Confronting Einstein Yang Mills Higgs Dark Energy in light of
  observations
  We study the observational aspects of Einstein Yang Mills Higgs Dark energy
model and constrain the parameter space from the latest observational data from
type Ia supernovae, observational Hubble data, baryon acoustic oscillation data
and cosmic microwave background radiation shift parameter data. It is found
from the analysis of data that the Higgs field in presence of gauge fields can
successfully describe the present accelerated expansion of the universe
consistent with the astrophysical observations.
