pith:FLM44QBS
Universal Relations with Dynamical Tides
Quasi-universal relations connect the static tidal deformability of neutron stars to its leading dynamical correction with at most 5 percent equation-of-state variation.
arxiv:2511.19626 v2 · 2025-11-24 · gr-qc · nucl-th
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Claims
We identify new quasi-universal relations between the static, dimensionless tidal deformability (Λ⁰) and its leading-order dynamical correction (Λ²), as well as between Λ⁰ and √(Λ⁰/Λ²) ≡ Mω*, ... the equation-of-state dependence does not exceed ∼5% for the Λ⁰–Λ² relation and ∼2.8% for the Λ⁰–Mω* relation.
That the 59 chosen equations of state form a representative sample and that the small-frequency expansion remains accurate in the relevant regime for binary neutron-star inspirals.
New quasi-universal relations connect static tidal deformability Λ⁰ to its dynamical correction Λ² and to Mω* with equation-of-state scatter below 5% and 2.8% respectively across 59 models.
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| First computed | 2026-05-18T03:09:32.953444Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/FLM44QBSVHUEICURFR55T3A7BL \
| jq -c '.canonical_record' \
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Canonical record JSON
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