Authors: Andrew Beckwith
This paper is to address what a fluctuation of a metric tensor becomes in early universe conditions. This metric fluctuation in conjunction with Barbour’s work on emergent time, allows for a lower bound to a graviton mass, and this lower bound mass for the graviton is contrasted with the NLED (non linear electrodynamic) calculations which may lead to an upper bound to a graviton mass. We show that the supposition of flat space uncertainty in energy is not supportable in initial phases of GR
Comments: 6 Pages. for the Marcel Grossman conference. The NLED argument is completely new, as a link to upper values of a graviton mass
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[v1] 2015-09-26 07:29:07
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