Authors: Andrew Beckwith
Initial temperature, particle count are tied into entropy genration, and we make a reference to the Riemannian Penrose inequality, in terms of , if it is an equality what it says about admissible frequencies, as to the early universe. The author is fully aware of the Riemannian Penrose inequality's usual application, black hole physics. Its application to early universe cosmology is due to assuming a non zero, but extremely small initial scale factor at the start of inflation. The frequency, of Eq.(12) is proportional to [1/ distance] with the distance ~ Area to the 1/3rd power. Which is used as a bound to make sense of the range of frequencies assumed in this problem
Comments: Re do of equation 12, with explanations of dimensional scaling put in ; 6 Pages. For Marcel Grossman 14. Details put in as to Riemannian Penrose inequality only being used here due to a non zero scale factor, initially.
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[v1] 2015-09-29 00:15:51
[v2] 2015-10-01 01:12:00
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