A kinetic theory for the growth of perturbations in an isotropic cosmological model, and the ultrarelativistic limit

Details A kinetic theory for the growth of perturbations in an isotropic cosmological model, and the ultrarelativistic limit A kinetic theory for the growth of perturbations in an isotropic cosmological model, and the ultrarelativistic limit

Oct 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978azh....55..922z&link_type=abstract

(Astronomicheskii Zhurnal, vol. 55, Sept.-Oct. 1978, p. 922-936.) Soviet Astronomy, vol. 22, Sept.-Oct. 1978, p. 528-535. Trans

Astronomy and Astrophysics

Astronomy

5

Astronomical Models, Cosmology, Gravitational Waves, Kinetic Theory, Perturbation Theory, Relativistic Particles, Expansion, Isotropic Media, Light Speed, Relativity, Universe, Wavelengths

Scientific paper

An analysis is presented of gravitational perturbations in an isotropic expanding universe that consists of relativistic gravitating particles. All short-wavelength perturbations in the ultrarelativistic gas comprising the universe will be propagated at the speed of light. A condition is established such that long-wavelength scalar and vector perturbations can grow.

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