Light propagation in a homogeneous and anisotropic universe

Abstract

This article proposes a comprehensive analysis of light propagation in an anisotropic and spatially homogeneous Bianchi I universe. After recalling that null geodesics are easily determined in such a spacetime, we derive the expressions of the redshift and direction drifts of light sources; by solving analytically the Sachs equation, we then obtain an explicit expression of the Jacobi matrix describing the propagation of narrow light beams. As a byproduct, we recover the old formula by Saunders for the angular diameter distance in a Bianchi I spacetime, but our derivation goes further since it also provides the optical shear and rotation. These results pave the way to the analysis of both supernovae data and weak lensing by the large-scale structure in Bianchi universes.

12 pages, no figure; v3 matches published version, except a minor typo in Eqs. (4.8), (4.10), now corrected

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• Late-Time Anisotropy Sourced by a 2-Form Field Non-Minimally Coupled to Cold Dark Matter
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• Algebraic symmetries of the observables on the sky: Variable emitters and observers
• Dirac procedure and the Hamiltonian formalism for cosmological perturbations in a Bianchi I universe
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