Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..523...75h&link_type=abstract
GRAVITATIONAL WAVES: Third Edoardo Amaldi Conference. AIP Conference Proceedings, Volume 523, pp. 75-81 (2000).
Astronomy and Astrophysics
Astrophysics
Wave Generation And Sources, Relativity And Gravitation, Black Holes
Scientific paper
Space-based gravitational-wave interferometers such as LISA will be sensitive to the inspiral of stellar mass compact objects into black holes with masses in the range of roughly 105 solar masses to (a few) 107 solar masses. During the last year of inspiral, the compact body spends several hundred thousand orbits spiraling from several Schwarzschild radii to the last stable orbit. The gravitational waves emitted from these orbits probe the strong-field region of the black hole spacetime and can make possible high precision tests and measurements of the black hole's properties. Measuring such waves will require a good theoretical understanding of the waves' properties, which in turn requires a good understanding of strong-field radiation reaction and of properties of the black hole's astrophysical environment which could complicate wave-form generation. In these proceedings, I review estimates of the rate at which such inspirals occur in the universe, and discuss what is being done and what must be done further in order to calculate the inspiral waveform. .
No associations
LandOfFree
Gravitational waves from inspiral into massive black holes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Gravitational waves from inspiral into massive black holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gravitational waves from inspiral into massive black holes will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1390662