Vacuum Non Singular Black Hole Solutions in Tetrad Theory of Gravitation

Details Vacuum Non Singular Black Hole Solutions in Tetrad Theory of Gravitation Vacuum Non Singular Black Hole Solutions in Tetrad Theory of Gravitation

2001-09-10

arxiv.org/abs/gr-qc/0109033v1

Gen.Rel.Grav. 34 (2002) 1047-1058

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

11 pages, LaTex, no figures, Submitted to GRG

Scientific paper

Starting from a spherically symmetric tetrad with three unknown functions of the radial coordinate, a general solution of M{\o}ller's field equations in case of spherical symmetry nonsingular black hole is derived. The previously obtained solutions are verified as special cases of the general solution. The general solution is characterized by an arbitrary function and two constants of integration. The general solution gives no more than the spherically symmetric nonsingular black hole solution. The energy content of the general solution depends on the asymptotic behavior of the arbitrary function, and is different from the standard one.

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