John W. Moffat, D. Vincent
Abstract
A solution of the field equations of the nonsymmetric theory of gravitation for the early universe starts with a far-from-equilibrium state and generates perturbations whose evolution is consistent with galaxy formation.
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A solution of the field equations of the nonsymmetric theory of gravitation for the early universe starts with a far-from-equilibrium state and generates perturbations whose evolution is consistent with galaxy formation.
Key concepts: Physics, Gravitation, Cosmology, Universe, Theoretical physics, Classical mechanics, Galaxy, Parameterized post-Newtonian formalism