Lensing in the McVittie metric
Oliver F. Piattella

TL;DR
This paper examines how cosmological expansion influences gravitational lensing by a point mass using the McVittie metric, finding that at leading order, expansion does not affect the bending angle.
Contribution
It provides an analytic expression for light bending in the McVittie metric with constant Hubble parameter, showing expansion effects are negligible at leading order.
Findings
Bending angle unaffected by cosmological expansion at leading order
Analytic expression derived for lensing in McVittie metric with constant Hubble
Expansion effects are minimal in the leading order approximation
Abstract
We investigate the effect of the cosmological expansion on the bending of light due to an isolated point-like mass. We adopt McVittie metric as the model for the geometry of the lens. Assuming a constant Hubble factor we find an analytic expression involving the bending angle, which turns out to be unaffected by the cosmological expansion at the leading order.
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Taxonomy
TopicsQuantum chaos and dynamical systems · Quantum Electrodynamics and Casimir Effect
