Probabilities in the Arkani-Hamed-Dimopolous-Kachru landscape
arXiv:hep-th/0611237 · doi:10.1088/1751-8113/40/26/017
Abstract
In a previous paper we found that in the context of the string theory ``discretuum'' proposed by Bousso and Polchinski, the cosmological constant probability distribution varies wildly. However, the successful anthropic predictions of the cosmological constant depend crucially on the assumption of a flat prior distribution. We conjectured that the staggered character of our Bousso-Polchinski distribution will arise in any landscape model which generates a dense spectrum of low-energy constants from a wide distribution of states in the parameter space of the fundamental theory. Here we calculate the volume distribution for in the simpler Arkani-Hamed-Dimopolous-Kachru landscape model, and indeed this conjecture is borne out.
arXiv comment12 pages, 4 figures
References in corpus (7)
- Quantization of Four-form Fluxes and Dynamical Neutralization of the Cosmological Constant
- Predictions from Quantum Cosmology
- Recycling universe
- The cosmological constant and the time of its dominance
- Nucleation Rates in Flat and Curved Space
- Probabilities in the Bousso-Polchinski multiverse
- Coincident brane nucleation and the neutralization of Λ
Cited by in corpus (11)
- Boltzmann brains and the scale-factor cutoff measure of the multiverse
- Predicting the cosmological constant with the scale-factor cutoff measure
- Properties of the scale factor measure
- Predictions from Star Formation in the Multiverse
- Global-Local Duality in Eternal Inflation
- Boundary definition of a multiverse measure
- Anthropic prediction in a large toy landscape
- Negative vacuum energy densities and the causal diamond measure
- Anthropic prediction for a large multi-jump landscape
- Reheating-volume measure in the landscape
- Multiverse rate equation including bubble collisions