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The quantum development of an asymptotically Euclidean Cauchy hypersurface

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abstract

In our model of quantum gravity the quantum development of a Cauchy hypersurface is governed by a wave equation derived as the result of a canonical quantization process. To find physically interesting solutions of the wave equation we employ the separation of variables by considering a temporal eigenvalue problem which has a complete countable set of eigenfunctions with positive eigenvalues and also a spatial eigenvalue problem which has a complete set of eigendistributions. Assuming that the Cauchy hypersurface is asymtotically Euclidean we prove that the temporal eigenvalues are also spatial eigenvalues and the product of corresponding eigenfunctions and eigendistributions, which will be smooth functions with polynomial growth, are the physically interesting solutions of the wave equation. We consider these solutions to describe the quantum development of the Cauchy hypersurface.

fields

gr-qc 1

years

2019 1

verdicts

REJECT 1

representative citing papers

Applications of canonical quantum gravity to cosmology

gr-qc · 2019-08-03 · reject · novelty 4.0

Dark energy and dark matter are proposed to be, respectively, the vacuum and ground-state eigenvalues of a density operator from canonical quantum gravity, yielding accelerating Friedmann solutions under assumed low temperatures and a negative cosmological constant.

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  • Applications of canonical quantum gravity to cosmology gr-qc · 2019-08-03 · reject · none · ref 12 · internal anchor

    Dark energy and dark matter are proposed to be, respectively, the vacuum and ground-state eigenvalues of a density operator from canonical quantum gravity, yielding accelerating Friedmann solutions under assumed low temperatures and a negative cosmological constant.