In scalar-tensor theories it is the two-derivative sigma-model interactions
that like to compete at low energies with the two-derivative interactions of
General Relativity (GR) $\unicode{x2014}$ at least once the dangerous
zero-derivative terms of the scalar potential are suppressed (such as by a
shift symmetry). But nontrivial two-derivative interactions require at least
two scalars to exist and so never arise in the single-scalar models most
commonly explored. Axio-dilaton models provide a well-motivated minimal class
of models for which these self-interactions can be explored. We review this
class of models and investigate whether these minimal two fields can suffice to
describe both Dark Matter and Dark Energy. We find that they can
$\unicode{x2014}$ the axion is the Dark Matter and the dilaton is the Dark
Energy $\unicode{x2014}$ and that they robustly predict several new phenomena
for the CMB and structure formation that can be sought in observations. These
include specific types of Dark Energy evolution and small space- and
time-dependent changes to particle masses post-recombination that alter the
Integrated Sachs-Wolfe effect, cause small changes to structure growth and
more.
Authors
Smith A; Mylova M; Brax P; Bruck CVD; Burgess CP; Davis A-C