Nature of Singularities in Vector-Tensor Theories of Gravity
  The Vector-Tensor (VT) theories of gravity are a class of alternative
theories to General Relativity (GR) that are characterized by the presence of a
dynamical vector field besides the metric. They are studied in attempts to
understand spontaneous Lorentz violation, to generate massive gravitons, and as
models of dark matter and dark energy. In this article, I outline how the
nature of singularities and horizons in VT theories differ greatly from GR even
under the same ordinary conditions. This is illustrated with Einsteinaether
theory where vacuum black hole solutions have naked singularities and vacuum
cosmological solutions have new singularities that are otherwise absent in GR.
It would be interesting to explore these deviations using gravitational waves
