Future singularity avoidance in semiclassical cosmology
DOI10.1007/S10714-012-1385-9zbMath1250.83045OpenAlexW2016389823MaRDI QIDQ715027
Publication date: 15 October 2012
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10714-012-1385-9
Relativistic cosmology (83F05) Quantum field theory on curved space or space-time backgrounds (81T20) Quantization of the gravitational field (83C45) Methods of quantum field theory in general relativity and gravitational theory (83C47) Space-time singularities, cosmic censorship, etc. (83C75) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Astrophysical cosmology (85A40)
Cites Work
- Unnamed Item
- Unnamed Item
- Particle production in an expanding universe dominated by dark energy fluid
- Stability of semiclassical gravity solutions with respect to quantum metric fluctuations
- A new type of isotropic cosmological models without singularity
- Quantum driven bounce of the future universe
- Quantum nature of the big bang: Improved dynamics
- Casimir effect in de Sitter and anti–de Sitter braneworlds
- Consistent loop quantum cosmology
- More general sudden singularities
- Quantum fields and ‘big rip’ expansion singularities
- Sudden future singularities
- Quantum spin dynamics (QSD): V. Quantum gravity as the natural regulator of the Hamiltonian constraint of matter quantum field theories
- Are loop quantum cosmos never singular?
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Uses of zeta regularization in QFT with boundary conditions: a cosmo-topological Casimir effect
- The Large Scale Structure of Space-Time
- QUANTUM EFFECTS AND STABILITY OF CHAMELEON COSMOLOGY
This page was built for publication: Future singularity avoidance in semiclassical cosmology