Pith Number

pith:45G56QNP

pith:2025:45G56QNPN46UAG3ONI3CCJQOGP

not attested not anchored not stored refs resolved

Inferring neutron-star Love-Q relations from gravitational waves in the hierarchical Bayesian framework

Jinwen Deng, Lijing Shao, Yiming Dong, Zhihao Zheng, Ziming Wang

A linear relation in log space between tidal deformability and quadrupole moment describes the neutron-star Love-Q relation well enough for next-generation gravitational wave detectors.

arxiv:2510.22137 v2 · 2025-10-25 · gr-qc · astro-ph.HE

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Add to your LaTeX paper

\usepackage{pith}
\pithnumber{45G56QNPN46UAG3ONI3CCJQOGP}

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Record completeness

1 Bitcoin timestamp

2 Internet Archive

3 Author claim open · sign in to claim

4 Citations open

5 Replications open

✓ Portable graph bundle live · download bundle · merged state

The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same current state with the deterministic merge algorithm.

Claims

C1strongest claim

A linear relation between lnΛ and lnQ is practically sufficient to describe the Love-Q relation with the precision expected from next-generation GW detectors; the characteristic length in dynamical Chern-Simons gravity can be constrained to 10 km or less.

C2weakest assumption

The simulated gravitational wave signals and noise properties accurately represent what real detectors will observe, and the selection of the 20 highest-SNR events with highest NS spins does not introduce bias into the recovered relation parameters.

C3one line summary

Hierarchical Bayesian inference on 20 high-SNR simulated binary neutron star events shows a linear lnΛ-lnQ relation suffices and constrains dynamical Chern-Simons gravity length scale to ≤10 km.

References

106 extracted · 106 resolved · 59 Pith anchors

[1] L. Shao and K. Yagi, Sci. Bull.67, 1946 (2022), arXiv:2209.03351 [gr-qc] 1946

[2] The Massive Pulsar PSR J1614-2230: Linking Quantum Chromodynamics, Gamma-ray Bursts, and Gravitational Wave Astronomy 2010 · arXiv:1010.5790

[3] Equation of state and neutron star properties constrained by nuclear physics and observation 2013 · arXiv:1303.4662

[4] A Massive Pulsar in a Compact Relativistic Binary 2013 · arXiv:1304.6875

[5] Neutron Star Observations: Prognosis for Equation of State Constraints 2007 · arXiv:astro-ph/0612440

Formal links

2 machine-checked theorem links

Receipt and verification

First computed	2026-05-26T01:03:17.257995Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

e74ddf41af6f3d401b6e6a3621260e33ff1095007fc78d7963e68825d2c12bf1

Aliases

arxiv: 2510.22137 · arxiv_version: 2510.22137v2 · doi: 10.48550/arxiv.2510.22137 · pith_short_12: 45G56QNPN46U · pith_short_16: 45G56QNPN46UAG3O · pith_short_8: 45G56QNP

Agent API

Resolver JSON Graph JSON Events JSON Schema Signing key

Verify this Pith Number yourself

curl -sH 'Accept: application/ld+json' https://pith.science/pith/45G56QNPN46UAG3ONI3CCJQOGP \
  | 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: e74ddf41af6f3d401b6e6a3621260e33ff1095007fc78d7963e68825d2c12bf1

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "d6b6bfea05e61b9e307e07847eb70b7ce8a946fd2ee87d5cce01b6c58b5f7603",
    "cross_cats_sorted": [
      "astro-ph.HE"
    ],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "gr-qc",
    "submitted_at": "2025-10-25T03:18:25Z",
    "title_canon_sha256": "c0a0701e2013f45dc1b1aa262a8fec5f5b4c881de62aab7853ca5830b62cf9e0"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2510.22137",
    "kind": "arxiv",
    "version": 2
  }
}