Authors: Carlos Castro
Recently, solutions to the $nonlinear$ Bohm-Poisson equation were found  with cosmological applications. We were able to obtain a value for the vacuum energy density of the same order of magnitude as the extremely small observed vacuum energy density, and explained the origins of its $repulsive$ gravitational nature. In this work we show how to obtain a value for the vacuum energy density which coincides $exactly$ with the extremely small observed vacuum energy density. This construction allows also to borrow the results over the past two decades pertaining the study of the Renormalization Group (RG) within the context of Weinberg's Asymptotic Safety scenario. The RG flow behavior of $ G $ shows that $ G $ $increases$ with distance, so that the magnitude of the repulsive force exemplified by $ - G < 0 $ becomes larger, and larger, as the universe expands. This is what is observed.
Comments: 9 Pages. submitted to Physics Letters B
[v1] 2017-10-24 01:42:13
Unique-IP document downloads: 44 times
Vixra.org is a pre-print repository rather than a journal. Articles hosted may not yet have been verified by peer-review and should be treated as preliminary. In particular, anything that appears to include financial or legal advice or proposed medical treatments should be treated with due caution. Vixra.org will not be responsible for any consequences of actions that result from any form of use of any documents on this website.
Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.