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Topological $R^4$ Inflation

John Ellis·Nemanja Kaloper·Keith A. Olive·Jun'ichi Yokoyama
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Abstract

We consider the possibility that higher-curvature corrections could drive inflation after the compactification to four dimensions. Assuming that the low-energy limit of the fundamental theory is eleven-dimensional supergravity to the lowest order, including curvature corrections and taking the descent from eleven dimensions to four via an intermediate five-dimensional theory, as favored by recent considerations of unification at some scale around $\sim 10^{16}$ GeV, we may obtain a simple model of inflation in four dimensions. The effective degrees of freedom are two scalar fields and the metric. The scalars arise as the large five-dimensional modulus and the self-interacting conformal mode of the metric. The effective potential has a local maximum in addition to the more usual minimum. However, the potential is quite flat at the top, and admits topological inflation. We show that the model can resolve cosmological problems and provide a mechanism for structure formation with very little fine tuning.

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John Ellis, Nemanja Kaloper, Keith A. Olive, Jun'ichi Yokoyama. 1999-01-29. Topological $R^4$ Inflation. https://doi.org/10.1103/physrevd.59.103503

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