Charged homogeneous cosmologies

Details Charged homogeneous cosmologies Charged homogeneous cosmologies

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...227...13f&link_type=abstract

Astrophysical Journal, Part 1, vol. 227, Jan. 1, 1979, p. 13, 14. NSF-supported research.

Physics

4

Charge Distribution, Cosmology, Electromagnetism, Maxwell Equation, Field Theory (Physics), Relativity

Scientific paper

The source-free Maxwell equations derived by Hughston and Jacobs (1970) for spatially homogeneous cosmologies are extended to include a source term corresponding to a cosmological charge density. It is shown that Maxwell's equations alone are sufficient to require the vanishing of the cosmological charge density in class A spacetimes. It is also found that charged solutions (where permitted) cannot be purely magnetic and that the only charged solutions in which the Poynting vector vanishes require the vanishing of the magnetic field.

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