On the hologram of de Sitter

2002/08/17 by Bruno Carneiro da Cunha · 1 citation
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Noncommutative and Quantum Gravity Theories #gr-qc #hep-th

paper · pdf · doi:10.1103/physrevd.66.124011

published as Phys.Rev. D66 (2002) 124011 · RevTeX 4, 8 pages, v3: Small clarifications on sections III and IV and references added/corrected, v4: typos

arxiv created 2002/08/17 · openalex publication_date 2002/12/26 · arxiv updated 2009/11/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

A careful reduction of three-dimensional gravity to the Liouville description is performed, where all gauge fixing and on-shell conditions come from the definition of asymptotic de Sitter spaces. The roles of both past and future infinities are discussed and the conditions space-time evolution imposes on both Liouville fields are made explicit. Space-times which correspond to nonequivalent profiles of the Liouville field at I^\ensuremath- and I⁺ are shown to exist. The qualitative implications of this for any tentative dual theory are presented.

Citations

• Quantum Gravity In De Sitter Space
• Quantum Fields in Curved Space
• 2 + 1 dimensional gravity as an exactly soluble system
• (Anti-) de Sitter Black Holes in higher derivative gravity and dual Conformal Field Theories
• The Stretched Horizon and Black Hole Complementarity
• The dS/CFT Correspondence
• The World as a Hologram

Cited by

• Comments on quantum aspects of three-dimensional de Sitter gravity