Authors: John A. Gowan
Following on from its primary role of providing negative energy during the "Big Bang", gravity plays two further major conservation roles in the evolving universe: 1) energy conservation (at all gravitational field strengths) for bound forms of energy, via the creation of time, history, and matter's temporal entropy drive; 2) symmetry conservation (at stellar and higher gravitational field strengths) via the conversion of bound to free energy (mass to light) in stars, supernovas, quasars, and related astrophysical processes, and ultimately and completely, via Hawking's "quantum radiance" of black holes. These secondary conservation roles, manifesting as the gravitational conversion of space to time and bound to free energy, are natural consequences of the mode of action of gravity's primary role, which is the creation of negative energy and entropy via the contraction, heating, and destruction of space (creating time), in contradistinction to the creation, expansion, and cooling of space by the positive energy and entropy of light.
Comments: 17 Pages. adding postscript
Unique-IP document downloads: 195 times
Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.