Energy conservation drives the expansion of the universe
J. M. Greben

TL;DR
This paper proposes a cosmological model driven by vacuum energy conservation, suggesting the universe's expansion is linked to decreasing vacuum energy and offering explanations for dark matter and cosmic acceleration.
Contribution
It introduces a novel cosmological theory where vacuum energy conservation dictates universe expansion and unifies particle physics with cosmology.
Findings
Vacuum energy density decreases as 1/t^3 over time.
The model explains dark matter as a matter term induced by vacuum energy.
It provides a potential explanation for the universe's recent acceleration.
Abstract
We develop a cosmological theory in which the evolution of the universe is controlled by the cosmological constant and dominated by the associated vacuum energy. The universe starts as a classical de Sitter space with an infinite effective vacuum energy density, which decreases subsequently like 1/t^3. The corresponding Friedmann-Robertson-Walker (FRW) scale factor also decreases over time, showing that the common assumption that it describes the expansion of the universe is incorrect and should be abandoned. Instead, the (cubic) expansion of the universe is needed to satisfy energy conservation. Once the vacuum energy density has decreased to the Planck level the first elementary particles can be created through a direct conversion of vacuum energy. After this epoch, the enormous kinetic energy enables a quick magnification of the number of particles through ordinary production…
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Taxonomy
TopicsCosmology and Gravitation Theories · Earth Systems and Cosmic Evolution · Relativity and Gravitational Theory
