Published November 1, 1978 | Version v1
Journal article

Black holes and gravitational waves. I. Circular orbits about a rotating hole

  • 1. W. K. Kellogg Radiation Laboratory, California Institute of Technology

Description

The gravitational waves emitted by test particles in circular orbits about rotating black holes are examined. The luminosity is determined as a function of the orbital radius and the Kerr angular momentum parameter. Several typical wave forms of the metric perturbation are illustrated as they might appear to a gravitational wave detector

Additional details

Publishing Information

Journal Title
Astrophys. J.
Journal Volume
225
Journal Issue
3
Series
Astrophys. J.
Journal Page Range
687-693

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
10446997
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
BLACK HOLES; DISTURBANCES; GENERAL RELATIVITY THEORY; GRAVITATION; GRAVITATIONAL FIELDS; GRAVITATIONAL WAVES; KERR FIELD; KERR METRIC; ROTATION; WAVE FORMS
Descriptors DEC
FIELD THEORIES; METRICS