Static spherically symmetric solutions in a new algebraically extended theory of gravity

Details Static spherically symmetric solutions in a new algebraically extended theory of gravity Static spherically symmetric solutions in a new algebraically extended theory of gravity

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987cqgra...4.1593k&link_type=abstract

Classical and Quantum Gravity (ISSN 0264-9381), vol. 4, Nov. 1, 1987, p. 1593-1608. NSERC-supported research.

Physics

11

Field Theory (Physics), Gravitation Theory, Spheres, Symmetry, Astronomical Models, Relativistic Theory, Space-Time Functions, Torsion

Scientific paper

The method of algebraic extension has yielded a new theory of gravitation in which the torsion is uniquely computable in terms of the generalized metric tensor. The field equations for this theory are solved in the static, spherically symmetric case. Two distinct solutions emerge which asymptotically approach flat space and have a Newtonian 'mass' parameter. In one of the solutions, this parameter arises in a manner analogous to general relativity; in the other solution, the mass parameter has a completely different origin intimately related to the algebraically extended structure of the theory. The possible experimental relevance of extended theories is discussed.

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