pith:Y5HUBNJI
Massive hybrid stars within the extended three-flavor quark-meson diquark model
The extended three-flavor quark-meson diquark model produces hybrid stars with masses and radii matching observations when vector and axial-vector mesons are included.
arxiv:2605.05816 v2 · 2026-05-07 · hep-ph · astro-ph.HE · nucl-th
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We show that it is possible to construct hybrid stars whose masses and radii are in agreement with recent astrophysical observations and perturbative QCD (pQCD). The addition of vector and axial vector mesons to the quark-meson diquark is essential, since it makes the EoS sufficiently stiff for intermediate densities. Our results suggest that stars with a mass larger than M∼2M⊙ have a quark core with a central density nB≥3.9nsat.
The mean-field approximation at zero temperature together with the specific choice of model parameters that are adjusted to simultaneously match astrophysical observations, the low-density nuclear equation of state, and perturbative QCD constraints at high density.
Adding vector and axial-vector mesons to the extended quark-meson diquark model produces a sufficiently stiff equation of state to support hybrid stars above 2 solar masses with quark cores at central densities of at least 3.9 times nuclear saturation density.
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| First computed | 2026-06-01T01:02:41.759681Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
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c74f40b528d06f61c2c3a748d8b5c65715310967303784a0761b7a62aa94b6f4
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Canonical record JSON
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