pith. sign in

arxiv: 1411.0046 · v1 · pith:OVVJ6GVLnew · submitted 2014-11-01 · 🌀 gr-qc

The Dispersion Relation for Matter Waves in a Two-Phase Vacuum

classification 🌀 gr-qc
keywords lambdawavesdispersionmatterrelationlesstheorytwo-phase
0
0 comments X
read the original abstract

The cosmological constant (lambda) of general relativity is a natural consequence of embedding Einstein's theory in a five-dimensional theory of the type needed for unification. The exact 5D solution for lambda less than 0 shows waves in ordinary 3D space with properties similar to those of de Broglie or matter waves. Here the dispersion relation is derived for matter waves in a toy two-phase model, where regions with lambda less than 0 and lambda greater than 0 average on the large scale to lambda = 0, thus providing in principle a resolution of the cosmological-constant problem. A striking result of the analysis is that the dispersion relation is bimodal, with a well-defined window of high-frequency transmission which effectively defines the speed of light.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.