A New View of the Cosmic Landscape
S.-H. Henry Tye

TL;DR
This paper proposes a new perspective on the cosmic landscape in string theory, suggesting that the short lifetime of meta-stable deSitter vacua explains the smallness of dark energy, based on resonance tunneling and landscape topography.
Contribution
It introduces a novel dynamical explanation for the small dark energy by analyzing the landscape's topography and resonance tunneling effects.
Findings
Meta-stable deSitter vacua have short lifetimes in the landscape.
Smaller vacuum energy correlates with longer vacuum lifetime.
Mapping landscape topography can test the proposed scenario.
Abstract
In this scenario, a generic meta-stable deSitter vacuum site in the cosmic landscape in string theory has a very short lifetime. Typically, the smaller is the vacuum energy of a meta-stable site, the longer is its lifetime. This view of the landscape can provide a qualitative dynamical explanation why the dark energy of our universe is so small. The argument for this scenario is based on resonance tunneling, a well-known quantum mechanical phenomenon, the topography of the landscape, and the vastness of the cosmic landscape. Mapping the topography of the landscape, even if only in a small region, will test the validity of this scenario.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Quantum Mechanics and Applications
