pith:WJCVWMAS
The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover
Non-parametric equation of state construction reveals early stiffening followed by softening in massive neutron stars.
arxiv:2605.08584 v2 · 2026-05-09 · astro-ph.HE · gr-qc · nucl-th
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Claims
By measuring the degree of this non-monotonic behavior in the posterior, we find evidence for a hadron-quark phase transition in the cores of the most massive neutron stars. This indicates that the non-perturbative quark matter is intrinsically soft, fundamentally distinguishing it from the stiff scenarios associated with the quark-star picture.
The global thermodynamic constraint is driven by the observationally required stiffening to support two-solar-mass neutron stars with relatively small radii for low-mass neutron stars, combined with the requirement not to overshoot perturbative QCD energy-density bounds.
Non-parametric EOS construction shows non-conformal behavior with evidence for soft quark matter and a hadron-quark phase transition in massive neutron star cores.
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Receipt and verification
| First computed | 2026-06-05T00:13:46.873394Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b2455b30129fd98ed09138020d6b018571cc9186c2ad4eaf4c64c907c082a3d7
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/WJCVWMAST7MY5UERHABA22YBQV \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: b2455b30129fd98ed09138020d6b018571cc9186c2ad4eaf4c64c907c082a3d7
Canonical record JSON
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"license": "http://creativecommons.org/publicdomain/zero/1.0/",
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