Published 1972
| Version v1
Journal article
Limits on gravitational radiation from two gravitationally bound black holes
Description
Upper bounds are computed for the energy emitted in gravitational radiation by two black holes falling into one another from rest at a range of separations. It is shown that before the ratio of total mass to proper separation exceeds 0·759 an event horizon must have formed around both.
Additional details
Identifiers
Publishing Information
- Journal Title
- Monthly Notices of the Royal Astronomical Society
- Journal Volume
- 159
- Journal Issue
- 1
- Series
- Mon. Notic. Roy. Astron. Soc.
- Journal Page Range
- 41P-45P
- ISSN
- 0035-8711
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 4047035
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- No Abstract
- Descriptors DEI
- BLACK HOLES; DISTANCE; EMISSION; ENERGY; EUCLIDEAN SPACE; GRAVITATIONAL RADIATION; MASS; MATHEMATICAL MODELS; TOPOLOGY
- Descriptors DEC
- MATHEMATICAL SPACE; MATHEMATICS; RADIATIONS; RIEMANN SPACE; SPACE
Optional Information
- Notes
- Brief communication.; Updated automatically by Metadata and Full-Text Enrichment Agent