Dark energy as stimulated emission of gravitons from a background brane
Peter L. Biermann, Benjamin C. Harms

TL;DR
This paper proposes that dark energy results from stimulated emission of gravitational wave solitons from a background brane, explaining its properties and suggesting potential observational tests.
Contribution
It introduces a novel model where dark energy arises from stimulated emission of gravitational waves from a background brane, with detailed energy transfer modeling.
Findings
Model explains dark energy's strength and evolution
Predicts detectable gravitational wave solitons
Suggests observational tests via pulsar timing and backgrounds
Abstract
The idea that dark energy is gravitational waves may explain its strength and its time-evolution provided that the additional energy comes from a background. A possible concept is that dark energy is the ensemble of coherent bursts (solitons) of gravitational waves originally produced by stimulated emission when the first generation of super-massive black holes was formed. These solitons get their initial energy as well as keep up their energy density throughout the evolution of the universe by stimulating emission from a background brane. We model this process by working out this energy transfer in a Boltzmann equation approach. The transit of these gravitational wave solitons may be detectable. Key tests include pulsar timing, clock jitter and the radio and neutrino backgrounds.
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Taxonomy
TopicsCosmology and Gravitation Theories · Pulsars and Gravitational Waves Research · Geophysics and Gravity Measurements
