{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:GQJZEV22U2RUX7RZAYGX4HSTDX","short_pith_number":"pith:GQJZEV22","schema_version":"1.0","canonical_sha256":"341392575aa6a34bfe39060d7e1e531dc940cec29fefda065eafe281568e09d8","source":{"kind":"arxiv","id":"2501.00090","version":3},"attestation_state":"computed","paper":{"title":"Scattering of wave dark matter by supermassive black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.GA","astro-ph.HE","hep-ph"],"primary_cat":"gr-qc","authors_text":"Giovanni Maria Tomaselli","submitted_at":"2024-12-30T19:00:00Z","abstract_excerpt":"Recent simulations of wave dark matter around black hole binaries revealed the formation of a universal density profile that co-rotates with the binary. We derive this profile from first principles, interpreting it as the steady state of a scattering process. We find that the scattering becomes particularly efficient when the ratio of the binary separation to the dark matter's de Broglie wavelength assumes certain discrete values, which can be interpreted as bound state resonances. After estimating the amount of dark matter that undergoes this type of scattering off supermassive black hole bin"},"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":"2501.00090","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2024-12-30T19:00:00Z","cross_cats_sorted":["astro-ph.CO","astro-ph.GA","astro-ph.HE","hep-ph"],"title_canon_sha256":"552bdb7a467a7b28fc9c30a58af95d8b54047fbe2aa202170d49d7df6fe336f1","abstract_canon_sha256":"1635fbd11707f5c4d42c630be1314be6b0681f61dff15c4bef46f8a674d71ea4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:43:04.108242Z","signature_b64":"qa7ltQjpkWJCT3x0B+3EmAETK7u5/dIR16eL5CGUoKKbvd8U07aE0GSqpBFZoDi1sOCKxxW+OQxTjEQjro4ADg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"341392575aa6a34bfe39060d7e1e531dc940cec29fefda065eafe281568e09d8","last_reissued_at":"2026-07-05T10:43:04.107693Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:43:04.107693Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Scattering of wave dark matter by supermassive black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.GA","astro-ph.HE","hep-ph"],"primary_cat":"gr-qc","authors_text":"Giovanni Maria Tomaselli","submitted_at":"2024-12-30T19:00:00Z","abstract_excerpt":"Recent simulations of wave dark matter around black hole binaries revealed the formation of a universal density profile that co-rotates with the binary. We derive this profile from first principles, interpreting it as the steady state of a scattering process. We find that the scattering becomes particularly efficient when the ratio of the binary separation to the dark matter's de Broglie wavelength assumes certain discrete values, which can be interpreted as bound state resonances. After estimating the amount of dark matter that undergoes this type of scattering off supermassive black hole bin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2501.00090","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/2501.00090/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":"2501.00090","created_at":"2026-07-05T10:43:04.107757+00:00"},{"alias_kind":"arxiv_version","alias_value":"2501.00090v3","created_at":"2026-07-05T10:43:04.107757+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2501.00090","created_at":"2026-07-05T10:43:04.107757+00:00"},{"alias_kind":"pith_short_12","alias_value":"GQJZEV22U2RU","created_at":"2026-07-05T10:43:04.107757+00:00"},{"alias_kind":"pith_short_16","alias_value":"GQJZEV22U2RUX7RZ","created_at":"2026-07-05T10:43:04.107757+00:00"},{"alias_kind":"pith_short_8","alias_value":"GQJZEV22","created_at":"2026-07-05T10:43:04.107757+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2507.04471","citing_title":"A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments","ref_index":58,"is_internal_anchor":false},{"citing_arxiv_id":"2510.17967","citing_title":"Scalar fields around black hole binaries in LIGO-Virgo-KAGRA","ref_index":62,"is_internal_anchor":false},{"citing_arxiv_id":"2512.13816","citing_title":"Stellar Superradiance and Low-Energy Absorption in Dense Nuclear Media","ref_index":136,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GQJZEV22U2RUX7RZAYGX4HSTDX","json":"https://pith.science/pith/GQJZEV22U2RUX7RZAYGX4HSTDX.json","graph_json":"https://pith.science/api/pith-number/GQJZEV22U2RUX7RZAYGX4HSTDX/graph.json","events_json":"https://pith.science/api/pith-number/GQJZEV22U2RUX7RZAYGX4HSTDX/events.json","paper":"https://pith.science/paper/GQJZEV22"},"agent_actions":{"view_html":"https://pith.science/pith/GQJZEV22U2RUX7RZAYGX4HSTDX","download_json":"https://pith.science/pith/GQJZEV22U2RUX7RZAYGX4HSTDX.json","view_paper":"https://pith.science/paper/GQJZEV22","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2501.00090&json=true","fetch_graph":"https://pith.science/api/pith-number/GQJZEV22U2RUX7RZAYGX4HSTDX/graph.json","fetch_events":"https://pith.science/api/pith-number/GQJZEV22U2RUX7RZAYGX4HSTDX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GQJZEV22U2RUX7RZAYGX4HSTDX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GQJZEV22U2RUX7RZAYGX4HSTDX/action/storage_attestation","attest_author":"https://pith.science/pith/GQJZEV22U2RUX7RZAYGX4HSTDX/action/author_attestation","sign_citation":"https://pith.science/pith/GQJZEV22U2RUX7RZAYGX4HSTDX/action/citation_signature","submit_replication":"https://pith.science/pith/GQJZEV22U2RUX7RZAYGX4HSTDX/action/replication_record"}},"created_at":"2026-07-05T10:43:04.107757+00:00","updated_at":"2026-07-05T10:43:04.107757+00:00"}