2005/01/31 by Guido Cognola, E. Elizalde, Emilio Elizalde +4 · 9 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Classical mechanics #Cosmological constant #Cosmology #Cosmology and Gravitation Theories #Dark energy #De Sitter space #De Sitter universe #Effective action #Gravitation #Loop quantum gravity #Mathematical physics #Noncommutative and Quantum Gravity Theories #Physics #Quantum #Quantum gravity #Quantum mechanics #Schwarzschild radius #Theoretical physics #Universe #astro-ph #de Sitter–Schwarzschild metric #gr-qc #hep-th
paper · pdf · doi:10.1088/1475-7516/2005/02/010
published as JCAP 0502:010,2005 · 25 pages, Latex file. Discussion enlarged, new references added. Version accepted in JCAP
arxiv created 2005/02/14 · openalex publication_date 2005/02/25 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/06
Motivated by the dark energy issue, the one-loop quantization approach for a family of relativistic cosmological theories is discussed in some detail. Specifically, general f ( R ) gravity at the one-loop level in a de Sitter universe is investigated, extending a similar program developed for the case of pure Einstein gravity. Using generalized zeta regularization, the one-loop effective action is explicitly obtained off shell, which allows us to study in detail the possibility of (de)stabilization of the de Sitter background by quantum effects. The one-loop effective action may also be useful for the study of the constant curvature black hole nucleation rate and it provides a plausible way of resolving the cosmological constant problem.