Abstract
SynopsisA general formalism for the description of high-frequency gravitational radiation is presented, and a justification is provided for the often made assumption that the energy of an isotropic field of gravitational radiation in a cosmological model may be represented by a perfect fluid.
Publisher
Cambridge University Press (CUP)
Reference11 articles.
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4. Gravitational Radiation and Observational Cosmology
Cited by
3 articles.
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