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Overall signature of the metric and the cosmological constant

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arxiv 2306.11502 v3 pith:JGQOHNDJ submitted 2023-06-20 hep-th gr-qc

classification hep-thgr-qc
keywords changesignatureclassicalmetricconstantcosmologicaldifferentgeneral
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We consider a little known aspect of signature change, where the overall sign of the metric is allowed to change, with physical implications. We show how, in different formulations of general relativity, this type of classical signature change across boundaries with a degenerate metric can be made consistent with a change in sign (and value) of the cosmological constant $\Lambda$. In particular, the separate "mostly plus" and "mostly minus" signature sectors of Lorentzian gravity are most naturally associated with different signs of $\Lambda$. We show how this general phenomenon allows for classical solutions where the open dS patch can arise from a portion of AdS space time. These can be interpreted as classical "imaginary space" extensions of the usual Lorentzian theory, with $a^2<0$.

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Forward citations

Cited by 6 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

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  4. Statistical consistency of sign-switching vacuum energy with cosmological observations

    astro-ph.CO 2026-03 conditional novelty 5.0 of 10

    Using exact non-Gaussian shift and posterior predictive tests, ΛsCDM improves CMB–BAO consistency and softens but does not resolve the Hubble tension, which persists at p≈4×10⁻⁴.

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    A covariant Moore-Penrose algorithm for complex degenerate metrics is formulated, but its uniqueness and torsion interpretation depend on an arbitrary auxiliary metric and the central proof is incomplete.

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    gr-qc 2025-01 conditional novelty 5.0 of 10

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