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Hybrid Equations of State for Neutron Stars with Hyperons and Deltas

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arxiv 2205.00559 v1 pith:6LQFTGV6 submitted 2022-05-01 astro-ph.HE astro-ph.SRnucl-th

A. Clevinger , J. Corkish , K. Aryal , V. Dexheimer This is my paper · ORCID
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keywords equationsstatehybridcontainhyperonsneutronstarsapplications
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In this contribution, we describe new chemically-equilibrated charge-neutral hybrid equations of state for neutron stars. They present a first-order phase transition to quark matter and differentiate by the particle population considered and how these particles interact. While some equations of state contain just nucleons and up, down-quarks, others also contain hyperons, Delta baryons, and strange quarks. The hybrid equations of state, together with corresponding hadronic ones, are available on the CompOSE repository and can be used for different astrophysical applications.

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  1. Astrophysical Constraints on Hadron--Quark Crossover in Hybrid Neutron Stars

    astro-ph.HE 2026-08 conditional novelty 5.0 of 10

    A Bayesian analysis of smooth hadron-quark crossover neutron stars using NICER and GW170817 data favors a broad, high-density mixed transition, disfavors pure quark cores, and makes a neutron-star interpretation of GW...

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