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We consider a scenario in which the inflaton $\phi$ is a pseudoscalar field non-minimally coupled to gravity through a term of the form ${\cal X} R \phi^2$.
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C. Germani and A. Kehagias, UV-Protected Inflation , Phys. Rev. Lett. 106
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2012
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2012
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K. Dimopoulos and M. Karciauskas, Parity Violating Statistical Anisotropy , JHEP 06
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2013
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2013
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2013
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R. Kallosh and A. Linde, Universality Class in Conformal Inflation , JCAP 1307
2013
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R. Kallosh and A. Linde, Non-minimal Inflationary Attractors , JCAP 1310
2013
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2017
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T. Tenkanen, Resurrecting Quadratic Inflation with a non-minimal coupling to gravity , JCAP 1712
2017
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V. Domcke, F. Muia, M. Pieroni and L. T. Witkowski, PBH dark matter from axion inflation , JCAP 1707
2017
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