Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity | Paper Citation Record

Observation 12be506c-7fa2-4afe-875c-2ff90405d843 · outbound

This paper cites Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity

Reference 1

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Observation ce6420f7-245e-4472-9d6a-def0a5effb96 · outbound

This paper cites tdBag model for strange quark matter tdBag [35] is a bag-like model inspired by the standard MIT bag model [ 36,37]1.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity tdBag model for strange quark matter tdBag [35] is a bag-like model inspired by the standard MIT bag model [ 36,37]1

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Observation d547355d-3af2-4631-a74a-cb1d22621825 · outbound

This paper cites Fraga et al.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Fraga et al

Reference 3

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Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Unresolved cited work

Reference 4

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Observation 2430d00e-50f3-4465-bbb9-4e9bd2843ecd · outbound

This paper cites vacuumless.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity vacuumless

Reference 5

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Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Unresolved cited work

Reference 6

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Observation 2eb793e9-1c09-4700-b16b-b59ad4cebfc5 · outbound

This paper cites Our procedure can be applied to study a variety of parameters and HM EoS choice and enables future studies of NSs binary containing SQM cores.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Our procedure can be applied to study a variety of parameters and HM EoS choice and enables future studies of NSs binary containing SQM cores

Reference 7

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Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Unresolved cited work

Reference 8

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Observation 8e1b3cab-90c5-4038-982f-dbaa9839bd05 · outbound

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Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Unresolved cited work

Reference 9

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Observation c879b4b0-23b6-4fae-a7e8-da67ad95f4ce · outbound

This paper cites The Inspiral We present the full gravitational waveform obtained from our simulations in Fig.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity The Inspiral We present the full gravitational waveform obtained from our simulations in Fig

Reference 10

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Observation 49568ec7-5356-45d3-b55f-b14987716465 · outbound

This paper cites 45.0 47.5 50.0 52.5 55.0 57.5 60.0 62.5 t[ms] 0.0 0.2 0.4 0.6 0.8 1.0 ρmax [g/cm3] ×1016 ρmax 0.00 0.02 0.04 0.06 M [M⊙] GW170817 Mej 1 2Mdisk Figure 7.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity 45.0 47.5 50.0 52.5 55.0 57.5 60.0 62.5 t[ms] 0.0 0.2 0.4 0.6 0.8 1.0 ρmax [g/cm3] ×1016 ρmax 0.00 0.02 0.04 0.06 M [M⊙] GW170817 Mej 1 2Mdisk Figure 7

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.440691Z

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Observation ad6dfc60-dcca-48e5-81ed-5832cb17fef6 · outbound

This paper cites Multimessenger Parameter Estimation of GW170817.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Multimessenger Parameter Estimation of GW170817

Reference 12

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Observation a70ba43f-d25f-4ea8-941e-092ed44966e4 · outbound

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

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

Reference 13

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Observation 8bff7709-b012-4725-a1f5-006eb4989663 · outbound

This paper cites Multi-messenger Observations of a Binary Neutron Star Merger.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Multi-messenger Observations of a Binary Neutron Star Merger

Reference 14

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Observation 3e106721-6e1e-4347-a824-cccaeafa9e09 · outbound

This paper cites Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

Reference 15

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Observation 54e73f3a-0900-4f24-ad31-9b08f38200ff · outbound

This paper cites Parameter Estimation for GW170817 using Relative Binning.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Parameter Estimation for GW170817 using Relative Binning

Reference 16

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Observation e13b942a-faea-44e2-bfa0-586d06711774 · outbound

This paper cites Tidal Deformabilities and Radii of Neutron Stars from the Observation of GW170817.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Tidal Deformabilities and Radii of Neutron Stars from the Observation of GW170817

Reference 17

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Observation 8017ad51-bfec-4cbc-8d10-2aa1d45ad09a · outbound

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

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Properties of the binary neutron star merger GW170817

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.468409Z

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Observation ed687f9e-a831-4cd4-8105-13a6d318d92b · outbound

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

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity GW170817: Measurements of Neutron Star Radii and Equation of State

Reference 19

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This paper cites GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

Reference 20

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Observation 10620419-ccd5-437a-9e95-81c1bc224beb · outbound

This paper cites GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.478943Z

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Observation 5f443b4d-d302-4014-9a8e-5185dcf287d7 · outbound

This paper cites Neutron-star radius constraints from GW170817 and future detections.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Neutron-star radius constraints from GW170817 and future detections

Reference 22

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Observation 06315c03-782d-4efb-be67-d8a3ae5ea1d4 · outbound

This paper cites Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations

Reference 23

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Observation 918b7c48-8ba8-4201-844d-900979e7aef5 · outbound

This paper cites The missing link: Merging neutron stars naturally produce jet-like structures and can power short Gamma-Ray Bursts.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity The missing link: Merging neutron stars naturally produce jet-like structures and can power short Gamma-Ray Bursts

Reference 24

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Observation 158c3ea7-a2b2-46e7-960b-6d934ef3f826 · outbound

This paper cites Multi-messenger Bayesian parameter inference of a binary neutron-star merger.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Multi-messenger Bayesian parameter inference of a binary neutron-star merger

Reference 25

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Observation 46a99fca-c0f1-4eb4-b5e6-3a2d733b530f · outbound

This paper cites Gravitational-wave constraints on the neutron-star-matter Equation of State.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Gravitational-wave constraints on the neutron-star-matter Equation of State

Reference 26

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Observation 7f442483-dab2-4d13-b030-b0259a70dfb0 · outbound

This paper cites New constraints on radii and tidal deformabilities of neutron stars from GW170817.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity New constraints on radii and tidal deformabilities of neutron stars from GW170817

Reference 27

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Observation c3752739-1d5b-4d87-9b62-a2e346899b0d · outbound

This paper cites Evidence for quark-matter cores in massive neutron stars.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Evidence for quark-matter cores in massive neutron stars

Reference 28

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Observation b0c36628-9d91-49ff-bc1f-f0c327f3e12d · outbound

This paper cites Signatures of quark-hadron phase transitions in general-relativistic neutron-star mergers.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Signatures of quark-hadron phase transitions in general-relativistic neutron-star mergers

Reference 29

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Observation 78ef91d4-e46c-4101-bada-8ad0a34dbd08 · outbound

This paper cites Identifying a first-order phase transition in neutron star mergers through gravitational waves.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Identifying a first-order phase transition in neutron star mergers through gravitational waves

Reference 30

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Observation b7850eb9-7f6f-4e92-be18-c8fe493fc6f2 · outbound

This paper cites Beyond second-order convergence in simulations of binary neutron stars in full general-relativity.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Beyond second-order convergence in simulations of binary neutron stars in full general-relativity

Reference 31

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Observation 938b5e79-fb77-4da6-86f4-8b9904954cf1 · outbound

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

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Exploring tidal effects of coalescing binary neutron stars in numerical relativity II: Longterm simulations

Reference 32

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Observation 96699d41-5945-4471-a0d4-42d2ff3547e5 · outbound

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

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Closed-form tidal approximants for binary neutron star gravitational waveforms constructed from high-resolution numerical relativity simulations

Reference 33

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Observation 3e05ff32-7409-45ea-9955-01c1cc4e4fb1 · outbound

This paper cites Sub-radian-accuracy gravitational waveforms of coalescing binary neutron stars in numerical relativity.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Sub-radian-accuracy gravitational waveforms of coalescing binary neutron stars in numerical relativity

Reference 34

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Observation d2555a13-ee79-49d6-bcd9-6212732d780c · outbound

This paper cites CoRe database of binary neutron star merger waveforms and its application in waveform development.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity CoRe database of binary neutron star merger waveforms and its application in waveform development

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.527475Z

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Observation 732fef48-4627-48a4-902c-aa4bd0590e8b · outbound

This paper cites A New Extended Model of Hadrons.Phys.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity A New Extended Model of Hadrons.Phys

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.574549Z

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Observation a0da15cf-f658-4c54-aa60-318a5544fc4f · outbound

This paper cites Magnetized Neutron Stars With Realistic Equations of State and Neutrino Cooling.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Magnetized Neutron Stars With Realistic Equations of State and Neutrino Cooling

Reference 37

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Observation 9c816f03-bf0e-498d-9e8f-f8c42b2783b8 · outbound

This paper cites The dynamical mass ejection from binary neutron star mergers: Radiation-hydrodynamics study in general relativity.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity The dynamical mass ejection from binary neutron star mergers: Radiation-hydrodynamics study in general relativity

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.538516Z

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Observation 3f04f5a8-d9d3-4adc-ab99-088dce373924 · outbound

This paper cites Effects of the microphysical Equation of State in the mergers of magnetized Neutron Stars With Neutrino Cooling.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Effects of the microphysical Equation of State in the mergers of magnetized Neutron Stars With Neutrino Cooling

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.542335Z

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Observation 3bd3d795-1653-4c66-9d10-7942e433cae7 · outbound

This paper cites Monte-Carlo closure for moment-based transport schemes in general relativistic radiation hydrodynamics simulations.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Monte-Carlo closure for moment-based transport schemes in general relativistic radiation hydrodynamics simulations

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.545820Z

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Observation f8e24310-f8b5-4d68-80be-50909b290bf3 · outbound

This paper cites GW170817, General Relativistic Magnetohydrodynamic Simulations, and the Neutron Star Maximum Mass.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity GW170817, General Relativistic Magnetohydrodynamic Simulations, and the Neutron Star Maximum Mass

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.549490Z

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Observation cc4614eb-06f1-4695-8afb-ccc958807dfb · outbound

This paper cites General relativistic magnetohydrodynamic simulations of binary neutron star mergers forming a long-lived neutron star.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity General relativistic magnetohydrodynamic simulations of binary neutron star mergers forming a long-lived neutron star

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.553272Z

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Observation 3dcb2221-cb8e-42f3-a05e-83ce5534946e · outbound

This paper cites Global simulations of strongly magnetized remnant massive neutron stars formed in binary neutron star mergers.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Global simulations of strongly magnetized remnant massive neutron stars formed in binary neutron star mergers

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.556836Z

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Observation b3cc82d8-06b2-44d5-a6c2-dc3a413f4312 · outbound

This paper cites They consider the ground state of matter to be three Fermi seas of deconﬁned quarks in equal proportions of up, down and strange ﬂavors.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity They consider the ground state of matter to be three Fermi seas of deconﬁned quarks in equal proportions of up, down and strange ﬂavors

Reference 44

Resolution: malformed identifier; no resolver link, observed 2026-08-14T14:29:00.424365Z

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Observation 7f8ffd84-2bf0-4802-af1a-bf068be4eb1b · outbound

This paper cites General-Relativistic Large-Eddy Simulations of Binary Neutron Star Mergers.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity General-Relativistic Large-Eddy Simulations of Binary Neutron Star Mergers

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.560770Z

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Observation 1abeb706-30a9-41f4-bfa0-08e5d83eb5bc · outbound

This paper cites General relativistic viscous hydrodynamics of differentially rotating neutron stars.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity General relativistic viscous hydrodynamics of differentially rotating neutron stars

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.564783Z

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Observation 4f696ca0-b121-497c-8e31-ba18b0ef6b41 · outbound

This paper cites Merger of compact stars in the two-families scenario.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Merger of compact stars in the two-families scenario

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.568262Z

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Observation 1fc70d1a-53ff-4e31-bc1c-173072dd244d · outbound

This paper cites Strange Matter.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Strange Matter

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.571587Z

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Observation 527c7d77-1679-4a1a-b1e3-8b261fd3442e · outbound

This paper cites THE MIT BAG MODEL.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity THE MIT BAG MODEL

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.577484Z

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Observation 426669f8-d535-4aff-9526-dc1ff966b00a · outbound

This paper cites Hybrid stars that masquerade as neutron stars.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Hybrid stars that masquerade as neutron stars

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.580130Z

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Observation 79708474-f800-4e9e-a665-efcb364df4d5 · outbound

This paper cites Color superconductivity in dense quark matter.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Color superconductivity in dense quark matter

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.583170Z

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Observation 2f457fcf-e166-4712-9d11-6af92e94a16b · outbound

This paper cites Color-flavor locked strange matter.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Color-flavor locked strange matter

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.586141Z

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Observation 47686bc2-cd28-4364-b5b6-c19c06d6963b · outbound

This paper cites Small, Dense Quark Stars from Perturbative QCD.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Small, Dense Quark Stars from Perturbative QCD

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.589505Z

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Observation ca8d9c8e-2eb7-4440-9a3a-37bfed7ef14f · outbound

This paper cites Vector interaction enhanced bag model for astrophysical applications.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Vector interaction enhanced bag model for astrophysical applications

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.593057Z

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Observation 212b9156-c50c-43bd-9da0-aa92afe666f5 · outbound

This paper cites Phase transition effects on the dynamical stability of hybrid neutron stars.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Phase transition effects on the dynamical stability of hybrid neutron stars

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.596995Z

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Observation d99344e6-5cac-46dd-baab-c983c6ba66cd · outbound

This paper cites Collapsed nuclei.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Collapsed nuclei

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.600639Z

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Observation a38e1a00-34d1-4781-a077-5a9e1322dea7 · outbound

This paper cites Cosmic Separation of Phases.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Cosmic Separation of Phases

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.604031Z

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Observation a1ad622e-3624-409f-a323-edd756a7ea15 · outbound

This paper cites Compact Stars: Nuclear Physics, Particle Physics, and General Relativity, 2 ed.; Springer: The address, 2000.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Compact Stars: Nuclear Physics, Particle Physics, and General Relativity, 2 ed.; Springer: The address, 2000

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.607280Z

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Observation 46e8a920-112a-4f0b-b6bc-923689a01104 · outbound

This paper cites Surface tension and curvature energy of quark matter in the NJL model.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Surface tension and curvature energy of quark matter in the NJL model

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.610565Z

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Observation db1ef07b-80f7-4b05-8d23-8ecb3a5f6c8f · outbound

This paper cites Dynamical Model of Elementary Particles Based on an Analogy with Superconductivity.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Dynamical Model of Elementary Particles Based on an Analogy with Superconductivity

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.614229Z

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Observation 63c07bd6-5511-4ec7-97f9-c0dd3eb6c87f · outbound

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

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity A unified equation of state of dense matter and neutron star structure

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.617794Z

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Observation ee98d37e-0c58-4763-9ed9-9b3039bbffc0 · outbound

This paper cites Calibration of Moving Puncture Simulations.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Calibration of Moving Puncture Simulations

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.621281Z

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Observation b4909ae5-51e7-4c33-89c5-557fc8174454 · outbound

This paper cites Numerical relativity simulations of binary neutron stars.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Numerical relativity simulations of binary neutron stars

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.625103Z

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Observation 5189230f-4b48-4937-ab44-79bc23b5a12d · outbound

This paper cites Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.629131Z

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Observation cc7b9e0d-5153-42de-86a1-31bd5e4a738f · outbound

This paper cites Gravitational waveforms from binary neutron star mergers with high-order WENO schemes in numerical relativity.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Gravitational waveforms from binary neutron star mergers with high-order WENO schemes in numerical relativity

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.632873Z

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Observation 70cc7c76-be20-4ce0-abb7-b586a0968d31 · outbound

This paper cites A new numerical method to construct binary neutron star initial data.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity A new numerical method to construct binary neutron star initial data

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.636564Z

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Observation 9803830c-389b-402c-ba28-ce424dff83d6 · outbound

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

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Constraints on a phenomenologically parameterized neutron-star equation of state

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.640184Z

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Observation 79c32faa-966a-4d3e-957a-53301899d8eb · outbound

This paper cites Instabilities in Close Neutron Star Binaries.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Instabilities in Close Neutron Star Binaries

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.643875Z

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Observation a8974c3c-767f-4130-842a-8328794939f5 · outbound

This paper cites Relativistic Numerical Method for Close Neutron Star Binaries.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Relativistic Numerical Method for Close Neutron Star Binaries

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.647422Z

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Observation 434c7d95-50e9-45f2-9c15-81fb64154a89 · outbound

This paper cites Conformal ``thin sandwich'' data for the initial-value problem of general relativity.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Conformal ``thin sandwich'' data for the initial-value problem of general relativity

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.651039Z

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Observation 8c0cd0c8-a024-4988-a9d7-3d98d4c3f99d · outbound

This paper cites Constructing quasi-equilibrium initial data for binary neutron stars with arbitrary spins.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Constructing quasi-equilibrium initial data for binary neutron stars with arbitrary spins

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.654372Z

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Observation 450d40d3-9e32-476f-8c42-266d984df0fd · outbound

This paper cites Binary Neutron Stars with Generic Spin, Eccentricity, Mass ratio, and Compactness - Quasi-equilibrium Sequences and First Evolutions.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Binary Neutron Stars with Generic Spin, Eccentricity, Mass ratio, and Compactness - Quasi-equilibrium Sequences and First Evolutions

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.657377Z

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Unavailable: canonical work link unavailable.

Observation 448e2a16-6501-4389-92bb-a3e8689e05b6 · outbound

This paper cites Initial data for binary neutron stars with adjustable eccentricity.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Initial data for binary neutron stars with adjustable eccentricity

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.660614Z

Source-reported events for the cited work

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Observation 6deae75e-58b1-4f60-a1c1-65646068e897 · outbound

This paper cites Reducing orbital eccentricity in initial data of binary neutron stars.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Reducing orbital eccentricity in initial data of binary neutron stars

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.664072Z

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Unavailable: canonical work link unavailable.

Observation f91efdd9-c18a-4596-b6bf-f6b7298bd7ef · outbound

This paper cites Constraint violation in free evolution schemes: comparing BSSNOK with a conformal decomposition of Z4.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Constraint violation in free evolution schemes: comparing BSSNOK with a conformal decomposition of Z4

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.667625Z

Source-reported events for the cited work

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Observation ca1d5a7e-ef81-48ba-abca-4d416080b144 · outbound

This paper cites Constraint damping for the Z4c formulation of general relativity.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Constraint damping for the Z4c formulation of general relativity

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.671104Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dc5cb1c0-718e-4f17-a279-20ad711dcc86 · outbound

This paper cites Compact binary evolutions with the Z4c formulation.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Compact binary evolutions with the Z4c formulation

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.674397Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 94eec824-d38a-4fcf-b9ba-782729f651c9 · outbound

This paper cites An improved weighted essentially non-oscillatory scheme for hyperbolic conservation laws.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity An improved weighted essentially non-oscillatory scheme for hyperbolic conservation laws

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.677766Z

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Observation f8b90ebc-f798-4afa-bf47-78a0daee5a1a · outbound

This paper cites High-resolution numerical relativity simulations of spinning binary neutron star mergers.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity High-resolution numerical relativity simulations of spinning binary neutron star mergers

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.681307Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 68217d01-c142-476a-b132-8d25232dbaff · outbound

This paper cites Binary Neutron Star Mergers.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Binary Neutron Star Mergers

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.684905Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 69328b24-54e3-4d40-8558-8f5f9ea5fdec · outbound

This paper cites Matter imprints in waveform models for neutron star binaries: tidal and self-spin effects.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Matter imprints in waveform models for neutron star binaries: tidal and self-spin effects

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.688693Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4ce158b7-af08-4a35-9f23-b02c0b8c6aba · outbound

This paper cites Gravitational waves and mass ejecta from binary neutron star mergers: Effect of the mass-ratio.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Gravitational waves and mass ejecta from binary neutron star mergers: Effect of the mass-ratio

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.692652Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8c17c92c-73e6-49ed-8a86-e2fdb1e957ff · outbound

This paper cites Gravitational waves and mass ejecta from binary neutron star mergers: Effect of the stars' rotation.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Gravitational waves and mass ejecta from binary neutron star mergers: Effect of the stars' rotation

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.696434Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b3fe394d-bd46-4b1d-b837-a981f22bc360 · outbound

This paper cites A simple model of complete precessing black-hole-binary gravitational waveforms.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity A simple model of complete precessing black-hole-binary gravitational waveforms

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.700319Z

Source-reported events for the cited work

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Observation f4d7507e-bc05-4efe-b3aa-85a6e48fa51f · outbound

This paper cites Tests of General Relativity with GW170817.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Tests of General Relativity with GW170817

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.704071Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d0de0b5d-d400-4081-86ef-0abc49111522 · outbound

This paper cites Constraining the Equation of State of Neutron Stars from Binary Mergers.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Constraining the Equation of State of Neutron Stars from Binary Mergers

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.707369Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1d11bb47-d7ce-4df9-8e7f-3f303a8b7799 · outbound

This paper cites Spectral properties of the post-merger gravitational-wave signal from binary neutron stars.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Spectral properties of the post-merger gravitational-wave signal from binary neutron stars

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.711795Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ab513a6b-01e4-4b25-858b-5d99fb613ab5 · outbound

This paper cites Gravitational-wave signal from binary neutron stars: a systematic analysis of the spectral properties.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Gravitational-wave signal from binary neutron stars: a systematic analysis of the spectral properties

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.715538Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b1e06f7f-6b7b-4353-8d43-96c010daf295 · outbound

This paper cites Measuring neutron-star properties via gravitational waves from binary mergers.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Measuring neutron-star properties via gravitational waves from binary mergers

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.718676Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 191e3292-61bf-4258-b3b3-e8c941688160 · outbound

This paper cites Gravitational waves and nonaxisymmetric oscillation modes in mergers of compact object binaries.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Gravitational waves and nonaxisymmetric oscillation modes in mergers of compact object binaries

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.721742Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4c368f6b-dab0-44cd-9f7c-375770641918 · outbound

This paper cites Equation-of-state dependence of the gravitational-wave signal from the ring-down phase of neutron-star mergers.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Equation-of-state dependence of the gravitational-wave signal from the ring-down phase of neutron-star mergers

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.724961Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6e31b725-10b2-44d0-8b2a-8aaadf4e8421 · outbound

This paper cites Revealing the high-density equation of state through binary neutron star mergers.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Revealing the high-density equation of state through binary neutron star mergers

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.728049Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5459dbe1-3f2b-4f1f-86aa-4f8db63ad53f · outbound

This paper cites Observing Gravitational Waves From The Post-Merger Phase Of Binary Neutron Star Coalescence.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Observing Gravitational Waves From The Post-Merger Phase Of Binary Neutron Star Coalescence

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.731450Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4a402242-db0c-4da9-872e-ee540f81483f · outbound

This paper cites A unified picture of the post-merger dynamics and gravitational wave emission in neutron-star mergers.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity A unified picture of the post-merger dynamics and gravitational wave emission in neutron-star mergers

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.734946Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cbe44726-2916-44c8-864e-826e12c3ab9c · outbound

This paper cites Modeling the complete gravitational wave spectrum of neutron star mergers.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Modeling the complete gravitational wave spectrum of neutron star mergers

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.738639Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9987e94c-d231-4738-8b7d-31032b8a8219 · outbound

This paper cites Gravitational waves and mass ejecta from binary neutron star mergers: Effect of large eccentricities.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Gravitational waves and mass ejecta from binary neutron star mergers: Effect of large eccentricities

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.742787Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 21256722-3157-4a38-a052-8eb14e18f75a · outbound

This paper cites Kilonovae.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Kilonovae

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.746338Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f822b7eb-63ec-4be4-bd22-7af0b0a6ee5a · outbound

This paper cites Modeling dynamical ejecta from binary neutron star mergers and implications for electromagnetic counterparts.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Modeling dynamical ejecta from binary neutron star mergers and implications for electromagnetic counterparts

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.750629Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 07f103c9-c38e-4646-a71e-a834e2757a45 · outbound

This paper cites Neutrino-Dominated Accretion and Supernovae.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Neutrino-Dominated Accretion and Supernovae

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.754374Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4d5e1107-8dd1-4a62-8c6c-4f3e6be70477 · outbound

This paper cites Nucleosynthesis in the Outflow from Gamma Ray Burst Accretion Disks.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Nucleosynthesis in the Outflow from Gamma Ray Burst Accretion Disks

Reference 100

Resolution: verified exact; local_arxiv, observed 2026-08-14T14:29:01.030478Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

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