{"as_of":"2026-08-05T00:24:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:24ad7daae0e82924157394cb68f7bd69a0e1248ac2c96f9f6e3cc2dfd4937afb","coverage":[{"denominator":107,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-31T20:45:39.059549Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-04T06:34:03.388597+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2607.28003/citation-record","integrity":"/paper/2607.28003/integrity","json":"/paper/2607.28003/citation-record.json","paper":"/paper/2607.28003"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:34.438559Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:34.438559Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:76db1dc2d8e9b650d4796a10dd4137504242cf2e2d694db1ca62559acf6d34a2","observation_id":"3444ed6b-f098-4681-b280-7867d6554876","resolution":{"observed_at":"2026-07-31T20:45:34.438559Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:34.488028Z","title":"For larger coupling simulations, we find that we can- not set ˆσarbitrarily low and still retain stability in the numerical evolution","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:34.488028Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:196d305a4fe31a3ddeb80d68636f808adec9d8798d68ce6d615905f809f620e3","observation_id":"3b3f033b-2abd-4b6f-8613-61f912ffe803","resolution":{"observed_at":"2026-07-31T20:45:34.488028Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:34.533827Z","title":"The GW strainhis ex- tracted at future null-infinityI + using data recorded at R/M= 170 for Cauchy Characteristic Evolution (CCE) —see also Sec","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:34.533827Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:cfc0a2ec54b0687dad16295bce5ea719e1e883e5f5ce94de46e984c51396a080","observation_id":"19f02dca-ae6d-4034-8aae-a2e2a0956f26","resolution":{"observed_at":"2026-07-31T20:45:34.533827Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:34.581538Z","title":"when computing phase differences as in our companionLetter[45]","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:34.581538Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:6cb5b4afd667c44d63fbe306e926b08cc7b4a191a0f589078215f758de8c3a94","observation_id":"4c5d58dc-6e8e-4b81-9272-30462e78a436","resolution":{"observed_at":"2026-07-31T20:45:34.581538Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:34.634618Z","title":"However, constraint-satisfying quasistationary initial data has not yet been constructed for scalarized binaries in this theory —in Ref","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:34.634618Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:bdcf39d94d347ad1da4d0fd2ea75e5086856ac29ed02b71fa659cfdbebe3e430","observation_id":"1f7b5757-0655-4577-be92-bf4f3e38ee4e","resolution":{"observed_at":"2026-07-31T20:45:34.634618Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:34.683154Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:34.683154Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:58802e3bf2ee07393b9134eb6d0558183998404cd0f74926d123147106331b17","observation_id":"27bf940e-d2cb-4db6-b27b-edda36b2dd24","resolution":{"observed_at":"2026-07-31T20:45:34.683154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:34.722611Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:34.722611Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:228f41cc4e26de89ada6a6cb1dd33887c77db26de60367a1395de1116fe54e22","observation_id":"b55c9a94-60be-470c-bbe2-31656800e799","resolution":{"observed_at":"2026-07-31T20:45:34.722611Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:34.765697Z","title":"Both Eab andB ab are symmetric spatial tensors","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:34.765697Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:38fce0d5b68fd1b4dc37666e8c539e0c72987b4d58567f595bd9b405fda7ed75","observation_id":"4cacc847-ccc8-42d3-81be-f124013e80ac","resolution":{"observed_at":"2026-07-31T20:45:34.765697Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:34.810376Z","title":"(5)] in two parts Hab =−8( ˆH (C) ab + ˆH (R) ab ),(D13) where ˆH (C) ab ≡C acbd∇c∇df(Ψ) (D14) ˆH (R) ab ≡(P acbd −C acbd)∇c∇df(Ψ),(D15) andP acbd was defined in Eq","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:34.810376Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:a1aa6530f814a49c143272bf1dfa55d1a9ad0bb8f2fb27d80aedbffeea42b707","observation_id":"87c52160-a210-4d39-a144-f79a203f5b77","resolution":{"observed_at":"2026-07-31T20:45:34.810376Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:34.845996Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:34.845996Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:055e59344997e55ecffe73d39a2bb8c4b26135f63c3e682cdaccc466deb4bf84","observation_id":"bb2cf47b-2fb6-440f-8a2d-5db25baca09c","resolution":{"observed_at":"2026-07-31T20:45:34.845996Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:34.884685Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:34.884685Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:078324dc248c299458e24074e472dd2bf434bb97fc75304143760c13d91324ff","observation_id":"e75323b8-f7de-45cb-a613-008599b6f279","resolution":{"observed_at":"2026-07-31T20:45:34.884685Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.07274","last_updated":"2015-12-02T03:09:26Z","snapshot_observed_at":"2026-07-06T04:07:31.249848Z","submitted_at":"2015-01-28T21:00:11Z","title":"Testing General Relativity with Present and Future Astrophysical Observations","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.07274","snapshot_observed_at":"2026-07-31T20:45:34.927096Z","title":"Bertiet al., Testing General Relativity with Present and Future Astrophysical Observations, Class","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:34.927096Z"},"links":{"cited_paper":"/paper/1501.07274","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:f22c6418f73d5db623e77a583d15be322f3c5a6d28f3fea4320fd9a1a86be516","observation_id":"a19fd1c6-82d0-4720-96d4-1e276f78d2b5","resolution":{"observed_at":"2026-07-31T20:45:34.927096Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.09241","last_updated":"2018-12-04T18:17:04Z","snapshot_observed_at":"2026-07-06T06:52:03.002610Z","submitted_at":"2018-07-24T17:24:45Z","title":"Dark Energy in light of Multi-Messenger Gravitational-Wave astronomy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.09241","snapshot_observed_at":"2026-07-31T20:45:34.939660Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:34.939660Z"},"links":{"cited_paper":"/paper/1807.09241","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:bcd457399d3960a016ac71f03d259ff46eb905c049cbd282d71fec2b0dfcea26","observation_id":"b88a5ad6-b46c-434b-945c-0d753cae8d24","resolution":{"observed_at":"2026-07-31T20:45:34.939660Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.12263","last_updated":"2025-08-29T11:52:35Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-03-15T21:04:14Z","title":"The Science of the Einstein Telescope","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.12263","snapshot_observed_at":"2026-07-31T20:45:34.966485Z","title":"Abacet al.(ET), The Science of the Einstein Tele- scope, (2025), arXiv:2503.12263 [gr-qc]","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:34.966485Z"},"links":{"cited_paper":"/paper/2503.12263","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:2e3ab3f14b985231b0640b4080510b0cba6c5ffc40626d10ae47b3a43cb1cc93","observation_id":"0125a9d0-df90-4c78-9aa7-84cd8147d0d3","resolution":{"observed_at":"2026-07-31T20:45:34.966485Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.09882","last_updated":"2021-10-06T14:54:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2021-09-20T23:34:33Z","title":"A Horizon Study for Cosmic Explorer: Science, Observatories, and Community","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.09882","snapshot_observed_at":"2026-07-31T20:45:35.006869Z","title":"Evanset al., A Horizon Study for Cosmic Explorer: Science, Observatories, and Community, arXiv:2109.09882 [astro-ph.IM] (2021)","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:35.006869Z"},"links":{"cited_paper":"/paper/2109.09882","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:5adb756324d5c52238e7c44a8ac72fc161cc112741419969a2642e4c0d625123","observation_id":"a812c76a-f6ce-451a-9787-d2ff15af6c02","resolution":{"observed_at":"2026-07-31T20:45:35.006869Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.07571","last_updated":"2024-02-12T11:06:12Z","snapshot_observed_at":"2026-08-02T13:54:50.876049Z","submitted_at":"2024-02-12T11:06:12Z","title":"LISA Definition Study Report","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.07571","snapshot_observed_at":"2026-07-31T20:45:35.079217Z","title":"Colpiet al.(LISA), LISA Definition Study Report, (2024), arXiv:2402.07571 [astro-ph.CO]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:35.079217Z"},"links":{"cited_paper":"/paper/2402.07571","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:0574c07a0f4d78a1e57ead371f07def0b718c43bf389858e03860e7df8073039","observation_id":"6fa9fa65-3e8f-4732-b722-753e56bc638a","resolution":{"observed_at":"2026-07-31T20:45:35.079217Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.07421","last_updated":"2017-11-10T00:49:58Z","snapshot_observed_at":"2026-07-06T05:48:03.249146Z","submitted_at":"2017-06-22T17:53:09Z","title":"Fixing extensions to General Relativity in the non-linear regime","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.07421","snapshot_observed_at":"2026-07-31T20:45:35.137434Z","title":"Cayuso, N","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:35.137434Z"},"links":{"cited_paper":"/paper/1706.07421","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:e859bd7895953d780039cba63eaada9d7172a35dd7ef77fc4747bebc99389e94","observation_id":"7ddd7e5d-d6f2-4e7e-ae49-cb4fad848dc4","resolution":{"observed_at":"2026-07-31T20:45:35.137434Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.05177","last_updated":"2018-11-22T11:22:53Z","snapshot_observed_at":"2026-07-06T07:07:32.090066Z","submitted_at":"2018-10-11T18:00:25Z","title":"Black holes and binary mergers in scalar Gauss-Bonnet gravity: scalar field dynamics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.05177","snapshot_observed_at":"2026-07-31T20:45:35.196324Z","title":"Witek, L","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:35.196324Z"},"links":{"cited_paper":"/paper/1810.05177","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:bb533aff75ead4d7ee13c0b8ec9804f0c396864d3c4c663b5548277ad643d3ff","observation_id":"17b33593-3044-4370-b3e4-da5238750d4c","resolution":{"observed_at":"2026-07-31T20:45:35.196324Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.12251","last_updated":"2019-09-26T16:57:32Z","snapshot_observed_at":"2026-07-06T08:24:54.691667Z","submitted_at":"2019-09-26T16:57:32Z","title":"Stability of rotating black holes in Einstein dilaton Gauss-Bonnet gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.12251","snapshot_observed_at":"2026-07-31T20:45:35.287868Z","title":"Okounkova, Stability of Rotating Black Holes in Ein- stein Dilaton Gauss-Bonnet Gravity, Phys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:35.287868Z"},"links":{"cited_paper":"/paper/1909.12251","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:1cdcb723f004aaaaeedc1623979c439858ead6af534ae44e4713433483933501","observation_id":"1ebdb8eb-f4cd-4b0e-bd01-2a30528b8e5b","resolution":{"observed_at":"2026-07-31T20:45:35.287868Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.02588","last_updated":"2020-05-08T03:16:13Z","snapshot_observed_at":"2026-07-06T08:35:15.491391Z","submitted_at":"2019-11-06T19:00:37Z","title":"Numerical relativity simulation of GW150914 beyond general relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.02588","snapshot_observed_at":"2026-07-31T20:45:35.382118Z","title":"Okounkova, L","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:35.382118Z"},"links":{"cited_paper":"/paper/1911.02588","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:09d75efa9bf7ec8db6532f250f4ea81e79d7215ef65c63a322710b40b80ede7e","observation_id":"8dff4133-33aa-4196-b755-c0b60c5160be","resolution":{"observed_at":"2026-07-31T20:45:35.382118Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.03571","last_updated":"2020-01-10T17:33:45Z","snapshot_observed_at":"2026-07-06T08:49:47.907635Z","submitted_at":"2020-01-10T17:33:45Z","title":"Numerical relativity simulation of GW150914 in Einstein dilaton Gauss-Bonnet gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.03571","snapshot_observed_at":"2026-07-31T20:45:35.455566Z","title":"Okounkova, Numerical relativity simulation of GW150914 in Einstein dilaton Gauss-Bonnet gravity, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:35.455566Z"},"links":{"cited_paper":"/paper/2001.03571","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:360cc6285f10fb690c48b3099edf05add565226ccb6340882788d18e07b15738","observation_id":"b688dfdb-b8b4-46ab-8268-8dc0713eda69","resolution":{"observed_at":"2026-07-31T20:45:35.455566Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00963","last_updated":"2019-04-01T16:54:50Z","snapshot_observed_at":"2026-07-06T07:43:06.427641Z","submitted_at":"2019-04-01T16:54:50Z","title":"Well-posedness of cubic Horndeski theories","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.00963","snapshot_observed_at":"2026-07-31T20:45:35.520430Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:35.520430Z"},"links":{"cited_paper":"/paper/1904.00963","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:5c0412f3ba474708310cb2e98a07ce024cc70a85c7cc0c970483acb1fe54bb5e","observation_id":"a1cef1be-6ce1-4e4b-ac7c-807d38943378","resolution":{"observed_at":"2026-07-31T20:45:35.520430Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.04327","last_updated":"2020-05-28T15:35:27Z","snapshot_observed_at":"2026-08-04T21:05:06.535100Z","submitted_at":"2020-03-09T18:00:05Z","title":"Well-posed formulation of scalar-tensor effective field theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.04327","snapshot_observed_at":"2026-07-31T20:45:35.587114Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:35.587114Z"},"links":{"cited_paper":"/paper/2003.04327","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:3fd43d1751cd5b2d9ab206d3285952880e5a5ca25ff155696ab1a6d2d0a6af85","observation_id":"3816ad0e-0e40-4e00-8bbb-2fb98aaca00e","resolution":{"observed_at":"2026-07-31T20:45:35.587114Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.08398","last_updated":"2020-05-28T15:32:47Z","snapshot_observed_at":"2026-07-06T09:05:40.749266Z","submitted_at":"2020-03-18T18:00:03Z","title":"Well-posed formulation of Lovelock and Horndeski theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.08398","snapshot_observed_at":"2026-07-31T20:45:35.654648Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:35.654648Z"},"links":{"cited_paper":"/paper/2003.08398","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:bd4b7ae9844ba52660fafa13904a4e8be550abc99b2f33ce1eeaf204d6340d9b","observation_id":"45664937-96a7-4dad-8c1c-55131a188d9b","resolution":{"observed_at":"2026-07-31T20:45:35.654648Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.13720","last_updated":"2020-06-19T18:05:11Z","snapshot_observed_at":"2026-07-06T09:23:58.059739Z","submitted_at":"2020-05-28T00:53:13Z","title":"Nonlinear/non-iterative treatment of EFT-motivated gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.13720","snapshot_observed_at":"2026-07-31T20:45:35.723378Z","title":"Cayuso and L","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:35.723378Z"},"links":{"cited_paper":"/paper/2005.13720","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:fa92f0e02f3214b2cd1437410517723e560399b62f1aedc18bf41fc86fd1957c","observation_id":"6d3a5046-e4a8-40f0-ae92-2802efc18722","resolution":{"observed_at":"2026-07-31T20:45:35.723378Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.03547","last_updated":"2021-02-20T20:52:47Z","snapshot_observed_at":"2026-07-06T10:12:22.062254Z","submitted_at":"2020-11-06T19:00:00Z","title":"Evolution of Einstein-scalar-Gauss-Bonnet gravity using a modified harmonic formulation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.03547","snapshot_observed_at":"2026-07-31T20:45:35.818721Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:35.818721Z"},"links":{"cited_paper":"/paper/2011.03547","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:338574f92a034381b0a1c986a028a14682870e9ab20496228f2b69776514143e","observation_id":"f76f62f4-1baa-457e-9de9-024b65067bac","resolution":{"observed_at":"2026-07-31T20:45:35.818721Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.05648","last_updated":"2022-02-15T15:48:25Z","snapshot_observed_at":"2026-07-06T11:28:24.094754Z","submitted_at":"2021-07-12T18:00:04Z","title":"No evidence of kinetic screening in simulations of merging binary neutron stars beyond general relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.05648","snapshot_observed_at":"2026-07-31T20:45:35.889930Z","title":"Bezares, R","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:35.889930Z"},"links":{"cited_paper":"/paper/2107.05648","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:7c560875466f15d206b8bf31e716a84a1ea2000e341fcccdba091165e88e5f29","observation_id":"d3b7e362-f069-4f6b-9f4c-7e62a2f27333","resolution":{"observed_at":"2026-07-31T20:45:35.889930Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.09186","last_updated":"2022-03-28T10:25:36Z","snapshot_observed_at":"2026-07-06T12:19:44.050065Z","submitted_at":"2021-12-16T20:18:29Z","title":"UV completions, fixing the equations and nonlinearities in $k$-essence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.09186","snapshot_observed_at":"2026-07-31T20:45:35.956120Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:35.956120Z"},"links":{"cited_paper":"/paper/2112.09186","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:3dc5403d02e996ae754720b1c7589ba264a4165f99904126774fbe882ab3e2b9","observation_id":"ecbb048c-8aed-455c-a231-93ee9f0639aa","resolution":{"observed_at":"2026-07-31T20:45:35.956120Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.15529","last_updated":"2022-02-21T18:41:19Z","snapshot_observed_at":"2026-07-06T12:23:52.936803Z","submitted_at":"2021-12-31T16:08:15Z","title":"Black Hole Binaries in Cubic Horndeski Theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.15529","snapshot_observed_at":"2026-07-31T20:45:36.025120Z","title":"Figueras and T","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.025120Z"},"links":{"cited_paper":"/paper/2112.15529","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:2a764d81fd535bd65ba2c1629629c56f8c790d89370539798aeb4ad08895aa54","observation_id":"7de69668-52f4-4d9b-8bfc-aaaa9f6e8c19","resolution":{"observed_at":"2026-07-31T20:45:36.025120Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.00014","last_updated":"2022-10-05T08:51:37Z","snapshot_observed_at":"2026-07-06T13:16:05.426540Z","submitted_at":"2022-05-31T18:00:01Z","title":"Fixing the dynamical evolution in scalar-Gauss-Bonnet gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.00014","snapshot_observed_at":"2026-07-31T20:45:36.089360Z","title":"Franchini, M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.089360Z"},"links":{"cited_paper":"/paper/2206.00014","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:de3c17c6b2eaf2f73158a7e187732ff5953e4ea580d50b618c8b6d6dfae5b62a","observation_id":"f063910c-6023-4b4c-b1e7-9e595af0c7d2","resolution":{"observed_at":"2026-07-31T20:45:36.089360Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.09235","last_updated":"2023-01-17T14:49:01Z","snapshot_observed_at":"2026-07-06T14:06:48.707061Z","submitted_at":"2022-10-17T16:29:45Z","title":"Nonlinear studies of binary black hole mergers in Einstein-scalar-Gauss-Bonnet gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.09235","snapshot_observed_at":"2026-07-31T20:45:36.176014Z","title":"Corman, J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.176014Z"},"links":{"cited_paper":"/paper/2210.09235","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:ef7391a831191c720746acdd663ba7bc8282f3dfc8071edef485f39e10313129","observation_id":"71b72a5e-c084-4bdc-9fef-88ad49424244","resolution":{"observed_at":"2026-07-31T20:45:36.176014Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.14470","last_updated":"2022-12-28T20:49:51Z","snapshot_observed_at":"2026-07-06T13:47:00.653824Z","submitted_at":"2022-08-30T18:00:31Z","title":"Well-posedness of the four-derivative scalar-tensor theory of gravity in singularity avoiding coordinates","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.14470","snapshot_observed_at":"2026-07-31T20:45:36.244987Z","title":"Arest´ e Sal´ o, K","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.244987Z"},"links":{"cited_paper":"/paper/2208.14470","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:9a14a4985ad0865e24153b0dc3a95527d025c7b3f02297f3a4fa61bf813ded4e","observation_id":"06fd34f3-e681-4273-9134-26eeeb804323","resolution":{"observed_at":"2026-07-31T20:45:36.244987Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.07246","last_updated":"2023-03-13T16:17:39Z","snapshot_observed_at":"2026-07-06T15:02:40.704180Z","submitted_at":"2023-03-13T16:17:39Z","title":"Modelling self-consistently beyond General Relativity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.07246","snapshot_observed_at":"2026-07-31T20:45:36.315852Z","title":"Cayuso, P","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.315852Z"},"links":{"cited_paper":"/paper/2303.07246","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:6799c46e3d9b98607a10734a1fe64def41cc05d918f75db0c5c12e9374a52378","observation_id":"08986ce8-58e9-4678-ab8d-152877df0f04","resolution":{"observed_at":"2026-07-31T20:45:36.315852Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.04725","last_updated":"2023-06-07T18:41:47Z","snapshot_observed_at":"2026-07-06T15:39:56.892976Z","submitted_at":"2023-06-07T18:41:47Z","title":"Nonlinear Evolution of Quadratic Gravity in 3+1 Dimensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.04725","snapshot_observed_at":"2026-07-31T20:45:36.381963Z","title":"Held and H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.381963Z"},"links":{"cited_paper":"/paper/2306.04725","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:105227548cbfac395d1c90bcb37e6a29ec57549152767e42e179b7a88174c960","observation_id":"30701f0b-e1c1-4ba9-b387-5aa2607d26c0","resolution":{"observed_at":"2026-07-31T20:45:36.381963Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.08775","last_updated":"2024-07-11T18:00:01Z","snapshot_observed_at":"2026-07-06T18:45:01.801741Z","submitted_at":"2024-07-11T18:00:01Z","title":"Well-posed initial value formulation of general effective field theories of gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.08775","snapshot_observed_at":"2026-07-31T20:45:36.447435Z","title":"Figueras, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.447435Z"},"links":{"cited_paper":"/paper/2407.08775","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:80b5c1894a8454f6804fb27ef6268fefee67a6762718aac8f7d7770e73ac1aa3","observation_id":"e8ee84e7-0c32-4885-93a1-fd89a4ddda94","resolution":{"observed_at":"2026-07-31T20:45:36.447435Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:36.546169Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.546169Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:aeb55ebd3639bbce1876af6d9c92854bbea3778a435675f7b9424297f706a71c","observation_id":"e3cdd512-3e17-45b1-aaff-e3ffd6dbca70","resolution":{"observed_at":"2026-07-31T20:45:36.546169Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:36.610220Z","title":"Figueras, ´A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.610220Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:927ac891c42eebfad8ff859a2bab7a324b1261c9434dc87cdc70126dc0a4ba7e","observation_id":"f60989c0-96a1-44f6-8740-4afcba57ee61","resolution":{"observed_at":"2026-07-31T20:45:36.610220Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0507014","last_updated":"2005-07-04T09:12:46Z","snapshot_observed_at":"2026-07-07T03:21:14.244391Z","submitted_at":"2005-07-04T09:12:46Z","title":"Evolution of Binary Black Hole Spacetimes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0507014","snapshot_observed_at":"2026-07-31T20:45:36.657284Z","title":"Pretorius, Evolution of binary black hole spacetimes, Phys","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.657284Z"},"links":{"cited_paper":"/paper/gr-qc/0507014","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:69ce9b305a9f6e19efb0de541d6e740f468e35b21f4033a7cb1ef6472a41b62f","observation_id":"6ec2494c-132b-49a5-b354-f05fa5b4ff4f","resolution":{"observed_at":"2026-07-31T20:45:36.657284Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0511103","last_updated":"2005-11-17T18:01:37Z","snapshot_observed_at":"2026-07-07T03:21:43.331487Z","submitted_at":"2005-11-17T18:01:37Z","title":"Gravitational wave extraction from an inspiraling configuration of merging black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0511103","snapshot_observed_at":"2026-07-31T20:45:36.693957Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.693957Z"},"links":{"cited_paper":"/paper/gr-qc/0511103","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:73f830a806f4f4cd09960dfb4f60856db83c8d2c6d14d415650b24776b5b3cb8","observation_id":"41229eda-51e5-4fd1-a22d-bca1871765f4","resolution":{"observed_at":"2026-07-31T20:45:36.693957Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0511048","last_updated":"2005-11-16T22:32:10Z","snapshot_observed_at":"2026-07-07T03:21:43.331487Z","submitted_at":"2005-11-09T20:30:35Z","title":"Accurate Evolutions of Orbiting Black-Hole Binaries Without Excision","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0511048","snapshot_observed_at":"2026-07-31T20:45:36.733196Z","title":"Campanelli, C","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.733196Z"},"links":{"cited_paper":"/paper/gr-qc/0511048","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:e926b192168a47a32e1c689ae226c339c38869fc15a06873824fcb5328ad1342","observation_id":"e9e28e5c-24b5-4467-bbe4-f8c97e4cf431","resolution":{"observed_at":"2026-07-31T20:45:36.733196Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.13654","last_updated":"2024-06-19T15:57:58Z","snapshot_observed_at":"2026-07-06T18:33:45.816337Z","submitted_at":"2024-06-19T15:57:58Z","title":"Inspiral-merger-ringdown waveforms in Einstein-scalar-Gauss-Bonnet gravity within the effective-one-body formalism","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.13654","snapshot_observed_at":"2026-07-31T20:45:36.771982Z","title":"Juli´ e, L","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.771982Z"},"links":{"cited_paper":"/paper/2406.13654","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:31a1618d8509c0e2edf444958b162b31b4fdc09ef3a4692ab3e50c0d02222a77","observation_id":"8ae66ca6-0267-4534-afec-e5895f9ec20f","resolution":{"observed_at":"2026-07-31T20:45:36.771982Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.6077","last_updated":"2013-12-18T16:36:08Z","snapshot_observed_at":"2026-07-06T03:11:45.494939Z","submitted_at":"2013-04-22T19:58:42Z","title":"A catalog of 174 binary black-hole simulations for gravitational-wave astronomy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.6077","snapshot_observed_at":"2026-07-31T20:45:36.809810Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.809810Z"},"links":{"cited_paper":"/paper/1304.6077","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:b8671895a599ce07f082ddfd2d1e46ad66fefac803727accf128edb5c4ad4d82","observation_id":"709cb17a-ad32-4392-9b41-3f0a1571d178","resolution":{"observed_at":"2026-07-31T20:45:36.809810Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.04831","last_updated":"2019-09-11T16:17:33Z","snapshot_observed_at":"2026-07-06T07:45:01.967120Z","submitted_at":"2019-04-09T18:00:00Z","title":"The SXS Collaboration catalog of binary black hole simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.04831","snapshot_observed_at":"2026-07-31T20:45:36.851508Z","title":"Boyleet al., The SXS Collaboration catalog of binary black hole simulations, Class","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.851508Z"},"links":{"cited_paper":"/paper/1904.04831","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:85b24fd38c378fb54c9b160f7a22f33767b7a046e57fd3deac8ae2632cd4acb8","observation_id":"85f10f0f-e6ce-4330-acd8-26eeb3c8e435","resolution":{"observed_at":"2026-07-31T20:45:36.851508Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:36.898870Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.898870Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:e216b1921d45020aebcc0461008c6ed40c1792661a99ac75d20b5f700dfabd18","observation_id":"e9fbfb4b-037a-4d08-a8a1-dcc5303bcf46","resolution":{"observed_at":"2026-07-31T20:45:36.898870Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:36.935079Z","title":"Armendariz-Picon, T","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.935079Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:c10aec27bc3882418e6e138d96dc3514885d72ecd66e608ecafa1fee59f4eef7","observation_id":"e6f1d6b8-a7b7-4eea-917d-9b564fb07746","resolution":{"observed_at":"2026-07-31T20:45:36.935079Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:36.980815Z","title":null,"venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:36.980815Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:fffb28290aaa8cb12548a3597773d7f1a18d226363d93236db51f7bf5dcbbb2b","observation_id":"4273318f-95c8-41b1-ba29-718d9140f46c","resolution":{"observed_at":"2026-07-31T20:45:36.980815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.12866","last_updated":"2019-07-27T11:46:49Z","snapshot_observed_at":"2026-08-02T13:13:13.040104Z","submitted_at":"2019-04-29T18:00:04Z","title":"Challenges to global solutions in Horndeski's theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.12866","snapshot_observed_at":"2026-07-31T20:45:37.019664Z","title":"Bernard, L","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.019664Z"},"links":{"cited_paper":"/paper/1904.12866","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:946f9ada5f042063c950817396cee5ca940405dc7032d8bc689a00cd800344b6","observation_id":"1e2edcac-fe46-4d22-889b-98f93b64ce57","resolution":{"observed_at":"2026-07-31T20:45:37.019664Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.07546","last_updated":"2021-03-22T16:10:50Z","snapshot_observed_at":"2026-08-04T21:06:40.368330Z","submitted_at":"2020-08-17T18:00:05Z","title":"K-dynamics: well-posed 1+1 evolutions in K-essence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.07546","snapshot_observed_at":"2026-07-31T20:45:37.061019Z","title":"Bezares, M","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.061019Z"},"links":{"cited_paper":"/paper/2008.07546","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:87cf8c5ba03883fb3164255a70d106dd705744773e42579c920a45a36b59cf77","observation_id":"dc4546d1-921a-445b-b811-6f587c1b0a46","resolution":{"observed_at":"2026-07-31T20:45:37.061019Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0702126","last_updated":"2007-02-25T20:49:46Z","snapshot_observed_at":"2026-07-07T03:23:50.925426Z","submitted_at":"2007-02-25T20:49:46Z","title":"Evolving relativistic fluid spacetimes using pseudospectral methods and finite differencing","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0702126","snapshot_observed_at":"2026-07-31T20:45:37.099474Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.099474Z"},"links":{"cited_paper":"/paper/gr-qc/0702126","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:6618ebaacc39c38665ebd02ff0b8d37734dd0d61ae882558ec2888068124b260","observation_id":"af0c6315-9103-4646-9565-5a79cba5776c","resolution":{"observed_at":"2026-07-31T20:45:37.099474Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0809.0002","last_updated":"2008-09-05T15:27:19Z","snapshot_observed_at":"2026-07-06T01:41:40.812259Z","submitted_at":"2008-08-29T20:00:37Z","title":"Evolving black hole-neutron star binaries in general relativity using pseudospectral and finite difference methods","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0809.0002","snapshot_observed_at":"2026-07-31T20:45:37.140479Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.140479Z"},"links":{"cited_paper":"/paper/0809.0002","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:e749ed9af48288a6e908dda790bd9a4709cec7f221ffa34aec7db969f3add085","observation_id":"a8daf930-42c8-41be-83ee-69230d5fed0f","resolution":{"observed_at":"2026-07-31T20:45:37.140479Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.11836","last_updated":"2023-06-13T05:48:42Z","snapshot_observed_at":"2026-07-06T15:19:08.624764Z","submitted_at":"2023-04-24T05:59:16Z","title":"Numerical simulations of black hole-neutron star mergers in scalar-tensor gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.11836","snapshot_observed_at":"2026-07-31T20:45:37.176877Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.176877Z"},"links":{"cited_paper":"/paper/2304.11836","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:d905f162e9a48b82a6916438e2134cc0043da494c7e8e67ff649a52802c8c93f","observation_id":"4b5174cc-0b61-4d2f-a304-236a3abda06c","resolution":{"observed_at":"2026-07-31T20:45:37.176877Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.19038","last_updated":"2024-09-30T17:14:46Z","snapshot_observed_at":"2026-07-06T18:37:51.919811Z","submitted_at":"2024-06-27T09:43:52Z","title":"Binary neutron star mergers using a discontinuous Galerkin-finite difference hybrid method","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.19038","snapshot_observed_at":"2026-07-31T20:45:37.216650Z","title":"Deppeet al., Binary neutron star mergers using a discontinuous Galerkin-finite difference hybrid method, Class","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.216650Z"},"links":{"cited_paper":"/paper/2406.19038","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:df84d8a1c19b261d90a6e3d5896bd4708f07c324da6ec30e202dcb688eb47ad0","observation_id":"df2d2393-b8cf-485c-bd92-7cbf21132b7d","resolution":{"observed_at":"2026-07-31T20:45:37.216650Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.15581","last_updated":"2024-12-18T01:20:15Z","snapshot_observed_at":"2026-07-06T18:19:21.735356Z","submitted_at":"2024-05-24T14:10:36Z","title":"Nonlinear studies of modifications to general relativity: Comparing different approaches","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.15581","snapshot_observed_at":"2026-07-31T20:45:37.261728Z","title":"Corman, L","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.261728Z"},"links":{"cited_paper":"/paper/2405.15581","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:d37495328c7036c4f412c4b16f4668225ccfbb99746a6e9be3268c08b746c82b","observation_id":"8669d646-2742-4dd0-9c61-7a40c5eec209","resolution":{"observed_at":"2026-07-31T20:45:37.261728Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.08410","last_updated":"2021-09-30T17:16:46Z","snapshot_observed_at":"2026-07-06T11:19:38.321360Z","submitted_at":"2021-06-15T20:03:53Z","title":"Numerical renormalization group-based approach to secular perturbation theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.08410","snapshot_observed_at":"2026-07-31T20:45:37.299720Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.299720Z"},"links":{"cited_paper":"/paper/2106.08410","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:86612fc84545d927d3e9856af49a2790beb45c45c79689e0f9960e8baf79163c","observation_id":"bac9492a-19eb-4521-8155-12c869db4924","resolution":{"observed_at":"2026-07-31T20:45:37.299720Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:37.344826Z","title":"Deppe, W","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.344826Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:d1f444e29de7e907461ffd45d28189ebd3b2f4523ca22b4ed8d5ba493ee32d05","observation_id":"e6414e75-cc77-46d4-977b-87273bfe685a","resolution":{"observed_at":"2026-07-31T20:45:37.344826Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:37.383811Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.383811Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:ce0ab7a800a4f412c1d094926261a81c17fbd981197fa59c356566b919b6cd1a","observation_id":"7120875f-78d1-4374-b6fd-ffa299a1dbaf","resolution":{"observed_at":"2026-07-31T20:45:37.383811Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.3622","last_updated":"2014-08-11T23:05:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2013-12-12T20:51:42Z","title":"Black hole hair in generalized scalar-tensor gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.3622","snapshot_observed_at":"2026-07-31T20:45:37.423784Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.423784Z"},"links":{"cited_paper":"/paper/1312.3622","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:05a6714ece5945661f0199548a295f1a5554cb48f85f26ff4461537ab9379c80","observation_id":"1eb7b206-d9f4-498a-9ac0-22f539314c58","resolution":{"observed_at":"2026-07-31T20:45:37.423784Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.1698","last_updated":"2014-11-24T21:21:37Z","snapshot_observed_at":"2026-07-06T03:51:11.258651Z","submitted_at":"2014-08-07T20:00:04Z","title":"Black hole hair in generalized scalar-tensor gravity: An explicit example","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.1698","snapshot_observed_at":"2026-07-31T20:45:37.467849Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.467849Z"},"links":{"cited_paper":"/paper/1408.1698","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:8cf4a6eca1048855be1a6531019a61ae67fd222dd6a5b004759e203c945f653c","observation_id":"b8c070cd-b740-4e42-ad7b-18aa58de0b5c","resolution":{"observed_at":"2026-07-31T20:45:37.467849Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.01766","last_updated":"2024-09-10T10:04:31Z","snapshot_observed_at":"2026-07-06T14:13:58.277553Z","submitted_at":"2022-11-03T12:45:58Z","title":"Spontaneous scalarization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.01766","snapshot_observed_at":"2026-07-31T20:45:37.508210Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.508210Z"},"links":{"cited_paper":"/paper/2211.01766","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:d52cd8c4eb8d777649825f4613b57cc244e6f4ed65540fd9fb9100e97559c0f2","observation_id":"7cb2d912-fc8a-4154-bce9-e092b83b2ef4","resolution":{"observed_at":"2026-07-31T20:45:37.508210Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.03568","last_updated":"2026-05-13T13:40:15Z","snapshot_observed_at":"2026-07-06T18:26:05.938067Z","submitted_at":"2024-06-05T18:30:33Z","title":"Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.03568","snapshot_observed_at":"2026-07-31T20:45:37.544843Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.544843Z"},"links":{"cited_paper":"/paper/2406.03568","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:df3002d3d1d4b9d48741e7021909940c647a99bd01eafc987211b38c80657d25","observation_id":"643063e9-233f-408a-ab90-325a746acacd","resolution":{"observed_at":"2026-07-31T20:45:37.544843Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.07897","last_updated":"2018-08-23T18:25:15Z","snapshot_observed_at":"2026-07-06T06:57:07.469745Z","submitted_at":"2018-08-23T18:25:15Z","title":"Towards the nonlinear regime in extensions to GR: assessing possible options","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.07897","snapshot_observed_at":"2026-07-31T20:45:37.583061Z","title":"Allwright and L","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.583061Z"},"links":{"cited_paper":"/paper/1808.07897","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:c7c85bcb85046a142b27d956338baf15fec00c37481e9c1a321fdc1ca58060e6","observation_id":"c1a947cb-efbd-46ad-a9d7-3926a48a88e6","resolution":{"observed_at":"2026-07-31T20:45:37.583061Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.08705","last_updated":"2024-03-13T17:09:32Z","snapshot_observed_at":"2026-07-06T17:44:04.908253Z","submitted_at":"2024-03-13T17:09:32Z","title":"Scalarization of isolated black holes in scalar Gauss-Bonnet theory in the fixing-the-equations approach","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.08705","snapshot_observed_at":"2026-07-31T20:45:37.623353Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.623353Z"},"links":{"cited_paper":"/paper/2403.08705","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:7e51158fdcf281fddfe27ae677318e4f744e86311c06988259928389bf466561","observation_id":"1c0b782a-6bcd-4f40-b079-7c19a10197de","resolution":{"observed_at":"2026-07-31T20:45:37.623353Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:37.663547Z","title":"Besharat, L","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.663547Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:abb39286be20d6c9e6b9bd08e86c0460b54e6211b40d91164d345da1737b49a8","observation_id":"6abe1613-21c4-4566-9b18-d37dc330bac1","resolution":{"observed_at":"2026-07-31T20:45:37.663547Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.00265","last_updated":"2025-01-07T23:53:58Z","snapshot_observed_at":"2026-07-06T19:24:57.163690Z","submitted_at":"2024-09-30T22:25:52Z","title":"Simulating binary black hole mergers using discontinuous Galerkin methods","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.00265","snapshot_observed_at":"2026-07-31T20:45:37.699713Z","title":"Lovelaceet al., Simulating binary black hole merg- ers using discontinuous Galerkin methods, Class","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.699713Z"},"links":{"cited_paper":"/paper/2410.00265","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:f29c8f32660a292a73c1d0974e2498bc361fd524f3584e26c051b827b458c8f9","observation_id":"aefdc39c-93aa-4576-9d0e-a7f79c5f6a6c","resolution":{"observed_at":"2026-07-31T20:45:37.699713Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.08635","last_updated":"2021-10-16T18:28:24Z","snapshot_observed_at":"2026-07-06T11:58:38.522979Z","submitted_at":"2021-10-16T18:28:24Z","title":"The SpECTRE Cauchy-characteristic evolution system for rapid, precise waveform extraction","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.08635","snapshot_observed_at":"2026-07-31T20:45:37.735772Z","title":"Moxon, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.735772Z"},"links":{"cited_paper":"/paper/2110.08635","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:dc942f105ddbeef2750bd32ea812a573fb718c1c3aaaae56fcfb9536e0555f49","observation_id":"bd90e28a-5aa0-49d0-9407-e218b3cf29c8","resolution":{"observed_at":"2026-07-31T20:45:37.735772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.06141","last_updated":"2025-02-11T16:08:12Z","snapshot_observed_at":"2026-07-06T19:12:53.753500Z","submitted_at":"2024-09-10T01:32:33Z","title":"Einstein-Klein-Gordon system via Cauchy-characteristic evolution: Computation of memory and ringdown tail","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.06141","snapshot_observed_at":"2026-07-31T20:45:37.775679Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.775679Z"},"links":{"cited_paper":"/paper/2409.06141","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:dcf57f145aa11931e7f9884db880d499c2b974ccb50f845c132399b0fd178700","observation_id":"48b9c4cb-625d-405e-b075-b296d0e00f17","resolution":{"observed_at":"2026-07-31T20:45:37.775679Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.12750","last_updated":"2023-10-10T08:47:57Z","snapshot_observed_at":"2026-07-06T15:19:46.421343Z","submitted_at":"2023-04-25T11:58:45Z","title":"Black hole hairs in scalar-tensor gravity and the lack thereof","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.12750","snapshot_observed_at":"2026-07-31T20:45:37.813925Z","title":"Capuano, L","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.813925Z"},"links":{"cited_paper":"/paper/2304.12750","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:fbf8f40b1654c4eee34997e527f3a9d0fe26ee42d853865de19aec68b8884a81","observation_id":"31f24bdb-e716-421d-87aa-1bc9aa34728a","resolution":{"observed_at":"2026-07-31T20:45:37.813925Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0711.2084","last_updated":"2007-11-13T23:33:36Z","snapshot_observed_at":"2026-07-06T01:35:43.677855Z","submitted_at":"2007-11-13T23:33:36Z","title":"Gauge Drivers for the Generalized Harmonic Einstein Equations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0711.2084","snapshot_observed_at":"2026-07-31T20:45:37.846319Z","title":"Lindblom, K","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.846319Z"},"links":{"cited_paper":"/paper/0711.2084","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:a9d9f55e52abf7422def27ca57c6c88463075a8258e2394890dd81943721ba72","observation_id":"66aa883e-a611-4d1e-8b79-1a3d69dc71ed","resolution":{"observed_at":"2026-07-31T20:45:37.846319Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.01468","last_updated":"2019-10-15T12:17:36Z","snapshot_observed_at":"2026-08-04T19:09:46.455195Z","submitted_at":"2019-02-04T21:40:11Z","title":"Hyperbolicity in Spherical Gravitational Collapse in a Horndeski Theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.01468","snapshot_observed_at":"2026-07-31T20:45:37.893528Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.893528Z"},"links":{"cited_paper":"/paper/1902.01468","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:54fa30a99135ec4e7f39ffc60652f34d2154070f230a9804df3822e81e673b8e","observation_id":"26bd35f2-8224-4d1b-86a8-0a71fbf8897f","resolution":{"observed_at":"2026-07-31T20:45:37.893528Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0804.4291","last_updated":"2008-05-15T15:30:34Z","snapshot_observed_at":"2026-07-06T01:38:44.610980Z","submitted_at":"2008-04-27T18:30:15Z","title":"Effective Field Theory for Inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0804.4291","snapshot_observed_at":"2026-07-31T20:45:37.930288Z","title":"Weinberg, Effective Field Theory for Inflation, Phys","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.930288Z"},"links":{"cited_paper":"/paper/0804.4291","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:ace00b01a7ae95f5c292d1047dba5195b59323f683bdaf05eaaf01451d592352","observation_id":"38845094-ac18-441b-a334-e8cb83aa4447","resolution":{"observed_at":"2026-07-31T20:45:37.930288Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0607056","last_updated":"2007-12-04T16:41:27Z","snapshot_observed_at":"2026-07-07T03:22:44.516364Z","submitted_at":"2006-07-13T17:49:22Z","title":"Solving Einstein's Equations With Dual Coordinate Frames","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0607056","snapshot_observed_at":"2026-07-31T20:45:37.967936Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.967936Z"},"links":{"cited_paper":"/paper/gr-qc/0607056","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:494fb24af74c5ca034ee1f235775a34f38059d061aae8555f1ada7ac2b290b56","observation_id":"33e1224e-6c57-4b6b-b07d-54f25e02709f","resolution":{"observed_at":"2026-07-31T20:45:37.967936Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:38.009072Z","title":"Friedrich, On the hyperbolicity of Einstein’s and other gauge field equations, Commun","venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.009072Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:7aa9b3bd3b6e3c24cedfeacc812fe7b6b45e5344dd56c5586fd925b021eccb5f","observation_id":"050ec91d-db42-40e3-88ca-ce7d6b62336c","resolution":{"observed_at":"2026-07-31T20:45:38.009072Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:38.030974Z","title":"Lindblom, M","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.030974Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:18c32c2dc220df99be2130db9ebccb1f331d80da406370c01d935ce0898142a8","observation_id":"6baba4a5-2d5a-47cd-9537-4b6ceee4148f","resolution":{"observed_at":"2026-07-31T20:45:38.030974Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.1780","last_updated":"2010-07-12T03:33:23Z","snapshot_observed_at":"2026-07-06T01:56:48.500109Z","submitted_at":"2009-08-12T19:42:21Z","title":"Ultra Relativistic Particle Collisions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0908.1780","snapshot_observed_at":"2026-07-31T20:45:38.069755Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.069755Z"},"links":{"cited_paper":"/paper/0908.1780","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:f86bc09720bfed0aef36c3168bb6a28616330d41cadd44fae36366dd6b8d6e4b","observation_id":"020689ef-4643-4673-a33c-1f889b696c83","resolution":{"observed_at":"2026-07-31T20:45:38.069755Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.3557","last_updated":"2009-09-21T19:56:59Z","snapshot_observed_at":"2026-07-06T02:00:39.439539Z","submitted_at":"2009-09-21T19:56:59Z","title":"Simulations of Binary Black Hole Mergers Using Spectral Methods","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.3557","snapshot_observed_at":"2026-07-31T20:45:38.106992Z","title":"Szilagyi, L","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.106992Z"},"links":{"cited_paper":"/paper/0909.3557","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:bee3024a02d0d47214674bc7c9ae17b6ff8f3537a25f740363e2725c7a3b8827","observation_id":"5879cab4-2aa9-4915-af14-3e4031ddbcfe","resolution":{"observed_at":"2026-07-31T20:45:38.106992Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.08682","last_updated":"2018-12-19T04:32:42Z","snapshot_observed_at":"2026-07-06T06:25:04.506480Z","submitted_at":"2018-02-23T18:59:30Z","title":"Critical behavior in 3-d gravitational collapse of massless scalar fields","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.08682","snapshot_observed_at":"2026-07-31T20:45:38.151147Z","title":"Deppe, L","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.151147Z"},"links":{"cited_paper":"/paper/1802.08682","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:8abf39c02c81fe63b85c58be5a6c05a9b8d09a9cba4c2feb053e9e03581e26c1","observation_id":"d37cea69-829a-47d5-8439-83a9aa1a4141","resolution":{"observed_at":"2026-07-31T20:45:38.151147Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.01190","last_updated":"2015-10-05T15:40:14Z","snapshot_observed_at":"2026-07-06T04:32:02.223550Z","submitted_at":"2015-10-05T15:40:14Z","title":"Formulation of discontinuous Galerkin methods for relativistic astrophysics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.01190","snapshot_observed_at":"2026-07-31T20:45:38.189840Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.189840Z"},"links":{"cited_paper":"/paper/1510.01190","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:c87ca517469d2193b792b2e25942a79fb9a20caf5b1a88a38f4fcb0ade82ce40","observation_id":"f904bd4e-ac31-4b91-bb45-8b54b3ae2bb0","resolution":{"observed_at":"2026-07-31T20:45:38.189840Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.6079","last_updated":"2013-04-26T16:19:54Z","snapshot_observed_at":"2026-07-06T03:00:40.964910Z","submitted_at":"2012-11-26T20:11:12Z","title":"Dynamical Excision Boundaries in Spectral Evolutions of Binary Black Hole Spacetimes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.6079","snapshot_observed_at":"2026-07-31T20:45:38.233470Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.233470Z"},"links":{"cited_paper":"/paper/1211.6079","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:30c02099ae775e18e77dc5c33dc249b5f644af67de64d1621026a48d363c566a","observation_id":"8564f125-95c9-45a5-82e9-a52e2b576b6f","resolution":{"observed_at":"2026-07-31T20:45:38.233470Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2508.08408","last_updated":"2025-08-13T02:53:20Z","snapshot_observed_at":"2026-07-06T22:11:28.636602Z","submitted_at":"2025-08-11T18:57:25Z","title":"Horizon tracking for asynchronous parallel black hole simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2508.08408","snapshot_observed_at":"2026-07-31T20:45:38.273320Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.273320Z"},"links":{"cited_paper":"/paper/2508.08408","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:987b68ecce8f53df59e3f981f891ca95c03eaea62c949ebdbbe5a0eacc32f60b","observation_id":"6e93ce62-984d-4c8c-ad85-305da8eeb286","resolution":{"observed_at":"2026-07-31T20:45:38.273320Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.06767","last_updated":"2022-04-18T15:18:07Z","snapshot_observed_at":"2026-07-06T12:07:56.233037Z","submitted_at":"2021-11-12T15:23:45Z","title":"A scalable elliptic solver with task-based parallelism for the SpECTRE numerical relativity code","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.06767","snapshot_observed_at":"2026-07-31T20:45:38.308925Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.308925Z"},"links":{"cited_paper":"/paper/2111.06767","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:e8459fa77b4c0530da7a5b0fa75d85474f799d08930d5a631e7a3d38c8f22399","observation_id":"8d30a23b-1fae-4d30-b136-a4860e200648","resolution":{"observed_at":"2026-07-31T20:45:38.308925Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06120","last_updated":"2024-10-24T16:37:28Z","snapshot_observed_at":"2026-07-06T18:12:22.193554Z","submitted_at":"2024-05-09T21:54:04Z","title":"Discontinuous Galerkin scheme for elliptic equations on extremely stretched grids","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.06120","snapshot_observed_at":"2026-07-31T20:45:38.343878Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.343878Z"},"links":{"cited_paper":"/paper/2405.06120","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:1aa0179ca3a64b5344b7541508898f6c6a6765aec071663e76255e9776d66c47","observation_id":"db4e5faa-333b-42a6-bb36-459a2ec2d960","resolution":{"observed_at":"2026-07-31T20:45:38.343878Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:38.383823Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.383823Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:61d42b1e1b18faccb72b6cadcc06133af700f1d5d4186d8e78f0fb91c4bd67d1","observation_id":"48cc2972-a68f-4df8-8f5e-ae654ccb159e","resolution":{"observed_at":"2026-07-31T20:45:38.383823Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.06895","last_updated":"2021-03-11T19:00:02Z","snapshot_observed_at":"2026-08-03T16:35:15.164932Z","submitted_at":"2021-03-11T19:00:02Z","title":"On the construction of asymptotically flat initial data in scalar-tensor effective field theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.06895","snapshot_observed_at":"2026-07-31T20:45:38.420478Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.420478Z"},"links":{"cited_paper":"/paper/2103.06895","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:d8e59fa424ae8e1431735b6caa7ada2e34a06037d3f220b75601e296431ea02e","observation_id":"8a87ac24-7c00-4ccb-bc36-b8432983ddf3","resolution":{"observed_at":"2026-07-31T20:45:38.420478Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.16791","last_updated":"2023-11-30T10:17:40Z","snapshot_observed_at":"2026-07-06T16:12:51.303563Z","submitted_at":"2023-08-31T15:08:09Z","title":"Solving the initial conditions problem for modified gravity theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.16791","snapshot_observed_at":"2026-07-31T20:45:38.455913Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.455913Z"},"links":{"cited_paper":"/paper/2308.16791","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:093c4ec67bee4bba47d203f7eb019195c6049961629e242b9e28b08ae9536f41","observation_id":"44a02415-1e39-4e3d-adb6-ce722562423e","resolution":{"observed_at":"2026-07-31T20:45:38.455913Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.08410","last_updated":"2025-03-04T22:51:41Z","snapshot_observed_at":"2026-07-06T18:29:44.841845Z","submitted_at":"2024-06-12T16:56:45Z","title":"Quasistationary hair for binary black hole initial data in scalar Gauss-Bonnet gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.08410","snapshot_observed_at":"2026-07-31T20:45:38.495673Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.495673Z"},"links":{"cited_paper":"/paper/2406.08410","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:197bb2740c3baacadcac679669aeec66c718cb4aec2cfc771620e3f5c28e1834","observation_id":"78714869-4eed-4542-aa53-7a5788656637","resolution":{"observed_at":"2026-07-31T20:45:38.495673Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:38.532170Z","title":"Christodoulou and R","venue":null,"work_id":null,"year":1971},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.532170Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:8779a694f24e74ce18d42e5aada807c16bd7c21063771e35b6ce77cfd51f663e","observation_id":"022476bf-a4b9-43c8-b443-594ea96d5f5a","resolution":{"observed_at":"2026-07-31T20:45:38.532170Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1012.1549","last_updated":"2011-05-31T16:07:39Z","snapshot_observed_at":"2026-07-06T02:20:19.201761Z","submitted_at":"2010-12-07T16:47:02Z","title":"Reducing orbital eccentricity of precessing black-hole binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1012.1549","snapshot_observed_at":"2026-07-31T20:45:38.568855Z","title":"Buonanno, L","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.568855Z"},"links":{"cited_paper":"/paper/1012.1549","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:9aeaf9fa7933a5ddfccc0b03db26c6b8c131580c948428f0549c7c082cba83c4","observation_id":"d062a58c-9c3b-47c3-8de7-2a223eb44bac","resolution":{"observed_at":"2026-07-31T20:45:38.568855Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.02300","last_updated":"2022-01-31T17:54:28Z","snapshot_observed_at":"2026-07-06T11:06:41.374888Z","submitted_at":"2021-05-05T19:50:04Z","title":"Fixing the BMS Frame of Numerical Relativity Waveforms","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.02300","snapshot_observed_at":"2026-07-31T20:45:38.607765Z","title":"Mitmanet al., Fixing the BMS frame of numerical relativity waveforms, Phys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.607765Z"},"links":{"cited_paper":"/paper/2105.02300","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:84a5af8e19e40a34ae331f02f5331b446f827051571ff428fb39482dbb7330fa","observation_id":"f83e26e1-872e-43e5-8274-5625822989cb","resolution":{"observed_at":"2026-07-31T20:45:38.607765Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.04356","last_updated":"2022-10-21T16:04:39Z","snapshot_observed_at":"2026-07-06T13:39:57.786408Z","submitted_at":"2022-08-08T18:23:01Z","title":"Fixing the BMS frame of numerical relativity waveforms with BMS charges","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.04356","snapshot_observed_at":"2026-07-31T20:45:38.643023Z","title":"Mitmanet al., Fixing the BMS frame of numerical relativity waveforms with BMS charges, Phys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.643023Z"},"links":{"cited_paper":"/paper/2208.04356","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:05b78ef19ed4c8066ceb325fabcef24bb0b3b0da49b60716ccd77f4c3382fd60","observation_id":"631ca85b-970b-40ea-a240-31eed24688e0","resolution":{"observed_at":"2026-07-31T20:45:38.643023Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:38.680392Z","title":"Boyle, K","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.680392Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:54a7254163f84c7826037c4a98d33900892b418bd49c0f980a40b2a79ac15705","observation_id":"2061408f-acf1-43f8-9303-6f65e4c74a1a","resolution":{"observed_at":"2026-07-31T20:45:38.680392Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.02055","last_updated":"2019-03-05T21:10:37Z","snapshot_observed_at":"2026-07-06T07:37:18.608385Z","submitted_at":"2019-03-05T21:10:37Z","title":"Classification of shift-symmetric Horndeski theories and hairy black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.02055","snapshot_observed_at":"2026-07-31T20:45:38.720087Z","title":"Saravani and T","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.720087Z"},"links":{"cited_paper":"/paper/1903.02055","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:0637bb6cef7e1b78caf0f08f09177e6055ce2a198c3989879994b25e0535830e","observation_id":"468f0db1-05b8-4101-9f94-5c6819ab03e4","resolution":{"observed_at":"2026-07-31T20:45:38.720087Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0707.4654","last_updated":"2008-02-25T15:55:56Z","snapshot_observed_at":"2026-07-06T01:32:51.693135Z","submitted_at":"2007-07-31T16:41:06Z","title":"Multipole expansions for energy and momenta carried by gravitational waves","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0707.4654","snapshot_observed_at":"2026-07-31T20:45:38.756762Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.756762Z"},"links":{"cited_paper":"/paper/0707.4654","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:a335fabd8fdc4539f5d4f20f9667aca1b97fefb0ab383f0f2d1f82a10593b652","observation_id":"d771c007-7489-46cc-9562-23ac536899b1","resolution":{"observed_at":"2026-07-31T20:45:38.756762Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.08955","last_updated":"2016-09-09T03:33:03Z","snapshot_observed_at":"2026-07-06T04:51:04.562947Z","submitted_at":"2016-03-29T20:35:18Z","title":"Theoretical Physics Implications of the Binary Black-Hole Mergers GW150914 and GW151226","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.08955","snapshot_observed_at":"2026-07-31T20:45:38.797862Z","title":"Yunes, K","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.797862Z"},"links":{"cited_paper":"/paper/1603.08955","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:a370ca2c22c948e1a9be3375fcbaeb88dbd2892fae2e0fc258f1d5fda6e138e8","observation_id":"b8e9c689-8e48-419a-b8dc-434742fce218","resolution":{"observed_at":"2026-07-31T20:45:38.797862Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.03208","last_updated":"2018-04-04T21:09:49Z","snapshot_observed_at":"2026-07-06T06:17:58.278569Z","submitted_at":"2018-01-10T01:23:14Z","title":"Extreme Gravity Tests with Gravitational Waves from Compact Binary Coalescences: (I) Inspiral-Merger","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.03208","snapshot_observed_at":"2026-07-31T20:45:38.837227Z","title":"Berti, K","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.837227Z"},"links":{"cited_paper":"/paper/1801.03208","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:58f823e99554402e2c90c2dc749d5ee512e84fe3fe336a15791ad15176796d31","observation_id":"bc101645-1cd6-4ba9-8be8-8667c0b9da5a","resolution":{"observed_at":"2026-07-31T20:45:38.837227Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.02668","last_updated":"2018-07-30T19:31:16Z","snapshot_observed_at":"2026-07-06T06:37:50.411108Z","submitted_at":"2018-05-07T18:00:06Z","title":"Black hole scalar charge from a topological horizon integral in Einstein-dilaton-Gauss-Bonnet gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.02668","snapshot_observed_at":"2026-07-31T20:45:38.874030Z","title":"Prabhu and L","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.874030Z"},"links":{"cited_paper":"/paper/1805.02668","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:207e3e59d0c30b589a8118fc73effdd6c951aadb8b75b1af6d3e646b7c2b1084","observation_id":"f163a383-9ea2-4669-97ea-c5cd2940fb24","resolution":{"observed_at":"2026-07-31T20:45:38.874030Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.07543","last_updated":"2019-10-15T12:46:50Z","snapshot_observed_at":"2026-07-06T07:40:01.196618Z","submitted_at":"2019-03-18T16:28:22Z","title":"Gravitational Collapse in Einstein dilaton Gauss-Bonnet Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.07543","snapshot_observed_at":"2026-07-31T20:45:38.909854Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.909854Z"},"links":{"cited_paper":"/paper/1903.07543","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:e4a0757ed622f42d61a6ec52a6dc213935c685c7875cdc7cae8867d21adf71e8","observation_id":"5c166e31-2542-4c9c-91b3-30cc7feb6361","resolution":{"observed_at":"2026-07-31T20:45:38.909854Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.08162","last_updated":"2018-01-24T19:45:08Z","snapshot_observed_at":"2026-08-04T16:54:16.262471Z","submitted_at":"2018-01-24T19:45:08Z","title":"The hangup effect in unequal mass binary black hole mergers and further studies of their gravitational radiation and remnant properties","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.08162","snapshot_observed_at":"2026-07-31T20:45:38.948229Z","title":"Healy and C","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.948229Z"},"links":{"cited_paper":"/paper/1801.08162","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:a52f387116ba773eab7a1d665df92fc5bc115b5022ad9cb20ed9c6826107e28d","observation_id":"b0a2dd82-e301-4835-91d7-093d4c7bd810","resolution":{"observed_at":"2026-07-31T20:45:38.948229Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:38.986476Z","title":null,"venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:38.986476Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:0096257a9fda17988993cd18331e003bc2c46e770c57e3807ab97bb23d83c897","observation_id":"2de75c15-d24b-49e1-bcda-031a57135174","resolution":{"observed_at":"2026-07-31T20:45:38.986476Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T20:45:39.025291Z","title":"Damour and G","venue":null,"work_id":null,"year":2093},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:39.025291Z"},"links":{"citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:392845b7720c3bc0ea9410d40a6740b2b2f953318f31e287c0bde58be2db4a31","observation_id":"0dc1d7a9-ed85-4f47-8038-0deead63a29e","resolution":{"observed_at":"2026-07-31T20:45:39.025291Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.02152","last_updated":"2015-12-29T17:36:57Z","snapshot_observed_at":"2026-07-06T04:32:22.478229Z","submitted_at":"2015-10-07T22:01:27Z","title":"Challenging the Presence of Scalar Charge and Dipolar Radiation in Binary Pulsars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.02152","snapshot_observed_at":"2026-07-31T20:45:39.059549Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:39.059549Z"},"links":{"cited_paper":"/paper/1510.02152","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:ad9a01312a49880ac082021a5e06cc4da52556b0587ba848f838ba6a99243473","observation_id":"864b47db-f9c3-41c4-a201-05c89ec78c5c","resolution":{"observed_at":"2026-07-31T20:45:39.059549Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-03T00:01:45.468920Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":99,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":107},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 100 of 107 outbound references and 0 inbound Pith citation observations for arXiv:2607.28003."}