A study of inhomogeneous massless scalar gauge fields in cosmology
  Why is the Universe so homogeneous and isotropic? We summarize a general
study of a $\gamma$-law perfect fluid alongside an inhomogeneous, massless
scalar gauge field (with homogeneous gradient) in anisotropic spaces with
General Relativity. The anisotropic matter sector is implemented as a $j$-form
(field-strength level), where $j\,\in\,\{1,3\}$, and the spaces studied are
Bianchi space-times of solvable type. Wald's no-hair theorem is extended to
include the $j$-form case. We highlight three new self-similar space-times: the
Edge, the Rope and Wonderland. The latter solution is so far found to exist in
the physical state space of types I,II, IV, VI$_0$, VI$_h$, VII$_0$ and
VII$_h$, and is a global attractor in I and V. The stability analysis of the
other types has not yet been performed. This paper is a summary of ~[1], with
some remarks towards new results which will be further laid out in upcoming
work.
