Can a slow and strong phase transition in neutron stars relieve major compact-star observation tensions?
astro-ph.HE, gr-qc, hep-ph, nucl-th
Submitted: 2026-06-15
Updated: 2026-10-10
Terminology
Sources
- Evidence for quark-matter cores in massive neutron stars
- Strongly interacting matter exhibits deconfined behavior in massive neutron stars
- Trace anomaly as signature of conformality in neutron stars
- First-order phase transitions in the cores of neutron stars
- XTE J1814-338: A potential hybrid star candidate
- Strange stars admixed with mirror dark matter: confronting observations of XTE J1814-338
- Macroscopic properties of the XTE J1814-338 as a dark matter admixed strange star
- How Neutron Star Observations Point Towards Exotic Matter: Existing Explanations and a Prospective Proposal
- Bayesian Inference of Dense-Matter Equations of State from Small-Radius Compact Stars with Twin-Star Scenarios
- A model-agnostic analysis of hybrid stars with reactive interfaces
- A Massive Pulsar in a Compact Relativistic Binary
- Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar
- Self-bound hybrid stars with strong phase transitions can relieve major compact star observation tensions
- Hybrid Quark Stars with Quark-Quark Phase Transitions
- Hybrid stars may have an inverted structure
- Radial and Non-Radial Oscillations of Inverted Hybrid Stars
- Rotational Properties of Inverted Hybrid Stars
- Hybrid Strangeon Stars
- Self-bound quark stars with a first-order two-to-three flavor phase transition
- Probing up-down quark matter via gravitational waves
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