Why the Universe Started from a Low Entropy State
arXiv:hep-th/0511102 · doi:10.1103/PhysRevD.74.123510
Abstract
We show that the inclusion of backreaction of massive long wavelengths imposes dynamical constraints on the allowed phase space of initial conditions for inflation, which results in a superselection rule for the initial conditions. Only high energy inflation is stable against collapse due to the gravitational instability of massive perturbations. We present arguments to the effect that the initial conditions problem {\it cannot} be meaningfully addressed by thermostatistics as far as the gravitational degrees of freedom are concerned. Rather, the choice of the initial conditions for the universe in the phase space and the emergence of an arrow of time have to be treated as a dynamic selection.
12 pages, 2 figs. Final version; agrees with accepted version in Phys. Rev. D
References in corpus (12)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- The Anthropic Landscape of String Theory
- Distributions of nonsupersymmetric flux vacua
- Inflation in AdS/CFT
- Low Energy Supersymmetry From the Landscape
- A Framework for the Landscape
- Can we predict for the Non-SUSY sector of the Landscape ?
- Spontaneous Creation of Inflationary Universes and the Cosmic Landscape
- The Landscape of String Theory and The Wave Function of the Universe
- Do We Have Evidence for New Physics in the Sky?
- A Fly in the SOUP
- Thermal gravity, black holes and cosmological entropy
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