Klein-Gordon Thermal Equation For A Preplanckian Universe
نویسندگان
چکیده
In this paper the quantum hyperbolic equation formulated in [1] is applied to the study of the propagation of the initial thermal state of the Universe. It is shown that the propagation depends on the barrier height. The Planck wall potential is introduced, VP = h̄/8tP = 1.25 10 GeV where tP is a Planck time. For the barrier height V < VP the master thermal equation is the modified Klein-Gordon equation, and for barrier height V > VP the master equation is the Klein-Gordon equation. The solutions of both type equations for Cauchy boundary conditions are discussed.
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