Bianchi universes de-Sitterize under a general inflaton potential when its relative variation α stays below 1, and this bound rules out models with α > 1.
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Constraining inflationary models via de-Sitterization of Bianchi Cosmologies
Bianchi universes de-Sitterize under a general inflaton potential when its relative variation α stays below 1, and this bound rules out models with α > 1.