Pith. sign in

REVIEW 4 cited by

Phase Transitions in Neutron Stars

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 1901.03252 v1 pith:GGJHBTAR submitted 2019-01-10 astro-ph.HE hep-phnucl-th

V. Dexheimer , L. T. T. Soethe , J. Roark , R. O. Gomes , S. O. Kepler , S. Schramm This is my paper · ORCID
classification astro-ph.HEhep-phnucl-th
keywords phasestarstransitionscorematterneutronassociatedcalculate
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

In this paper we review the most common descriptions for the first order phase transition to deconfined quark matter in the core of neutron stars. We also present a new description of these phase transitions in the core of proto-neutron stars, in which more constraints are enforced so as to include trapped neutrinos. Finally, we calculate the emission of gravitational waves associated with deconfinement phase transitions, discuss the possibility of their detection, and how this would provide information about the equation of state of dense matter.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 4 Pith papers

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

  1. Globally Charged Vacuum Decay

    hep-ph 2026-06 unverdicted novelty 7.0 of 10

    For a U(1)-charged scalar, the Euclidean bounce for vacuum decay loses O(4) symmetry at finite charge, lowers the barrier and increases the rate, while charge rearrangement imposes a subluminal terminal velocity on th...

  2. How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition

    astro-ph.HE 2026-08 conditional novelty 6.0 of 10

    A Bayesian analysis of mock neutron star radius measurements shows that precision radii mainly constrain the symmetry-energy parameters L and Ksym and the quark transition density, while transition strength and quark ...

  3. Probing up-down quark matter via gravitational waves

    astro-ph.HE 2019-08 conditional novelty 5.0 of 10

    Up-down quark stars in the two-families scenario yield tidal deformabilities compatible with GW170817, constraining the effective bag constant to approximately 50 MeV/fm^3.

  4. Quantifying the Information Gain from Future High-Precision Radius Measurements for Identifying Twin Neutron Stars

    astro-ph.HE 2026-07 reject novelty 4.0 of 10

    The paper claims a radius precision of ~0.2 km is enough to extract most Bayesian information for identifying twin neutron stars, but its own distinguishability and entropy analyses suggest notable gains remain down t...

Pith tools