Wave optics of the solar gravity lens

Abstract

It is well known that the solar gravitational field can be considered as a telescope with a prime focus at locations beyond 550 au. In this work we present a new derivation of the wave-optical properties of the system, by adapting the arrival-time formalism from gravitational lensing. At the diffraction limit the angular resolution is similar to that of a notional telescope with the diameter of the Sun, and the maximum light amplification is $8\pi 4GM/(c^2\lambda )$, enough to detect a 1 W laser on Proxima Centauri b pointed in the general direction of the Sun. Extended sources, however, would be blurred by the wings of the point spread function into the geometrical-optics regime of gravitational lensing. Broad-band sources would have to further contend with the solar corona. Imaging an exoplanet surface as advocated in the literature, without attempting to reach the diffraction limit, appears achievable. For diffraction-limited imaging (sub-km scales from 100 pc) nearby neutron stars appear to be most plausible targets.

References in corpus (5)

• A terrestrial planet candidate in a temperate orbit around Proxima Centauri
• The Cosmic Horseshoe: Discovery of an Einstein Ring around a Giant Luminous Red Galaxy
• Diffraction of electromagnetic waves by an extended gravitational lens
• Searching for Planets Orbiting Alpha Centauri A with the James Webb Space Telescope
• Interstellar communication. II. Application to the solar gravitational lens