pith:FHB7UHGT
Maximal mass of neutron stars constrained by neutron star observations
Neutron star observations constrain the maximum mass to 2.2-2.3 solar masses with weak dependence on the baseline equation of state.
arxiv:2605.00437 v2 · 2026-05-01 · astro-ph.HE · hep-ph · nucl-th
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Claims
We find that the maximum-mass distributions are largely determined by observational constraints and show only weak sensitivity to the choice of baseline EOS, favoring values around 2.2-2.3 M⊙ when the most robust constraints are applied.
That the constructed families of causal hybrid EOSs, obtained by matching baseline hadronic models to an extended linear sigma model and enforcing pQCD asymptotics, adequately span the physically allowed high-density behavior without missing important phase transitions or other degrees of freedom.
Bayesian analysis of causal hybrid EOS models constrained by neutron-star observations favors a maximum mass of 2.2-2.3 solar masses with radius near 12 km, largely independent of the hadronic baseline.
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Receipt and verification
| First computed | 2026-07-09T01:20:05.144639Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
29c3fa1cd3a3433ae149ee2936b6dcdc411227ce94ca3a509d8c85285d4ea717
Aliases
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Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/FHB7UHGTUNBTVYKJ5YUTNNW43R \
| 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: 29c3fa1cd3a3433ae149ee2936b6dcdc411227ce94ca3a509d8c85285d4ea717
Canonical record JSON
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