Cosmology With A Dark Refraction Index

TL;DR

This paper explores how a cosmic fluid's refractive index influences light propagation in cosmology, potentially explaining supernova observations without cosmic acceleration and offering new interpretations of inhomogeneity effects.

Contribution

It introduces a model linking the cosmic fluid's refractive index to cosmological observations, extending optical metric theory to explain supernova data and inhomogeneity effects.

Findings

Refraction index can fit supernova Hubble curve without acceleration.

Inhomogeneity effects like Sachs-Wolfe can be modeled as refraction.

The theory applies to gravitational waves and neutrino fluxes.

Abstract

We review Gordon's optical metric and the transport equations for the amplitude and polarization of a geometrical optics wave traveling in a gravity field. We apply the theory to the FLRW cosmologies by associating a refraction index with the cosmic fluid. We then derive an expression for the accumulated effect of a refraction index on the distance redshift relations and fit the Hubble curve of current supernova observations with a non-accelerating cosmological model. We also show that some observational effects caused by inhomogeneities, e.g. the Sachs-Wolfe effect, can be interpreted as being caused by an effective index of refraction, and hence this theory could extend to other speed of light communications such as gravitational radiation and neutrino fluxes.