Verifying the no-hair property of massive compact objects with intermediate-mass-ratio inspirals in advanced gravitational-wave detectors
The detection of gravitational waves from the inspiral of a neutron star or stellar-mass black hole into an intermediate-mass black hole (IMBH) promises an entirely new look at strong-field gravitational physics. Gravitational waves from these intermediate-mass-ratio inspirals (IMRIs), systems with...
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Format: | Article |
Language: | English |
Published: |
American Physical Society,
2012-08-10T12:51:05Z.
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Subjects: | |
Online Access: | Get fulltext |