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Linearisation Instabilities of the Massive Nonsymmetric Gravitational Theory

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arxiv gr-qc/9603062 v2 pith:BVSXQT2X submitted 1996-03-29 gr-qc

classification gr-qc
keywords datagravitationallinearisationmassivenonsymmetrictheoryantisymmetricapproximation
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The massive nonsymmetric gravitational theory is shown to posses a linearisation instability at purely GR field configurations, disallowing the use of the linear approximation in these situations. It is also shown that arbitrarily small antisymmetric sector Cauchy data leads to singular evolution unless an ad hoc condition is imposed on the initial data hypersurface.

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    Massive one-form fields, with a reconstructed self-interacting potential, can support traversable wormholes while ordinary matter in a specially tuned case satisfies all classical energy conditions.

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