On the formation of black holes in non-symmetric gravity

Details On the formation of black holes in non-symmetric gravity On the formation of black holes in non-symmetric gravity

1995-06-19

arxiv.org/abs/gr-qc/9506033v1

Phys.Rev.Lett.75:2455-2459,1995

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

9 pages, ordinary LaTex.

Scientific paper

10.1103/PhysRevLett.75.2455

It has been recently suggested that the Non-symmetric Gravitational Theory (NGT) is free of black holes. Here, we study the linear version of NGT. We find that even with spherical symmetry the skew part of the metric is generally non-static. In addition, if the skew field is initially regular, it will remain regular everywhere and, in particular, at the horizon. Therefore, in the fully-nonlinear theory, if the initial skew-field is sufficiently small, the formation of a black hole is to be anticipated.

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