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Gravitational radiation from extreme kerr black hole
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Nakamura, Takashi Sasaki, Misao |
| Copyright Year | 1989 |
| Description | Gravitational radiation induced by a test particle falling into an extreme Kerr black hole was investigated analytically. Assuming the radiation is dominated by the infinite sequence of quasi-normal modes which has the limiting frequency m/(2M), where m is an azimuthal eigenvalue and M is the mass of the black hole, it was found that the radiated energy diverges logarithmically in time. Then the back reaction to the black hole was evaluated by appealing to the energy and angular momentum conservation laws. It was found that the radiation has a tendency to increase the ratio of the angular momentum to mass of the black hole, which is completely different from non-extreme case, while the contribution of the test particle is to decrease it. |
| File Size | 731424 |
| Page Count | 20 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19890017423 |
| Archival Resource Key | ark:/13960/t9c58hc6g |
| Language | English |
| Publisher Date | 1989-05-17 |
| Access Restriction | Open |
| Subject Keyword | Astrophysics Conservation Laws Neutron Stars Emission Spectra Gravitational Waves Angular Momentum Eigenvalues Mass Distribution Black Holes Astronomy Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Technical Report |
