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Quantum corrections to gravity and their implications for cosmology and astrophysics

TLDR
The quantum contributions to the gravitational action are relatively easy to calculate in the higher derivative sector of the theory as mentioned in this paper, however, the applications to the post-inflationary cosmology and astrophysics require the corrections to the Einstein-Hilbert action and to the cosmological constant, and those we can not derive yet in a consistent and safe way.
Abstract
The quantum contributions to the gravitational action are relatively easy to calculate in the higher derivative sector of the theory. However, the applications to the post-inflationary cosmology and astrophysics require the corrections to the Einstein-Hilbert action and to the cosmological constant, and those we can not derive yet in a consistent and safe way. At the same time, if we assume that these quantum terms are covariant and that they have relevant magnitude, their functional form can be defined up to a single free parameter, which can be defined on the phenomenological basis. It turns out that the quantum correction may lead, in principle, to surprisingly strong and interesting effects in astrophysics and cosmology.

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Inflation with an antisymmetric tensor field

TL;DR: In this paper, the authors investigate the possibility of inflation with models of antisymmetric tensor field having minimal and non-minimal couplings to gravity, and they find that the nonminimal models, through the introduction of a nonminical coupling to gravity can give rise to stable de-Sitter solutions with a bound on the coupling parameters.
References
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Journal ArticleDOI

The Cosmological Constant Problem

TL;DR: In this article, five different approaches to the cosmological constant problem are described, and a brief review of the history of this problem is given. But none of the approaches are considered in this paper.
Journal ArticleDOI

Infrared Singularities and Massive Fields

TL;DR: In this paper, it is shown in the context of a simple model of gauge mesons coupled to massive fermions that the heavy fields decouple at low momenta except for their contribution to renormalization effects.
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Renormalizable asymptotically free quantum theory of gravity

TL;DR: In this paper, it was shown that higher derivative quantum gravity is asymptotically free in all essential coupling constants by the calculation of one-loop counterterms and the solution of the corresponding renormalization group (RG) equations.
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The cored distribution of dark matter in spiral galaxies

TL;DR: In this article, a new method for extracting rotation curves from Hi data cubes is presented; this method takes into account the existence of a warp and minimises projection effects; the rotation curves obtained are tested by taking them as input to construct model data cubes that are compared to the observed ones.
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