On the dynamics of single-vertex states in quantum-reduced loop gravity

Abstract In this article we examine a Hamiltonian constraint operator governing the dynamics of simple quantum states, whose graph consists of a single six-valent vertex, in quantum-reduced loop gravity. To this end, we first derive the action of the Hamiltonian constraint on generic basis states in the Hilbert space of quantum-reduced loop gravity. Specializing to the example of the single-vertex states, we find that the Euclidean part of the Hamiltonian bears a close formal similarity to the Hamiltonian constraint of Bianchi I models in loop quantum cosmology. Extending the formal analogy to the Lorentzian part of the Hamiltonian suggests a possible modified definition of the Hamiltonian constraint for loop quantum cosmology, in which the Lorentzian part, corresponding to the scalar curvature of the spatial surfaces, is not assumed to be identically vanishing, and is represented by a non-trivial operator in the quantum theory.

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Publication Details

Journal
Classical and Quantum Gravity
Published
2025-04-16
DOI
https://doi.org/10.1088/1361-6382/adcdb9
Primary Topic
Noncommutative and Quantum Gravity Theories
Type
article
Field-Weighted Citation Impact
0.00

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On the dynamics of single-vertex states in quantum-reduced loop gravity

Ilkka Mäkinen
Classical and Quantum Gravity
Noncommutative and Quantum Gravity Theories
article

On the dynamics of single-vertex states in quantum-reduced loop gravity

Ilkka Mäkinen
article en

Abstract

Abstract In this article we examine a Hamiltonian constraint operator governing the dynamics of simple quantum states, whose graph consists of a single six-valent vertex, in quantum-reduced loop gravity. To this end, we first derive the action of the Hamiltonian constraint on generic basis states in the Hilbert space of quantum-reduced loop gravity. Specializing to the example of the single-vertex states, we find that the Euclidean part of the Hamiltonian bears a close formal similarity to the Hamiltonian constraint of Bianchi I models in loop quantum cosmology. Extending the formal analogy to the Lorentzian part of the Hamiltonian suggests a possible modified definition of the Hamiltonian constraint for loop quantum cosmology, in which the Lorentzian part, corresponding to the scalar curvature of the spatial surfaces, is not assumed to be identically vanishing, and is represented by a non-trivial operator in the quantum theory.

Classical and Quantum GravityVol. 42(9)
National Centre for Nuclear Research (PL)
Narodowe Centrum Nauki, Narodowym Centrum Nauki
Openalex Percentile: Top 94%
Noncommutative and Quantum Gravity Theories
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