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arXiv · gr-qc/9509053

Cosmological perturbations and classical change of signature

Jerome Martin
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Abstract

Cosmological perturbations on a manifold admitting signature change are studied. The background solution consists in a Friedmann-Lemaitre-Robertson- Walker (FLRW) Universe filled by a constant scalar field playing the role of a cosmological constant. It is shown that no regular solution exist satisfying the junction conditions at the surface of change. The comparison with similar studies in quantum cosmology is made.

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Jerome Martin. 1995-09-27. Cosmological perturbations and classical change of signature. https://doi.org/10.1103/physrevd.52.6708

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