Inhomogeneous cosmology - Gravitational radiation in Bianchi backgrounds

Details Inhomogeneous cosmology - Gravitational radiation in Bianchi backgrounds Inhomogeneous cosmology - Gravitational radiation in Bianchi backgrounds

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...253....1a&link_type=abstract

Astrophysical Journal, Part 1, vol. 253, Feb. 1, 1982, p. 1-18.

Mathematics

51

Astronomical Models, Background Radiation, Cosmology, Gravitational Waves, Polarization (Waves), Inhomogeneity, Plane Waves, Singularity (Mathematics), Space-Time Functions, Wave Equations

Scientific paper

An exact formalism is developed for describing cosmological models with strong, long wavelength gravitational waves of general polarization, propagating over backgrounds corresponding to Bianchi types I through VII. A new metric which exhibits the appropriate symmetries of two equivalent independent polarizations of gravitational waves is introduced and discussed. The formalism is applied to an empty type I cosmology, and it is shown how the original z-dependent chaotic singularity structure transforms itself into gravitational radiation propagating along the z-axis in a Bianchi I background.

Affiliated with

Also associated with

No associations

Rating

Inhomogeneous cosmology - Gravitational radiation in Bianchi backgrounds does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Inhomogeneous cosmology - Gravitational radiation in Bianchi backgrounds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Inhomogeneous cosmology - Gravitational radiation in Bianchi backgrounds will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1646665