Inflation inside non-topological defects and scalar black holes

TL;DR

This paper explores inflation phenomena inside non-topological defects and scalar black holes within a gravity-scalar-electromagnetic framework, revealing new inflationary behaviors in these non-topological structures.

Contribution

It introduces a non-topological counterpart to topological inflation, demonstrating inflation inside boson stars and scalar black holes in a unified Einstein-Maxwell-scalar model.

Findings

Inflation occurs inside boson stars with strong gravity.

Scalar black holes can develop inflationary regions.

The phenomenon extends topological inflation to non-topological objects.

Abstract

In this paper, we demonstrate that a phenomenon described as "topological inflation" during which inflation occurs inside the core of topological defects, has a non-topological counterpart. This appears in a simple set-up containing Einstein gravity coupled minimally to an electromagnetic field as well as a self-interacting, complex valued scalar field. The U(1) symmetry of the model is unbroken and leads to the existence of globally regular solutions, so-called boson stars, that develop a horizon for sufficiently strong gravitational coupling. We also find that the same phenomenon exists for black holes with scalar hair.