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arxiv: astro-ph/9407040 · v2 · submitted 1994-07-14 · 🌌 astro-ph · hep-ph

Mutated Hybrid Inflation

classification 🌌 astro-ph hep-ph
keywords modelinflationbecauseconfigurationcorrespondsdensitydescribedfields
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A new model of inflation is described. An unusual form for the inflationary potential is obtained because the inflaton corresponds to a non-trivial path in the configuration space of the two real scalar fields of the model. The model predicts a spectral index $n = 1 - 3/2N \simeq 0.97$ for the density perturbations and negligible gravitational waves.

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