Charged Einstein-aether black holes and Smarr formula
  In the framework of the Einstein-Maxwell-aether theory, we present two new
classes of exact charged black hole solutions, which are asymptotically flat
and possess the universal as well as Killing horizons. We also construct the
Smarr formulas, and calculate the temperatures of the horizons, using the Smarr
mass-area relation. We find that, in contrast to the neutral case, such
obtained temperature is not proportional to its surface gravity at any of the
two kinds of the horizons. Einstein-Maxwell-aether black holes with the
cosmological constant and their topological cousins are also given.
