Cooling of hybrid neutron stars with microscopic equations of state

and D. Zappal\`a; G. F. Burgio; H.-J. Schulze; J.-B. Wei

REVIEW

Cooling of hybrid neutron stars with microscopic equations of state

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 2003.08079 v1 pith:Q57OPHM2 submitted 2020-03-18 nucl-th astro-ph.HEastro-ph.SR

J.-B. Wei , G. F. Burgio , H.-J. Schulze , and D. Zappalà This is my paper · ORCID

classification nucl-thastro-ph.HEastro-ph.SR

keywords neutroncoolingdifferenthybridmicroscopicmodelsstarsstate

verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments

read the original abstract

We model the cooling of hybrid neutron stars combining a microscopic nuclear equation of state in the Brueckner-Hartree-Fock approach with different quark models. We then analyze the neutron star cooling curves predicted by the different models and single out the preferred ones. We find that the possibility of neutron p-wave pairing can be excluded in our scenario.

Discussion (0). Continue with ORCID to comment.

Pith tools