Closed FRW holography: a time-dependent ER=EPR realization

• Published in: The journal of high energy physics 2024-05, Vol.2024 (5), p.219-63, Article 219
• Main Authors: Franken, Victor, Partouche, Hervé, Rondeau, François, Toumbas, Nicolaos
• Format: Article
• Language: English
• Subjects: Big bang cosmology; Black holes; Classical and Quantum Gravitation; Cosmological models; Cosmology; de Sitter space; Dictionaries; Elementary Particles; Entanglement; Entropy; Gauge-Gravity Correspondence; Gravity; Holography; Observers; Physics; Physics and Astronomy; Quantum Field Theories; Quantum Field Theory; Quantum Physics; Radiation; Regular Article - Theoretical Physics; Relativity Theory; Screens; Spacetime; String Theory; Time dependence
• ISSN: 1029-8479; 1029-8479
• DOI: 10.1007/JHEP05(2024)219

A bstract We extend a recent de Sitter holographic proposal and entanglement entropy prescription to generic closed FRW cosmologies in arbitrary dimensions, and propose that for large classes of bouncing and Big Bang/Big Crunch cosmologies, the full spacetime can be encoded holographically on two holographic screens, associated to two antipodal observers. In the expanding phase, the two screens lie at the apparent horizons. In the contracting phase, there is an infinite number of possible trajectories of the holographic screens, which can be grouped in equivalence classes. In each class the effective holographic theory can be derived from a pair of “parent” screens on the apparent horizons. A number of cases including moduli dominated cosmologies escape our discussion, and it is expected that two antipodal observers and their associated screens do not suffice to reconstruct these cosmologies. The leading contributions to the entanglement entropy between the screens arise from a minimal extremal trapped or anti-trapped surface lying in the region between them. This picture entails a time-dependent realization of the ER=EPR conjecture, where an effective geometrical bridge connecting the screens via the minimal extremal surface emerges from entanglement. For the Big Crunch contracting cases, the screens disentangle and the geometrical bridge closes off when the minimal extremal trapped sphere hits the Big Crunch singularity at a finite time before the collapse of the Universe. Semiclassical, thermal corrections are incorporated in the cases of radiation dominated cosmologies.