{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:ABIMEYIM7CZSB2P5DWDWRMVCX4","short_pith_number":"pith:ABIMEYIM","schema_version":"1.0","canonical_sha256":"0050c2610cf8b320e9fd1d8768b2a2bf1c231dc1ecd50814c878f1fb2ae1d3f3","source":{"kind":"arxiv","id":"1803.10204","version":2},"attestation_state":"computed","paper":{"title":"Gravitational waves from quasinormal modes of a class of Lorentzian wormholes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"S. Aneesh, Sayan Kar, Sukanta Bose","submitted_at":"2018-03-27T17:41:04Z","abstract_excerpt":"Quasinormal modes of a two-parameter family of Lorentzian wormhole spacetimes, which arise as solutions in a specific scalar-tensor theory associated with braneworld gravity, are obtained using standard numerical methods. Being solutions in a scalar-tensor theory, these wormholes can exist with matter satisfying the Weak Energy Condition. If one posits that the end-state of stellar-mass binary black hole mergers, of the type observed in GW150914, can be these wormholes, then we show how their properties can be measured from their distinct signatures in the gravitational waves emitted by them a"},"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":"1803.10204","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2018-03-27T17:41:04Z","cross_cats_sorted":[],"title_canon_sha256":"1e305fc375b0ab9642b5159708be6f4da69d1bd45e3b7e38576052304ac687c0","abstract_canon_sha256":"b0d75b65cc98517b36bc8a12afc92927a108328fd1846fdb8fcdecfb15c477a5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:11:49.501047Z","signature_b64":"R8/+fnGoFKI6rXFP2x/myb9fL9tbDZQeQjiV0+Es+PiLfRSa+/5nNrzfhNBOmip1dZa70Ovz2N2q/b6TQeUOBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0050c2610cf8b320e9fd1d8768b2a2bf1c231dc1ecd50814c878f1fb2ae1d3f3","last_reissued_at":"2026-05-18T00:11:49.500435Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:11:49.500435Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational waves from quasinormal modes of a class of Lorentzian wormholes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"S. Aneesh, Sayan Kar, Sukanta Bose","submitted_at":"2018-03-27T17:41:04Z","abstract_excerpt":"Quasinormal modes of a two-parameter family of Lorentzian wormhole spacetimes, which arise as solutions in a specific scalar-tensor theory associated with braneworld gravity, are obtained using standard numerical methods. Being solutions in a scalar-tensor theory, these wormholes can exist with matter satisfying the Weak Energy Condition. If one posits that the end-state of stellar-mass binary black hole mergers, of the type observed in GW150914, can be these wormholes, then we show how their properties can be measured from their distinct signatures in the gravitational waves emitted by them a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1803.10204","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":"1803.10204","created_at":"2026-05-18T00:11:49.500537+00:00"},{"alias_kind":"arxiv_version","alias_value":"1803.10204v2","created_at":"2026-05-18T00:11:49.500537+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1803.10204","created_at":"2026-05-18T00:11:49.500537+00:00"},{"alias_kind":"pith_short_12","alias_value":"ABIMEYIM7CZS","created_at":"2026-05-18T12:32:13.499390+00:00"},{"alias_kind":"pith_short_16","alias_value":"ABIMEYIM7CZSB2P5","created_at":"2026-05-18T12:32:13.499390+00:00"},{"alias_kind":"pith_short_8","alias_value":"ABIMEYIM","created_at":"2026-05-18T12:32:13.499390+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.21533","citing_title":"Long-lived quasinormal modes of Asymptotically de Sitter Black Holes in Generalized Proca Theory","ref_index":110,"is_internal_anchor":true},{"citing_arxiv_id":"2605.12113","citing_title":"Quasinormal Spectra of Fields of Various Spin in Asymptotically de Sitter Black Holes within Generalized Proca Theory","ref_index":82,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03659","citing_title":"Long-lived massive scalar modes, grey-body factors, and absorption cross sections of the Reissner--Nordstr\\\"om-like brane-world black hole","ref_index":88,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ABIMEYIM7CZSB2P5DWDWRMVCX4","json":"https://pith.science/pith/ABIMEYIM7CZSB2P5DWDWRMVCX4.json","graph_json":"https://pith.science/api/pith-number/ABIMEYIM7CZSB2P5DWDWRMVCX4/graph.json","events_json":"https://pith.science/api/pith-number/ABIMEYIM7CZSB2P5DWDWRMVCX4/events.json","paper":"https://pith.science/paper/ABIMEYIM"},"agent_actions":{"view_html":"https://pith.science/pith/ABIMEYIM7CZSB2P5DWDWRMVCX4","download_json":"https://pith.science/pith/ABIMEYIM7CZSB2P5DWDWRMVCX4.json","view_paper":"https://pith.science/paper/ABIMEYIM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1803.10204&json=true","fetch_graph":"https://pith.science/api/pith-number/ABIMEYIM7CZSB2P5DWDWRMVCX4/graph.json","fetch_events":"https://pith.science/api/pith-number/ABIMEYIM7CZSB2P5DWDWRMVCX4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ABIMEYIM7CZSB2P5DWDWRMVCX4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ABIMEYIM7CZSB2P5DWDWRMVCX4/action/storage_attestation","attest_author":"https://pith.science/pith/ABIMEYIM7CZSB2P5DWDWRMVCX4/action/author_attestation","sign_citation":"https://pith.science/pith/ABIMEYIM7CZSB2P5DWDWRMVCX4/action/citation_signature","submit_replication":"https://pith.science/pith/ABIMEYIM7CZSB2P5DWDWRMVCX4/action/replication_record"}},"created_at":"2026-05-18T00:11:49.500537+00:00","updated_at":"2026-05-18T00:11:49.500537+00:00"}