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We study the possibility that the approximate time shift symmetry during inflation is promoted to the full invariance under time reparametrization t \to \tilde t(t), or equivalently under field redefinition of the inflaton \phi \to \tilde\phi(\phi).
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A. Wang, D. Wands and R. Maartens, “Scalar field perturbations in Horava-Lifshitz cosmology,” JCAP
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