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Bouncing Galileon Cosmologies

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TLDR
In this article, nonsingular, homogeneous and isotropic bouncing solutions of the conformal Galileon model were presented, and it was shown that such solutions necessarily begin with a radiation-dominated contracting phase.
Abstract
We present nonsingular, homogeneous and isotropic bouncing solutions of the conformal Galileon model. We show that such solutions necessarily begin with a radiation-dominated contracting phase. This is followed by a quintom scenario in which the background equation of state crosses the cosmological constant boundary allowing for a nonsingular bounce which in turn is followed by Galilean Genesis. We analyze the spectrum of cosmological perturbations in this background. Our results show that the fluctuations evolve smoothly and without any pathology, but the adiabatic modes form a blue tilted spectrum. In order to achieve a scale-invariant primordial power spectrum as required by current observations, we introduce a light scalar field coupling to the Galileon kinetically. We find two couplings which yield a scale-invariant spectrum, one of which requires a fine tuning of the initial conditions. This model also predicts a blue tilted spectrum of gravitational waves stemming from quantum vacuum fluctuations in the contracting phase.

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From Satisfying to Violating the Null Energy Condition

TL;DR: In this paper, the authors construct a theory that admits a time-dependent solution smoothly interpolating between a null energy condition (NEC)-satisfying phase at early times and a NEC-violating phase at late times.
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When Matter Matters

TL;DR: In this article, it was shown that without any other matter present in the spatially flat Friedmann universe, the perturbations of the Galileon scalar field propagate with a speed at most equal to the speed of light.
Journal ArticleDOI

DBI Realizations of the Pseudo-Conformal Universe and Galilean Genesis Scenarios

TL;DR: The pseudo-conformal universe as discussed by the authors is an alternative to inflation in which the early universe is described by a conformal field theory on approximately flat space-time, and the fields develop time-dependent expectation values, spontaneously breaking the conformal symmetries to a de Sitter subalgebra.
Journal ArticleDOI

The Paths of Gravity in Galileon Cosmology

TL;DR: In this paper, the authors explore three classes of Galileon models: standard uncoupled, linearly or derivatively coupled to matter, and investigate the expansion history with particular attention to early time and late time attractors, as well as linear perturbations.
Journal ArticleDOI

Note on the production of scale-invariant entropy perturbation in the Ekpyrotic universe

TL;DR: In this paper, the authors considered the stable production of the scale-invariant entropy perturbation in the Ekpyrotic universe via non-minimal couplings.
References
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Dynamics of dark energy

TL;DR: In this article, the authors review the observational evidence for the current accelerated expansion of the universe and present a number of dark energy models in addition to the conventional cosmological constant, paying particular attention to scalar field models such as quintessence, K-essence and tachyon.
Journal ArticleDOI

Cosmological imprint of an energy component with general equation of state

TL;DR: In this article, the authors examine the possibility that a significant component of the energy density of the universe has an equation of state different from that of matter, radiation, or cosmological constant.
Journal ArticleDOI

4D Gravity on a Brane in 5D Minkowski Space

TL;DR: In this article, the authors propose a mechanism by which four-dimensional Newtonian gravity emerges on a 3-brane in 5D Minkowski space with an infinite size extra dimension.
Book

Theory of Cosmological Perturbations

TL;DR: In this paper, the authors present in a manifestly gauge-invariant form the theory of classical linear gravitational perturbations in part I, and a quantum theory of cosmological perturbation in part II.
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