Thermal hybrid inflation in a braneworld

Natural braneworld inflation and baryogenesis

In natural inflation models, the inflaton is a pseudo Nambu-Goldstone boson and the flatness of the potential is protected by shift symmetries. In this framework, a successful inflation requires the global symmetry to be spontaneously broken at a scale close to the Planck mass. Such a high value of the spontaneous breaking scale may not be legitimate in an effective field theory. On the other h...

Thermal hybrid inflation in brane world

In conventional scenario of thermal inflation, the requirement from the reheating temperature puts a lower bound on the mass of the inflaton field. At the same time, the mass of the inflaton field and the height of the potential during thermal inflation is intimately related. With these conditions, the conventional models for thermal inflation are quite restricted. Naively, one may expect that ...

The consistency relation in braneworld inflation

Degeneracy of consistency equations in braneworld inflation

In a Randall–Sundrum type II inflationary scenario we compute perturbation amplitudes and spectral indices up to next-to-lowest order in the slowroll parameters, starting from the well-known lowest-order result for a de Sitter brane. Using two different prescriptions for the tensor amplitude, we show that the braneworld consistency equations are not degenerate with respect to the standard relat...

Dark energy in Chaotic Braneworld Inflation

In this paper, we show that in the framework of chaotic braneworld inflation, after preheating, the remaining oscillating inflaton field can play the role of dark matter with the observed level. Augmented by a non-zero effective cosmological constant Λ4 on the brane, triple unification of inflation, dark matter and dark energy by a single field is realized. Our model perhaps is the simplest one...