Abstract

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 is realised in some non-standard scenario such as Warm inflation or the Braneworld scenario. Dimopoulos and Owen (Phys Rev D 94(6): 063518, 2016) 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 correct choice of equation of states (w_{re}), one can also satisfy the recently proposed Trans–Planckian Censorship Conjecture (TCC).

Highlights

  • Of the models to survive the hard reality of observations

  • With the recent theoretical constraints coming from the String theorists, going by the name of Swampland Conjectures (SC) [8,9,10,11] or the Trans-Planckian Conjecture (TCC) [12,13], the whole idea of inflationary cosmology is in an existential crisis

  • Power law plateau model realised in the RS I I brane world [22], is much more robust in the sense that to satisfy

Read more

Summary

Introduction

Power law plateau model realised in the RS I I brane world [22], is much more robust in the sense that to satisfy.

RS I I braneworld
Swampland conjecture and TCC
Power-law plateau type potential
Analysis of inflationary observables
Reheating analysis
Bound on tensor to scalar ratio from TCC
Conclusion
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call