  We argue that more cosmological solutions in massive gravity can be obtained
if the metric tensor and the tensor $\Sigma_{\mu\nu}$ defined by
St\"{u}ckelberg fields take the homogeneous and isotropic form. The standard
cosmology with matter and radiation dominations in the past can be recovered
and $\Lambda$CDM model is easily obtained. The dynamical evolution of the
universe is modified at very early times.
