Space Time Matter inflation

Abstract

We study a model of power-law inflationary inflation using the Space-Time-Matter (STM) theory of gravity for a five dimensional (5D) canonical metric that describes an apparent vacuum. In this approach the expansion is governed by a single scalar (neutral) quantum field. In particular, we study the case where the power of expansion of the universe is $p\gg 1$. This kind of model is more successful than others in accounting for galaxy formation.

accepted in JMP

References in corpus (2)

• Inflationary cosmology from STM theory of gravity
• An exact solution of the five-dimensional Einstein equations with four-dimensional de Sitter-like expansion

Cited by in corpus (6)

• A Class of Anisotropic Five-Dimensional Solutions for the Early Universe
• A confirmation of agreement of different approaches for scalar gauge-invariant metric perturbations during inflation
• Passing to an effective 4D phantom cosmology from 5D vacuum theory of gravity
• Fierz-Pauli equation for massive gravitons from Induced Matter theory of gravity
• Dirac equation in a de Sitter expansion for massive neutrinos from modern Kaluza-Klein theory
• Scalar Metric fluctuations in space time matter inflation