paper

Torsion and Chern-Simons gravity in 4D space-times from a Geometrodynamical four-form

arXiv:2404.17798

Abstract

The space-time geometry in any inertial frame is described by the line-element . Now, not only the Minkowski metric is invariant under proper Lorentz transformations, the totally antisymmetric Levi-Civita tensor too is. In general relativity (GR), of the flat space-time gets generalized to a dynamical, space-time dependent metric tensor that characterizes a curved space-time geometry. In the present study, it is put forward that the flat space-time Levi-Civita tensor gets elevated to a dynamical four-form field in curved space-time manifolds, i.e. , so that . It is shown that this geometrodynamical four-form field extends GR by leading naturally to a torsion in the theory as well as to a Chern-Simons gravity. It is demonstrated that the scalar-density associated with may be used to construct a generalized exterior derivative that converts a p-form density to a (p+1)-form density of identical weight. It is argued that the scalar-density associated with corresponds to an axion-like pseudo-scalar field in the Minkowski space-time, and that it can also masquerade as dark matter. Thereafter, we provide a simple semi-classical analysis in which a self-gravitating Bose-Einstein condensate of such ultra-light pseudo-scalars leads to the formation of a supermassive black hole. A brief analysis of propagation of weak gravitational waves in the presence of is also considered in this article.

Appeared in the Proceedings of the Third Minkowski Meeting that was held at Albena (Bulgaria) in September, 2023