2011, Vol.14, No.2, pp.126-137
In this work on the basis of author's previous results and within
the scope of the Generalized Uncertainty Principle, a model of the
high energy deformation for a particular case of Einstein's
equations is developed. In the process a thermodynamic description
of General Relativity is used. And the deformation is understood
as an extension of a particular theory by inclusion of one or
several additional parameters in such a way that the initial
theory appears in the limiting transition. The possibility for
the high energy deformation of Einstein's equations within the
scope of both equilibrium thermodynamics and non-equilibrium
thermodynamics is examined.
Key words:
gravitational thermodynamics, high energy deformation of Einstein's equations,
Early Universe
Full text: Acrobat PDF (147KB)
Copyright © Nonlinear Phenomena in Complex Systems. Last updated: September 28, 2011