Solutions to the field equations of the Nonsymmetric Gravitational Theory with $g_[i0] = 0$ are obtained for the homogeneous, plane-symmetric, time-dependent case, both in vacuum and in the presence of a perfect fluid. Cosmological consequences include a dependence of the speed of light on its polarisation, as in a birefringent crystal
26 pages and 5 figures. Published version26 pages and 5 figures. Published version26 pages and 5 fig...
We have found exact constant solutions for the cosmological density parameter using a generalization...
A particular model providing a dynamical cancellation of a cosmological constant entering in Einstei...
We examine gravitational waves in an isolated axi--symmetric reflexion symmetric NGT system. The str...
12 pages12 pages12 pagesWe consider spatially homogeneous and isotropic Friedmann-Robertson-Walker (...
Classically, the physics of the universe is described by Newton\u27s Laws of Motion and Newton\u27s ...
We consider the linearized nonsymmetric theory of gravitation (NGT) within the background of an expa...
General Relativity and its higher derivative extensions have symmetric teleparallel reformulations i...
We generalize the results of Randall and Sundrum to a wider class of four-dimensional space-times in...
We derive the effects of a nonzero cosmological constant Λ on gravitational wave propagation in the ...
Proceeding from a homogeneous and isotropic Friedmann universe a conceptional problem concerning lig...
In this article on the basis of a new definition of spacetime symmetry, which is in accordance with ...
Plane symmetric inhomogeneous cosmological models for perfect fluid distribution are investigated in...
In cosmological group field theory (GFT) models for quantum gravity coupled to a massless scalar fie...
A plane-symmetric non-static cosmological model representing a bulk viscous fluid distribution has b...
26 pages and 5 figures. Published version26 pages and 5 figures. Published version26 pages and 5 fig...
We have found exact constant solutions for the cosmological density parameter using a generalization...
A particular model providing a dynamical cancellation of a cosmological constant entering in Einstei...
We examine gravitational waves in an isolated axi--symmetric reflexion symmetric NGT system. The str...
12 pages12 pages12 pagesWe consider spatially homogeneous and isotropic Friedmann-Robertson-Walker (...
Classically, the physics of the universe is described by Newton\u27s Laws of Motion and Newton\u27s ...
We consider the linearized nonsymmetric theory of gravitation (NGT) within the background of an expa...
General Relativity and its higher derivative extensions have symmetric teleparallel reformulations i...
We generalize the results of Randall and Sundrum to a wider class of four-dimensional space-times in...
We derive the effects of a nonzero cosmological constant Λ on gravitational wave propagation in the ...
Proceeding from a homogeneous and isotropic Friedmann universe a conceptional problem concerning lig...
In this article on the basis of a new definition of spacetime symmetry, which is in accordance with ...
Plane symmetric inhomogeneous cosmological models for perfect fluid distribution are investigated in...
In cosmological group field theory (GFT) models for quantum gravity coupled to a massless scalar fie...
A plane-symmetric non-static cosmological model representing a bulk viscous fluid distribution has b...
26 pages and 5 figures. Published version26 pages and 5 figures. Published version26 pages and 5 fig...
We have found exact constant solutions for the cosmological density parameter using a generalization...
A particular model providing a dynamical cancellation of a cosmological constant entering in Einstei...