How Neutron Star Observations Point Towards Exotic Matter: Existing Explanations and a Prospective Proposal

TL;DR

This paper explores how neutron star observations suggest the presence of exotic matter in their cores, proposing a new hybrid star model with a slow phase transition and a novel quark matter equation of state to reconcile observational constraints.

Contribution

It introduces a slow stable hybrid star configuration with a new non-CSS parametrization, aiming to better match neutron star observational data and dense matter microphysics constraints.

Findings

Neutron star observations favor exotic matter in cores.

The proposed hybrid star model can satisfy current observational constraints.

Significant tensions and open questions remain due to model assumptions.

Abstract

Multi-messenger astronomical observations of neutron stars, together with more precise calculations and constraints coming from dense matter microphysics, are generating tension with regard to equations of state models used to describe neutron star cores. Assuming an abrupt first-order phase transition with a slow conversion speed between phases, we propose different slow stable hybrid star configurations aiming to reconcile all current constraints simultaneously; within this framework, we also introduce a novel non-CSS parametrization to the quark matter equation of state and discuss its strengths and limitations. We analyze our model results in conjunction with a review of other relevant theoretical possibilities existing in the literature. We found that modern neutron star observations seem to favor the existence of some type of exotic matter in the neutron star cores; in particular, our slow stable hybrid star scenario remains a proposal capable of satisfying these constraints. However, due both to the existing skepticism regarding some of the adopted hypotheses in most extreme neutron star measurements and to the precise adjustment needed for the equation-of-state parameters, significant tension and open questions remain.