From Quark Matter to Strange Machos

TL;DR

This paper explores the diverse equilibrium configurations of strange-matter stars, revealing complex properties and potential observable low-mass objects like strange dwarfs and planetary-mass stars, which could be detected via microlensing.

Contribution

It provides a comprehensive analysis of strange-matter star sequences, introducing new stable categories and low-mass objects not previously characterized.

Findings

Identification of two distinct stable strange dwarf categories.

Prediction of very-low-mass strange stellar objects comparable to planets.

Potential detectability of these objects through gravitational microlensing.

Abstract

This paper gives an overview of the properties of all possible equilibrium sequences of compact strange-matter stars with nuclear crusts, which range from strange stars to strange dwarfs. In contrast to their non-strange counterparts, --neutron stars and white dwarfs--, their properties are determined by two (rather than one) parameters, the central star density and the density at the base of the nuclear crust. This leads to stellar strange-matter configurations whose properties are much more complex than those of the conventional sequence. As an example, two generically different categories of stable strange dwarfs are found, which could be the observed white dwarfs. Furthermore we find very-low-mass strange stellar objects, with masses as small as those of Jupiter or even lighter planets. Such objects, if abundant enough in our Galaxy, should be seen by the presently performed gravitational microlensing searches.