Some Observable Effects of Modified Gravity in Cosmology and Astrophysics

TL;DR

This thesis explores observable effects of modified gravity theories in cosmology and astrophysics, including early universe dynamics, singularity formation, and gravitational repulsion, offering insights into alternative gravity models.

Contribution

It provides new analyses of $R^2$ gravity effects, singularity prevention mechanisms, and gravitational repulsion phenomena in astrophysical contexts.

Findings

Radiation-dominated epoch behavior in $R^2$ gravity

Mechanisms for preventing curvature singularities

Potential for gravitational repulsion in spherically symmetric solutions

Abstract

In Chapter 1 I present the current picture of the universe and briefly review the cosmological constant problem and some of the theories proposed to solve it. The following Chapters essentially contain the published papers with some modifications and additions: in Chapter 2 I study the radiation-dominated epoch in $R^2$ gravity, gravitational particle production and its implications for the early and contemporary universe; in Chapter 3 I investigate the formation of curvature singularities in contracting astronomical systems; in Chapter 4, I discuss some mechanisms to prevent such singularities and calculate the related cosmic-ray production; finally, in Chapter 5, I deal with spherically symmetric solutions and explore the possibility of gravitational repulsion.