Super Hilltop Inflation
arXiv:0812.2731 · doi:10.1088/1475-7516/2009/03/012
Abstract
In this paper, we consider logarithmic radiative corrections and higher order terms to the supersymmetric hilltop F- and D-term hybrid inflation models. Conventional F- and D-term hybrid inflation only predicts $n_s \gae 0.98$. We show that via a positive quadratic and a negative quartic correction the spectral index can be reduced to suggested from latest WMAP result and also cosmic string problem appeared in SUSY hybrid inflation can be solved with mild tuning of the parameters if $κ\lae 0.01$ for F-term inflation and $g \lae 0.05$ for D-term inflation.
12 pages, 8 figures, to be published in JCAP
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Cited by in corpus (22)
- Dark Matter Evidence, Particle Physics Candidates and Detection Methods
- Observable Spectra of Induced Gravitational Waves from Inflation
- Observable induced gravitational waves from an early matter phase
- Supersymmetric Hybrid Inflation Redux
- Gravitational production of super-Hubble-mass particles: an analytic approach
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- Kähler-driven Tribrid Inflation
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- Primordial non-Gaussianity in warm inflation using formalism
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- Reheating constraints on mutated hilltop inflation
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- Higher order terms in the inflaton potential and the lower bound on the tensor to scalar ratio r
- Large non-Gaussianity generated after D-term Inflation by Right-Handed Sneutrino Curvaton
- A double-running inflaton mass for a flat potential and an assisted hilltop inflation