Abstract
Decoupled, separable equations describing perturbations of a Kerr black hole are derived. These equations can be used to study black-hole processes involving scalar, electromagnetic, neutrino or gravitational fields. A number of astrophysical applications are made: Misner's idea that gravitational synchrotron radiation might explain Weber's observations is shown to be untenable; rotating black holes are shown to be stable against small perturbations; energy amplification by "superradiant scattering" of waves off a rotating black hole is computed; the "spin down" (loss of angular momentum) of a rotating black hole caused by a stationary non-axisymmetric perturbation is calculated.
Item Type: | Thesis (Dissertation (Ph.D.)) |
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Subject Keywords: | Physics |
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Degree Grantor: | California Institute of Technology |
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Division: | Physics, Mathematics and Astronomy |
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Major Option: | Physics |
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Awards: | Einstein Prize (APS), 2021. Member of the US National Academy of Sciences, 2003. Fellow of the American Academy of Arts and Sciences, 1996. |
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Thesis Availability: | Public (worldwide access) |
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Research Advisor(s): | |
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Group: | TAPIR, Astronomy Department |
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Thesis Committee: | |
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Defense Date: | 19 July 1973 |
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Additional Information: | Einstein Prize citation: "For outstanding contributions to observational tests of general relativity with theories of gravitational waves, astrophysical black holes, and neutron stars." |
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Funders: | Funding Agency | Grant Number |
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Pretoria Portland Cement Company | UNSPECIFIED | United States Steel Foundation | UNSPECIFIED | NSF | GP-28027 | NSF | GP-27304 |
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Record Number: | CaltechETD:etd-08022006-094950 |
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Persistent URL: | https://resolver.caltech.edu/CaltechETD:etd-08022006-094950 |
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DOI: | 10.7907/N3AW-PV92 |
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Related URLs: | |
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ORCID: | |
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Default Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. |
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ID Code: | 2997 |
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Collection: | CaltechTHESIS |
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Deposited By: |
Imported from ETD-db
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Deposited On: | 02 Aug 2006 |
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Last Modified: | 09 Oct 2020 22:24 |
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