Bianchi type electromagnetic cosmology - Type I Hamiltonian

Details Bianchi type electromagnetic cosmology - Type I Hamiltonian Bianchi type electromagnetic cosmology - Type I Hamiltonian

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...254..425r&link_type=abstract

Astrophysical Journal, Part 1, vol. 254, Mar. 15, 1982, p. 425-436. Consejo Nacional de Ciencia y Tecnologia

Physics

5

Astronomical Models, Cosmology, Dynamic Models, Electromagnetic Fields, Hamiltonian Functions, Interstellar Magnetic Fields, Anisotropic Media, Field Theory (Physics), Maxwell Equation, Variational Principles

Scientific paper

The dynamical effects of spatially homogeneous magnetic fields on anisotropic Bianchi Type I cosmological models are studied. Some general features to be expected of cosmic magnetic fields which are too weak to influence cosmic dynamics are pointed out, and the potentials affecting the evolution of anisotropy for diagonal, symmetric, and general metrics are obtained by means of the Arnowitt, Deser, and Misner Hamiltonian formalism.

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