{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:IA2I2JVO33AVKKWPYMXJD26HM3","short_pith_number":"pith:IA2I2JVO","schema_version":"1.0","canonical_sha256":"40348d26aedec1552acfc32e91ebc766d1482645f622c8272f8bf6c5260da5ce","source":{"kind":"arxiv","id":"1808.10732","version":1},"attestation_state":"computed","paper":{"title":"Gravitational Waves from Dark Boson Star binary mergers","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Carlos Palenzuela, Miguel Bezares","submitted_at":"2018-08-31T13:23:57Z","abstract_excerpt":"Gravitational wave astronomy might allow us to detect the coalescence of low-brightness astrophysical compact objects which are extremely difficult to be observed with current electromagnetic telescopes. Besides classical sources like black holes and neutron stars, other candidates include Exotic Compact Objects (ECOs), which could exist in theory but have never yet been observed in Nature. Among different possibilities, here we consider Dark Stars, astrophysical compact objects made of dark matter such that only interact with other stars through gravity. We study numerically the dynamics and "},"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":"1808.10732","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2018-08-31T13:23:57Z","cross_cats_sorted":[],"title_canon_sha256":"44848c0534093b7727ff6766e1305a616d64978cd6f49d80bf7167683d461d5a","abstract_canon_sha256":"49a0210285aa82c7cc6e39772c5e8bd0e2b8906bbfeee43bce4d30507b6dc114"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:59:22.339912Z","signature_b64":"b219njZD+TGzDRVp1b13AzfjXO84OIvcV4c6dweGP/mHQHT4vfKZ+JKTA+sdavkSVSUYHQnoMyI6if0HbmVfCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"40348d26aedec1552acfc32e91ebc766d1482645f622c8272f8bf6c5260da5ce","last_reissued_at":"2026-05-17T23:59:22.339577Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:59:22.339577Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational Waves from Dark Boson Star binary mergers","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Carlos Palenzuela, Miguel Bezares","submitted_at":"2018-08-31T13:23:57Z","abstract_excerpt":"Gravitational wave astronomy might allow us to detect the coalescence of low-brightness astrophysical compact objects which are extremely difficult to be observed with current electromagnetic telescopes. Besides classical sources like black holes and neutron stars, other candidates include Exotic Compact Objects (ECOs), which could exist in theory but have never yet been observed in Nature. Among different possibilities, here we consider Dark Stars, astrophysical compact objects made of dark matter such that only interact with other stars through gravity. We study numerically the dynamics and "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1808.10732","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":""},"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":"1808.10732","created_at":"2026-05-17T23:59:22.339629+00:00"},{"alias_kind":"arxiv_version","alias_value":"1808.10732v1","created_at":"2026-05-17T23:59:22.339629+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1808.10732","created_at":"2026-05-17T23:59:22.339629+00:00"},{"alias_kind":"pith_short_12","alias_value":"IA2I2JVO33AV","created_at":"2026-05-18T12:32:28.185984+00:00"},{"alias_kind":"pith_short_16","alias_value":"IA2I2JVO33AVKKWP","created_at":"2026-05-18T12:32:28.185984+00:00"},{"alias_kind":"pith_short_8","alias_value":"IA2I2JVO","created_at":"2026-05-18T12:32:28.185984+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1202.5809","citing_title":"Dynamical Boson Stars","ref_index":55,"is_internal_anchor":true},{"citing_arxiv_id":"2604.15240","citing_title":"Boson star-black hole binaries: initial data and head-on collisions","ref_index":78,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IA2I2JVO33AVKKWPYMXJD26HM3","json":"https://pith.science/pith/IA2I2JVO33AVKKWPYMXJD26HM3.json","graph_json":"https://pith.science/api/pith-number/IA2I2JVO33AVKKWPYMXJD26HM3/graph.json","events_json":"https://pith.science/api/pith-number/IA2I2JVO33AVKKWPYMXJD26HM3/events.json","paper":"https://pith.science/paper/IA2I2JVO"},"agent_actions":{"view_html":"https://pith.science/pith/IA2I2JVO33AVKKWPYMXJD26HM3","download_json":"https://pith.science/pith/IA2I2JVO33AVKKWPYMXJD26HM3.json","view_paper":"https://pith.science/paper/IA2I2JVO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1808.10732&json=true","fetch_graph":"https://pith.science/api/pith-number/IA2I2JVO33AVKKWPYMXJD26HM3/graph.json","fetch_events":"https://pith.science/api/pith-number/IA2I2JVO33AVKKWPYMXJD26HM3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IA2I2JVO33AVKKWPYMXJD26HM3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IA2I2JVO33AVKKWPYMXJD26HM3/action/storage_attestation","attest_author":"https://pith.science/pith/IA2I2JVO33AVKKWPYMXJD26HM3/action/author_attestation","sign_citation":"https://pith.science/pith/IA2I2JVO33AVKKWPYMXJD26HM3/action/citation_signature","submit_replication":"https://pith.science/pith/IA2I2JVO33AVKKWPYMXJD26HM3/action/replication_record"}},"created_at":"2026-05-17T23:59:22.339629+00:00","updated_at":"2026-05-17T23:59:22.339629+00:00"}