Neural quantum states on K5 yield two families of approximate physical states for the Thiemann-ordered Hamiltonian constraint in Abelianized Euclidean LQG: one flat with non-zero volume (non-normalizable) and one normalizable with zero volume, close to Ashtekar-Lewandowski and Dittrich-Geiller vacua
Thiemann, Modern Canonical Quantum Gen- eral Relativity, Cambridge University Press
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A van der Waals-inspired modification to general relativity renders the gravitational coupling dynamical, providing a mechanism to avoid Big Bang and black hole singularities.
The quantum parameter ζ modifies quasinormal frequency spectra of charged effective black holes with Λ, preserving non-monotonic behaviors while adding new features to overtone outbursts and complex-imaginary mode interactions.
The Holst model with β=0 yields 10 differential constraints, 21 algebraic constraints, and 6 evolution equations that exactly account for all 37 field components while leaving lapse and shift unconstrained.
For genuine 3D collapsing Bianchi I initial conditions in mLQC-I, quantum effects damp shear exponentially after the bounce, yielding an isotropic attractor independent of matter content under the weak energy condition.
citing papers explorer
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Finding and characterising physical states of Euclidean Abelianized loop quantum gravity using neural quantum states
Neural quantum states on K5 yield two families of approximate physical states for the Thiemann-ordered Hamiltonian constraint in Abelianized Euclidean LQG: one flat with non-zero volume (non-normalizable) and one normalizable with zero volume, close to Ashtekar-Lewandowski and Dittrich-Geiller vacua
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Van der Waals Gravity Theory
A van der Waals-inspired modification to general relativity renders the gravitational coupling dynamical, providing a mechanism to avoid Big Bang and black hole singularities.
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Quasinormal modes of charged covariant effective black holes with a cosmological constant
The quantum parameter ζ modifies quasinormal frequency spectra of charged effective black holes with Λ, preserving non-monotonic behaviors while adding new features to overtone outbursts and complex-imaginary mode interactions.
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A Lagrangian framework for canonical analysis for the Holst model with $\beta = 0$
The Holst model with β=0 yields 10 differential constraints, 21 algebraic constraints, and 6 evolution equations that exactly account for all 37 field components while leaving lapse and shift unconstrained.
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Genericness of quantum damping of cosmological shear in modified loop quantum cosmology
For genuine 3D collapsing Bianchi I initial conditions in mLQC-I, quantum effects damp shear exponentially after the bounce, yielding an isotropic attractor independent of matter content under the weak energy condition.