Thin accretion disk onto slowly rotating black holes in Einstein-Æther theory

Abstract The accretion disk is formed by particles moving in closed orbits around a compact object, whose physical properties and the electromagnetic radiation characteristics are determined space-time geometry object. In this paper, we study optical appearance of emitted from thin two types black hole solution Einstein-Æther theory. We investigate detail effects æther field on energy flux, temperature distribution, spectrum slowly rotating holes. Then plot ray-traced redshifted image as well intensity polarization profile lensed found that simulation, only has certain effect central shadow area disk.