A viable Starobinsky-like inflationary scenario in the light of Planck
  and BICEP2 results
  The recent CMB data from Planck and BICEP2 observations have opened a new
window for inflationary cosmology. In this Essay we compare three
Starobinsky-like inflationary scenarios: (i) the original Starobinsky proposal;
(ii) a family of dynamically broken SUGRA models; and (iii) a class of
"decaying" vacuum $\Lambda(H)$ cosmologies. We then focus on the $\Lambda(H)$
variant, which spans the complete cosmic history of the universe from an early
inflationary stage, followed by the "graceful exit" into the standard radiation
regime, the matter epoch and, finally, the late-time accelerated expansion.
Computing the effective potential we find that the "running" $\Lambda(H)$
models also provide a prediction for the tensor-to-scalar ratio of the CMB
spectrum, $r \simeq 0.16$, which is compatible to within $1\sigma$ with the
value $r=0.20^{+0.07}_{-0.05}$ recently measured by the BICEP2 collaboration.
