Quantum of volume in de Sitter space
Jakub Mielczarek, Wlodzimierz Piechocki

TL;DR
This paper explores the quantization of a flat cosmological model with a scalar field and positive cosmological constant using loop quantum cosmology, revealing a discrete volume spectrum and proposing a link between the cosmological constant and quantum geometry scale.
Contribution
It introduces a scale-dependent Hamiltonian in loop quantum cosmology and investigates the potential interpretation of the cosmological constant as a running parameter.
Findings
The volume operator spectrum is discrete and depends on $\Lambda$.
A relationship between the quantum of volume and the lattice cell size is established.
The possibility of interpreting $\Lambda$ as a running constant is discussed.
Abstract
We apply the nonstandard loop quantum cosmology method to quantize a flat Friedmann-Robertson-Walker cosmological model with a free scalar field and the cosmological constant . Modification of the Hamiltonian in terms of loop geometry parametrized by a length introduces a scale dependence of the model. The spectrum of the volume operator is discrete and depends on . Relating quantum of the volume with an elementary lattice cell leads to an explicit dependence of on . Based on this assumption, we investigate the possibility of interpreting as a running constant.
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