Power Law Plateau Inflation Potential In The RS $II$ Braneworld Evading
  Swampland Conjecture
  In the recent time, inflationary cosmology is facing an existential crisis
due to the proposed Swampland criterion which aims to evade any (meta-)stable
de Sitter construction within the String landscape. It is been realised that a
single field slow roll inflation is inconsistent with the Swampland criterion
unless the inflationary model in realised in some non standard scenario such as
Warm inflation or the Braneworld scenario. In \cite{Dimopoulos}, Dimopoulos and
Owen introduced a new class of model of inflation dubbed as the power law
plateau inflation in the standard cold inflationary scenario. But to realise
this model in the standard scenario consistent with observation, they had to
introduce a phase of thermal inflation. In this paper we have analysed this
model in the braneworld scenario to show that for some choice of the parameters
defining the model class, one can have an observationally consistent power law
plateau without any phase of thermal inflation. We have also shown that, for
the correct choice of model parameters, one can easily satisfy the Swampland
criterion. Besides, for a particular choice of the potential one can also
satisfy the recently proposed Trans-Planckian Censorship Conjecture.
