  Einstein-Maxwell-dilaton theory is an interesting theory of gravity for
studying scalar fields in the context of no-hair theorem. In this work, we
consider static charged dilaton and charged, slowly rotating dilaton black
holes in Einstein-Maxwell-dilaton gravity. We investigate the accretion process
in thin disks around such black holes, using the Novikov-Thorne model. The
electromagnetic flux, temperature distribution, energy conversion efficiency
and also innermost stable circular orbits of thin disks are obtained and
effects of dilaton and rotation parameters are studied. For the static and
slowly rotating black holes the results are compared to that of Schwarzschild
and Kerr, respectively.
