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Null energy condition and superluminal propagation

TLDR
In this paper, the null energy condition is violated in a large class of situations, including isotropic solids and fluids relevant for cosmology, and the existence of superluminal modes is shown to imply the presence of instabilities.
Abstract
We study whether a violation of the null energy condition necessarily implies the presence of instabilities. We prove that this is the case in a large class of situations, including isotropic solids and fluids relevant for cosmology. On the other hand we present several counter-examples of consistent effective field theories possessing a stable background where the null energy condition is violated. Two necessary features of these counter-examples are the lack of isotropy of the background and the presence of superluminal modes. We argue that many of the properties of massive gravity can be understood by associating it to a solid at the edge of violating the null energy condition. We briefly analyze the difficulties of mimicking u H > 0 in scalar tensor theories of gravity.

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Cosmological and astrophysical observables from field theory in curved backgrounds

TL;DR: In this paper, the authors introduce tools for the evaluation of (a) the observational consistency of an effective field theory of gravity, and (b) the potential modifications of theories equipped with diffeomorphism invariance.
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Wormhole modeling in $R^2$ gravity with linear trace term

TL;DR: In this paper, the modification of general relativity (in particular, the theory of gravity defined by Harko et al. ) is considered, to study the traversable wormhole solutions.
Journal ArticleDOI

Construction of the conserved ζ via the effective action for perfect fluids

TL;DR: In this article, the curvature perturbation γ i j is conserved outside the horizon in the same manner as γ is. But the authors focus on the case where the existence of such conserved ζ is guaranteed: a universe dominated by a perfect fluid with adiabatic pressure.
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Fluids, Superfluids and Supersolids: Dynamics and Cosmology of Self Gravitating Media

TL;DR: In this article, cosmological perturbations for a generic self-gravitating media described by four derivatively-coupled scalar fields are computed. But the authors focus on the dark sector.
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Reissner–Nordström and Charged Gas Spheres

TL;DR: In this article, the authors proposed to treat the photon gas as part of the dynamics of a polytropic stellar system, in which the mass distribution extends to infinity, the boundary between bulk and atmosphere being defined by an abrupt change in the poly-tropic index, triggered by the density.
References
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Book

The Large Scale Structure of Space-Time

TL;DR: In this paper, the authors discuss the General Theory of Relativity in the large and discuss the significance of space-time curvature and the global properties of a number of exact solutions of Einstein's field equations.
Book

General Relativity

Robert Wald
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.
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