Paper Citation Record · LEDGER

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides

As of 11 August 2026, this Paper Citation Record lists 100 of 129 outbound references and 5 inbound Pith citation observations for arXiv:2501.13064.

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2501.13064 v2

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measured 100 of 129 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-10T16:33:20.174351Z

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

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Source: paper_references, paper_reference_links, observed 2026-08-10T10:40:00.398819Z

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Source: pith, observed 2026-07-10T15:07:19.518197Z

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100 of 129 outbound references displayed

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Outbound references

Observation 2e4d8910-8793-47b0-8927-716f31b22d26 · outbound

This paper cites The two approaches are equivalent when only the f-modes are considered, yet our model is more flexible in incorporating other modes (e.g., gravity and pressure modes).

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides The two approaches are equivalent when only the f-modes are considered, yet our model is more flexible in incorporating other modes (e.g., gravity and pressure modes)

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.376520Z

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Observation 09bc628d-19d9-448b-a2ed-d5e06997eec6 · outbound

This paper cites For the frame dragging terms [H (eff) fr and H (eff) t,LS], we do not replace Pϕ by µr√u[1 + ...] in order to capture the correct back-reaction torque (as discussed in Sec.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides For the frame dragging terms [H (eff) fr and H (eff) t,LS], we do not replace Pϕ by µr√u[1 + ...] in order to capture the correct back-reaction torque (as discussed in Sec

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.386868Z

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Observation 09431f9f-00bd-4d90-955a-1c59362750ea · outbound

This paper cites an unresolved cited work.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Unresolved cited work

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.396070Z

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Observation 0c7eeed4-36d8-4851-b7db-6056235488b6 · outbound

This paper cites Numerical Relativity Simulations of Precessing Binary Neutron Star Mergers.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Numerical Relativity Simulations of Precessing Binary Neutron Star Mergers

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.468064Z

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Observation fa1ee42a-1a28-4c4b-80a5-46467ed16c48 · outbound

This paper cites This is achieved by scaling length and time by1/M, frequency byM, energy and linear momentum by1/µ, and angular momentum by1/(µM ).

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides This is achieved by scaling length and time by1/M, frequency byM, energy and linear momentum by1/µ, and angular momentum by1/(µM )

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.406443Z

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Observation 70448d52-d6fa-4a42-b233-734bcfb31f1e · outbound

This paper cites (110) The detuning is to be compared with Eqs.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides (110) The detuning is to be compared with Eqs

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.416500Z

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Observation 9b0b88b7-34d1-45c4-998f-ca5aeae9705d · outbound

This paper cites Equilibrium, Stability and Orbital Evolution of Close Binary Systems.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Equilibrium, Stability and Orbital Evolution of Close Binary Systems

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.493105Z

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Observation 70f000c9-7909-44a4-8f5a-ecea95427725 · outbound

This paper cites 2q∗ aqaωa⟨ξa, iˆez × ξa⟩ + X b 2q∗ aqbΩ ⟨ˆez × ξa, ˆez × ξb⟩ # , ≃ +X a.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides 2q∗ aqaωa⟨ξa, iˆez × ξa⟩ + X b 2q∗ aqbΩ ⟨ˆez × ξa, ˆez × ξb⟩ # , ≃ +X a

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.435134Z

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Observation 09bdb34b-6df5-491e-a242-2e79da002d67 · outbound

This paper cites GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.442593Z

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Observation e982bfb1-7b02-46ca-9bf5-ce552ce0caf0 · outbound

This paper cites GW170817: Measurements of Neutron Star Radii and Equation of State.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides GW170817: Measurements of Neutron Star Radii and Equation of State

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.454647Z

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Observation 76028673-0c08-4d42-bff6-854d28491b59 · outbound

This paper cites Exploring tidal effects of coalescing binary neutron stars in numerical relativity II: Longterm simulations.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Exploring tidal effects of coalescing binary neutron stars in numerical relativity II: Longterm simulations

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.460374Z

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Observation 99d03b6d-32c6-4375-a6c4-51731610bb2c · outbound

This paper cites Measurability of the tidal polarizability of neutron stars in late-inspiral gravitational-wave signals.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Measurability of the tidal polarizability of neutron stars in late-inspiral gravitational-wave signals

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.527083Z

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Observation ca77a39c-48a9-4d87-a116-f144ca4f72c8 · outbound

This paper cites Gravitational waveforms from SpEC simulations : neutron star-neutron star and low-mass black hole-neutron star binaries.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Gravitational waveforms from SpEC simulations : neutron star-neutron star and low-mass black hole-neutron star binaries

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.478493Z

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Observation 685dd830-a6fe-46c2-b45b-a4c0758ae5a8 · outbound

This paper cites Hydrodynamic Instability and Coalescence of Binary Neutron Stars.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Hydrodynamic Instability and Coalescence of Binary Neutron Stars

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.484799Z

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Observation 11b7b69a-716b-4650-a178-1d47128edf57 · outbound

This paper cites Time-domain effective-one-body gravitational waveforms for coalescing compact binaries with nonprecessing spins, tides and self-spin effects.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Time-domain effective-one-body gravitational waveforms for coalescing compact binaries with nonprecessing spins, tides and self-spin effects

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.547644Z

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Observation db5380e9-f426-4cde-bdcc-6c28a7aa5ae5 · outbound

This paper cites in” replaced by “or.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides in” replaced by “or

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.369127Z

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Observation 3e81aa9d-38d4-4535-a97f-3973462a001b · outbound

This paper cites Constraining neutron star tidal Love numbers with gravitational wave detectors.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Constraining neutron star tidal Love numbers with gravitational wave detectors

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.500149Z

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Observation 537b44d7-ba9c-4412-9a10-ee8efb11c79e · outbound

This paper cites Improved resummation of post-Newtonian multipolar waveforms from circularized compact binaries.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Improved resummation of post-Newtonian multipolar waveforms from circularized compact binaries

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.506958Z

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Observation 57582702-75c5-47c8-9e24-71f0ac8606ea · outbound

This paper cites Tidal deformability of neutron stars with realistic equations of state and their gravitational wave signatures in binary inspiral.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Tidal deformability of neutron stars with realistic equations of state and their gravitational wave signatures in binary inspiral

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.513484Z

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Observation 8e56d808-24fd-410c-bdb6-edef6fad509e · outbound

This paper cites Effective action approach to higher-order relativistic tidal interactions in binary systems and their effective one body description.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Effective action approach to higher-order relativistic tidal interactions in binary systems and their effective one body description

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.518966Z

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Observation 7e2c9045-01c4-4aaa-992a-a26a457309e3 · outbound

This paper cites Gravitational self-force corrections to two-body tidal interactions and the effective one-body formalism.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Gravitational self-force corrections to two-body tidal interactions and the effective one-body formalism

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.533981Z

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Observation 96305710-2644-4efb-845b-437d44242791 · outbound

This paper cites Modeling the dynamics of tidally-interacting binary neutron stars up to merger.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Modeling the dynamics of tidally-interacting binary neutron stars up to merger

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.541369Z

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Observation 5aa0902f-c0d5-48bd-a1f8-a5c069637a16 · outbound

This paper cites Fast Rotating Relativistic Stars: Spectra and Stability without Approximation.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Fast Rotating Relativistic Stars: Spectra and Stability without Approximation

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.627422Z

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Observation 9c812c12-fb6e-4f78-aa01-03e945988d22 · outbound

This paper cites Dynamical Tides in General Relativity: Effective Action and Effective-One-Body Hamiltonian.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Dynamical Tides in General Relativity: Effective Action and Effective-One-Body Hamiltonian

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.555643Z

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Observation 40ee9bed-3f6e-4b06-b9c1-33b371bc709d · outbound

This paper cites Effects of neutron-star dynamic tides on gravitational waveforms within the effective-one-body approach.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Effects of neutron-star dynamic tides on gravitational waveforms within the effective-one-body approach

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.572036Z

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Observation f47a6d38-1ec7-43e5-8a7f-6db05710c776 · outbound

This paper cites Spin effects on neutron star fundamental-mode dynamical tides: phenomenology and comparison to numerical simulations.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Spin effects on neutron star fundamental-mode dynamical tides: phenomenology and comparison to numerical simulations

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.581886Z

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Observation d8a23b45-a0b2-435e-bd4b-4b13967f5292 · outbound

This paper cites Ranjan Mohanty, U.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Ranjan Mohanty, U

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.587879Z

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Observation cbd54773-628c-4729-8aab-ccad70ae8826 · outbound

This paper cites Multipolar universal relations between f-mode frequency and tidal deformability of compact stars.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Multipolar universal relations between f-mode frequency and tidal deformability of compact stars

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.594028Z

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Observation 85d2d538-444f-47e2-8590-f1152e6b51bf · outbound

This paper cites an unresolved cited work.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Unresolved cited work

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.604003Z

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Observation c708d623-c6d7-4a94-8e74-a44b66f6b6ad · outbound

This paper cites Gravitational wave asteroseismology of fast rotating neutron stars with realistic equations of state.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Gravitational wave asteroseismology of fast rotating neutron stars with realistic equations of state

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.613606Z

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Observation e0e778f6-a096-4b87-a7b7-eb6f75620bce · outbound

This paper cites New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.685904Z

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Unavailable: canonical work link unavailable.

Observation 49bb8e8a-3514-438b-a789-605afb95eadd · outbound

This paper cites Rapidly rotating neutron stars: Universal relations and EOS inference.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Rapidly rotating neutron stars: Universal relations and EOS inference

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.637541Z

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Observation 5533b227-69b3-4dd6-8191-b5dfb9255fe9 · outbound

This paper cites Beyond the linear tide: impact of the non-linear tidal response of neutron stars on gravitational waveforms from binary inspirals.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Beyond the linear tide: impact of the non-linear tidal response of neutron stars on gravitational waveforms from binary inspirals

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.644485Z

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Observation 0b1b0f4e-7c39-440f-804e-b7eceb3a9533 · outbound

This paper cites Resonance Locking of Anharmonic $g$-Modes in Coalescing Neutron Star Binaries.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Resonance Locking of Anharmonic $g$-Modes in Coalescing Neutron Star Binaries

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.652532Z

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Observation 755e241e-916e-4972-b095-10fd5da0bf60 · outbound

This paper cites Closed-form tidal approximants for binary neutron star gravitational waveforms constructed from high-resolution numerical relativity simulations.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Closed-form tidal approximants for binary neutron star gravitational waveforms constructed from high-resolution numerical relativity simulations

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.660242Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 018c2bd8-20f9-4ba6-bc98-ae95ddcfa057 · outbound

This paper cites Frequency-domain gravitational waveform models for inspiraling binary neutron stars.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Frequency-domain gravitational waveform models for inspiraling binary neutron stars

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.666617Z

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Unavailable: canonical work link unavailable.

Observation b8509608-66dd-4528-a239-632e1a532902 · outbound

This paper cites Improving the NRTidal model for binary neutron star systems.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Improving the NRTidal model for binary neutron star systems

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.673106Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 751143db-a738-4720-b0dc-764cf750c3e6 · outbound

This paper cites Analytically improved and numerical-relativity informed effective-one-body model for coalescing binary neutron stars.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Analytically improved and numerical-relativity informed effective-one-body model for coalescing binary neutron stars

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.679085Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ecaf1a6c-f440-46aa-862e-0067bb525e53 · outbound

This paper cites Rotating Love: The dynamical tides of spinning Newtonian stars.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Rotating Love: The dynamical tides of spinning Newtonian stars

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.746630Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e1345b39-e17e-4c8e-a636-4df1acf7fc81 · outbound

This paper cites Frequency domain model of $f$-mode dynamic tides in gravitational waveforms from compact binary inspirals.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Frequency domain model of $f$-mode dynamic tides in gravitational waveforms from compact binary inspirals

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.692608Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6ef0422e-c244-4773-bb14-b02f02895dc9 · outbound

This paper cites The sum of Love: Exploring the effective tidal deformability of neutron stars.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides The sum of Love: Exploring the effective tidal deformability of neutron stars

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.699926Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c6894710-f6cb-4b5d-aa36-fa861c1ca15c · outbound

This paper cites Andersson and P.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Andersson and P

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.706336Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 15a1427b-8814-4387-8ffe-66b95791cdcb · outbound

This paper cites Dynamical tides in superfluid neutron stars.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Dynamical tides in superfluid neutron stars

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.714349Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 85ccad4f-44e2-4e1f-9867-3f0a6b041b1b · outbound

This paper cites Resonant tides in binary neutron star mergers: analytical-numerical relativity study.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Resonant tides in binary neutron star mergers: analytical-numerical relativity study

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.725800Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 14d488e4-f325-41ff-b6fe-a7e4f59694ca · outbound

This paper cites The Last Three Seconds: Packed Message delivered by Tides in Binary Neutron Star Mergers.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides The Last Three Seconds: Packed Message delivered by Tides in Binary Neutron Star Mergers

Reference 45

Resolution: verified exact; local_arxiv, observed 2026-08-10T16:33:23.453271Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 41aadd8a-f226-4e47-bb23-f695f33f324c · outbound

This paper cites Gravitoelectric dynamical tides at second post-Newtonian order.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Gravitoelectric dynamical tides at second post-Newtonian order

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.740424Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 56e8a4f9-374e-45d6-bca2-7aba2dddd674 · outbound

This paper cites An instability due to the nonlinear coupling of p-modes to g-modes: Implications for coalescing neutron star binaries.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides An instability due to the nonlinear coupling of p-modes to g-modes: Implications for coalescing neutron star binaries

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.820698Z

Source-reported events for the cited work

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Observation ede7d709-d887-42a7-b169-6b17758b4ef4 · outbound

This paper cites General relativistic dynamical tides in binary inspirals, without modes.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides General relativistic dynamical tides in binary inspirals, without modes

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.752772Z

Source-reported events for the cited work

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Observation 3f3ed5ce-90ba-43be-bfc2-acf3cd106085 · outbound

This paper cites Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.758427Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 10b323d5-661b-4be1-8059-8b4c31547430 · outbound

This paper cites an unresolved cited work.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Unresolved cited work

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.764418Z

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Observation 901118d1-3913-42cd-b70a-d811cbdcf6fe · outbound

This paper cites Resonant Oscillations and Tidal Heating in Coalescing Binary Neutron Stars.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Resonant Oscillations and Tidal Heating in Coalescing Binary Neutron Stars

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.770787Z

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Observation a3495fd9-30b1-42d5-827a-7fcb81ae4bb3 · outbound

This paper cites Nonlinear mode coupling in rotating stars and the r-mode instability in neutron stars.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Nonlinear mode coupling in rotating stars and the r-mode instability in neutron stars

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.791100Z

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Observation 9e44c177-e4b5-4be8-b4c2-535e28e73679 · outbound

This paper cites Excitation of f-modes during mergers of spinning binary neutron star.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Excitation of f-modes during mergers of spinning binary neutron star

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.799899Z

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Observation 0c0c891f-2160-4aba-b271-63c09f8c7da3 · outbound

This paper cites Dynamical tides during the inspiral of rapidly spinning neutron stars: Solutions beyond mode resonance.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Dynamical tides during the inspiral of rapidly spinning neutron stars: Solutions beyond mode resonance

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.809291Z

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Observation 90f28da3-4874-42ec-8ec5-58f0d61f1b70 · outbound

This paper cites Effective one-body approach to general relativistic two-body dynamics.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Effective one-body approach to general relativistic two-body dynamics

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.891211Z

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Observation e463da04-b041-4fae-968b-43e8e5a64169 · outbound

This paper cites The stability of tidally deformed neutron stars to three- and four-mode coupling.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides The stability of tidally deformed neutron stars to three- and four-mode coupling

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.832270Z

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Observation 2565f0e0-2f87-4eb6-b47d-3b2108097e8b · outbound

This paper cites Growth rate of the tidal p-mode g-mode instability in coalescing binary neutron stars.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Growth rate of the tidal p-mode g-mode instability in coalescing binary neutron stars

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.844614Z

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Observation 5bd20257-7f23-4757-9e89-8411c0b06dd4 · outbound

This paper cites Impact of the tidal p-g instability on the gravitational wave signal from coalescing binary neutron stars.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Impact of the tidal p-g instability on the gravitational wave signal from coalescing binary neutron stars

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.856662Z

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Observation c5c80eee-9c00-4aa7-9706-bd5a651c3aea · outbound

This paper cites Constraining the p-mode--g-mode tidal instability with GW170817.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Constraining the p-mode--g-mode tidal instability with GW170817

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.864469Z

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Observation 9629db00-d14d-4e9f-ac3a-8be7b0aad2ca · outbound

This paper cites Urca reactions during neutron star inspiral.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Urca reactions during neutron star inspiral

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.870110Z

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Observation 2c975ef9-996d-4154-953d-117c7aed0047 · outbound

This paper cites Dissipative tidal effects to next-to-leading order and constraints on the dissipative tidal deformability using gravitational wave data.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Dissipative tidal effects to next-to-leading order and constraints on the dissipative tidal deformability using gravitational wave data

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.876382Z

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Observation 1d945dfb-1dd2-4101-b75b-2182a3503262 · outbound

This paper cites Campanelli, C.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Campanelli, C

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.884410Z

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Observation 1a9a8777-af86-4e22-bb3e-456155035d8b · outbound

This paper cites Properties of the binary neutron star merger GW170817.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Properties of the binary neutron star merger GW170817

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.956040Z

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Observation 28225e48-fb4d-4ec2-97f0-261510050085 · outbound

This paper cites A unified equation of state of dense matter and neutron star structure.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides A unified equation of state of dense matter and neutron star structure

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.897586Z

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Observation 67c3ac72-cbae-4ae5-bc66-b04874dc4aa1 · outbound

This paper cites Christensen-Dalsgaard, Lecture Notes on Stellar Oscillations(Institut for Fysik og Astronomi, Aarhus Universitet, 1998).

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Christensen-Dalsgaard, Lecture Notes on Stellar Oscillations(Institut for Fysik og Astronomi, Aarhus Universitet, 1998)

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.906876Z

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Observation 4b351916-6519-4170-aebf-1548a91ecd86 · outbound

This paper cites Gravitomagnetic resonant excitation of Rossby modes in coalescing neutron star binaries.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Gravitomagnetic resonant excitation of Rossby modes in coalescing neutron star binaries

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.915724Z

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Observation 3b59b1ba-318e-453b-8828-96eb0dcc8d9d · outbound

This paper cites Goldstein, C.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Goldstein, C

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.924648Z

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Observation 848db00a-481a-4656-8b5f-0b42ca00e6bb · outbound

This paper cites Poisson and C.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Poisson and C

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.934875Z

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Observation 7545718b-2bed-4cb9-9236-4c21c514f4ec · outbound

This paper cites Post-1-Newtonian tidal effects in the gravitational waveform from binary inspirals.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Post-1-Newtonian tidal effects in the gravitational waveform from binary inspirals

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.941949Z

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Observation 82a1c4f8-1125-4c71-9693-9b8957564c8d · outbound

This paper cites Constraints on a phenomenologically parameterized neutron-star equation of state.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Constraints on a phenomenologically parameterized neutron-star equation of state

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.948963Z

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Observation 2d714958-7c72-4c29-b10e-7ccd52a3aa0f · outbound

This paper cites The complete non-spinning effective-one-body metric at linear order in the mass ratio.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides The complete non-spinning effective-one-body metric at linear order in the mass ratio

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.020976Z

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Observation 10e12fe8-6760-426c-8662-8d19290148dc · outbound

This paper cites an unresolved cited work.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Unresolved cited work

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.964070Z

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Observation 02bfe71d-9db4-4d97-8733-13cfb26249a1 · outbound

This paper cites Tidal dissipation in stars and giant planets.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Tidal dissipation in stars and giant planets

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.970382Z

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Observation 3241e47e-bfa8-4180-b95b-aa782d7534f4 · outbound

This paper cites Fourth post-Newtonian effective-one-body Hamiltonians with generic spins.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Fourth post-Newtonian effective-one-body Hamiltonians with generic spins

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.977259Z

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Observation 4940acd1-0e94-4a5a-963d-de40af1c7131 · outbound

This paper cites 56 and 60) to 1 PN order.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides 56 and 60) to 1 PN order

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.428239Z

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Observation 24dca6aa-1f9b-44a9-b2b7-353e37c7e1ab · outbound

This paper cites First Law of Mechanics for Black Hole Binaries with Spins.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides First Law of Mechanics for Black Hole Binaries with Spins

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.983654Z

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Observation d64f3cc9-8212-4bec-a020-b80bce99dd68 · outbound

This paper cites Coalescence of Two Spinning Black Holes: An Effective One-Body Approach.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Coalescence of Two Spinning Black Holes: An Effective One-Body Approach

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.990616Z

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Observation 7c031143-6935-452c-93f7-b938c81cafe3 · outbound

This paper cites Transition from inspiral to plunge in precessing binaries of spinning black holes.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Transition from inspiral to plunge in precessing binaries of spinning black holes

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.998462Z

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Observation 5f1ffd4a-c0b3-4bd4-8047-34a1586cc32e · outbound

This paper cites Final spin of a coalescing black-hole binary: an Effective-One-Body approach.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Final spin of a coalescing black-hole binary: an Effective-One-Body approach

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.006977Z

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Observation 59d703cb-cbe7-42df-bdcf-e6ee5563588f · outbound

This paper cites Effective one body approach to the dynamics of two spinning black holes with next-to-leading order spin-orbit coupling.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Effective one body approach to the dynamics of two spinning black holes with next-to-leading order spin-orbit coupling

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.028150Z

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Observation 912f6b0a-77a9-47c8-9d4c-64c01d6ed21e · outbound

This paper cites Inspiral-merger-ringdown multipolar waveforms of nonspinning black-hole binaries using the effective-one-body formalism.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Inspiral-merger-ringdown multipolar waveforms of nonspinning black-hole binaries using the effective-one-body formalism

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.035647Z

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Observation 930bebef-6ea5-4cc3-9886-329af3e19779 · outbound

This paper cites an unresolved cited work.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Unresolved cited work

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.043141Z

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Observation 17f6e576-9c7d-4162-8930-9cd4d91d23f8 · outbound

This paper cites First-post-Newtonian quadrupole tidal interactions in binary systems.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides First-post-Newtonian quadrupole tidal interactions in binary systems

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.055218Z

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Observation 986dbb85-703f-4b5f-9652-1456265776df · outbound

This paper cites Renormalizing Love: tidal effects at the third post-Newtonian order.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Renormalizing Love: tidal effects at the third post-Newtonian order

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.060200Z

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Observation 7471fd88-cae9-4bcb-92a7-719e37c104f4 · outbound

This paper cites Post-Newtonian Theory for Gravitational Waves.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Post-Newtonian Theory for Gravitational Waves

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.068306Z

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Observation d3e6a18e-6cc6-40b9-9d08-71e7b010ca4d · outbound

This paper cites Gravitational Recoil during Binary Black Hole Coalescence using the Effective One Body Approach.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Gravitational Recoil during Binary Black Hole Coalescence using the Effective One Body Approach

Reference 86

Resolution: verified exact; local_arxiv, observed 2026-08-10T16:33:22.005843Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 8574904f-59c7-4b36-ab51-542756965250 · outbound

This paper cites Spin effects in the inspiral of coalescing compact binaries.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Spin effects in the inspiral of coalescing compact binaries

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.081659Z

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Observation c2ef7411-f986-436e-8680-d1dc2ad50ad7 · outbound

This paper cites An improved effective-one-body Hamiltonian for spinning black-hole binaries.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides An improved effective-one-body Hamiltonian for spinning black-hole binaries

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.089980Z

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Observation 4b7a601b-6047-4b86-be1f-802b8ead30a0 · outbound

This paper cites Extending the effective-one-body Hamiltonian of black-hole binaries to include next-to-next-to-leading spin-orbit couplings.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Extending the effective-one-body Hamiltonian of black-hole binaries to include next-to-next-to-leading spin-orbit couplings

Reference 89

Resolution: verified exact; local_arxiv, observed 2026-08-10T16:33:21.873000Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 174a52c2-888f-4097-861e-9950cb465734 · outbound

This paper cites Prototype effective-one-body model for nonprecessing spinning inspiral-merger-ringdown waveforms.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Prototype effective-one-body model for nonprecessing spinning inspiral-merger-ringdown waveforms

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.102609Z

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Observation e8cde60f-9cb3-41da-9728-252c414964da · outbound

This paper cites Gravitational waves from inspiraling compact binaries: The quadrupole-moment term.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Gravitational waves from inspiraling compact binaries: The quadrupole-moment term

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.108504Z

Source-reported events for the cited work

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Observation d63f4c1f-5a07-4592-9cca-5fd619c44b35 · outbound

This paper cites Testing the binary black hole nature of a compact binary coalescence.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Testing the binary black hole nature of a compact binary coalescence

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.115996Z

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Observation 877dd6b8-3fa7-4804-bbea-7f525793aecb · outbound

This paper cites Observability of dynamical tides in merging eccentric neutron star binaries.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Observability of dynamical tides in merging eccentric neutron star binaries

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.122857Z

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Observation 6e28d92d-6fff-4bcb-9812-61db95cd36cc · outbound

This paper cites Haberland, J.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Haberland, J

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.130335Z

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Observation cf02d283-fcea-418d-b3b0-35360965e84e · outbound

This paper cites Reisenegger and P.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Reisenegger and P

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.137921Z

Source-reported events for the cited work

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Observation 75955737-e8cd-4bd2-9e09-ff4b8cf83b6b · outbound

This paper cites Resonant tidal excitation of superfluid neutron stars in coalescing binaries.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Resonant tidal excitation of superfluid neutron stars in coalescing binaries

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.145963Z

Source-reported events for the cited work

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Observation c0db9493-7b6c-4f5b-a717-0ecc836b99a7 · outbound

This paper cites Dynamical tides in coalescing superfluid neutron star binaries with hyperon cores and their detectability with third generation gravitational-wave detectors.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Dynamical tides in coalescing superfluid neutron star binaries with hyperon cores and their detectability with third generation gravitational-wave detectors

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.154011Z

Source-reported events for the cited work

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Observation 90161a59-6e8c-49a1-86ce-1d73506063ed · outbound

This paper cites General-relativistic treatment of tidal $g$-mode resonances in coalescing binaries of neutron stars. I. Theoretical framework and crust breaking.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides General-relativistic treatment of tidal $g$-mode resonances in coalescing binaries of neutron stars. I. Theoretical framework and crust breaking

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.161162Z

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Observation aaba65bb-109c-43a7-914d-950596493d36 · outbound

This paper cites General-relativistic treatment of tidal $g$-mode resonances in coalescing binaries of neutron stars. II. As triggers for precursor flares of short gamma-ray bursts.

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.168234Z

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Observation 2f704d18-e740-401d-9eb9-c52b232b2b9a · outbound

This paper cites Neutron star g-modes in the relativistic Cowling approximation.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Neutron star g-modes in the relativistic Cowling approximation

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.174351Z

Source-reported events for the cited work

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Pith citing papers

Observation 2cda26a2-e236-4d7e-9fc6-6c6348aed45a · inbound

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The error budget of binary neutron star merger simulations for configurations with high spin Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-07T11:40:36.103140Z

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Observation 3360aef2-96e3-4bfb-8705-c6ecc444519d · inbound

Universal Relations with Dynamical Tides cites this paper.

Universal Relations with Dynamical Tides Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides

Reference 53

Resolution: verified exact; arxiv_id, observed 2026-05-17T05:54:08.555506Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 82b13fc7-1b70-43b1-9d95-f2ef4d2f4c64 · inbound

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The Good, the Bad, and the Subtle: Relativistic mode sums for neutron-star tidal response Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides

Reference 25

Resolution: metadata mismatch; arxiv_id, observed 2026-05-12T02:16:15.961959Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation a1b2840e-5ddf-4efc-8cd5-077228699165 · inbound

Nonlinear hydrodynamics in spinning neutron stars: Theoretical universal relations and equilibrium solutions cites this paper.

Nonlinear hydrodynamics in spinning neutron stars: Theoretical universal relations and equilibrium solutions Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides

Reference 34

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Oscillations of Dissipative Neutron Stars: The Impact of Hyperonic Reaction Rates cites this paper.

Oscillations of Dissipative Neutron Stars: The Impact of Hyperonic Reaction Rates Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides

Reference 64

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