Towards the self-adjointness of a Hamiltonian operator in loop quantum gravity
arXiv:1805.08644 · doi:10.1103/PhysRevD.98.086014
Abstract
Although the physical Hamiltonian operator can be constructed in the deparameterized model of loop quantum gravity coupled to a scalar field, its property is still unknown. This open issue is attacked in this paper by considering an operator representing the square of the physical Hamiltonian operator acting nontrivially on two-valent spin networks. The Hilbert space preserved by the graphing changing operator is consist of spin networks with a single two-valent non-degenerate vertex. The matrix element of are explicitly worked out in a suitable basis. It turns out that the operator is essentially self-adjoint, which implies a well-defined physical Hamiltonian operator in for the deparameterized model.
References in corpus (38)
- Background Independent Quantum Gravity: A Status Report
- Discreteness of area and volume in quantum gravity
- Loop Quantum Cosmology: A Status Report
- Quantum Nature of the Big Bang: Improved dynamics
- Quantum Theory of Gravity I: Area Operators
- Real Ashtekar Variables for Lorentzian Signature Space-times
- Quantum Spin Dynamics (QSD)
- Barbero's Hamiltonian derived from a generalized Hilbert-Palatini action
- Quantization of diffeomorphism invariant theories of connections with local degrees of freedom
- Dust as a Standard of Space and Time in Canonical Quantum Gravity
- Differential Geometry on the Space of Connections via Graphs and Projective Limits
- Uniqueness of diffeomorphism invariant states on holonomy-flux algebras
- Partial and Complete Observables for Canonical General Relativity
- Fundamental Structure of Loop Quantum Gravity
- The Phoenix Project: Master Constraint Programme for Loop Quantum Gravity
- Quantum Spin Dynamics (QSD) II
- The physical hamiltonian in nonperturbative quantum gravity
- Algebraic Quantum Gravity (AQG) IV. Reduced Phase Space Quantisation of Loop Quantum Gravity
- Gravity quantized
- Reduced Phase Space Quantization and Dirac Observables
- Representation Theory of Analytic Holonomy C* Algebras
- New scalar constraint operator for loop quantum gravity
- Hamiltonian operator for loop quantum gravity coupled to a scalar field
- The flat FRW model in LQC: the self-adjointness
- Master Constraint Operator in Loop Quantum Gravity
- A regularization of the hamiltonian constraint compatible with the spinfoam dynamics
- Hamiltonian Renormalisation I: Derivation from Osterwalder-Schrader Reconstruction
- Topological Measure and Graph-Differential Geometry on the Quotient Space of Connections
- A symmetric scalar constraint for loop quantum gravity
- New Hamiltonian constraint operator for loop quantum gravity
- New volume and inverse volume operators for loop quantum gravity
- operator for canonical quantum gravity
- Hamiltonian Renormalisation IV. Renormalisation Flow of D+1 dimensional free scalar fields and Rotation Invariance
- Relational Evolution of Observables for Hamiltonian-Constrained Systems
- 2+1 Sector of 3+1 Gravity
- Graphical method in loop quantum gravity: I. Derivation of the closed formula for the matrix element of the volume operator
- Causal structure and degenerate phase boundaries
- Graphical method in loop quantum gravity: II. The Hamiltonian constraint and inverse volume operators
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- Shadow and stability of quantum-corrected black holes
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- Reduced Phase Space Quantization of Black Holes: Path Integrals, and Effective Dynamics
- Alternative dynamics in loop quantum Brans-Dicke cosmology
- Consistency check on the fundamental and alternative flux operators in loop quantum gravity
- Loop quantum cosmology from an alternative Hamiltonian
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- Loop quantum cosmology from an alternative Hamiltonian. II. Including the Lorentzian term
- Dynamics in canonical models of loop quantum gravity
- Covariant effective spacetimes of spherically symmetric electrovacuum with a cosmological constant
- Geometrical Quantum Time in the Model of Euclidean Quantum Gravity
- Loop Quantum Vector-Tensor Gravity and Its Spherically Symmetric Model
- Realization of Dirac quantization in loop quantum gravity