Using Generalized General Relativity to Study the Emission of Gravity Waves and Generation of Elementary Particles by Black Hole and Astronomical Objects

Abstract

In this study the generalized gravitational field equation has been adopted to see how gravitational waves can be generated. First one assumes spherically symmetric body solution. At the beginning of the work a useful expression for the time metric has been also obtained in terms of the potential for all fields including strong fields when the body is spherically symmetric. In this case standing, time oscillating, and radially decaying gravitational waves can be generated. However, if the black hole a quires a mass that exceeds a certain critical value a travelling gravitational waves can be emitted with wave length shorter than a certain critical wave length. The singularity black hole problem and the infinite self-mass of elementary particles are one of the long-standing problems in physics. Using the expression of energy in a potential dependent special relativity an advanced model has been constructed. According to this model the energy at which both radius and mass give minimum energy, determine the self-mass and minimum radius. The self-mass was found to be finite, dependent on vacuum energy and coupling constant. The radius was found to be dependent on the short-range field coupling constant.