On the Consistency of the Wheeler-DeWitt Equation in the Quantized Eddington-inspired Born-Infeld Gravity
arXiv:1810.10918 · doi:10.1088/1475-7516/2018/12/032
Abstract
We re-examine the quantum geometrodynamical approach within the Eddington-inspired-Born-Infeld theory of gravity, which was first proposed in our previous work [1]. A thorough analysis of the classical Hamiltonian with constraints is carried and the correctness and self-consistency of the modified Wheeler-DeWitt equation (WDW) is studied. We find that based on the newly obtained WDW equation derived with the use of the Dirac brackets, the conclusion reached in Ref.[1] can be corroborated. The big rip singularity present in the classical theory, and induced by a phantom perfect fluid, is expected to be avoided when quantum effects encoded on the modified WDW equation are taken into account.
14 pages
References in corpus (5)
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Worse than a big rip?
- Cosmology with Eddington-inspired Gravity
- Eddington-Born-Infeld cosmology: a cosmographic approach, a tale of doomsdays and the fate of bound structures
- Towards the Quantization of Eddington-inspired-Born-Infeld Theory
Cited by in corpus (8)
- Cosmological constraints of phantom dark energy models
- Ricci-Based Gravity theories and their impact on Maxwell and nonlinear electromagnetic models
- Phantom singularities and their quantum fate: general relativity and beyond
- The classical and quantum fate of the Little Sibling of the Big Rip in cosmology
- The little rip in classical and quantum cosmology
- Classical and quantum cosmology: The big rip, the little rip and the little sibling of the big rip
- Eddington-inspired-Born-Infeld tensorial instabilities neutralized in a quantum approach
- Quantum relativistic cosmology: dynamical interpretation and tunneling universe