Authors: M. A. Thomas
This is Part II of the original presentation by the same title. In this slideshow I will attempt to extend the domain of the theory to higher energies in the extremal gravities present at ~ 2M☉ neutron stars and smaller black holes. At these higher energies and stronger gravities the theory moves into supergravity theories. These are not quantum gravities but are the lower limit of such. Extremal gravities are still comparatively weak compared to strong space-time curvatures near singularities. The Planck energies are still relatively far away and rolled up in very small compactifications. It is not currently known where the energies of supergravities lie.
Comments: 23 Pages. This is a PDF of a Powerpoint Presentation (23 Slides)
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[v1] 2020-03-05 14:17:54
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