Observational consequences of an interacting multiverse
arXiv:1705.09889 · doi:10.3390/universe3020049
Abstract
The observability of the multiverse is at the very root of its physical significance as a scientific proposal. In this conference we present, within the third quantization formalism, an interacting scheme between the wave functions of different universes and analyze the effects of some particular values of the coupling function. One of the main consequences of the interaction between universes can be the appearance of a pre-inflationary stage in the evolution of the universes that might leave observable consequences in the properties of the CMB.
8 pages, 4 figures. Proceedings of the conference given in the Varying Constants and Fundamental Cosmology meeting (VARCOSMOFUN-16) held in Szczecin, Poland, 12-17th September 2016
References in corpus (7)
- Black Hole Remnants in the Early Universe
- Impact of quantum entanglement on spectrum of cosmological fluctuations
- Testing Predictions of the Quantum Landscape Multiverse 2: The Exponential Inflationary Potential
- Testing Predictions of the Quantum Landscape Multiverse 1: The Starobinsky Inflationary Potential
- Cosmological Avatars of the Landscape II: CMB and LSS Signatures
- Inflation After False Vacuum Decay: New Evidence from BICEP2
- Predictions of the Quantum Landscape Multiverse