced by the disk matter are indeed capable of modifying the companion’s motion and, hence, the gravitational wave signal emitted from the system. The nature and significance of the effect depends crucially on the flow parameters of the disk, e.g. velocity, density profiles of the flow. Therefore, on one hand, one needs to incorporate these effects while theoretically modelling the gravitational wave signal emitted from such systems. On the other hand, by studying the emitted gravitational wave signals profile, one could infer about the nature of the accretion disk, which has been, till date, done only by observing the electro-magnetic signals coming from it. This multi-messenger astronomy was for the first time conceived and worked out during our research work." @default.
- W2895718133 created "2018-10-12" @default.
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- W2895718133 date "2018-01-01" @default.
- W2895718133 modified "2023-09-27" @default.
- W2895718133 title "Gravitational Wave Emission from Binary Mergers: Ideal Versus Real Picture" @default.
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- W2895718133 doi "https://doi.org/10.1007/978-3-319-94607-8_4" @default.
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