Modified Gravity (MOG), Cosmology and Black Holes

TL;DR

This paper introduces a covariant modified gravity theory (MOG) with additional scalar and vector fields, explores its cosmological solutions, and analyzes black hole properties, including the behavior of scalar fields and radiation.

Contribution

It formulates a new covariant MOG theory with scalar and vector fields, deriving cosmological solutions and analyzing black hole characteristics within this framework.

Findings

Cosmological solutions are derived for a homogeneous and isotropic universe.

Black holes in MOG are stationary, axisymmetric, and have spherical topology.

The scalar field is constant around isolated black holes, preventing monopole radiation.

Abstract

A covariant modified gravity (MOG) is formulated by adding to general relativity two new degrees of freedom, a scalar field gravitational coupling strength $G= 1/\chi$ and a gravitational spin 1 vector field $\phi_\mu$. The $G$ is written as $G=G_N(1+\alpha)$ where $G_N$ is Newton's constant, and the gravitational source charge for the vector field is $Q_g=\sqrt{\alpha G_N}M$, where $M$ is the mass of a body. Cosmological solutions of the theory are derived in a homogeneous and isotropic cosmology. Black holes in MOG are stationary as the end product of gravitational collapse and are axisymmetric solutions with spherical topology. It is shown that the scalar field $\chi$ is constant everywhere for an isolated black hole with asymptotic flat boundary condition. A consequence of this is that the scalar field loses its monopole moment radiation.