Kinetically modified non-minimal inflation with exponential frame function
Abstract We consider supersymmetric (SUSY) and non-SUSY models of chaotic inflation based on the $$\phi ^n$$ ϕ n potential with $$n=2$$ n = 2 or 4. We show that the coexistence of an exponential non-minimal coupling to gravity $$f_\mathcal{R}=\mathrm{e}^{c_\mathcal{R}\phi ^{p}}$$ f R = e c R ϕ p wit...
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| Format: | Article |
| Language: | English |
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SpringerOpen
2017-09-01
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| Series: | European Physical Journal C: Particles and Fields |
| Online Access: | http://link.springer.com/article/10.1140/epjc/s10052-017-5165-2 |