Wave-theoretical description of the solar gravitational lens
arXiv:1703.05783 · doi:10.1103/PhysRevD.95.084041
Abstract
We discuss the propagation of electromagnetic (EM) waves in the post-Newtonian approximation of the general theory of relativity. We consider diffraction of EM waves in the static gravitational field of a massive monopole. We develop a wave-theoretical description of the solar gravitational lens (SGL) and show that with its enormous magnifying power of (for m) and angular resolution of arcsec, the SGL may be used for direct megapixel imaging of an exoplanet.
5 pages
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