Neutron Star Structure with Hyperons and Quarks

G. F. Burgio; H.-J. Schulze (INFN Sezione di Catania; Italy); M. Baldo

Neutron Star Structure with Hyperons and Quarks

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv astro-ph/0312446 v1 pith:A4Z3ZTRT submitted 2003-12-17 astro-ph nucl-th

M. Baldo , G. F. Burgio , H.-J. Schulze (INFN Sezione di Catania , Italy) This is my paper · ORCID

classification astro-phnucl-th

keywords hyperonsmatterneutronparticularquarkstarsapproachattention

verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments

read the original abstract

We discuss the high-density nuclear equation of state within the Brueckner-Hartree-Fock approach. Particular attention is paid to the effects of nucleonic three-body forces, the presence of hyperons, and the joining with an eventual quark matter phase. The resulting properties of neutron stars, in particular the mass-radius relation, are determined. It turns out that stars heavier than 1.3 solar masses contain necessarily quark matter.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

First-order phase transition from hypernuclear matter to deconfined quark matter obeying new constraints from compact star observations
nucl-th 2019-08 conditional novelty 6.0 of 10

A hybrid neutron star model with an intermediate hypernuclear shell and a stiff color-superconducting quark core can reach 2.2 solar masses and satisfies current mass and radius constraints.

Pith tools