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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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Galileons in the Sky

TL;DR: The existence of a non-renormalization theorem for Galileon scalar fields makes them especially attractive candidates for inflation as well as for late-time acceleration in braneworld models as mentioned in this paper.
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Stability of the Einstein static universe in f ( R , T ) gravity

TL;DR: In this article, the existence and stability of an ES universe in the context of f(R, T) modified theories of gravity is studied. And the authors suggest that modifications in f(T, R) gravity would lead to stable solutions which are unstable in f (R) gravity model and also investigate homogeneous scalar perturbations for the mentioned models.
Journal ArticleDOI

Two Field Matter Bounce Cosmology

TL;DR: In this article, the authors re-examine the non-singular matter bounce scenario and study the evolution of both curvature and entropy fluctuations through the bounce, and show that both have a scale-invariant spectrum which is blue-tilted on small scales.
Journal ArticleDOI

Evolution of cosmological perturbations and the production of non-Gaussianities through a nonsingular bounce: Indications for a no-go theorem in single field matter bounce cosmologies

TL;DR: In this article, the authors studied the dynamics of the cosmological perturbations evolving through a nonsingular bouncing phase described by a generic single scalar field Lagrangian minimally coupled to Einstein gravity.
Journal ArticleDOI

Unbraiding the bounce: superluminality around the corner

TL;DR: In this paper, the cosmological bounce solution of Ijjas and Steinhardt was studied and the exact structure of the Lagrangian was reconstructed for a possible UV-completion.
References
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Journal ArticleDOI

Dynamics of dark energy

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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.
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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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