A class of Bianchi type VI cosmological models with electromagnetic field

Details A class of Bianchi type VI cosmological models with electromagnetic field A class of Bianchi type VI cosmological models with electromagnetic field

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...204..322d&link_type=abstract

Astrophysical Journal, vol. 204, Mar. 1, 1976, pt. 1, p. 322-329.

Physics

24

Astronomical Models, Cosmology, Electromagnetic Fields, Field Theory (Physics), Relativity, Einstein Equations, Hubble Diagram, Ideal Fluids, Kinematics, Mathematical Models, Maxwell Equation

Scientific paper

The 'parallel-propagation' solution of the Einstein-Maxwell equations found by Tariq and Tupper (1974) is generalized to represent the solution of the field equations for a perfect-fluid distribution both with and without an electromagnetic field. All the solutions admit a three-parameter group of isometries of Bianchi type VI and form a subclass of the Bianchi type VI models found by Ellis and MacCallum (1969). The perfect-fluid models in this subclass automatically satisfy the Hawking-Penrose strong energy condition, while those models which represent perfect fluid with electromagnetism have a current four-vector which is either spacelike or zero. Properties of these models are discussed and are compared with those of another subclass found by Ellis and MacCallum.

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