The Entropic Landscape
arXiv:1001.1155 · doi:10.1103/PhysRevD.82.123523
Abstract
We initiate a quantitative exploration of the entire landscape. Predictions thus far have focused on subsets of landscape vacua that share most properties with our own. Using the entropic principle (the assumption that entropy production traces the formation of complex structures such as observers), we derive six predictions that apply to the whole landscape. Typical observers find themselves in a flat universe, at the onset of vacuum domination, surrounded by a recently produced bath of relativistic quanta. These quanta are neither very dilute nor condensed, and thus appear as a roughly thermal background. Their characteristic wavelength is of order the inverse fourth root of the vacuum energy. These predictions hold for completely arbitrary observers, in arbitrary vacua with potentially exotic particle physics and cosmology. They agree with observation: We live in a flat universe at the onset of vacuum domination, whose dominant entropy production process (the glow of galactic dust) has recently produced a radiation bath (the cosmic infrared background). This radiation is marginally dilute, relativistic, and has a wavelength of order 100 microns, as predicted.
40 pages and 3 figures, references added
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- The Multiverse Interpretation of Quantum Mechanics
- Life at the Interface of Particle Physics and String Theory
- Inflation after False Vacuum Decay: Observational Prospects after Planck
- Technically natural dark energy from Lorentz breaking
- A geometric solution to the coincidence problem, and the size of the landscape as the origin of hierarchy
- The Cosmological Constant Problem, Dark Energy, and the Landscape of String Theory
- The string landscape and low energy supersymmetry
- Geometric origin of coincidences and hierarchies in the landscape
- Boundary definition of a multiverse measure
- Vacuum Structure and the Arrow of Time
- Why Comparable? A Multiverse Explanation of the Dark Matter-Baryon Coincidence
- Supersymmetry Breaking and the Cosmological Constant
- Deformed compact extra space as dark matter candidate
- New Scale Factor Measure
- New Inflation in the Landscape and Typicality of the Observed Cosmic Perturbation
- Anthropic Origin of the Neutrino Mass from Cooling Failure
- Ab Initio Estimates of the Size of the Observable Universe
- Dark Matter Annihilations in the Causal Diamond
- A Computational Anthropic Principle: Where is the Hardest Problem in the Multiverse?
- Anthropic Estimates for Many Parameters of Physics and Astronomy