Generation of gravitational waves by the anisotropic phases in the early universe

Details Generation of gravitational waves by the anisotropic phases in the early universe Generation of gravitational waves by the anisotropic phases in the early universe

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.229..357d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 229, Dec. 1, 1987, p. 357-370.

Statistics

Computation

17

Anisotropic Media, Evolution (Development), Gravitational Waves, Universe, Computational Astrophysics, Energy Distribution, Stress Tensors, Temperature Gradients

Scientific paper

The authors discuss possible anisotropic and inhomogeneous phases in the early universe at relatively late epochs corresponding to the temperatures 300 MeV - 1 TeV. The anisotropy and inhomogeneity of the stress-energy tensor at the horizon scale gives rise to the generation of a stochastic gravitational wave background. Both the amplitude and spectral energy density of this background are estimated. The authors also discuss the possibility of the detection of this background by the planned gravitational wave detectors.

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