Quantum Gravity and String Theory


Introduction to Gravitation

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

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Submission history

[v1] 14 Nov 2009
[v2] 12 Oct 2010
[v3] 2011-12-09 20:41:06
[v4] 2011-12-12 09:18:37
[v5] 2012-08-11 13:27:48
[v6] 2012-09-15 12:17:36
[v7] 2014-06-23 14:51:25
[v8] 2014-08-28 16:32:39

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