{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:VGCQYQSCF7EX7IWFLUC4D7M732","short_pith_number":"pith:VGCQYQSC","schema_version":"1.0","canonical_sha256":"a9850c42422fc97fa2c55d05c1fd9fde8e9e893df8140f15673f7a4d0e245b64","source":{"kind":"arxiv","id":"2201.06113","version":2},"attestation_state":"computed","paper":{"title":"Gravitational waves and kicks from the merger of unequal mass, highly compact boson stars","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Carlos Palenzuela, Enrico Barausse, Mateja Bo\\v{s}kovi\\'c, Miguel Bezares, Paolo Pani, Steven Liebling","submitted_at":"2022-01-16T18:42:58Z","abstract_excerpt":"Boson stars have attracted much attention in recent decades as simple, self-consistent models of compact objects and also as self-gravitating structures formed in some dark-matter scenarios. Direct detection of these hypothetical objects through electromagnetic signatures would be unlikely because their bosonic constituents are not expected to interact significantly with ordinary matter and radiation. However, binary boson stars might form and coalesce emitting a detectable gravitational wave signal which might distinguish them from ordinary compact object binaries containing black holes and n"},"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":"2201.06113","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/publicdomain/zero/1.0/","primary_cat":"gr-qc","submitted_at":"2022-01-16T18:42:58Z","cross_cats_sorted":[],"title_canon_sha256":"d46b87fa754b8beaeb6b986bc7789bb6b9229be181379da597a4ef64a007b3ab","abstract_canon_sha256":"18ba8a52899813b30a6cc8842bb9a652887b49de6ad18e955837b59f65f2bd31"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:58:14.993770Z","signature_b64":"6wlUkREjKG7kF9OEuypnYm9Lgtogn5So0OG5RKhTs+bfMv8zJi0WpO4Wzv40pK+MVtOBjWUqv3bEuRSmsjymAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a9850c42422fc97fa2c55d05c1fd9fde8e9e893df8140f15673f7a4d0e245b64","last_reissued_at":"2026-07-05T04:58:14.993347Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:58:14.993347Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational waves and kicks from the merger of unequal mass, highly compact boson stars","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Carlos Palenzuela, Enrico Barausse, Mateja Bo\\v{s}kovi\\'c, Miguel Bezares, Paolo Pani, Steven Liebling","submitted_at":"2022-01-16T18:42:58Z","abstract_excerpt":"Boson stars have attracted much attention in recent decades as simple, self-consistent models of compact objects and also as self-gravitating structures formed in some dark-matter scenarios. Direct detection of these hypothetical objects through electromagnetic signatures would be unlikely because their bosonic constituents are not expected to interact significantly with ordinary matter and radiation. However, binary boson stars might form and coalesce emitting a detectable gravitational wave signal which might distinguish them from ordinary compact object binaries containing black holes and n"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2201.06113","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2201.06113/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":"2201.06113","created_at":"2026-07-05T04:58:14.993405+00:00"},{"alias_kind":"arxiv_version","alias_value":"2201.06113v2","created_at":"2026-07-05T04:58:14.993405+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2201.06113","created_at":"2026-07-05T04:58:14.993405+00:00"},{"alias_kind":"pith_short_12","alias_value":"VGCQYQSCF7EX","created_at":"2026-07-05T04:58:14.993405+00:00"},{"alias_kind":"pith_short_16","alias_value":"VGCQYQSCF7EX7IWF","created_at":"2026-07-05T04:58:14.993405+00:00"},{"alias_kind":"pith_short_8","alias_value":"VGCQYQSC","created_at":"2026-07-05T04:58:14.993405+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.26436","citing_title":"Massive boson stars: Waveform-based branch diagnosis with neural reconstruction","ref_index":54,"is_internal_anchor":false},{"citing_arxiv_id":"2605.19572","citing_title":"Timing-Window Mechanism for Chain-Like Transients in Collisions of Radially Excited Boson Stars","ref_index":42,"is_internal_anchor":false},{"citing_arxiv_id":"2605.19572","citing_title":"Timing-Window Mechanism for Chain-Like Transients in Collisions of Radially Excited Boson Stars","ref_index":41,"is_internal_anchor":false},{"citing_arxiv_id":"2512.15242","citing_title":"Massive boson stars: Stability and GW emission in head-on mergers","ref_index":54,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25582","citing_title":"Lessons from binary dynamics of inspiralling equal-mass boson-star mergers","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15240","citing_title":"Boson star-black hole binaries: initial data and head-on collisions","ref_index":80,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VGCQYQSCF7EX7IWFLUC4D7M732","json":"https://pith.science/pith/VGCQYQSCF7EX7IWFLUC4D7M732.json","graph_json":"https://pith.science/api/pith-number/VGCQYQSCF7EX7IWFLUC4D7M732/graph.json","events_json":"https://pith.science/api/pith-number/VGCQYQSCF7EX7IWFLUC4D7M732/events.json","paper":"https://pith.science/paper/VGCQYQSC"},"agent_actions":{"view_html":"https://pith.science/pith/VGCQYQSCF7EX7IWFLUC4D7M732","download_json":"https://pith.science/pith/VGCQYQSCF7EX7IWFLUC4D7M732.json","view_paper":"https://pith.science/paper/VGCQYQSC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2201.06113&json=true","fetch_graph":"https://pith.science/api/pith-number/VGCQYQSCF7EX7IWFLUC4D7M732/graph.json","fetch_events":"https://pith.science/api/pith-number/VGCQYQSCF7EX7IWFLUC4D7M732/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VGCQYQSCF7EX7IWFLUC4D7M732/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VGCQYQSCF7EX7IWFLUC4D7M732/action/storage_attestation","attest_author":"https://pith.science/pith/VGCQYQSCF7EX7IWFLUC4D7M732/action/author_attestation","sign_citation":"https://pith.science/pith/VGCQYQSCF7EX7IWFLUC4D7M732/action/citation_signature","submit_replication":"https://pith.science/pith/VGCQYQSCF7EX7IWFLUC4D7M732/action/replication_record"}},"created_at":"2026-07-05T04:58:14.993405+00:00","updated_at":"2026-07-05T04:58:14.993405+00:00"}