Quantum geometrodynamics: whence, whither?
arXiv:0812.0295 · doi:10.1007/s10714-008-0750-1
Abstract
Quantum geometrodynamics is canonical quantum gravity with the three-metric as the configuration variable. Its central equation is the Wheeler--DeWitt equation. Here I give an overview of the status of this approach. The issues discussed include the problem of time, the relation to the covariant theory, the semiclassical approximation as well as applications to black holes and cosmology. I conclude that quantum geometrodynamics is still a viable approach and provides insights into both the conceptual and technical aspects of quantum gravity.
25 pages; invited contribution for the Proceedings of the seminar "Quantum Gravity: Challenges and Perspectives", Bad Honnef, Germany, April 2008
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- Classical and quantum cosmology of the little rip abrupt event
- Can the Arrow of Time be understood from Quantum Cosmology?
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- Quantum mechanics allows setting initial conditions at a cosmological singularity: Gowdy model example
- Baryogenesis in cosmological models with symmetric and asymmetric quantum bounces
- Cosmological models with asymmetric quantum bounces
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- Comparing Quantum Gravity Models: String Theory, Loop Quantum Gravity, and Entanglement gravity versus -QGR
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- M-theory Calabi-Yau Quantum Mechanics
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- Space, Time, Matter in Quantum Gravity
- Hilbert spaces built over metrics of fixed signature
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- Semiclassical Length Measure from a Quantum-Gravity Wave Function