Properties of fluctuating states in loop quantum cosmology
arXiv:1906.03146 · doi:10.3390/math7070645
Abstract
In loop quantum cosmology, the values of volume fluctuations and correlations determine whether the dynamics of an evolving state exhibits a bounce. Of particular interest are states that are supported only on either the positive or the negative part of the spectrum of the Hamiltonian that generates this evolution. It is shown here that the restricted support on the spectrum does not significantly limit the possible values of volume fluctuations.
12 pages
References in corpus (7)
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Cited by in corpus (5)
- Annihilation-to-nothing: a quantum gravitational boundary condition for the Schwarzschild black hole
- Bounce Models within Teleparallel modified gravity
- Non-bouncing solutions in loop quantum cosmology
- A note on non singular Einstein-Aether cosmologies
- Equivalent Hamiltonian approach to quantum cosmology of integrable models