Sayantan Choudhury, Supratik Pal
We propose a model of inflation in the framework of brane cosmology driven by
background supergravity. Starting from bulk supergravity we construct the
inflaton potential on the brane and employ it to investigate for the
consequences to inflationary paradigm. To this end, we derive the expressions
for the important parameters in brane inflation, which are somewhat different
from their counterparts in standard cosmology, using the one loop radiative
corrected potential. We further estimate the observable parameters and find
them to fit well with recent observational data by confronting with WMAP7 using
CAMB. We also analyze the typical energy scale of brane inflation with our
model, which resonates well with present estimates from cosmology and standard
model of particle physics.
View original:
http://arxiv.org/abs/1102.4206
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