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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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Non-singular bounce scenarios in loop quantum cosmology and the effective field description

TL;DR: In this article, the authors compare the dynamics in loop quantum cosmology and in a non-singular bouncing effective field model with a nonstandard kinetic term at both the background and perturbative levels.
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An extended matter bounce scenario: current status and challenges

TL;DR: In this article, an extended model of the matter bounce cosmology is proposed, in which the universe has experienced a quasi-matter contracting phase with a variable background equation of state parameter.
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Hidden Negative Energies in Strongly Accelerated Universes

TL;DR: In this paper, it was shown that theories of cosmological acceleration which have equation of state, w, such that 1+w is small but positive may still secretly violate the null energy condition.
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Dynamical analysis of generalized Galileon cosmology

TL;DR: In this paper, a detailed dynamical analysis of generalized Galileon cosmology, incorporating also the requirements of ghost and instabilities absence, was performed, and it was shown that there are not any new stable late-time solutions apart from those of standard quintessence.
Journal ArticleDOI

The Effective Field Theory of nonsingular cosmology: II

TL;DR: Based on the Effective Field Theory (EFT) of cosmological perturbations, the authors explicitly clarified the pathology in nonsingular cubic Galileon models and showed how to cure it in EFT with new insights into this issue.
References
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Journal ArticleDOI

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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