{"as_of":"2026-08-10T02:54:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:03a9efc5309e86a0084fc0357e3998e0d73dd4c9c46bd1431916e25120b838e5","coverage":[{"denominator":172,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-09T05:33:08.230985Z","state":"measured"},{"denominator":103,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":103,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-09T00:07:29.728685Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-06-29T20:33:58.147033Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.03223","snapshot_observed_at":"2026-08-09T00:07:29.728685Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.03973","last_updated":"2025-02-06T11:06:13Z","snapshot_observed_at":"2026-08-09T05:48:47.263112Z","submitted_at":"2025-02-06T11:06:13Z","title":"Axisymmetric stability of neutron stars as extreme rotators in massive scalar-tensor theory","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-09T00:07:29.728685Z"},"links":{"cited_paper":"/paper/2502.03223","citing_paper":"/paper/2502.03973"},"observation_digest":"sha256:a9a7cc9083bbc5b4f1598aff45ab8b9541cdbbb4e0e2879c3f6c9074047a82a9","observation_id":"cf8e7a0d-ade3-48e8-8c8f-aeb2607fe4d4","resolution":{"observed_at":"2026-08-09T00:07:29.728685Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"cited_work":{"arxiv_id":"2502.03223","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.03223","snapshot_observed_at":"2026-06-29T20:33:58.147033Z","title":null,"venue":null,"work_id":"f926a360-77d3-4357-a4e4-f2c8296fdc4b","year":2025},"citing_paper":{"arxiv_id":"2605.26228","last_updated":"2026-05-25T18:00:28Z","snapshot_observed_at":"2026-08-01T21:44:38.475132Z","submitted_at":"2026-05-25T18:00:28Z","title":"Donutization Inside Neutron Stars: Shell-Localized Scalar Fields","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-06-29T20:33:28.058638Z"},"links":{"cited_paper":"/paper/2502.03223","citing_paper":"/paper/2605.26228"},"observation_digest":"sha256:d4e82520fcffeecab46f87163d812a7e86807b77645b6a1109a9ab95bb4ea7b4","observation_id":"91588b2e-1337-43e7-ab41-181e0b289469","resolution":{"observed_at":"2026-06-29T20:33:58.148281Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.03223","snapshot_observed_at":"2026-07-31T03:49:42.228479Z","title":"T.-L., & Shibata, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.28556","last_updated":"2026-07-30T17:22:50Z","snapshot_observed_at":"2026-08-07T09:36:30.126110Z","submitted_at":"2026-07-30T17:22:50Z","title":"Spinning down neutron-star merger remnants with the Tayler-Spruit dynamo: Global simulations reveal the formation of massive disks and neutron-rich ejecta","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-07-31T03:49:42.228479Z"},"links":{"cited_paper":"/paper/2502.03223","citing_paper":"/paper/2607.28556"},"observation_digest":"sha256:b380766798d73d3aa5837511c121f8617f443ab19bcb80df0523365257b1e677","observation_id":"4261daac-9c99-484d-95e1-dcd8425ca502","resolution":{"observed_at":"2026-07-31T03:49:42.228479Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2502.03223/citation-record","integrity":"/paper/2502.03223/integrity","json":"/paper/2502.03223/citation-record.json","paper":"/paper/2502.03223"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T05:33:07.730233Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.730233Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:11b2cb636b1fb1473ec5018af6c8d3d1f6f6d432a8acb5d0023981bacc92945f","observation_id":"58dc4e7c-62f7-416e-b3f1-d9f58161a530","resolution":{"observed_at":"2026-08-09T05:33:07.730233Z","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":"2026-08-09T05:33:07.712933Z","title":"Both Total Variation Di- minishing Lax-Friedrich (TVDLF) [108–110] and HLLC [12, 13, 111] approximate Riemann solvers are imple- mented in SACRA-2D","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.712933Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:8e1320710369b7b4a3256c038685d74b5d11ec2719c6e3144a21d999405d8fbf","observation_id":"3fad7353-ec26-4d89-9bc6-8e5417842047","resolution":{"observed_at":"2026-08-09T05:33:07.712933Z","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":"2026-08-09T05:33:07.719182Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.719182Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:b153d94078c66a30ba7611e32673130b24f9c1ae19a0550dec12c303939af7a5","observation_id":"f414325c-61a5-4664-a7e3-5c012bb74b6c","resolution":{"observed_at":"2026-08-09T05:33:07.719182Z","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":"2026-08-09T05:33:07.724617Z","title":"We implement the primitive recovery proce- dure for GRHD mentioned in Appendix C of [116]","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.724617Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:5e972ca1da9f8c023daf6040a5cc67c391074e70a7a32244f97cf82e8749e2d7","observation_id":"84084484-531f-410a-a3ff-5279e3b7458c","resolution":{"observed_at":"2026-08-09T05:33:07.724617Z","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":"2026-08-09T05:33:07.735512Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.735512Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:d85a1d56b7164e780f2764ac4fc208e90a3da56a3a4a793fe62324fb659103bc","observation_id":"70669aca-6fb0-408c-a284-bb1e2ea7180b","resolution":{"observed_at":"2026-08-09T05:33:07.735512Z","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":"2026-08-09T05:33:07.740840Z","title":"(49) In SACRA 2D, we numerically solve Eq","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.740840Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:bc0fb2fe3acbdcae7c9ae8caf024e1c43a7c1a24fe3e9499185a1f1bb9ae9392","observation_id":"6c611894-771b-45a7-a762-3b2153867f32","resolution":{"observed_at":"2026-08-09T05:33:07.740840Z","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":"2026-08-09T05:33:07.746822Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.746822Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:a06f1a642652ab4fe8528025526be26ffee339b572c8e6b2955d15f30413925e","observation_id":"1411175d-89ef-4045-8811-b0d0846f922d","resolution":{"observed_at":"2026-08-09T05:33:07.746822Z","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":"2026-08-09T05:33:07.751944Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.751944Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:0a75e27e7e7a3160d94896b6f8bf95913695c94082bdd4ed8c4f204c64cd41c2","observation_id":"d5304a43-d9af-41a1-8b29-e1800ef00b3a","resolution":{"observed_at":"2026-08-09T05:33:07.751944Z","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":"2026-08-09T05:33:07.756877Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.756877Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:11cee61c3dcafc65d3f0e413374932b0e79475a46ff6e9e022cbcb2fab72935c","observation_id":"d5bfe728-1436-46bf-9b2c-e530cf3c39a5","resolution":{"observed_at":"2026-08-09T05:33:07.756877Z","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":"2026-08-09T05:33:07.762070Z","title":"Under axisymmetry, the mo- mentum constraints Mx and My evaluated are effec- tively Mϖ and Mϕ in cylindrical coordinates, respec- tively","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.762070Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:e9db8e72af422ad6e28999b0470834c9d4e3512381444c175d56055912e3e46c","observation_id":"83b6a02e-4312-4001-86d3-d86223a36c52","resolution":{"observed_at":"2026-08-09T05:33:07.762070Z","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":"2026-08-09T05:33:07.766985Z","title":"Here, ka and la 9 are outgoing and ingoing null vectors, respectively, where ma is a complex null vector satisfying −kala = 1 = ma ¯ma","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.766985Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:bd2ef78900518e89e8da419388319ffbdf639eef1faa0113060244137b592caa","observation_id":"fe93d17f-afed-4e7f-8617-17ba5aa49483","resolution":{"observed_at":"2026-08-09T05:33:07.766985Z","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":"2026-08-09T05:33:07.772249Z","title":"Assuming that the apparent horizon contains the coordinate center (x, z) = (0, 0), the horizon radius H can be represented as a function of polar angle θ as r = H(θ)","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.772249Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:db627d1bc03700c6b30aefae95d6d1bd125df70d21ba907f515ce39accbfe603","observation_id":"c43f55a7-2396-4651-a619-f5e7fca14234","resolution":{"observed_at":"2026-08-09T05:33:07.772249Z","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":"2026-08-09T05:33:07.776959Z","title":"Specifically, we consider a non-rotating black hole in the so-called maximal trumpet coordinate, which is time-independent under BSSN formalism with the puncture gauge","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.776959Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:7858ff146b3612ad5f8ee129d2461df5a5222a42aa3960c9f5d3f7ffb6a0a4cc","observation_id":"2bddcccc-4fca-4c1c-acdc-a520e51ceb1d","resolution":{"observed_at":"2026-08-09T05:33:07.776959Z","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":"2026-08-09T05:33:07.782010Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.782010Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:0109f6fb5ed33344242fc4579e74469da3bb9092c8d264cf6d1462a9514a0341","observation_id":"fd27ec01-fd2e-408e-bb4b-92f10fca94fb","resolution":{"observed_at":"2026-08-09T05:33:07.782010Z","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":"2026-08-09T05:33:07.786652Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.786652Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:d48f76f2a2d239ca5ea8fc89a8f5ae1c9132cbdfcd0be5f0fcb16e01320faced","observation_id":"0afa7ed6-ce50-4383-9ca7-3fbf15acc886","resolution":{"observed_at":"2026-08-09T05:33:07.786652Z","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":"2026-08-09T05:33:07.791532Z","title":"For this test, the cylindrical coordinates in SACRA-2D are converted to the Cartesian coordinates","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.791532Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:8143a2a99a6c2aee6c53fc62ccfa7cd169b17a2d16b885cc98af7f7e99a9d2cc","observation_id":"0b5b1af6-33b6-45bb-91cb-b0a2fe6c1966","resolution":{"observed_at":"2026-08-09T05:33:07.791532Z","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":"2026-08-09T05:33:07.796243Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.796243Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:cabbec714e4f9b6ed3cb8fe6adf145f5c634fc90953ba60c0d1574b0c8c70e58","observation_id":"3712a007-82a6-4c9b-8628-93af70394e2f","resolution":{"observed_at":"2026-08-09T05:33:07.796243Z","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":"2026-08-09T05:33:07.801215Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.801215Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:6652657effdc876adf90ac932975782529975478a5c86f3a495dccadf9a280c2","observation_id":"dfc48119-879d-4d40-9f90-ca2da4526f1d","resolution":{"observed_at":"2026-08-09T05:33:07.801215Z","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":"2026-08-09T05:33:07.806297Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.806297Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:4c99f248996625db56dddde6725ac98ffa80628f527edf7b39c417c2636106d3","observation_id":"731117a0-b94b-4584-b656-0938c5e42b2b","resolution":{"observed_at":"2026-08-09T05:33:07.806297Z","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":"2026-08-09T05:33:07.811513Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.811513Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:0b1f20da2dc266a38c75d05929d181b526ac0ab5514959075733d2b425adcfd4","observation_id":"5524417e-9d9f-40fa-9b17-c0e2aac17fb9","resolution":{"observed_at":"2026-08-09T05:33:07.811513Z","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":"2026-08-09T05:33:07.816641Z","title":"We consider uniformly rotating neutron stars in both the stable and unstable branches indicated as the red crosses in Fig","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.816641Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:a485b05a31f9b0c22c059c0b4c6ba21f3c951be4627c78c6f2eb205e40961c21","observation_id":"6013fab1-164d-4222-aabe-c3827eae4c1a","resolution":{"observed_at":"2026-08-09T05:33:07.816641Z","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":"2026-08-09T05:33:07.821474Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.821474Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:c5a76dee29f8ed732e467be3e3bec6cd05cff522c50526a9a080602accbef08d","observation_id":"9f0836b4-5ad0-48d9-8281-c7eaef9d8a25","resolution":{"observed_at":"2026-08-09T05:33:07.821474Z","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":"2026-08-09T05:33:07.826778Z","title":"Harten, P","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.826778Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:30749826c07990836c3538c08c182c766fb17675f4a77824e95470672cb71d56","observation_id":"3e160e21-8885-470a-a64a-98752c4a03a8","resolution":{"observed_at":"2026-08-09T05:33:07.826778Z","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":"2026-08-09T05:33:07.832003Z","title":"M¨ osta, B","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.832003Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:23dfee3c0bc6408e48694f841945ccaf417dff9820ef85c8c7bb9dfacf23fefb","observation_id":"165627bc-1bf6-462f-8556-6dfb20d99464","resolution":{"observed_at":"2026-08-09T05:33:07.832003Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.07276","last_updated":"2015-08-18T15:54:55Z","snapshot_observed_at":"2026-08-06T15:35:14.620493Z","submitted_at":"2015-01-28T21:00:12Z","title":"IllinoisGRMHD: An Open-Source, User-Friendly GRMHD Code for Dynamical Spacetimes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.07276","snapshot_observed_at":"2026-08-09T05:33:07.836924Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.836924Z"},"links":{"cited_paper":"/paper/1501.07276","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:bf129574634c4873c5479a8aaf40fa2ba23af323ee902e8ae4dfc73de3036b0c","observation_id":"0d8717e6-31f3-4708-b8e0-23fcaa006963","resolution":{"observed_at":"2026-08-09T05:33:07.836924Z","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":"2026-08-09T05:33:07.842519Z","title":"Bernuzzi and T","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.842519Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:b1d932d355d1c5bb7a3402544e2d7108de5027d3e47586bb97d282f030ffec45","observation_id":"588fb137-b67f-47a4-9d76-700a8ec98578","resolution":{"observed_at":"2026-08-09T05:33:07.842519Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.10328","last_updated":"2020-03-13T10:18:11Z","snapshot_observed_at":"2026-08-07T03:58:22.028680Z","submitted_at":"2019-07-24T09:46:10Z","title":"Beyond second-order convergence in simulations of magnetised binary neutron stars with realistic microphysics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.10328","snapshot_observed_at":"2026-08-09T05:33:07.847440Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.847440Z"},"links":{"cited_paper":"/paper/1907.10328","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:c14a6759c52a380ab3c5858eb363de30e43cd185ccaa42f83eb440e9eab9d8ff","observation_id":"8c07330d-abdc-4155-8d4e-3b1c7347b48e","resolution":{"observed_at":"2026-08-09T05:33:07.847440Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.00870","last_updated":"2020-04-02T08:34:58Z","snapshot_observed_at":"2026-08-03T23:33:38.436902Z","submitted_at":"2020-04-02T08:34:58Z","title":"GRMHD large eddy simulations with gradient subgrid-scale model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.00870","snapshot_observed_at":"2026-08-09T05:33:07.853715Z","title":"Vigan` o, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.853715Z"},"links":{"cited_paper":"/paper/2004.00870","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:b85c68c3246402346d0043acf8e1b6be80b8c7511bb1de6d58b27f96c1ebdf56","observation_id":"764be903-7c69-4616-b552-532ec53e55f3","resolution":{"observed_at":"2026-08-09T05:33:07.853715Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.10174","last_updated":"2021-03-12T18:50:39Z","snapshot_observed_at":"2026-08-03T15:34:32.882093Z","submitted_at":"2020-12-18T11:33:44Z","title":"Spritz: General Relativistic Magnetohydrodynamics with Neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.10174","snapshot_observed_at":"2026-08-09T05:33:07.859015Z","title":"Cipolletta, J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.859015Z"},"links":{"cited_paper":"/paper/2012.10174","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:2f9ad2f6fefaf683ef4fdbdf0e9a7c2734f237ff326c7471bc8932b40ebe0c5e","observation_id":"78f0a762-5095-4164-ab61-91406ede1def","resolution":{"observed_at":"2026-08-09T05:33:07.859015Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.14518","last_updated":"2020-10-27T18:00:01Z","snapshot_observed_at":"2026-07-06T10:09:10.434213Z","submitted_at":"2020-10-27T18:00:01Z","title":"High-accuracy waveforms for black hole-neutron star systems with spinning black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.14518","snapshot_observed_at":"2026-08-09T05:33:07.864257Z","title":"Foucart, A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.864257Z"},"links":{"cited_paper":"/paper/2010.14518","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:e64f78a064419d1d165f4387e641b84fa409be1bdc707ae45d358a93776b075e","observation_id":"e8989e2a-e6ca-4f64-90e4-727e04e6a7aa","resolution":{"observed_at":"2026-08-09T05:33:07.864257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.04621","last_updated":"2023-04-26T13:36:17Z","snapshot_observed_at":"2026-07-06T12:06:35.380847Z","submitted_at":"2021-11-08T16:48:57Z","title":"General-relativistic neutrino-radiation magnetohydrodynamic simulation of seconds-long black hole-neutron star mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.04621","snapshot_observed_at":"2026-08-09T05:33:07.869347Z","title":"Hayashi, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.869347Z"},"links":{"cited_paper":"/paper/2111.04621","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:261568c5ec202762507214ddb9903b0765761f21d3bd25815b082e5bf24e8bb1","observation_id":"ffc9bfa3-54a7-499b-87b1-7584191d79ed","resolution":{"observed_at":"2026-08-09T05:33:07.869347Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.14858","last_updated":"2023-05-09T14:57:24Z","snapshot_observed_at":"2026-08-09T16:50:09.877424Z","submitted_at":"2021-11-29T19:00:01Z","title":"A New Moment-Based General-Relativistic Neutrino-Radiation Transport Code: Methods and First Applications to Neutron Star Mergers","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.14858","snapshot_observed_at":"2026-08-09T05:33:07.874453Z","title":"Radice, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.874453Z"},"links":{"cited_paper":"/paper/2111.14858","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:c592c84843be829a6fc6d2328886b9a2bc72b09d9924cad3f0f2d0232635074f","observation_id":"64637c5c-c8d0-4530-9730-b5cb496f902f","resolution":{"observed_at":"2026-08-09T05:33:07.874453Z","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":"2026-08-09T05:33:07.879466Z","title":"Kurganov and E","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.879466Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:7937cec03090e79bb4c264672c8c9150932c23648c165b1087daf36057659a19","observation_id":"919ce712-d64d-457f-bf87-973d8364564a","resolution":{"observed_at":"2026-08-09T05:33:07.879466Z","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":"2026-08-09T05:33:07.884218Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.884218Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:252d45d661fe996dd975bcd624cb9de2615ccbf28416bcb4175321bcb07adf7b","observation_id":"6c691554-900a-4388-8e4d-052746365a9d","resolution":{"observed_at":"2026-08-09T05:33:07.884218Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0506414","last_updated":"2005-08-31T10:04:39Z","snapshot_observed_at":"2026-07-07T00:51:24.821839Z","submitted_at":"2005-06-17T14:34:37Z","title":"An HLLC Riemann Solver for Relativistic Flows: I. Hydrodynamics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0506414","snapshot_observed_at":"2026-08-09T05:33:07.888873Z","title":"Mignone and G","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.888873Z"},"links":{"cited_paper":"/paper/astro-ph/0506414","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:396f82ffffc706fa36631fd6de2eb081ebed0edbbed2a8cd3900fed0451c8c30","observation_id":"11f46cd5-245b-4364-b2cd-853c153df5f2","resolution":{"observed_at":"2026-08-09T05:33:07.888873Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0811.1483","last_updated":"2008-11-10T14:57:53Z","snapshot_observed_at":"2026-07-06T01:47:37.889204Z","submitted_at":"2008-11-10T14:57:53Z","title":"A five-wave HLL Riemann solver for relativistic MHD","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0811.1483","snapshot_observed_at":"2026-08-09T05:33:07.893910Z","title":"Mignone, M","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.893910Z"},"links":{"cited_paper":"/paper/0811.1483","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:b98cce3d558b1f22cd3cc42b182b26d3990ea8e07443e5b7c4cd52eb31616a11","observation_id":"30869d2c-dc1f-4dff-b845-19942ac9383b","resolution":{"observed_at":"2026-08-09T05:33:07.893910Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.00267","last_updated":"2018-08-01T11:11:42Z","snapshot_observed_at":"2026-07-06T06:53:28.543858Z","submitted_at":"2018-08-01T11:11:42Z","title":"Hydrodynamic convection in accretion discs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.00267","snapshot_observed_at":"2026-08-09T05:33:07.898776Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.898776Z"},"links":{"cited_paper":"/paper/1808.00267","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:a5f7da2a4ee7a5096d5449c64fb65649355a0e6f09c311fdc10bf7d25ead52ba","observation_id":"238bb7d0-3aa5-4370-aa09-e9244418cf0c","resolution":{"observed_at":"2026-08-09T05:33:07.898776Z","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":"2026-08-09T05:33:07.903666Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.903666Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:b6a11c8ce80ffb1552abc60e2f3a190034d1fb38aea1298177a603e8b1f9a2e3","observation_id":"399902bb-c12f-4520-9d8f-b14531849946","resolution":{"observed_at":"2026-08-09T05:33:07.903666Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.04487","last_updated":"2022-05-09T18:00:14Z","snapshot_observed_at":"2026-08-01T05:39:29.130354Z","submitted_at":"2022-05-09T18:00:14Z","title":"Implementation of advanced Riemann solvers in a neutrino-radiation magnetohydrodynamics code in numerical relativity and its application to a binary neutron star merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.04487","snapshot_observed_at":"2026-08-09T05:33:07.908619Z","title":"Kiuchi, L","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.908619Z"},"links":{"cited_paper":"/paper/2205.04487","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:f838a750d8e0e1852be04328e317a4c3c7e8dee37b0c736b40793529258fc2cc","observation_id":"1b09d799-db1b-417a-bf9a-cd310f25a3a6","resolution":{"observed_at":"2026-08-09T05:33:07.908619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.00943","last_updated":"2016-07-03T20:17:30Z","snapshot_observed_at":"2026-07-06T04:35:12.575616Z","submitted_at":"2015-11-03T15:24:33Z","title":"An Extension of the Athena++ Code Framework for GRMHD Based on Advanced Riemann Solvers and Staggered-Mesh Constrained Transport","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.00943","snapshot_observed_at":"2026-08-09T05:33:07.913591Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.913591Z"},"links":{"cited_paper":"/paper/1511.00943","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:da3ec0896a871c3542aac715d2b28eb07b4dd3f7db0b73beb0664ce7f541c296","observation_id":"f2bd8dbf-24bd-4ad0-851a-8c273331b22d","resolution":{"observed_at":"2026-08-09T05:33:07.913591Z","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":"2026-08-09T05:33:07.918489Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.918489Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:d886bce8239ceb0c5aef9da9ea379f25a38a3ddb190dcc09eb9a54fe5fe0d7cf","observation_id":"6b600551-bd5a-47b7-87f7-078411ed2f7e","resolution":{"observed_at":"2026-08-09T05:33:07.918489Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0805.2712","last_updated":"2008-05-18T04:11:42Z","snapshot_observed_at":"2026-07-06T01:39:38.346814Z","submitted_at":"2008-05-18T04:11:42Z","title":"Evolution of neutron stars with toroidal magnetic fields: Axisymmetric simulation in full general relativity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0805.2712","snapshot_observed_at":"2026-08-09T05:33:07.923320Z","title":"Kiuchi, M","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.923320Z"},"links":{"cited_paper":"/paper/0805.2712","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:ee89ae2e69fe26b03d14f1af68355c8d3c67092a3d63dcbf45cf7d666719207d","observation_id":"096a5d7d-89cc-4e41-9037-985f740a693e","resolution":{"observed_at":"2026-08-09T05:33:07.923320Z","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":"2026-08-09T05:33:07.928259Z","title":"Shibata, ApJ 595, 992 (2003), arXiv:astro- ph/0310020 [astro-ph]","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.928259Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:653ce6af7149f34e1f7940409eeb4b7c41fa7e6980dd3c52a606c13caa2ef5fe","observation_id":"19051787-86e6-4d65-a65a-f72154cc3f09","resolution":{"observed_at":"2026-08-09T05:33:07.928259Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0402184","last_updated":"2004-02-09T04:33:15Z","snapshot_observed_at":"2026-08-07T17:32:48.327137Z","submitted_at":"2004-02-09T04:33:15Z","title":"Gravitational waves from axisymmetrically oscillating neutron stars in general relativistic simulations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0402184","snapshot_observed_at":"2026-08-09T05:33:07.933338Z","title":"Shibata and Y.-I","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.933338Z"},"links":{"cited_paper":"/paper/astro-ph/0402184","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:4dbcd1f79ca45cdbc8984372f2b5f9d1deac872a43bc099a74b0a81743c13945","observation_id":"6566b515-a840-436b-94df-58a311b3b79d","resolution":{"observed_at":"2026-08-09T05:33:07.933338Z","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":"2026-08-09T05:33:07.938795Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.938795Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:b94691df1de5b732f94f5fda73ac9994354bdbe6d23a207cdd910e9069615514","observation_id":"b942fa05-a128-434b-b3ba-3e2d588543b6","resolution":{"observed_at":"2026-08-09T05:33:07.938795Z","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":"2026-08-09T05:33:07.943673Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.943673Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:eeaad98ef6bcd25f6d529654b81ce0654ab36a9f2e4764637086146610edb922","observation_id":"15e08033-9db6-4422-812b-61fa366781d9","resolution":{"observed_at":"2026-08-09T05:33:07.943673Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0510653","last_updated":"2005-12-09T21:58:10Z","snapshot_observed_at":"2026-08-08T10:16:56.279179Z","submitted_at":"2005-10-24T15:16:06Z","title":"Collapse of magnetized hypermassive neutron stars in general relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0510653","snapshot_observed_at":"2026-08-09T05:33:07.948540Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.948540Z"},"links":{"cited_paper":"/paper/astro-ph/0510653","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:59321bda7e1bbd82ce64c2a2eaaa2b6c2f7a80390f3996cba87fc2a93a4831d7","observation_id":"f0361aef-a59d-4deb-818b-9b7edf81c1f5","resolution":{"observed_at":"2026-08-09T05:33:07.948540Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0511142","last_updated":"2005-11-04T21:07:54Z","snapshot_observed_at":"2026-07-07T00:55:41.327148Z","submitted_at":"2005-11-04T21:07:54Z","title":"Magnetized hypermassive neutron star collapse: a central engine for short gamma-ray bursts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0511142","snapshot_observed_at":"2026-08-09T05:33:07.953984Z","title":"Shibata, M","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.953984Z"},"links":{"cited_paper":"/paper/astro-ph/0511142","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:4ef20a00b478f1a3f9c76281d6c286c78ffd38eed5d13631e50b2f5986f296f7","observation_id":"bbf67bf9-51da-43d1-a0a9-8226fbfb3c43","resolution":{"observed_at":"2026-08-09T05:33:07.953984Z","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":"2026-08-09T05:33:07.959179Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.959179Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:cb32c2e87448dd1ac14d321851e8a1334fde8130983adaaf58cba54a8fdb88f6","observation_id":"5b2a4990-eab9-47ca-a506-98d43dc18cee","resolution":{"observed_at":"2026-08-09T05:33:07.959179Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.10303","last_updated":"2017-03-30T03:53:11Z","snapshot_observed_at":"2026-07-06T05:35:47.750465Z","submitted_at":"2017-03-30T03:53:11Z","title":"General relativistic viscous hydrodynamics of differentially rotating neutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.10303","snapshot_observed_at":"2026-08-09T05:33:07.967732Z","title":"Shibata, K","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.967732Z"},"links":{"cited_paper":"/paper/1703.10303","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:5c46306ee5558917ac2e1b3a06752fd6db5d0fb232cdf8aa23ad056c68da3871","observation_id":"ada1f06d-8a2a-460b-80e6-7aca4b4d4395","resolution":{"observed_at":"2026-08-09T05:33:07.967732Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0403036","last_updated":"2004-03-09T03:59:22Z","snapshot_observed_at":"2026-07-07T03:18:59.127978Z","submitted_at":"2004-03-09T03:59:22Z","title":"New criterion for direct black hole formation in rapidly rotating stellar collapse","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0403036","snapshot_observed_at":"2026-08-09T05:33:07.973313Z","title":"Sekiguchi and M","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.973313Z"},"links":{"cited_paper":"/paper/gr-qc/0403036","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:6d3ddf91d22b33d2b3cf4bdd60c10cbe5a58a315c6ecbe596e0ddb821ed1792b","observation_id":"eb3e4c96-6834-42d7-b9fc-490b3264b8c9","resolution":{"observed_at":"2026-08-09T05:33:07.973313Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0504567","last_updated":"2005-04-26T07:23:10Z","snapshot_observed_at":"2026-08-08T16:01:48.877513Z","submitted_at":"2005-04-26T07:23:10Z","title":"Axisymmetric collapse simulations of rotating massive stellar cores in full general relativity: Numerical study for prompt black hole formation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0504567","snapshot_observed_at":"2026-08-09T05:33:07.978806Z","title":"Sekiguchi and M","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.978806Z"},"links":{"cited_paper":"/paper/astro-ph/0504567","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:a3566696f713d35670f0155dd81280fa1c2d365e8cfe11bd0aa92bb0c5713f13","observation_id":"173c3e22-5873-4865-9c46-cc13c42f7b4f","resolution":{"observed_at":"2026-08-09T05:33:07.978806Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0402040","last_updated":"2004-02-08T12:23:13Z","snapshot_observed_at":"2026-08-10T01:06:07.580996Z","submitted_at":"2004-02-08T12:23:13Z","title":"Gravitational waves from axisymmetric rotating stellar core collapse to a neutron star in full general relativity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0402040","snapshot_observed_at":"2026-08-09T05:33:07.983891Z","title":"Shibata and Y.-I","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.983891Z"},"links":{"cited_paper":"/paper/gr-qc/0402040","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:c633ae1ca95c775eabf72e44509594d0a024a9f9e4bf8556a31712e1f9921672","observation_id":"fa960fc5-1c68-4b11-baa6-3978559c657e","resolution":{"observed_at":"2026-08-09T05:33:07.983891Z","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":"2026-08-09T05:33:07.988751Z","title":"Shibata, Y","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.988751Z"},"links":{"citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:3b7161437ecb58cb439ea357102861de51da3fffa8df4196e2bc3c132b5d2ed5","observation_id":"0a403fe9-8bea-493c-8fe9-2f103bbbdcff","resolution":{"observed_at":"2026-08-09T05:33:07.988751Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1202.2487","last_updated":"2012-05-29T06:53:21Z","snapshot_observed_at":"2026-07-06T02:42:43.660863Z","submitted_at":"2012-02-12T03:49:21Z","title":"Fully General Relativistic Simulations of Core-Collapse Supernovae with An Approximate Neutrino Transport","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.2487","snapshot_observed_at":"2026-08-09T05:33:07.993543Z","title":"Kuroda, K","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.993543Z"},"links":{"cited_paper":"/paper/1202.2487","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:fa7a07609f410b2f69f4776b0b91e3d0682fde20bf7624f6bad4f12cf1aec2b3","observation_id":"283157c4-e7d2-41ed-aff5-e6a120e9ab94","resolution":{"observed_at":"2026-08-09T05:33:07.993543Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.04467","last_updated":"2021-06-11T07:37:24Z","snapshot_observed_at":"2026-08-08T11:49:32.529769Z","submitted_at":"2021-02-08T19:00:01Z","title":"Ultra-delayed neutrino-driven explosion of rotating massive-star collapse","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.04467","snapshot_observed_at":"2026-08-09T05:33:07.998641Z","title":"Fujibayashi, K","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:07.998641Z"},"links":{"cited_paper":"/paper/2102.04467","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:ee947746fbc757f7e89deaaa4ba5343c9376f903d0aaf25882826cd937bfc712","observation_id":"37665da1-421a-4e3e-95a8-2ab326d88299","resolution":{"observed_at":"2026-08-09T05:33:07.998641Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.03958","last_updated":"2023-09-05T10:31:17Z","snapshot_observed_at":"2026-07-06T14:28:05.906581Z","submitted_at":"2022-12-07T21:12:27Z","title":"Collapse of rotating massive stars leading to black hole formation and energetic supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.03958","snapshot_observed_at":"2026-08-09T05:33:08.003771Z","title":"Fujibayashi, Y","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.003771Z"},"links":{"cited_paper":"/paper/2212.03958","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:c959f5754253b74d498529cad9ec1caae8113f0e1b474141a8f601d877a130dd","observation_id":"8a6c05f4-894f-4741-9f30-36feaee44f06","resolution":{"observed_at":"2026-08-09T05:33:08.003771Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.02161","last_updated":"2023-09-05T11:58:26Z","snapshot_observed_at":"2026-07-06T16:14:26.899440Z","submitted_at":"2023-09-05T11:58:26Z","title":"Supernova-like explosion of massive rotating stars from disks surrounding a black hole","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.02161","snapshot_observed_at":"2026-08-09T05:33:08.009044Z","title":"Fujibayashi, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.009044Z"},"links":{"cited_paper":"/paper/2309.02161","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:1e1bf59ca9b0b114e5bcc65afff23830f25a97a6c66cc93cc3fce8dd8728551a","observation_id":"4ee5f712-8559-44ef-ae6c-5896fd97f0f0","resolution":{"observed_at":"2026-08-09T05:33:08.009044Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.12086","last_updated":"2023-09-21T13:57:25Z","snapshot_observed_at":"2026-08-07T17:16:37.301373Z","submitted_at":"2023-09-21T13:57:25Z","title":"Outflow energy and black-hole spin evolution in collapsar scenarios","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.12086","snapshot_observed_at":"2026-08-09T05:33:08.014137Z","title":"Shibata, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.014137Z"},"links":{"cited_paper":"/paper/2309.12086","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:0777f2885db6ca8632d25fbad6d03d513b40e16e6f2f4e4366a30a03203edabd","observation_id":"286c36be-bfcd-415a-8407-3aa15f1ab11e","resolution":{"observed_at":"2026-08-09T05:33:08.014137Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.02077","last_updated":"2025-02-04T07:54:06Z","snapshot_observed_at":"2026-08-09T13:23:01.514286Z","submitted_at":"2025-02-04T07:54:06Z","title":"Self-consistent scenario for jet and stellar explosion in collapsar: General relativistic magnetohydrodynamics simulation with dynamo","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.02077","snapshot_observed_at":"2026-08-09T05:33:08.019558Z","title":"Shibata, S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.019558Z"},"links":{"cited_paper":"/paper/2502.02077","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:f3f15647b09bd2ee68dc6ce6f1a3ac659a505f0389837ff3e25601f4ef8d8ccf","observation_id":"ef7997db-cbb6-4d52-b13c-75508c24cf5c","resolution":{"observed_at":"2026-08-09T05:33:08.019558Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0205091","last_updated":"2002-05-07T05:56:17Z","snapshot_observed_at":"2026-07-07T00:26:21.116642Z","submitted_at":"2002-05-07T05:56:17Z","title":"Collapse of a Rotating Supermassive Star to a Supermassive Black Hole: Fully Relativistic Simulations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0205091","snapshot_observed_at":"2026-08-09T05:33:08.024639Z","title":"Shibata and S","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.024639Z"},"links":{"cited_paper":"/paper/astro-ph/0205091","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:49614dd7d1d1133ce85b4d35cb42bbb8adb67d2b1effb617e52ef5a2afa2c09a","observation_id":"6b8ad74e-1285-42f9-a05f-f0b299bb8748","resolution":{"observed_at":"2026-08-09T05:33:08.024639Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0706.2360","last_updated":"2007-10-28T18:24:52Z","snapshot_observed_at":"2026-07-06T01:28:40.706351Z","submitted_at":"2007-06-15T20:00:30Z","title":"Magnetorotational collapse of very massive stars to black holes in full general relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0706.2360","snapshot_observed_at":"2026-08-09T05:33:08.029684Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.029684Z"},"links":{"cited_paper":"/paper/0706.2360","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:ab190201ffeb498c87e117ac37d8f5e0f9bbc2c6918c200a8531d2b750fba236","observation_id":"3033f0c2-9bb7-4bca-9a82-2c0bd104e3b9","resolution":{"observed_at":"2026-08-09T05:33:08.029684Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.3090","last_updated":"2012-02-01T10:31:53Z","snapshot_observed_at":"2026-07-06T02:32:27.733250Z","submitted_at":"2011-08-15T20:27:12Z","title":"Relativistic collapse and explosion of rotating supermassive stars with thermonuclear effects","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.3090","snapshot_observed_at":"2026-08-09T05:33:08.035373Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.035373Z"},"links":{"cited_paper":"/paper/1108.3090","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:e00e06a01544ae3fc06bfb8d4f2cc967dadae68a9394c0801165b07f211b0fcf","observation_id":"d4764cff-d744-4bf9-b366-92e0f83ca0b0","resolution":{"observed_at":"2026-08-09T05:33:08.035373Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.07147","last_updated":"2016-06-23T01:01:51Z","snapshot_observed_at":"2026-07-06T05:00:59.523166Z","submitted_at":"2016-06-23T01:01:51Z","title":"Gravitational waves from supermassive stars collapsing to a supermassive black hole","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.07147","snapshot_observed_at":"2026-08-09T05:33:08.041178Z","title":"Shibata, Y","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.041178Z"},"links":{"cited_paper":"/paper/1606.07147","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:6918b5f04c5c592a861f0164a6f2c2187e35c165154b3a2f8ed12d713e33d489","observation_id":"def241e1-170f-42e1-9bd3-6fd37249ccb0","resolution":{"observed_at":"2026-08-09T05:33:08.041178Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.00433","last_updated":"2017-04-03T05:54:47Z","snapshot_observed_at":"2026-07-06T05:36:16.123121Z","submitted_at":"2017-04-03T05:54:47Z","title":"Gravitational Collapse of Rotating Supermassive Stars including Nuclear Burning Effects","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.00433","snapshot_observed_at":"2026-08-09T05:33:08.047149Z","title":"Uchida, M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.047149Z"},"links":{"cited_paper":"/paper/1704.00433","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:6473a9d760e5a94371ac1fbfd089f441248f825952f0c76ecb6d329d4d06c311","observation_id":"3c690d53-2e2d-4c3e-80d3-0a0e7236e168","resolution":{"observed_at":"2026-08-09T05:33:08.047149Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.10502","last_updated":"2018-09-27T13:10:54Z","snapshot_observed_at":"2026-07-06T07:04:39.537654Z","submitted_at":"2018-09-27T13:10:54Z","title":"Black Hole Formation and Explosion from Rapidly Rotating Very Massive Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.10502","snapshot_observed_at":"2026-08-09T05:33:08.052750Z","title":"Uchida, M","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.052750Z"},"links":{"cited_paper":"/paper/1809.10502","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:9a0cda801e3bf00c2209e59423c3f2a0ddd6aab6128b419914ef6dd93fb157a4","observation_id":"2e21bfd7-4a58-429b-9e79-faa08c5d8a9f","resolution":{"observed_at":"2026-08-09T05:33:08.052750Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.11572","last_updated":"2024-08-21T12:28:53Z","snapshot_observed_at":"2026-07-06T19:04:00.888268Z","submitted_at":"2024-08-21T12:28:53Z","title":"Powerful explosions from the collapse of rotating supermassive stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.11572","snapshot_observed_at":"2026-08-09T05:33:08.058157Z","title":"Fujibayashi, C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.058157Z"},"links":{"cited_paper":"/paper/2408.11572","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:f1815af8396a2f5745306bae2185d48837c9d3747a2ab5ff65b036866b135762","observation_id":"f8d8b4c3-2e67-4170-8fe4-c9b23bd9d0ef","resolution":{"observed_at":"2026-08-09T05:33:08.058157Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0805.3099","last_updated":"2008-08-20T22:14:26Z","snapshot_observed_at":"2026-07-06T01:38:38.867843Z","submitted_at":"2008-05-20T15:09:30Z","title":"NADA: A new code for studying self-gravitating tori around black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0805.3099","snapshot_observed_at":"2026-08-09T05:33:08.063763Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.063763Z"},"links":{"cited_paper":"/paper/0805.3099","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:eeb1f1e2ba5c1778bfcef879568ac0689e5413d863944d593619156fbaa942d4","observation_id":"c5411a2f-0115-49e0-886f-a7711b9d1958","resolution":{"observed_at":"2026-08-09T05:33:08.063763Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1004.3102","last_updated":"2010-04-19T06:22:47Z","snapshot_observed_at":"2026-08-03T21:09:34.302755Z","submitted_at":"2010-04-19T06:22:47Z","title":"Influence of self-gravity on the runaway instability of black hole-torus systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.3102","snapshot_observed_at":"2026-08-09T05:33:08.069013Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.069013Z"},"links":{"cited_paper":"/paper/1004.3102","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:fdf0d368434700c95bb5264d34ebe20a54d8f7741331cb0c8ccd252521387f72","observation_id":"9ba6962a-1984-46c5-8d84-3d6fc3ddce15","resolution":{"observed_at":"2026-08-09T05:33:08.069013Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1206.5911","last_updated":"2012-06-26T08:13:10Z","snapshot_observed_at":"2026-07-06T02:50:38.748297Z","submitted_at":"2012-06-26T08:13:10Z","title":"Radiation Magnetohydrodynamics for Black Hole-Torus System in Full General Relativity: A Step toward Physical Simulation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.5911","snapshot_observed_at":"2026-08-09T05:33:08.074315Z","title":"Shibata and Y","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.074315Z"},"links":{"cited_paper":"/paper/1206.5911","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:8789c3c7bd331573f66bbf970b4692466db180538bfb87be8483cb71a8100073","observation_id":"3947723e-0079-4c7d-8e0d-12e6b9d694a6","resolution":{"observed_at":"2026-08-09T05:33:08.074315Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0907.2760","last_updated":"2009-12-18T08:10:47Z","snapshot_observed_at":"2026-07-06T01:56:36.639996Z","submitted_at":"2009-07-16T08:33:39Z","title":"Higher-dimensional numerical relativity: Formulation and code tests","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0907.2760","snapshot_observed_at":"2026-08-09T05:33:08.079696Z","title":"Yoshino and M","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.079696Z"},"links":{"cited_paper":"/paper/0907.2760","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:918f1c2da50ed54bd749978e0dd9b9e26a751bc26bd002ccbbf44875803074b4","observation_id":"77657f17-7ac7-491c-94c3-067ed35986ae","resolution":{"observed_at":"2026-08-09T05:33:08.079696Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.10191","last_updated":"2017-07-17T23:59:24Z","snapshot_observed_at":"2026-07-06T05:35:45.732137Z","submitted_at":"2017-03-29T18:32:27Z","title":"Properties of Neutrino-driven Ejecta from the Remnant of Binary Neutron Star Merger : Purely Radiation Hydrodynamics Case","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.10191","snapshot_observed_at":"2026-08-09T05:33:08.086026Z","title":"Fujibayashi, Y","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.086026Z"},"links":{"cited_paper":"/paper/1703.10191","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:36cda151b4558edaab96960bad29447522bc2df6ee450c0c2a770d969920fda9","observation_id":"d391262a-13f4-4ab3-a88e-f2d09648ab51","resolution":{"observed_at":"2026-08-09T05:33:08.086026Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.04467","last_updated":"2020-01-13T19:00:00Z","snapshot_observed_at":"2026-08-08T13:10:51.151066Z","submitted_at":"2020-01-13T19:00:00Z","title":"Mass ejection from disks surrounding a low-mass black hole: Viscous neutrino-radiation hydrodynamics simulation in full general relativity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.04467","snapshot_observed_at":"2026-08-09T05:33:08.091389Z","title":"Fujibayashi, M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.091389Z"},"links":{"cited_paper":"/paper/2001.04467","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:bb2357e95a7eb8c5c7ad616033e7b503b6046b9ffa72ee4a99f75ffe04a2c29a","observation_id":"c2860eda-9cdc-4763-b9f2-734253dc4269","resolution":{"observed_at":"2026-08-09T05:33:08.091389Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.03895","last_updated":"2020-09-08T18:00:00Z","snapshot_observed_at":"2026-07-06T09:53:55.894497Z","submitted_at":"2020-09-08T18:00:00Z","title":"Viscous evolution of a massive disk surrounding stellar-mass black holes in full general relativity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.03895","snapshot_observed_at":"2026-08-09T05:33:08.096600Z","title":"Fujibayashi, M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.096600Z"},"links":{"cited_paper":"/paper/2009.03895","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:83c95ce35743e0cd7a7b5e8e9c20164d9d446fd3227e72effe7e6879b1cffb00","observation_id":"5e05403f-cb56-4581-84bf-08b93124aa07","resolution":{"observed_at":"2026-08-09T05:33:08.096600Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.01346","last_updated":"2021-02-02T06:46:56Z","snapshot_observed_at":"2026-07-06T10:37:43.118444Z","submitted_at":"2021-02-02T06:46:56Z","title":"Long-term evolution of a merger-remnant neutron star in general relativistic magnetohydrodynamics I: Effect of magnetic winding","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.01346","snapshot_observed_at":"2026-08-09T05:33:08.101891Z","title":"Shibata, S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.101891Z"},"links":{"cited_paper":"/paper/2102.01346","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:6a506b52f7fb825b894fa7f82dd55af7530f37c3edf3cc66e12e899aeb6b4edc","observation_id":"977cf1b2-871d-40a9-ba20-b7a8d1b73a52","resolution":{"observed_at":"2026-08-09T05:33:08.101891Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.08732","last_updated":"2021-09-17T19:26:25Z","snapshot_observed_at":"2026-07-06T11:48:52.330589Z","submitted_at":"2021-09-17T19:26:25Z","title":"Long-term evolution of neutron-star merger remnants in general relativistic resistive-magnetohydrodynamics with a mean-field dynamo term","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.08732","snapshot_observed_at":"2026-08-09T05:33:08.107987Z","title":"Shibata, S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.107987Z"},"links":{"cited_paper":"/paper/2109.08732","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:6acf620f9faa54a74d7e553ea17d005b35516e5d2e66c2e6dba4fea453ece269","observation_id":"7b5c5579-3f99-4eef-b1ad-1766e628e6bc","resolution":{"observed_at":"2026-08-09T05:33:08.107987Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.05557","last_updated":"2022-10-18T21:49:50Z","snapshot_observed_at":"2026-07-06T13:08:56.050466Z","submitted_at":"2022-05-11T15:04:13Z","title":"Comprehensive study of mass ejection and nucleosynthesis in binary neutron star mergers leaving short-lived massive neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.05557","snapshot_observed_at":"2026-08-09T05:33:08.113448Z","title":"Fujibayashi, K","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.113448Z"},"links":{"cited_paper":"/paper/2205.05557","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:1953e71f97083d0af20f5719a3d1a8eb41ef93a702c0f4824d5e5ef57aa06610","observation_id":"dfaeb1df-8efa-4811-8a27-78d5132be8fa","resolution":{"observed_at":"2026-08-09T05:33:08.113448Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.0627","last_updated":"2013-10-04T10:34:54Z","snapshot_observed_at":"2026-07-06T03:24:35.221990Z","submitted_at":"2013-10-02T09:10:30Z","title":"Coalescence of binary neutron stars in a scalar-tensor theory of gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.0627","snapshot_observed_at":"2026-08-09T05:33:08.118903Z","title":"Shibata, K","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.118903Z"},"links":{"cited_paper":"/paper/1310.0627","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:8d6bfbaf45eba716fa449e9cdfaaee5b0893947bb00731fc237c942aad70ad50","observation_id":"4af61dd6-5de0-41e7-903c-c5f9481a77b3","resolution":{"observed_at":"2026-08-09T05:33:08.118903Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1410.0738","last_updated":"2015-01-27T08:20:46Z","snapshot_observed_at":"2026-07-06T03:56:19.212671Z","submitted_at":"2014-10-03T01:41:31Z","title":"Quasiequilibrium sequences of binary neutron stars undergoing dynamical scalarization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.0738","snapshot_observed_at":"2026-08-09T05:33:08.124503Z","title":"Taniguchi, M","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.124503Z"},"links":{"cited_paper":"/paper/1410.0738","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:772c156fe98fe2f8d8ec7658105ff27dad7f2511ac163a67cb309d62ef12f336","observation_id":"6c44594c-cf7e-4021-97ad-b01e7edc0f4b","resolution":{"observed_at":"2026-08-09T05:33:08.124503Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.01709","last_updated":"2023-09-04T16:42:23Z","snapshot_observed_at":"2026-07-06T16:14:09.494600Z","submitted_at":"2023-09-04T16:42:23Z","title":"Binary neutron star mergers in massive scalar-tensor theory: Quasi-equilibrium states and dynamical enhancement of the scalarization","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.01709","snapshot_observed_at":"2026-08-09T05:33:08.129630Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.129630Z"},"links":{"cited_paper":"/paper/2309.01709","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:926926056529884ac227aef5fd86f9ad6dbd7b2f44139ae02bab9db945fd5db6","observation_id":"a16af902-3012-4f69-92b3-4c460f4f0214","resolution":{"observed_at":"2026-08-09T05:33:08.129630Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.05211","last_updated":"2024-06-07T18:51:51Z","snapshot_observed_at":"2026-08-08T06:55:37.352090Z","submitted_at":"2024-06-07T18:51:51Z","title":"Binary neutron star mergers in massive scalar-tensor theory: Properties of post-merger remnants","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.05211","snapshot_observed_at":"2026-08-09T05:33:08.134552Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.134552Z"},"links":{"cited_paper":"/paper/2406.05211","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:05a0de9dd9379679940c9752f569d64b6ae5f3d750de67e7ea0519023036fe84","observation_id":"3d952fdc-140b-4c94-aeac-c656c722a1d7","resolution":{"observed_at":"2026-08-09T05:33:08.134552Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.00137","last_updated":"2024-09-30T18:18:47Z","snapshot_observed_at":"2026-08-06T04:52:10.872615Z","submitted_at":"2024-09-30T18:18:47Z","title":"Accessing universal relations of binary neutron star waveforms in massive scalar-tensor theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.00137","snapshot_observed_at":"2026-08-09T05:33:08.140101Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.140101Z"},"links":{"cited_paper":"/paper/2410.00137","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:f17a376f1d2f772a430352342d829b07b418b1ed8fe0636a16e24626d001e17e","observation_id":"f98e77b2-ccf5-4f61-a475-41cdaee44885","resolution":{"observed_at":"2026-08-09T05:33:08.140101Z","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":"2026-08-09T05:47:49.070118Z","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":"2026-08-09T05:33:08.145376Z","title":"Witek, L","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.145376Z"},"links":{"cited_paper":"/paper/1810.05177","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:5aa360fd7f6fb0c33f9d06a29f657d5582cb63168e93ec453ea96c6bf90b8fc0","observation_id":"221a8be9-2196-4ba1-888c-804d7eb47321","resolution":{"observed_at":"2026-08-09T05:33:08.145376Z","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":"2026-08-09T02:23:02.989009Z","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":"2026-08-09T05:33:08.150614Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.150614Z"},"links":{"cited_paper":"/paper/1903.07543","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:f28b6caad736c0d92fc4ded1b6611e64b4552ba511a27aac246a238c700c100c","observation_id":"220fca2f-2f37-4811-a484-156515c3a083","resolution":{"observed_at":"2026-08-09T05:33:08.150614Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.11027","last_updated":"2020-02-10T16:31:21Z","snapshot_observed_at":"2026-07-06T08:39:49.849549Z","submitted_at":"2019-11-25T16:22:44Z","title":"Scalarized Black Hole dynamics in Einstein dilaton Gauss-Bonnet Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.11027","snapshot_observed_at":"2026-08-09T05:33:08.155794Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.155794Z"},"links":{"cited_paper":"/paper/1911.11027","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:fc33d2d68b10bd03cd4d46567b18ade17b3550c5a34faaacd544738705a67da0","observation_id":"d0cc152d-1eb4-4431-999c-88426edcf585","resolution":{"observed_at":"2026-08-09T05:33:08.155794Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.10436","last_updated":"2021-07-15T09:37:57Z","snapshot_observed_at":"2026-08-08T13:39:47.838278Z","submitted_at":"2020-12-18T18:54:51Z","title":"Dynamical descalarization in binary black hole mergers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.10436","snapshot_observed_at":"2026-08-09T05:33:08.161077Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.161077Z"},"links":{"cited_paper":"/paper/2012.10436","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:d5f9c31ffa6ae921fb0ba2c49d355241b00a1fa60516a9c35bf5546071d49f69","observation_id":"a95ec0c0-1a89-487f-ae24-50078797f62f","resolution":{"observed_at":"2026-08-09T05:33:08.161077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.09488","last_updated":"2022-11-28T16:25:31Z","snapshot_observed_at":"2026-08-09T07:47:38.859890Z","submitted_at":"2022-08-19T18:00:02Z","title":"Binary neutron star mergers in Einstein-scalar-Gauss-Bonnet gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.09488","snapshot_observed_at":"2026-08-09T05:33:08.166100Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.166100Z"},"links":{"cited_paper":"/paper/2208.09488","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:5362f08ad0612a751128ba17420910e2c8b912a225b7066ba50e925753aaab23","observation_id":"8b936a7c-c9cb-4592-8e0e-113f8c6fc630","resolution":{"observed_at":"2026-08-09T05:33:08.166100Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.11596","last_updated":"2023-02-22T19:00:14Z","snapshot_observed_at":"2026-08-08T23:36:43.202897Z","submitted_at":"2023-02-22T19:00:14Z","title":"Dynamical Scalarization during Neutron Star Mergers in scalar-Gauss-Bonnet Theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.11596","snapshot_observed_at":"2026-08-09T05:33:08.171489Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.171489Z"},"links":{"cited_paper":"/paper/2302.11596","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:87433a3496f8b0b7143eb80859ab53a24622ad6128d9b6c4d1216f77e54f8d80","observation_id":"e6ee952e-41da-407f-9e01-5db5a691f790","resolution":{"observed_at":"2026-08-09T05:33:08.171489Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1407.6727","last_updated":"2015-01-22T19:19:02Z","snapshot_observed_at":"2026-07-06T03:49:59.959272Z","submitted_at":"2014-07-24T20:22:27Z","title":"The Initial Value Formulation of Dynamical Chern-Simons Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.6727","snapshot_observed_at":"2026-08-09T05:33:08.176568Z","title":"Delsate, D","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.176568Z"},"links":{"cited_paper":"/paper/1407.6727","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:3576da45f8ed1f6b0055477b16d621d21d06cd92d33db48bcc27099c76ef3078","observation_id":"0f286089-0c4b-4531-9268-cbc79837b185","resolution":{"observed_at":"2026-08-09T05:33:08.176568Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.08789","last_updated":"2019-11-15T14:34:14Z","snapshot_observed_at":"2026-07-06T08:01:47.566114Z","submitted_at":"2019-06-20T18:00:22Z","title":"Numerical binary black hole collisions in dynamical Chern-Simons gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.08789","snapshot_observed_at":"2026-08-09T05:33:08.181522Z","title":"Okounkova, L","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.181522Z"},"links":{"cited_paper":"/paper/1906.08789","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:cb3be15969bd07e916670bfd904d609a447328271637a28466526037449b80c0","observation_id":"2a75c7b0-db3f-4186-9e98-d1c6677feff1","resolution":{"observed_at":"2026-08-09T05:33:08.181522Z","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":"2026-08-08T15:21:09.260716Z","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":"2026-08-09T05:33:08.186365Z","title":"Okounkova, L","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.186365Z"},"links":{"cited_paper":"/paper/1911.02588","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:20b6308883f7347ab1c99fbe9629c9202a56ff0df4fb714f7a09bff0018a1da7","observation_id":"612efff2-f2e8-4ad3-98a7-6a7e6813ffe6","resolution":{"observed_at":"2026-08-09T05:33:08.186365Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.07704","last_updated":"2023-05-12T18:01:04Z","snapshot_observed_at":"2026-07-06T15:26:38.838948Z","submitted_at":"2023-05-12T18:01:04Z","title":"Black Holes in Massive Dynamical Chern-Simons gravity: scalar hair and quasibound states at decoupling","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.07704","snapshot_observed_at":"2026-08-09T05:33:08.191568Z","title":"Richards, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.191568Z"},"links":{"cited_paper":"/paper/2305.07704","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:606ea6154c66cd9472f3bdeb5f5a0453f928417a4be4499d6a3d396464abaaee","observation_id":"7a81d579-d104-4cc8-a805-87b52f375e51","resolution":{"observed_at":"2026-08-09T05:33:08.191568Z","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":"2026-08-09T05:33:08.196589Z","title":"Bezares, R","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.196589Z"},"links":{"cited_paper":"/paper/2107.05648","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:c65a133ac90870bbdd0e4c54782389d3713f57f4096b95397fb4e0b39b1737f2","observation_id":"bbe1113f-37a5-4581-af56-76c715f724cf","resolution":{"observed_at":"2026-08-09T05:33:08.196589Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.12139","last_updated":"2023-02-21T12:00:27Z","snapshot_observed_at":"2026-07-06T14:08:49.704572Z","submitted_at":"2022-10-21T17:50:20Z","title":"Properties of scalar wave emission in a scalar-tensor theory with kinetic screening","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.12139","snapshot_observed_at":"2026-08-09T05:33:08.201327Z","title":"Shibata and D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.201327Z"},"links":{"cited_paper":"/paper/2210.12139","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:d3dd3a11667828a86fbc7f7fde890d37d7c92b49231fc7b5fda40bcdf1a7eda2","observation_id":"6e21174d-8abc-4a4b-b638-7514382ff76d","resolution":{"observed_at":"2026-08-09T05:33:08.201327Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.04175","last_updated":"2016-06-22T13:20:32Z","snapshot_observed_at":"2026-07-06T04:52:52.890087Z","submitted_at":"2016-04-14T14:51:37Z","title":"Highly compact neutron stars in scalar-tensor theories of gravity: Spontaneous scalarization versus gravitational collapse","version":2},"cited_work":{"arxiv_id":"1604.04175","doi":null,"metadata_source":"pith","pith_arxiv_id":"1604.04175","snapshot_observed_at":"2026-08-09T05:33:10.019243Z","title":"Highly compact neutron stars in scalar-tensor theories of gravity: Spontaneous scalarization versus gravitational collapse","venue":"gr-qc","work_id":"66538837-14e2-4d40-8c9e-37cf59882f7e","year":2016},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.206139Z"},"links":{"cited_paper":"/paper/1604.04175","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:6246fe56a925e7293c75d1e56e3cd7064561be1442a1b33ebf6e96110fd8c915","observation_id":"8c64855d-044c-4485-a6d5-2c44a7d94d39","resolution":{"observed_at":"2026-08-09T05:33:10.025094Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1708.03651","last_updated":"2017-12-01T12:35:46Z","snapshot_observed_at":"2026-08-05T10:33:37.049506Z","submitted_at":"2017-08-11T18:19:06Z","title":"Long-lived inverse chirp signals from core collapse in massive scalar-tensor gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.03651","snapshot_observed_at":"2026-08-09T05:33:08.211176Z","title":"Sperhake, C","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.211176Z"},"links":{"cited_paper":"/paper/1708.03651","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:764c8d251b5f0cfbe3ec71d3b95d8caa91c2b349dd4dab714b3bb32ad170ab61","observation_id":"6d561202-b520-4846-87cc-73d79e0f52bd","resolution":{"observed_at":"2026-08-09T05:33:08.211176Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.04835","last_updated":"2019-08-29T07:13:51Z","snapshot_observed_at":"2026-08-09T23:57:36.686289Z","submitted_at":"2018-12-12T07:37:44Z","title":"Numerical studies on core collapse supernova in self-interacting massive scalar-tensor gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.04835","snapshot_observed_at":"2026-08-09T05:33:08.216150Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.216150Z"},"links":{"cited_paper":"/paper/1812.04835","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:8b9e0ffcad144fec3a6ec5a2b09eba053eef0babead51f1c6e5a7cf2b6db48ba","observation_id":"368e1f02-8177-4bdd-922d-8770985366b7","resolution":{"observed_at":"2026-08-09T05:33:08.216150Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.11999","last_updated":"2021-10-15T15:07:57Z","snapshot_observed_at":"2026-07-06T10:52:11.851830Z","submitted_at":"2021-03-22T16:47:20Z","title":"Dynamical Formation of Scalarized Black Holes and Neutron Stars through Stellar Core Collapse","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.11999","snapshot_observed_at":"2026-08-09T05:33:08.220943Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.220943Z"},"links":{"cited_paper":"/paper/2103.11999","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:ca28b8776763cdb415ba0f236291e685c05aaa86b83c9017052b48e3d6f81274","observation_id":"086ef7db-b373-42ab-9152-caf1c01e918c","resolution":{"observed_at":"2026-08-09T05:33:08.220943Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.08543","last_updated":"2021-05-18T14:22:50Z","snapshot_observed_at":"2026-08-03T05:20:59.552320Z","submitted_at":"2021-05-18T14:22:50Z","title":"Nonlinear evolution and non-uniqueness of scalarized neutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.08543","snapshot_observed_at":"2026-08-09T05:33:08.225861Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.225861Z"},"links":{"cited_paper":"/paper/2105.08543","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:bd2f1ae1d66847cd128c1d14122a767c51f19b604eeaa94ebb2bbf7ffd6b87c2","observation_id":"5c2b7b89-b1b5-40e7-b646-fe2b257df7e9","resolution":{"observed_at":"2026-08-09T05:33:08.225861Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.03672","last_updated":"2022-08-31T16:21:31Z","snapshot_observed_at":"2026-07-06T12:45:17.935007Z","submitted_at":"2022-03-07T19:11:07Z","title":"Gravitational waves from accretion-induced descalarization in massive scalar-tensor theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.03672","snapshot_observed_at":"2026-08-09T05:33:08.230985Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-09T05:33:08.230985Z"},"links":{"cited_paper":"/paper/2203.03672","citing_paper":"/paper/2502.03223"},"observation_digest":"sha256:38bdac8cabd992792c0eb138b8dad9f842ec21a2098bacf2f4b8bb6041214c64","observation_id":"5285f4a3-5c54-408e-b115-acae848a4eb5","resolution":{"observed_at":"2026-08-09T05:33:08.230985Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2502.03223","last_updated":"2025-02-05T14:41:39Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-09T07:48:03.159202Z","submitted_at":"2025-02-05T14:41:39Z","title":"SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":99,"verified_exact":1,"verified_fuzzy":0},"total_outbound_references":172},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 100 of 172 outbound references and 3 inbound Pith citation observations for arXiv:2502.03223."}