{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:PECZWJRZC4MGI2W7TVL7E77Y4D","short_pith_number":"pith:PECZWJRZ","schema_version":"1.0","canonical_sha256":"79059b26391718646adf9d57f27ff8e0d775ffcf93b577b5b7c7e3483ba45fc7","source":{"kind":"arxiv","id":"2504.15334","version":1},"attestation_state":"computed","paper":{"title":"Discovering $\\mu$Hz gravitational waves and ultra-light dark matter with binary resonances","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Adrien Bourgoin, Alexander C. Jenkins, Aurelien Hees, Diego Blas, Joshua W. Foster, M\\'iriam Herrero-Valea, Xiao Xue","submitted_at":"2025-04-21T18:00:00Z","abstract_excerpt":"In the presence of a weak gravitational wave (GW) background, astrophysical binary systems act as high-quality resonators, with efficient transfer of energy and momentum between the orbit and a harmonic GW leading to potentially detectable orbital perturbations. In this work, we develop and apply a novel modeling and analysis framework that describes the imprints of GWs on binary systems in a fully time-resolved manner to study the sensitivity of lunar laser ranging, satellite laser ranging, and pulsar timing to both resonant and nonresonant GW backgrounds. We demonstrate that optimal data col"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2504.15334","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2025-04-21T18:00:00Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"dfc8ca44486496f8eaa4eb7c9636d61d569c7245861da062b34c4bf34adeed76","abstract_canon_sha256":"d9b3c214ec3ab33a0b21795cc511c6833553489281f07807641c4c3e7a732321"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:52:00.975842Z","signature_b64":"/LIQLJaP2CXZwmQ4AAvA+xo1Fi0xJcUmvg/ephqoOEFEWegqUCmNtvXHEyyK7QxreTC5zTuKtd1/q+MFEOKbBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"79059b26391718646adf9d57f27ff8e0d775ffcf93b577b5b7c7e3483ba45fc7","last_reissued_at":"2026-07-05T10:52:00.975437Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:52:00.975437Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Discovering $\\mu$Hz gravitational waves and ultra-light dark matter with binary resonances","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Adrien Bourgoin, Alexander C. Jenkins, Aurelien Hees, Diego Blas, Joshua W. Foster, M\\'iriam Herrero-Valea, Xiao Xue","submitted_at":"2025-04-21T18:00:00Z","abstract_excerpt":"In the presence of a weak gravitational wave (GW) background, astrophysical binary systems act as high-quality resonators, with efficient transfer of energy and momentum between the orbit and a harmonic GW leading to potentially detectable orbital perturbations. In this work, we develop and apply a novel modeling and analysis framework that describes the imprints of GWs on binary systems in a fully time-resolved manner to study the sensitivity of lunar laser ranging, satellite laser ranging, and pulsar timing to both resonant and nonresonant GW backgrounds. We demonstrate that optimal data col"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2504.15334","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2504.15334/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2504.15334","created_at":"2026-07-05T10:52:00.975495+00:00"},{"alias_kind":"arxiv_version","alias_value":"2504.15334v1","created_at":"2026-07-05T10:52:00.975495+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2504.15334","created_at":"2026-07-05T10:52:00.975495+00:00"},{"alias_kind":"pith_short_12","alias_value":"PECZWJRZC4MG","created_at":"2026-07-05T10:52:00.975495+00:00"},{"alias_kind":"pith_short_16","alias_value":"PECZWJRZC4MGI2W7","created_at":"2026-07-05T10:52:00.975495+00:00"},{"alias_kind":"pith_short_8","alias_value":"PECZWJRZ","created_at":"2026-07-05T10:52:00.975495+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2607.00072","citing_title":"Precision Solar System Dynamics for Ultralight Dark Matter Search","ref_index":58,"is_internal_anchor":false},{"citing_arxiv_id":"2605.04110","citing_title":"High-Power AM-CW Lunar Laser Ranging as a $\\mu$Hz SGWB Detector","ref_index":7,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06082","citing_title":"Hunting Dark Matter with the Einstein Telescope","ref_index":79,"is_internal_anchor":false},{"citing_arxiv_id":"2604.21013","citing_title":"Archival Multiband Gravitational-Wave Signals from Massive Black Hole Binary Mergers","ref_index":112,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26092","citing_title":"Sensitivity of binary pulsar timing to spin-0 and spin-1 ultralight dark matter","ref_index":39,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PECZWJRZC4MGI2W7TVL7E77Y4D","json":"https://pith.science/pith/PECZWJRZC4MGI2W7TVL7E77Y4D.json","graph_json":"https://pith.science/api/pith-number/PECZWJRZC4MGI2W7TVL7E77Y4D/graph.json","events_json":"https://pith.science/api/pith-number/PECZWJRZC4MGI2W7TVL7E77Y4D/events.json","paper":"https://pith.science/paper/PECZWJRZ"},"agent_actions":{"view_html":"https://pith.science/pith/PECZWJRZC4MGI2W7TVL7E77Y4D","download_json":"https://pith.science/pith/PECZWJRZC4MGI2W7TVL7E77Y4D.json","view_paper":"https://pith.science/paper/PECZWJRZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2504.15334&json=true","fetch_graph":"https://pith.science/api/pith-number/PECZWJRZC4MGI2W7TVL7E77Y4D/graph.json","fetch_events":"https://pith.science/api/pith-number/PECZWJRZC4MGI2W7TVL7E77Y4D/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PECZWJRZC4MGI2W7TVL7E77Y4D/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PECZWJRZC4MGI2W7TVL7E77Y4D/action/storage_attestation","attest_author":"https://pith.science/pith/PECZWJRZC4MGI2W7TVL7E77Y4D/action/author_attestation","sign_citation":"https://pith.science/pith/PECZWJRZC4MGI2W7TVL7E77Y4D/action/citation_signature","submit_replication":"https://pith.science/pith/PECZWJRZC4MGI2W7TVL7E77Y4D/action/replication_record"}},"created_at":"2026-07-05T10:52:00.975495+00:00","updated_at":"2026-07-05T10:52:00.975495+00:00"}