Journal
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Volume -, Issue 12, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2007/12/004
Keywords
inflation; cosmology of theories beyond the SM; physics of the early universe; power spectrum
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Using analytic expressions, we explore the parameter space for hilltop inflation models with a potential of the form V-0 +/- m(2)phi(2) - a phi(p). With the positive sign and p > 2 this converts the original hybrid inflation model into a hilltop model, allowing the spectral index to agree with the observed value n = 0.95. In some cases the observed value is theoretically favored, while in others there is only the generic prediction |n-1| less than or similar to 1.
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