A metric on the space of neutron star models in general relativity and modified gravity

TL;DR

This paper introduces a geometric distance measure on the space of neutron star models in general relativity and modified gravity, enabling quantitative comparison of stellar models based on their metrics.

Contribution

It develops a mathematical formalism to define a Riemannian metric on the space of neutron star models, facilitating quantitative analysis of their similarities and differences.

Findings

Constructed a configuration manifold for neutron star models

Provided examples illustrating the use of the metric in stellar structure analysis

Established a foundation for future studies on neutron star model comparison

Abstract

Some pairs of neutron star models can intuitively be thought of as being `closer' together than others, in the sense that more precise observations might be required to distinguish between them than would be necessary for other pairs. In this paper, borrowing ideas from the study of geometrodynamics, we introduce a mathematical formalism to define a geometric distance between stellar models, to provide a quantitative meaning to this notion of closeness. In particular, it is known that the set of all metrics on a Riemannian manifold itself admits the structure of a Riemannian manifold (`configuration manifold'), which comes equipped with a canonical metric. By thinking of a stationary star as being a particular $3+1$ metric, the structure of which is determined through the Tolman-Oppenheimer-Volkoff relations and their generalisations, points on a suitably restricted configuration manifold can be thought of as representing different stars, and distances between these points can be computed. We develop the necessary mathematical machinery to build the configuration manifold of neutron star models, and provide some worked examples to illustrate how this space might be used in future studies of stellar structure.