The Generalized Hartle-Hawking Initial State: Quantum Field Theory on Einstein Conifolds

Details The Generalized Hartle-Hawking Initial State: Quantum Field Theory on Einstein Conifolds The Generalized Hartle-Hawking Initial State: Quantum Field Theory on Einstein Conifolds

1999-03-16

arxiv.org/abs/gr-qc/9903062v1

Phys.Rev. D60 (1999) 064013

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Revtex 3, 31 pages, 4 epsf figures

Scientific paper

10.1103/PhysRevD.60.064013

Recent arguments have indicated that the sum over histories formulation of quantum amplitudes for gravity should include sums over conifolds, a set of histories with more general topology than that of manifolds. This paper addresses the consequences of conifold histories in gravitational functional integrals that also include scalar fields. This study will be carried out explicitly for the generalized Hartle-Hawking initial state, that is the Hartle-Hawking initial state generalized to a sum over conifolds. In the perturbative limit of the semiclassical approximation to the generalized Hartle-Hawking state, one finds that quantum field theory on Einstein conifolds is recovered. In particular, the quantum field theory of a scalar field on de Sitter spacetime with $RP^3$ spatial topology is derived from the generalized Hartle-Hawking initial state in this approximation. This derivation is carried out for a scalar field of arbitrary mass and scalar curvature coupling. Additionally, the generalized Hartle-Hawking boundary condition produces a state that is not identical to but corresponds to the Bunch-Davies vacuum on $RP^3$ de Sitter spacetime. This result cannot be obtained from the original Hartle-Hawking state formulated as a sum over manifolds as there is no Einstein manifold with round $RP^3$ boundary.

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