Chaotic inflation on the brane and the Swampland Criteria
  In this paper, we show that single-field chaotic inflation on the brane with
the potential $V=a \phi^p$ is compatible with the Swampland criteria. The
spectral index and the running spectral index are within experimental bounds
for $0<p \leq 2$. The tensor to scalar ratio is within observational bounds if
$p \lesssim \mathcal{O}(1)$.
