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Galilean Genesis: An Alternative to inflation

TLDR
In this paper, a cosmological scenario is proposed, in which standard inflation is replaced by an expanding phase with a drastic violation of the Null Energy Condition (NEC): the model is based on the recently introduced Galileon theories, which allow NEC violating solutions without instabilities.
Abstract
We propose a novel cosmological scenario, in which standard inflation is replaced by an expanding phase with a drastic violation of the Null Energy Condition (NEC): >> H2. The model is based on the recently introduced Galileon theories, which allow NEC violating solutions without instabilities. The unperturbed solution describes a Universe that is asymptotically Minkowski in the past, expands with increasing energy density until it exits the regime of validity of the effective field theory and reheats. This solution is a dynamical attractor and the Universe is driven to it, even if it is initially contracting. The study of perturbations of the Galileon field reveals some subtleties, related to the gross violation of the NEC and it shows that adiabatic perturbations are cosmologically irrelevant. The model, however, suggests a new way to produce a scale invariant spectrum of isocurvature perturbations, which can later be converted to adiabatic: the Galileon is forced by symmetry to couple to the other fields as a dilaton; the effective metric it yields on the NEC violating solution is that of de Sitter space, so that all light scalars will automatically acquire a nearly scale-invariant spectrum of perturbations.

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Modified Gravity and Cosmology

TL;DR: A comprehensive survey of recent work on modified theories of gravity and their cosmological consequences can be found in this article, where the authors provide a reference tool for researchers and students in cosmology and gravitational physics, as well as a selfcontained, comprehensive and up-to-date introduction to the subject as a whole.
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Massive Gravity

TL;DR: In this paper, a review of recent progress in massive gravity is presented, showing how different theories of massive gravity emerge from a higher-dimensional theory of general relativity, leading to the Dvali-Gabadadze-Porrati model, cascading gravity and ghost-free massive gravity.
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Beyond the cosmological standard model

TL;DR: A review of the state of the art in the field of modified gravity can be found in this article, where the authors identify the guiding principles for rigorous and consistent modifications of the standard model, and discuss the prospects for empirical tests.
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Imperfect Dark Energy from Kinetic Gravity Braiding

TL;DR: In this paper, the authors introduce a large class of scalar-tensor models with interactions containing the second derivatives of the scalar field but not leading to additional degrees of freedom.
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Beyond the Cosmological Standard Model

TL;DR: A review of the current state of the field and a framework for anticipating developments in the next decade can be found in this paper, where the authors identify the guiding principles for rigorous and consistent modifications of the standard model, and discuss the prospects for empirical tests.
References
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Journal ArticleDOI

Non-Gaussian features of primordial fluctuations in single field inflationary models

TL;DR: In this article, the three point correlation functions for primordial scalar and tensor fluctuations in single field inflationary models were computed in the slow roll limit, where the answer is given terms of the two usual slow roll parameters.
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Galileon as a local modification of gravity

TL;DR: In this article, the authors study the connection between self-acceleration and the presence of ghosts for a quite generic class of theories that modify gravity in the infrared, defined as those that at distances shorter than cosmological, reduce to a certain generalization of the Dvali-Gabadadze-Porrati (DGP) effective theory.
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Generating the curvature perturbation without an inflaton

TL;DR: In this article, the curvaton is light during a period of cosmological inflation, when it acquires a perturbation with an almost scale-invariant spectrum.
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The Effective Field Theory of Inflation

TL;DR: The effective field theory of inflation as discussed by the authors is the most general theory describing the fluctuations around a quasi de Sitter background, in the case of single field models, in which the scalar mode can be eaten by the metric by going to unitary gauge.
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Causality, analyticity and an IR obstruction to UV completion

TL;DR: In this paper, it was shown that low-energy effective field theories described by local, Lorentz invariant Lagrangians, secretly exhibit macroscopic non-locality and cannot be embedded in any UV theory whose S-matrix satisfies canonical analyticity constraints.
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