A new observable for holographic cosmology

Abstract The double-cone geometry is a saddle of the gravitational path integral, which explains the chaotic statistics of the spectrum of black hole microstates. This geometry is the usual AdS-Schwarzschild black hole, but with a periodic identification of the time coordinate; the resulting singula...

Full description

Bibliographic Details
Main Authors: Joydeep Chakravarty, Alexander Maloney, Keivan Namjou, Simon F. Ross
Format: Article
Language:English
Published: SpringerOpen 2024-10-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP10(2024)184