{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:TP3OUTLW4XKNY3FK7O3RQTAOKL","short_pith_number":"pith:TP3OUTLW","schema_version":"1.0","canonical_sha256":"9bf6ea4d76e5d4dc6caafbb7184c0e52eb234213e72b82ed9dacdc203f6cf737","source":{"kind":"arxiv","id":"1712.01396","version":2},"attestation_state":"computed","paper":{"title":"Gravitational-Wave Fringes at LIGO: Detecting Compact Dark Matter by Gravitational Lensing","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Chang Sub Shin, Sunghoon Jung","submitted_at":"2017-12-04T22:36:46Z","abstract_excerpt":"Utilizing gravitational-wave (GW) lensing opens a new way to understand the small-scale structure of the universe. We show that, in spite of its coarse angular resolution and short duration of observation, LIGO can detect the GW lensing induced by compact structures, in particular by compact dark matter (DM) or primordial black holes of $10 - 10^5 \\, M_\\odot$, which remain interesting DM candidates. The lensing is detected through GW frequency chirping, creating the natural and rapid change of lensing patterns: \\emph{frequency-dependent amplification and modulation} of GW waveforms. As a highe"},"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":"1712.01396","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-12-04T22:36:46Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"d07aa7d52e257e0faea3ad5c27c2a1610be311d6948e8aac85adcdc6ce75ce6e","abstract_canon_sha256":"5dc5815bb3cd192613ee9ed3b63db446c3b434553d0020862285aaeeaf8ec436"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:54:44.285524Z","signature_b64":"/mBaAtAgQGG4HX/V7trgtuRy2ozgH//oqTlQoG3ny940mX8P76IDuOd2Kper6GJwLZINwtrXG71t8zOJd2xVDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9bf6ea4d76e5d4dc6caafbb7184c0e52eb234213e72b82ed9dacdc203f6cf737","last_reissued_at":"2026-05-17T23:54:44.285088Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:54:44.285088Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational-Wave Fringes at LIGO: Detecting Compact Dark Matter by Gravitational Lensing","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Chang Sub Shin, Sunghoon Jung","submitted_at":"2017-12-04T22:36:46Z","abstract_excerpt":"Utilizing gravitational-wave (GW) lensing opens a new way to understand the small-scale structure of the universe. We show that, in spite of its coarse angular resolution and short duration of observation, LIGO can detect the GW lensing induced by compact structures, in particular by compact dark matter (DM) or primordial black holes of $10 - 10^5 \\, M_\\odot$, which remain interesting DM candidates. The lensing is detected through GW frequency chirping, creating the natural and rapid change of lensing patterns: \\emph{frequency-dependent amplification and modulation} of GW waveforms. As a highe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1712.01396","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"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":"1712.01396","created_at":"2026-05-17T23:54:44.285170+00:00"},{"alias_kind":"arxiv_version","alias_value":"1712.01396v2","created_at":"2026-05-17T23:54:44.285170+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1712.01396","created_at":"2026-05-17T23:54:44.285170+00:00"},{"alias_kind":"pith_short_12","alias_value":"TP3OUTLW4XKN","created_at":"2026-05-18T12:31:46.661854+00:00"},{"alias_kind":"pith_short_16","alias_value":"TP3OUTLW4XKNY3FK","created_at":"2026-05-18T12:31:46.661854+00:00"},{"alias_kind":"pith_short_8","alias_value":"TP3OUTLW","created_at":"2026-05-18T12:31:46.661854+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":5,"sample":[{"citing_arxiv_id":"2606.21519","citing_title":"Wave-optics imprints of dark matter subhalos on strongly lensed gravitational waves. II. Saddle images and detectability","ref_index":28,"is_internal_anchor":true},{"citing_arxiv_id":"2606.17765","citing_title":"Effective description of lensed gravitational waves diffracted by stellar fields","ref_index":91,"is_internal_anchor":true},{"citing_arxiv_id":"2606.12792","citing_title":"Identification of Lensed Gravitational-Wave Beat Patterns by LISA","ref_index":36,"is_internal_anchor":true},{"citing_arxiv_id":"2605.21584","citing_title":"Wave-optics gravitational wave lensing in modified gravity","ref_index":51,"is_internal_anchor":true},{"citing_arxiv_id":"2505.20996","citing_title":"Parameter inference of millilensed gravitational waves using neural spline flows","ref_index":23,"is_internal_anchor":true},{"citing_arxiv_id":"2604.08179","citing_title":"GW231123: False Massive Graviton Signatures from Unmodeled Point-Mass Lensing","ref_index":24,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TP3OUTLW4XKNY3FK7O3RQTAOKL","json":"https://pith.science/pith/TP3OUTLW4XKNY3FK7O3RQTAOKL.json","graph_json":"https://pith.science/api/pith-number/TP3OUTLW4XKNY3FK7O3RQTAOKL/graph.json","events_json":"https://pith.science/api/pith-number/TP3OUTLW4XKNY3FK7O3RQTAOKL/events.json","paper":"https://pith.science/paper/TP3OUTLW"},"agent_actions":{"view_html":"https://pith.science/pith/TP3OUTLW4XKNY3FK7O3RQTAOKL","download_json":"https://pith.science/pith/TP3OUTLW4XKNY3FK7O3RQTAOKL.json","view_paper":"https://pith.science/paper/TP3OUTLW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1712.01396&json=true","fetch_graph":"https://pith.science/api/pith-number/TP3OUTLW4XKNY3FK7O3RQTAOKL/graph.json","fetch_events":"https://pith.science/api/pith-number/TP3OUTLW4XKNY3FK7O3RQTAOKL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TP3OUTLW4XKNY3FK7O3RQTAOKL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TP3OUTLW4XKNY3FK7O3RQTAOKL/action/storage_attestation","attest_author":"https://pith.science/pith/TP3OUTLW4XKNY3FK7O3RQTAOKL/action/author_attestation","sign_citation":"https://pith.science/pith/TP3OUTLW4XKNY3FK7O3RQTAOKL/action/citation_signature","submit_replication":"https://pith.science/pith/TP3OUTLW4XKNY3FK7O3RQTAOKL/action/replication_record"}},"created_at":"2026-05-17T23:54:44.285170+00:00","updated_at":"2026-05-17T23:54:44.285170+00:00"}