The Inflationary Energy Scale in Braneworld Cosmology

Details The Inflationary Energy Scale in Braneworld Cosmology The Inflationary Energy Scale in Braneworld Cosmology

2003-06-16

arxiv.org/abs/astro-ph/0306311v1

Phys.Rev. D68 (2003) 083505

Astronomy and Astrophysics

Astrophysics

10 pages, 3 figures

Scientific paper

10.1103/PhysRevD.68.083505

Upper bounds on the energy scale at the end of inflation in the Randall-Sundrum type II braneworld scenario are derived. The analysis is made exact by introducing new parameters that represent extensions of the Hubble flow parameters. Only very weak assumptions about the form of the inflaton potential are made. In the high energy and slow roll regime the bounds depend on the amplitude of gravitational waves produced during inflation and become stronger as this amplitude increases.

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