Extended Effective Field Theory of Inflation
arXiv:1802.03040 · doi:10.1007/JHEP02(2018)172
Abstract
We present a general framework where the effective field theory of single field inflation is extended by the inclusion of operators with mass dimension 3 and 4 in the unitary gauge. These higher dimensional operators introduce quartic and sextic corrections to the dispersion relation. We study the regime of validity of this extended effective field theory of inflation and the effect of these higher dimensional operators on CMB observables associated with scalar perturbations, such as the speed of sound, the amplitude of the power spectrum and the tensor-to-scalar ratio. Tensor perturbations remain instead, unaltered.
new version matches the published version, includes adding few citations and correcting few typos
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- Formation and Abundance of Late Forming Primordial Black Holes as Dark Matter
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- Non-Minimal M-flation
- Inflationary Cosmology with Quantum Gravitational Effects and the Swampland Conjectures
- Constraining Violations of the Weak Equivalence Principle in the Dark Sector
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- Cosmological perturbation theory with trinity of scalar fields