Lattice Refining LQC and the Matter Hamiltonian
William Nelson, Mairi Sakellariadou (King's College, London)

TL;DR
This paper investigates how different lattice refinement models in loop quantum cosmology constrain matter content by analyzing the Hamiltonian constraint with various operator properties.
Contribution
It introduces a parametrization of lattice refinement and matter Hamiltonian, analyzing their effects on wave-function solutions in loop quantum cosmology.
Findings
Constraints on parameter space (A, δ) restrict matter content.
Solutions depend on self-adjointness of Hamiltonian.
Physical restrictions limit supported matter types.
Abstract
In the context of loop quantum cosmology, we parametrise the lattice refinement by a parameter, , and the matter Hamiltonian by a parameter, . We then solve the Hamiltonian constraint for both a self-adjoint, and a non-self-adjoint Hamiltonian operator. Demanding that the solutions for the wave-functions obey certain physical restrictions, we impose constraints on the two-dimensional, , parameter space, thereby restricting the types of matter content that can be supported by a particular lattice refinement model.
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