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A semi-analytical approach to perturbations in mutated hilltop inflation (1010.5924v3)
Published 28 Oct 2010 in astro-ph.CO, gr-qc, and hep-th
Abstract: We study cosmological perturbations and observational aspects for mutated hilltop model of inflation. Employing mostly analytical treatment, we evaluate observable parameters during inflation as well as post-inflationary perturbations. This further leads to exploring observational aspects related to Cosmic Microwave Background (CMB) radiation. This semi-analytical treatment reduces complications related to numerical computation to some extent for studying the different phenomena related to CMB angular power spectrum for mutated hilltop inflation.
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