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The flat FRW model in LQC: self-adjointness

Wojciech Kamiński and Jerzy Lewandowski

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The flat Friedman–Robertson–Walker (FRW) model coupled to the massless scalar field according to the improved, background scale-independent version of Ashtekar, Pawłowski and Singh [1] is considered. The core of the theory is addressed directly: the APS construction of the quantum Hamiltonian is analyzed under the assumption that the cosmological constant Λ ≤ 0. We prove the essential self-adjointness of the operator whose square-root defines in [1] the quantum Hamiltonian operator and therefore provide the explicit definition. If Λ < 0, then the spectrum is discrete. In the Λ = 0 case, the essential and absolutely continuous spectra of the operator are derived. The latter operator is related in the unitary way to the absolutely continuous part of the quantum mechanics operator a\big({-}\frac{\partial^2}{\partial y^2} - \frac{b}{{\rm cosh}^2\hat{y}}\big) (a, b > 0 being some constants) plus a trace class operator.


PACS

98.80.Cq Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.)

98.80.Es Observational cosmology (including Hubble constant, distance scale, cosmological constant, early Universe, etc)

95.30.Sf Relativity and gravitation

04.60.Pp Loop quantum gravity, quantum geometry, spin foams

98.80.Qc Quantum cosmology

MSC

83C45 Quantization of the gravitational field

83F05 Cosmology

47L30 Abstract operator algebras on Hilbert spaces

85A40 Cosmology (For relativistic cosmology, see 83F05)

81R15 Operator algebra methods (See also 46Lxx, 81T05)

Subjects

Gravitation and cosmology

Astrophysics and astroparticles

Dates

Issue 3 (7 February 2008)

Received 26 August 2007, in final form 5 December 2007

Published 14 January 2008



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