{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:M32PGYIEQE2CWCF53PQSMZLBNM","short_pith_number":"pith:M32PGYIE","schema_version":"1.0","canonical_sha256":"66f4f3610481342b08bddbe12665616b3dd4fdf4ad863107c35472a11559d823","source":{"kind":"arxiv","id":"2107.04601","version":3},"attestation_state":"computed","paper":{"title":"Bridging the $\\mu$Hz gap in the gravitational-wave landscape with binary resonance","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Alexander C. Jenkins, Diego Blas","submitted_at":"2021-07-09T18:00:02Z","abstract_excerpt":"Gravitational-wave (GW) astronomy is transforming our understanding of the Universe by probing phenomena invisible to electromagnetic observatories. A comprehensive exploration of the GW frequency spectrum is essential to fully harness this potential. Remarkably, current methods have left the $\\mu$Hz frequency band almost untouched. Here, we show that this $\\mu$Hz gap can be filled by searching for deviations in the orbits of binary systems caused by their resonant interaction with GWs. In particular, we show that laser ranging of the Moon and artificial satellites around the Earth, as well as"},"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":"2107.04601","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2021-07-09T18:00:02Z","cross_cats_sorted":["astro-ph.IM","gr-qc","hep-ph"],"title_canon_sha256":"a7a70fb7e54ce3c14bd9ebc9b3810fe79e392c7f500967268a88187dea1d5511","abstract_canon_sha256":"b7acd619af84da0934457ab484088e3b6b873b6eafe10f92928688a3a0bdd754"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:03:48.843832Z","signature_b64":"LIVBjtFmBEUqbDURJzA140CcVhGsIZYBG3OIQOu6eymafCNz0phmqB5FV6qfNB/7rS+wPqGtTSxK024hwmU7Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"66f4f3610481342b08bddbe12665616b3dd4fdf4ad863107c35472a11559d823","last_reissued_at":"2026-07-05T04:03:48.843352Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:03:48.843352Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Bridging the $\\mu$Hz gap in the gravitational-wave landscape with binary resonance","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Alexander C. Jenkins, Diego Blas","submitted_at":"2021-07-09T18:00:02Z","abstract_excerpt":"Gravitational-wave (GW) astronomy is transforming our understanding of the Universe by probing phenomena invisible to electromagnetic observatories. A comprehensive exploration of the GW frequency spectrum is essential to fully harness this potential. Remarkably, current methods have left the $\\mu$Hz frequency band almost untouched. Here, we show that this $\\mu$Hz gap can be filled by searching for deviations in the orbits of binary systems caused by their resonant interaction with GWs. In particular, we show that laser ranging of the Moon and artificial satellites around the Earth, as well as"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2107.04601","kind":"arxiv","version":3},"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/2107.04601/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":"2107.04601","created_at":"2026-07-05T04:03:48.843410+00:00"},{"alias_kind":"arxiv_version","alias_value":"2107.04601v3","created_at":"2026-07-05T04:03:48.843410+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2107.04601","created_at":"2026-07-05T04:03:48.843410+00:00"},{"alias_kind":"pith_short_12","alias_value":"M32PGYIEQE2C","created_at":"2026-07-05T04:03:48.843410+00:00"},{"alias_kind":"pith_short_16","alias_value":"M32PGYIEQE2CWCF5","created_at":"2026-07-05T04:03:48.843410+00:00"},{"alias_kind":"pith_short_8","alias_value":"M32PGYIE","created_at":"2026-07-05T04:03:48.843410+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2607.00072","citing_title":"Precision Solar System Dynamics for Ultralight Dark Matter Search","ref_index":55,"is_internal_anchor":false},{"citing_arxiv_id":"2605.21474","citing_title":"Gravitational Waves from Black Hole Reheating: The Scalar-Induced Component","ref_index":243,"is_internal_anchor":false},{"citing_arxiv_id":"2605.21477","citing_title":"Opening the Window of Ultra-Light PBHs by Exorcising the Poltergeist","ref_index":83,"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":2,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/M32PGYIEQE2CWCF53PQSMZLBNM","json":"https://pith.science/pith/M32PGYIEQE2CWCF53PQSMZLBNM.json","graph_json":"https://pith.science/api/pith-number/M32PGYIEQE2CWCF53PQSMZLBNM/graph.json","events_json":"https://pith.science/api/pith-number/M32PGYIEQE2CWCF53PQSMZLBNM/events.json","paper":"https://pith.science/paper/M32PGYIE"},"agent_actions":{"view_html":"https://pith.science/pith/M32PGYIEQE2CWCF53PQSMZLBNM","download_json":"https://pith.science/pith/M32PGYIEQE2CWCF53PQSMZLBNM.json","view_paper":"https://pith.science/paper/M32PGYIE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2107.04601&json=true","fetch_graph":"https://pith.science/api/pith-number/M32PGYIEQE2CWCF53PQSMZLBNM/graph.json","fetch_events":"https://pith.science/api/pith-number/M32PGYIEQE2CWCF53PQSMZLBNM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/M32PGYIEQE2CWCF53PQSMZLBNM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/M32PGYIEQE2CWCF53PQSMZLBNM/action/storage_attestation","attest_author":"https://pith.science/pith/M32PGYIEQE2CWCF53PQSMZLBNM/action/author_attestation","sign_citation":"https://pith.science/pith/M32PGYIEQE2CWCF53PQSMZLBNM/action/citation_signature","submit_replication":"https://pith.science/pith/M32PGYIEQE2CWCF53PQSMZLBNM/action/replication_record"}},"created_at":"2026-07-05T04:03:48.843410+00:00","updated_at":"2026-07-05T04:03:48.843410+00:00"}