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Introduction to modified gravity and gravitational alternative for dark energy

TLDR
In this paper, a review of modified gravities considered as a gravitational alternative for dark energy is presented, and the possibility to explain the coincidence problem as the manifestation of the universe expansion in such models is mentioned.
Abstract: 
We review various modified gravities considered as gravitational alternative for dark energy. Specifically, we consider the versions of f(R), f(G) or f(R, G) gravity, model with non-linear gravitational coupling or string-inspired model with Gauss-Bonnet-dilaton coupling in the late universe where they lead to cosmic speed-up. It is shown that some of such theories may pass the Solar System tests. On the same time, it is demonstrated that they have quite rich cosmological structure: they may naturally describe the effective (cosmological constant, quintessence or phantom) late-time era with a possible transition from decceleration to acceleration thanks to gravitational terms which increase with scalar curvature decrease. The possibility to explain the coincidence problem as the manifestation of the universe expansion in such models is mentioned. The late (phantom or quintessence) universe filled with dark fluid with inhomogeneous equation of state (where inhomogeneous terms are originated from the modifi...

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Journal ArticleDOI

f ( R ) theories of gravity

TL;DR: In this article, the authors present a review of the most important aspects of the different classes of modified gravity theories, including higher-order curvature invariants and metric affine.
Journal ArticleDOI

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.
Journal ArticleDOI

f(R) theories

TL;DR: Various applications of f(R) theories to cosmology and gravity — such as inflation, dark energy, local gravity constraints, cosmological perturbations, and spherically symmetric solutions in weak and strong gravitational backgrounds are reviewed.
Journal ArticleDOI

Extended Theories of Gravity

TL;DR: Extended Theories of Gravity as discussed by the authors can be considered as a new paradigm to cure shortcomings of General Relativity at infrared and ultraviolet scales, which is an approach that, by preserving the undoubtedly positive results of Einstein's theory, is aimed to address conceptual and experimental problems recently emerged in astrophysics, cosmology and High Energy Physics.
Journal ArticleDOI

$f(R,T)$ gravity

TL;DR: In this article, the authors considered a modified theory of gravity, where the gravitational Lagrangian is given by an arbitrary function of the Ricci scalar and of the trace of the stress-energy tensor.
References
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Journal ArticleDOI

Cosmological constant—the weight of the vacuum

TL;DR: A review of cosmological constants can be found in this paper, where the authors discuss several aspects of the Cosmological Constant problem from both cosmology and theoretical perspectives.
Journal ArticleDOI

Modified gravity with negative and positive powers of curvature: Unification of inflation and cosmic acceleration

TL;DR: A modified gravity, which eliminates the need for dark energy and which seems to be stable, is considered in this article, where the terms with positive powers of curvature support the inflationary epoch while the terms that serve as effective dark energy, supporting current cosmic acceleration.
Journal ArticleDOI

Properties of singularities in the (phantom) dark energy universe

TL;DR: In this paper, the properties of future singularities are investigated in the universe dominated by dark energy including the phantom-type fluid. And the authors classify the finite-time singularities into four classes and explicitly present the models which give rise to these singularities by assuming the form of the equation of state of dark energy.
Book

Effective Action in Quantum Gravity

TL;DR: In this paper, the renormalization group method in curved space-time with torsion was used to solve the problem of quantum field theory in a curved space time and effective action.
Journal ArticleDOI

Late-time cosmology in (phantom) scalar-tensor theory: dark energy and the cosmic speed-up

TL;DR: In this article, the authors considered late-time cosmology in a (phantom) scalar-tensor theory with an exponential potential, as a dark energy model with equation of state parameter close to -1 (a bit above or below this value).
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