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Quantum Schwarzschild-(A)dS black holes: unitarity and singularity resolution
We consider the canonical quantisation of spherically symmetric spacetimes within unimodular gravity, leaving sign choices in the metric general enough to include both the interior and exterior Schwarzschild-(Anti-)de Sitter spacetime.
Steffen Gielen, Sofie Ried
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Time evolution in canonical quantum gravity is trivial
The Wheeler-DeWitt (WdW) equation does not describe any explicit time evolution of the wave function, and somehow related to this issue, there is no natural way of defining an invariant inner product that provides a viable probability interpretation.
openaire +2 more sources
Quantum Gravity Spacetime: Universe vs. Multiverse. [PDF]
Tessarotto M, Cremaschini C.
europepmc +1 more source
Planar Black Holes and Entanglement Entropy in Analog Gravity Models. [PDF]
Bilic N, Zingg T.
europepmc +1 more source
Entropy of a Quasi-de Sitter Spacetime and the Role of Specific Heat. [PDF]
Luongo O, Azizinia M, Boshkayev K.
europepmc +1 more source
Master field equations for spherically symmetric gravitational fields beyond general relativity. [PDF]
Carballo-Rubio R.
europepmc +1 more source
Tunneling between Multiple Histories as a Solution to the Information Loss Paradox. [PDF]
Chen P, Sasaki M, Yeom DH, Yoon J.
europepmc +1 more source
Entropic Dynamics Approach to Relational Quantum Mechanics. [PDF]
Caticha A, Saleem H.
europepmc +1 more source
Minimum Spacetime Length and the Thermodynamics of Spacetime. [PDF]
Rossi V, Cacciatori SL, Pesci A.
europepmc +1 more source

