The dark aftermath of Higgs inflation
  In this letter we study the dynamics of the late Universe when a nonminimally
coupled Higgs field is present. In general, the nonminimal coupling leads to a
nontrivial mixing between the gravitational degrees of freedom and the
Goldstone massless bosons. We know that this is irrelevant during the
inflationary phase. In contrast, in the late Universe the nonminimal coupling
affects the classical equations of motion, leading to an acceleration of the
expansion rate or to a collapse that forms Q-balls.
