Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr | Paper Citation Record

Observation b31460a6-bd10-46ee-94e7-bf067823a17e · outbound

This paper cites Observation of Gravitational Waves from a Binary Black Hole Merger.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Observation of Gravitational Waves from a Binary Black Hole Merger

Reference 1

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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.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

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Observation e0cbc7c1-1f8e-4d8d-96ed-ccd61c413cd3 · outbound

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Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run

Reference 3

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Observation 3271790c-9449-4c20-8805-3df8f10c335c · outbound

This paper cites GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run

Reference 4

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Observation 7c29d392-ea5a-4c34-bdd5-18d8d95de3b7 · outbound

This paper cites GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run

Reference 5

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This paper cites GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run

Reference 6

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Observation 93d0e003-223e-43e8-8403-ffac214f8276 · outbound

This paper cites Black Hole Spectroscopy and Tests of General Relativity with GW250114.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Black Hole Spectroscopy and Tests of General Relativity with GW250114

Reference 7

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Observation 36064646-c73d-4ba0-a9f4-68d1b442d63c · outbound

This paper cites Black hole spectroscopy: from theory to experiment.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Black hole spectroscopy: from theory to experiment

Reference 8

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Observation d3367f8e-3735-46a0-8f15-0a4ebb22bfc8 · outbound

This paper cites Quasi-Normal Modes of Stars and Black Holes.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Quasi-Normal Modes of Stars and Black Holes

Reference 9

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.563235Z

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Observation 2530031e-d6c8-4a20-b05f-ebd65a5584b4 · outbound

This paper cites Nollert, TOPICAL REVIEW: Quasinormal modes: the characteristic ‘sound’ of black holes and neutron stars, Class.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Nollert, TOPICAL REVIEW: Quasinormal modes: the characteristic ‘sound’ of black holes and neutron stars, Class

Reference 10

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Observation 1aa05c61-2231-4e0f-9f1c-9a756f248ee3 · outbound

This paper cites Quasinormal modes of black holes and black branes.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Quasinormal modes of black holes and black branes

Reference 11

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Observation c2841a0d-6d3c-4a41-8407-0e03b1be3a26 · outbound

This paper cites Quasinormal modes of black holes: from astrophysics to string theory.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Quasinormal modes of black holes: from astrophysics to string theory

Reference 12

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Observation 04eea347-6e9f-4bc8-9a00-4309f45c3d93 · outbound

This paper cites Testing General Relativity with Black Hole Quasi-Normal Modes.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Testing General Relativity with Black Hole Quasi-Normal Modes

Reference 13

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.566796Z

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Observation 8f712d88-098e-4b6e-8d75-442bb9d7f3ee · outbound

This paper cites an unresolved cited work.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Unresolved cited work

Reference 14

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Observation ae870c2d-3bff-4b65-9408-bb11a001004f · outbound

This paper cites The Science of the Einstein Telescope.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr The Science of the Einstein Telescope

Reference 15

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Observation b3071fb1-3d2f-4437-bfb0-c38dffb5630d · outbound

This paper cites LISA Definition Study Report.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr LISA Definition Study Report

Reference 16

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Observation dfce6b98-4215-47d3-9679-da791843c14c · outbound

This paper cites Testing General Relativity with Present and Future Astrophysical Observations.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Testing General Relativity with Present and Future Astrophysical Observations

Reference 17

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Observation d1998808-bc33-4b7c-b557-fd3df8d0965a · outbound

This paper cites Prospects for Fundamental Physics with LISA.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Prospects for Fundamental Physics with LISA

Reference 18

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.430022Z

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Observation 9b960141-58cb-4126-8416-8d6d67093fc0 · outbound

This paper cites Regge and J.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Regge and J

Reference 19

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Observation 196d4557-f811-42a4-a21c-db6d531fa3b8 · outbound

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Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Unresolved cited work

Reference 20

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Observation f94ddeb6-7f7b-4ade-b448-461bdd82a1d6 · outbound

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Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Unresolved cited work

Reference 21

Resolution: unresolved; raw_fallback, observed 2026-05-16T14:41:02.874252Z

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Observation 17d56270-121b-41ac-af9f-b6d1edf11529 · outbound

This paper cites Quasi-normal modes of rotating black holes in Einstein-dilaton Gauss-Bonnet gravity: the first order in rotation.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Quasi-normal modes of rotating black holes in Einstein-dilaton Gauss-Bonnet gravity: the first order in rotation

Reference 22

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.396267Z

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Observation cbf4cac5-5153-4ead-80c9-7d5cbfd9b087 · outbound

This paper cites Quasinormal modes of slowly-rotating black holes in dynamical Chern-Simons gravity.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Quasinormal modes of slowly-rotating black holes in dynamical Chern-Simons gravity

Reference 23

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.471128Z

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Observation abd44054-9d18-4597-86b9-c8500db0ab73 · outbound

This paper cites Analytical computation of quasi-normal modes of slowly-rotating black-holes in dCS gravity.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Analytical computation of quasi-normal modes of slowly-rotating black-holes in dCS gravity

Reference 24

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.534088Z

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Observation 8a9ec034-fa35-4e06-b695-0b0882e87300 · outbound

This paper cites Quasi-normal modes of rotating black holes in Einstein-dilaton Gauss-Bonnet gravity: the second order in rotation.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Quasi-normal modes of rotating black holes in Einstein-dilaton Gauss-Bonnet gravity: the second order in rotation

Reference 25

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.427311Z

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Observation f4b8c653-a2c7-433b-b57b-dca459db155d · outbound

This paper cites The universal Teukolsky equations and black hole perturbations in higher-derivative gravity.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr The universal Teukolsky equations and black hole perturbations in higher-derivative gravity

Reference 26

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.531193Z

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Observation 50db0354-0385-4c48-8ae5-139533df975a · outbound

This paper cites Perturbations of spinning black holes in dynamical Chern-Simons gravity I. Slow rotation equations.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Perturbations of spinning black holes in dynamical Chern-Simons gravity I. Slow rotation equations

Reference 27

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.313169Z

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Observation c20fe1dd-022e-4153-82cd-55674f39948d · outbound

This paper cites Teukolsky equation for near-extremal black holes beyond general relativity: near-horizon analysis.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Teukolsky equation for near-extremal black holes beyond general relativity: near-horizon analysis

Reference 28

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.452842Z

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Observation 66448a8f-833a-41ad-b8a8-5917a532ef66 · outbound

This paper cites Higher-derivative corrections to the Kerr quasinormal mode spectrum.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Higher-derivative corrections to the Kerr quasinormal mode spectrum

Reference 29

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.354441Z

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Observation e61850d4-8c1a-498a-bfbc-a3f552ea4875 · outbound

This paper cites Quasi-normal mode frequencies and gravitational perturbations of black holes with any subextremal spin in modified gravity through METRICS: the scalar-Gauss-Bonnet gravity case.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Quasi-normal mode frequencies and gravitational perturbations of black holes with any subextremal spin in modified gravity through METRICS: the scalar-Gauss-Bonnet gravity case

Reference 30

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.518980Z

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Observation f25b1b24-a044-4118-926d-9555c09f42c2 · outbound

This paper cites Ringing out General Relativity: Quasi-normal mode frequencies for black holes of any spin in modified gravity.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Ringing out General Relativity: Quasi-normal mode frequencies for black holes of any spin in modified gravity

Reference 31

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.445163Z

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Observation c671b2db-deea-46d0-add9-a6c63a7bc288 · outbound

This paper cites Quasinormal modes of rapidly rotating Einstein-Gauss-Bonnet-dilaton black holes.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Quasinormal modes of rapidly rotating Einstein-Gauss-Bonnet-dilaton black holes

Reference 32

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.335883Z

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Observation a9c4b15a-0552-4568-b6d8-9bb48b265c8b · outbound

This paper cites an unresolved cited work.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Unresolved cited work

Reference 33

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.414167Z

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Observation 010f88bf-5ec1-481a-b1f3-068a95993ae8 · outbound

This paper cites Perturbations of spinning black holes beyond General Relativity: Modified Teukolsky equation.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Perturbations of spinning black holes beyond General Relativity: Modified Teukolsky equation

Reference 34

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.474007Z

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Observation a8369d41-7851-46d4-9f9b-9000d439b5dd · outbound

This paper cites An approach to computing spectral shifts for black holes beyond Kerr.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr An approach to computing spectral shifts for black holes beyond Kerr

Reference 35

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.409344Z

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Observation 0016f5d4-422b-46d4-9051-ccf7fc31654f · outbound

This paper cites Parametrized quasi-normal mode framework for modified Teukolsky equations.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Parametrized quasi-normal mode framework for modified Teukolsky equations

Reference 36

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.387469Z

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Observation 5be370f9-98bc-497f-a75b-8e6bc71d1469 · outbound

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Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Unresolved cited work

Reference 37

Resolution: unresolved; raw_fallback, observed 2026-05-16T14:41:02.885291Z

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Observation af1d84cc-7178-48e2-a35e-2d8e322471d6 · outbound

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Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Unresolved cited work

Reference 38

Resolution: unresolved; raw_fallback, observed 2026-05-16T14:41:02.877996Z

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No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation a0e5db22-10c3-43ca-82e0-663668213898 · outbound

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Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Unresolved cited work

Reference 39

Resolution: unresolved; raw_fallback, observed 2026-05-16T14:41:02.865481Z

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Observation 3abc51a5-c177-486f-9e3b-60e65dceff7d · outbound

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Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Unresolved cited work

Reference 40

Resolution: unresolved; raw_fallback, observed 2026-05-16T14:41:02.879860Z

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Observation 8602b14c-778e-4455-9c28-605a030568dd · outbound

This paper cites Black hole scalarization induced by the spin -- 2+1 time evolution.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Black hole scalarization induced by the spin -- 2+1 time evolution

Reference 41

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.476731Z

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Observation 766b5633-e6bf-433f-91b0-0b427f6bdff2 · outbound

This paper cites vibrations.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr vibrations

Reference 42

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T14:41:02.883669Z

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Observation ff2a570b-c723-4be4-bec4-dab36d07a0f3 · outbound

This paper cites Ferrari and B.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Ferrari and B

Reference 43

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T14:41:02.881780Z

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Observation 70959b9f-2a7e-459e-af2f-8ce59c7fe6dd · outbound

This paper cites Post-Kerr black hole spectroscopy.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Post-Kerr black hole spectroscopy

Reference 44

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.513247Z

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Observation 1a59290c-e538-4d70-a861-fb91f449cc4c · outbound

This paper cites Axisymmetric black holes allowing for separation of variables in the Klein-Gordon and Hamilton-Jacobi equation.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Axisymmetric black holes allowing for separation of variables in the Klein-Gordon and Hamilton-Jacobi equation

Reference 45

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.527878Z

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Observation f18f0a10-6be8-478a-afec-df0651a754f2 · outbound

This paper cites Pedrotti,Studies on Quasi-Normal Modes and Shad- ows of Black Holes, Master’s thesis, Trento U.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Pedrotti,Studies on Quasi-Normal Modes and Shad- ows of Black Holes, Master’s thesis, Trento U

Reference 46

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T14:41:02.887836Z

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Observation 6e8a4512-882c-4974-971f-86b7d879e4d9 · outbound

This paper cites Quasinormal modes-shadow correspondence for rotating regular black holes.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Quasinormal modes-shadow correspondence for rotating regular black holes

Reference 47

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.413851Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation aff8c10b-5bb7-4b95-9a61-f5fcbb8c6a67 · outbound

This paper cites Berti, V.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Berti, V

Reference 48

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.483149Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation b4dc0765-3fd5-4e09-8807-97bc1a4ea71c · outbound

This paper cites The Quasinormal Mode Spectrum of a Kerr Black Hole in the Eikonal Limit.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr The Quasinormal Mode Spectrum of a Kerr Black Hole in the Eikonal Limit

Reference 49

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.455281Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation eb4f5cbf-fcf4-4385-918e-5f2bab03152f · outbound

This paper cites Eikonal quasinormal modes of black holes beyond General Relativity.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Eikonal quasinormal modes of black holes beyond General Relativity

Reference 50

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.373707Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation cdc2fa77-f6f2-4b6c-93d3-7982f0900616 · outbound

This paper cites an unresolved cited work.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Unresolved cited work

Reference 51

Resolution: unresolved; raw_fallback, observed 2026-05-16T14:41:02.876134Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 280cf415-26a2-46e7-b3b2-93e35b90d092 · outbound

This paper cites Black Hole Shadow and other Observables away from the Horizon: Extending the Effective Metric Descriptions.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Black Hole Shadow and other Observables away from the Horizon: Extending the Effective Metric Descriptions

Reference 52

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.442132Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation b781c69c-60e1-4855-a03a-008e4d727659 · outbound

This paper cites Del Piano, C.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Del Piano, C

Reference 53

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.419450Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation b0f7753b-81a4-44c2-b1f6-d8810a882694 · outbound

This paper cites Photon Rings around Kerr and Kerr-like Black Holes.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Photon Rings around Kerr and Kerr-like Black Holes

Reference 54

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.461454Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 9057d25d-d648-4b1b-81e4-1443ea3082c0 · outbound

This paper cites A Metric for Rapidly Spinning Black Holes Suitable for Strong-Field Tests of the No-Hair Theorem.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr A Metric for Rapidly Spinning Black Holes Suitable for Strong-Field Tests of the No-Hair Theorem

Reference 55

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.347483Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 76a935f2-17e5-40d3-88ac-00109fede5b2 · outbound

This paper cites General parametrization of axisymmetric black holes in metric theories of gravity.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr General parametrization of axisymmetric black holes in metric theories of gravity

Reference 56

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.379402Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation a48028d6-9933-41c1-a91c-c77b66f9fd9b · outbound

This paper cites On the connection of spacetime separability and spherical photon orbits.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr On the connection of spacetime separability and spherical photon orbits

Reference 57

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.492698Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 640f7f6e-bb48-430f-b9cc-7205dcc43cf4 · outbound

This paper cites Thermal behavior of a radially deformed black hole spacetime.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Thermal behavior of a radially deformed black hole spacetime

Reference 58

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.467530Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 22f8a0a9-e005-4050-a35b-30c69a7b40bf · outbound

This paper cites Superradiance in Kerr-like black holes.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Superradiance in Kerr-like black holes

Reference 59

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.486380Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation cab38c09-34b5-43f0-928b-4f90d1128866 · outbound

This paper cites Preserving Kerr symmetries in deformed spacetimes.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Preserving Kerr symmetries in deformed spacetimes

Reference 60

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.470480Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 3e8ef1b4-bd29-4c6a-a868-5a9f52011d9e · outbound

This paper cites Dynamics of Scalar Fields in the Background of Rotating Black Holes.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Dynamics of Scalar Fields in the Background of Rotating Black Holes

Reference 61

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.431203Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 9600a9ef-cc68-4468-8a39-910f6fed2984 · outbound

This paper cites A family of solutions to the inverse problem in gravitation: building a theory around a metric.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr A family of solutions to the inverse problem in gravitation: building a theory around a metric

Reference 62

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.400129Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 50fc3f11-9b95-48bd-a2a8-3241fb7db93c · outbound

This paper cites Exact theory for the Rezzolla-Zhidenko metric and self-consistent calculation of quasinormal modes.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Exact theory for the Rezzolla-Zhidenko metric and self-consistent calculation of quasinormal modes

Reference 63

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.422479Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 7377108b-8294-4cca-97bf-3722cd8780c4 · outbound

This paper cites Testing the black hole "no-hair" hypothesis.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Testing the black hole "no-hair" hypothesis

Reference 64

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.343389Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 45d73f65-2d1e-434a-bae9-039a79a84009 · outbound

This paper cites Are LIGO's Black Holes Made From Smaller Black Holes?.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Are LIGO's Black Holes Made From Smaller Black Holes?

Reference 65

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.312464Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 332b8394-4d15-4c8d-9726-031006aa304e · outbound

This paper cites Nonlinear Effects In Black Hole Ringdown From Scattering Experiments I: spin and initial data dependence of quadratic mode coupling.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Nonlinear Effects In Black Hole Ringdown From Scattering Experiments I: spin and initial data dependence of quadratic mode coupling

Reference 66

Resolution: metadata mismatch; arxiv_id, observed 2026-05-16T14:41:02.450181Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation dab04f67-b47c-4497-af9d-dd4b0db8cd37 · outbound

This paper cites De Amicis et al., (2024), arXiv:2412.06887 [gr-qc].

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr De Amicis et al., (2024), arXiv:2412.06887 [gr-qc]

Reference 67

Resolution: metadata mismatch; arxiv_id, observed 2026-05-16T14:41:02.496111Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation b4b17bb1-453b-4f90-a417-dfa9302fb18e · outbound

This paper cites Quasinormal-mode spectrum of Kerr black holes and its geometric interpretation.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Quasinormal-mode spectrum of Kerr black holes and its geometric interpretation

Reference 68

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.468186Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation a0872dbe-c87f-4a52-9426-896095a26cee · outbound

This paper cites Geodesic stability, Lyapunov exponents and quasinormal modes.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Geodesic stability, Lyapunov exponents and quasinormal modes

Reference 69

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.504638Z

Source-reported events for the cited work

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Observation 13279797-1537-4800-82d4-8b7bedb468d8 · outbound

This paper cites Are eikonal quasinormal modes linked to the unstable circular null geodesics?.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Are eikonal quasinormal modes linked to the unstable circular null geodesics?

Reference 70

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.320537Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 79b4ccd3-9eb7-47ab-8e3b-993318b9e7c9 · outbound

This paper cites Capozziello and V.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Capozziello and V

Reference 71

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T14:41:02.889975Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation f4655816-9616-4395-9f19-3c239a52b238 · outbound

This paper cites Comparing Equivalent Gravities: common features and differences.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Comparing Equivalent Gravities: common features and differences

Reference 72

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.318923Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 3c34f754-2db1-4f19-a832-9e679a884d83 · outbound

This paper cites The Equivalence Principle as a Noether Symmetry.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr The Equivalence Principle as a Noether Symmetry

Reference 73

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.479880Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 1755f942-842c-4375-ad67-7165cadf59ad · outbound

This paper cites Black Hole Ringing, Quasinormal Modes, and Light Rings.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Black Hole Ringing, Quasinormal Modes, and Light Rings

Reference 74

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.476722Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation fb461f1b-9682-47d6-870d-3bb0c61152a4 · outbound

This paper cites Further clarification on quasinormal modes/circular null geodesics correspondence.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Further clarification on quasinormal modes/circular null geodesics correspondence

Reference 75

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.524649Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 4edceb13-5fcc-4cb3-8ab5-ee2d3a677801 · outbound

This paper cites qnm: A Python package for calculating Kerr quasinormal modes, separation constants, and spherical-spheroidal mixing coefficients.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr qnm: A Python package for calculating Kerr quasinormal modes, separation constants, and spherical-spheroidal mixing coefficients

Reference 76

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.327802Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 99c4a8e1-ddad-4f45-9f50-ee9827aaa112 · outbound

This paper cites Quantifying Systematic Biases in Black Hole Spectroscopy.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Quantifying Systematic Biases in Black Hole Spectroscopy

Reference 77

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.327948Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation b47224d1-d72e-4762-b440-2aca7fcb1311 · outbound

This paper cites Measuring deviations from the Kerr geometry with black hole ringdown.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Measuring deviations from the Kerr geometry with black hole ringdown

Reference 78

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.499019Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation b47d3519-57e5-447b-bb7a-f7058bf1f29f · outbound

This paper cites Listening to the Universe with Next Generation Ground-Based Gravitational-Wave Detectors.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Listening to the Universe with Next Generation Ground-Based Gravitational-Wave Detectors

Reference 79

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.521963Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation b6d0ab04-cae1-4cc6-8159-12644cdf4e54 · outbound

This paper cites About the Significance of Quasinormal Modes of Black Holes.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr About the Significance of Quasinormal Modes of Black Holes

Reference 80

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.516235Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation e288b15f-9fe1-4a85-b2a2-676b4afe111d · outbound

This paper cites Stability of the fundamental quasinormal mode in time-domain observations against small perturbations.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Stability of the fundamental quasinormal mode in time-domain observations against small perturbations

Reference 81

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.463801Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 688a70d9-639b-4559-a374-c9a874a5042f · outbound

This paper cites Quasinormal modes in higher derivative gravity: testing the black hole parametrization and sensitivity of overtones.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Quasinormal modes in higher derivative gravity: testing the black hole parametrization and sensitivity of overtones

Reference 82

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.438558Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 15dba2d8-d187-42c9-9f64-8764688dea74 · outbound

This paper cites Probing higher curvature gravity via ringdown with overtones.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Probing higher curvature gravity via ringdown with overtones

Reference 83

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.448648Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation a94cbe55-7fa8-4edb-af2f-9d89c286a2f4 · outbound

This paper cites Steppohn, S.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Steppohn, S

Reference 84

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.473701Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation a9cd7ec3-a7a9-4f82-b5a1-b777829f942e · outbound

This paper cites Isospectrality in Effective Field Theory Extensions of General Relativity.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Isospectrality in Effective Field Theory Extensions of General Relativity

Reference 85

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.382854Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 8f71dd10-43e2-476b-8497-3aac9431a111 · outbound

This paper cites Thomopoulos, S.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Thomopoulos, S

Reference 86

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.507424Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 6568f7e8-146c-49e4-941b-ad67310380ed · outbound

This paper cites Seidel and S.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Seidel and S

Reference 87

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T14:41:02.872613Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 7717367a-feab-4d48-a3f4-6de78e9f6ddb · outbound

This paper cites an unresolved cited work.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Unresolved cited work

Reference 88

Resolution: unresolved; raw_fallback, observed 2026-05-16T14:41:02.869340Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 41ad126f-1f86-484d-b033-70e321924e10 · outbound

This paper cites Quasinormal modes of rotating black holes beyond general relativity in the WKB approximation.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Quasinormal modes of rotating black holes beyond general relativity in the WKB approximation

Reference 89

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.489496Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 7ca6a90a-a17f-42d7-896e-fa0535fba52f · outbound

This paper cites an unresolved cited work.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Unresolved cited work

Reference 90

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.510428Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation ded2b396-5ec5-4696-8587-5aa45fe51af4 · outbound

This paper cites an unresolved cited work.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Unresolved cited work

Reference 91

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.403671Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 6da1eab7-697a-45b9-a928-c46ea049189e · outbound

This paper cites Late time tails from momentarily stationary, compact initial data in Schwarzschild spacetimes.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Late time tails from momentarily stationary, compact initial data in Schwarzschild spacetimes

Reference 92

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.367036Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 925a71c3-0d37-4ce7-86c8-d9966626e6b2 · outbound

This paper cites Scalar-field perturbations from a particle orbiting a black hole using numerical evolution in 2+1 dimensions.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Scalar-field perturbations from a particle orbiting a black hole using numerical evolution in 2+1 dimensions

Reference 93

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.396634Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 72743b22-abe6-423d-8e13-4cc0d180378f · outbound

This paper cites Numerical integration of the Teukolsky Equation in the time domain.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Numerical integration of the Teukolsky Equation in the time domain

Reference 94

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.335219Z

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No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation daa23a7c-c5f8-4e8f-8e0e-c4957455d390 · outbound

This paper cites Mode-Coupling in Rotating Gravitational Collapse of a Scalar Field.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Mode-Coupling in Rotating Gravitational Collapse of a Scalar Field

Reference 95

Resolution: verified exact; local_arxiv, observed 2026-05-16T14:41:02.410381Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 65eeea40-cf90-4f72-92ee-0114e98002c7 · outbound

This paper cites BlackJAX: Composable Bayesian inference in JAX.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr BlackJAX: Composable Bayesian inference in JAX

Reference 96

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:41:02.502010Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 3a36b2ad-8757-4762-905b-131aada07442 · outbound

This paper cites Bradbury, R.

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr Bradbury, R

Reference 97

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T14:41:02.871042Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

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