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Dynamical Mechanism for Varying Light Velocity as a Solution to Cosmological Problems

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arxiv astro-ph/9812481 v2 pith:FAMPU52T submitted 1998-12-30 astro-ph gr-qchep-th

classification astro-phgr-qchep-th
keywords fieldmatterequationsdescribesdynamicallightmechanismproblems
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abstract

A dynamical model for varying light velocity in cosmology is developed, based on the idea that there are two metrics in spacetime. One metric $g_{\mu\nu}$ describes the standard gravitational vacuum, and the other ${\hat g}_{\mu\nu} =g_{\mu\nu}+\beta\psi_\mu\psi_\nu$ describes the geometry through which matter fields propagate. Matter propagating causally with respect to $\hat{g}_{\mu\nu}$ can provide acausal contributions to the matter stress-energy tensor in the field equations for $g_{\mu\nu}$, which, as we explicitly demonstrate with perfect fluid and scalar field matter models, provides a mechanism for the solution of the horizon, flatness and magnetic monopole problems in an FRW universe. The field equations also provide a ``graceful exit'' to the inflationary epoch since below an energy scale (related to the mass of $\psi_\mu$) we recover exactly the standard FRW field equations.

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Cited by 2 Pith papers

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

  1. Alleviating the Hubble Tension via Cosmological Time Dilation in the meVSL Model

    physics.gen-ph 2025-09 reject novelty 3.0 of 10

    The meVSL model's parameter b reduces the baryon drag sound horizon, raising inferred H0, and changes the cosmological time-dilation exponent to n=1-b/4; the paper forecasts SN sample sizes to detect this.

  2. Revisiting Varying Speed of Light in Cosmology: Insights from the Friedmann-Lema\^itre-Robertson-Walker Metric

    physics.gen-ph 2025-05 reject novelty 2.0 of 10

    A varying speed of light in FLRW is presented as gauge freedom via the lapse function, but the key variational derivation omits the √-g measure and the claimed Hubble-tension resolution contradicts Eq. (30).

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