Breaking of spatial diffeomorphism invariance, inflation and the spectrum of cosmological perturbations

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Abstract

Standard inflationary models yield a characteristic signature of a primordial power spectrum with a red tensor and scalar tilt. Nevertheless, Cannone et al. [1] recently suggested that, by breaking the assumption of spatial diffeomorphism invariance in the context of the effective field theory of inflation, a blue tensor spectrum can be achieved without violating the Null Energy Condition. In this context, we explore in which cases the inflationary model of [2] can yield a blue tilt of the tensor modes along with a red tilt in the scalar spectrum. Ultimately, we analyze under which conditions the model of [3] can reproduce the specific consistency relation of String Gas Cosmology.

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Graef, L. L., & Brandenberger, R. (2015). Breaking of spatial diffeomorphism invariance, inflation and the spectrum of cosmological perturbations. Journal of Cosmology and Astroparticle Physics, 2015(10). https://doi.org/10.1088/1475-7516/2015/10/009

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