Matrix Multiverses Meet Multiple Mythologies
Sidan A, Tom Banks, Willy Fischler
Abstract
We present a model in which asymptotically de Sitter universes of various types, and de Sitter (dS) radii Rn, live in the interiors of black holes in a maximally entropic flat p = ρ Friedmann-Robertson-Walker universe. These dS universes clearly have many quantum states. We argue that they decay and equilibrate with the maximal entropy universe on time scales of order αn Rn ln (Rn /δn), where αn are model-dependent dimensionless constants and δn are the initial distances between the shell, satisfying the Israel junction conditions, and the dS horizon. These are time-scales as viewed by a detector following a trajectory far from the would-be cosmological horizon. These times are all exponentially shorter than dS recurrence times, which have no meaning in this model. It is impossible for a detector inside one of the dS universes to determine whether it is actually part of such a structure. This model could be used as the basis for claiming that certain constants of nature or cosmological initial conditions were chosen to have mathematically unnatural values because other values could not lead to any form of intelligent life.
Create a lesson
Related papers
When duality changes the poles: SL(2,Z) transformations of linear response EFTs
Andrea Amoretti, Daniel K. Brattan, Jonas Rongen
The Geometry of the CKM matrix, the Standard Model and RG fixed points
Brian P. Dolan, Charles Nash
Auxiliary Field Deformations of the Lambda Model
Christian Ferko, Cian Luke Martin, Pranat Sharma
Carrollian axion electrodynamics
Hemant Rathi, Ashish Shukla
The geometry of multiloop Feynman Integrals from the Scattering Facet
José Ríos-Sánchez, Germán Rodrigo
Deep learning emergent spacetime from fermionic spectral functions in holography
Koji Hashimoto, Hyun-Sik Jeong, Keun-Young Kim et al.