{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:POJYW6XUUY7WSGQMO2P7YR4JY5","short_pith_number":"pith:POJYW6XU","schema_version":"1.0","canonical_sha256":"7b938b7af4a63f691a0c769ffc4789c7769dad93daa04e4da7e0050c8c71a475","source":{"kind":"arxiv","id":"2501.15397","version":1},"attestation_state":"computed","paper":{"title":"Astrophysical properties of static black holes embedded in a Dehnen type dark matter halo with the presence of quintessential field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Ahmad Al-Badawi, Sanjar Shaymatov","submitted_at":"2025-01-26T04:37:23Z","abstract_excerpt":"From an astrophysical perspective, the composition of black holes (BHs), dark matter (DM), and dark energy can be an intriguing physical system. In this study, we consider Schwarzschild BHs embedded in a Dehnen-type DM halo exhibiting a quintessential field. This study examines the horizons, shadows, deflection angle, and quasinormal modes (QNMs) of the effective BH spacetime and how they are affected by the dark sector. The Schwarzschild BH embodied in a Dehnen-type DM halo exhibiting a quintessential field possesses two horizons: the event horizon and the cosmological horizon. We demonstrate"},"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":"2501.15397","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2025-01-26T04:37:23Z","cross_cats_sorted":[],"title_canon_sha256":"324764d1f811c9d8b39ce057978b57adbf6fef15b8e444c099e4b92f7c29d13f","abstract_canon_sha256":"b0e5973b9f28d6729a17dc3c4a94c9fa1866363b539c457acb12046c9041d1f2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:05:28.691237Z","signature_b64":"VtHskShG5IoBHEzZMPphaJMfMD02lAv6C9zDSEnPgaAZurx6DVJbsdlxMMFUeRY1HqYpYMRmUUltjPK4EO4GBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7b938b7af4a63f691a0c769ffc4789c7769dad93daa04e4da7e0050c8c71a475","last_reissued_at":"2026-07-05T10:05:28.690749Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:05:28.690749Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Astrophysical properties of static black holes embedded in a Dehnen type dark matter halo with the presence of quintessential field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Ahmad Al-Badawi, Sanjar Shaymatov","submitted_at":"2025-01-26T04:37:23Z","abstract_excerpt":"From an astrophysical perspective, the composition of black holes (BHs), dark matter (DM), and dark energy can be an intriguing physical system. In this study, we consider Schwarzschild BHs embedded in a Dehnen-type DM halo exhibiting a quintessential field. This study examines the horizons, shadows, deflection angle, and quasinormal modes (QNMs) of the effective BH spacetime and how they are affected by the dark sector. The Schwarzschild BH embodied in a Dehnen-type DM halo exhibiting a quintessential field possesses two horizons: the event horizon and the cosmological horizon. We demonstrate"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2501.15397","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2501.15397/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":"2501.15397","created_at":"2026-07-05T10:05:28.690809+00:00"},{"alias_kind":"arxiv_version","alias_value":"2501.15397v1","created_at":"2026-07-05T10:05:28.690809+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2501.15397","created_at":"2026-07-05T10:05:28.690809+00:00"},{"alias_kind":"pith_short_12","alias_value":"POJYW6XUUY7W","created_at":"2026-07-05T10:05:28.690809+00:00"},{"alias_kind":"pith_short_16","alias_value":"POJYW6XUUY7WSGQM","created_at":"2026-07-05T10:05:28.690809+00:00"},{"alias_kind":"pith_short_8","alias_value":"POJYW6XU","created_at":"2026-07-05T10:05:28.690809+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2607.00812","citing_title":"Gravitational Wave Signatures of Schwarzschild Black Hole in a Generalized Dehnen-Type $(1,4,\\gamma)$ Dark Matter Halo","ref_index":39,"is_internal_anchor":false},{"citing_arxiv_id":"2605.22210","citing_title":"Constraints on Schwarzschild Black Hole in a Generalized Dehnen-Type $(1,4,\\gamma)$ Dark Matter Halo via the S2 Star Orbit around Sgr A$^\\star$","ref_index":50,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/POJYW6XUUY7WSGQMO2P7YR4JY5","json":"https://pith.science/pith/POJYW6XUUY7WSGQMO2P7YR4JY5.json","graph_json":"https://pith.science/api/pith-number/POJYW6XUUY7WSGQMO2P7YR4JY5/graph.json","events_json":"https://pith.science/api/pith-number/POJYW6XUUY7WSGQMO2P7YR4JY5/events.json","paper":"https://pith.science/paper/POJYW6XU"},"agent_actions":{"view_html":"https://pith.science/pith/POJYW6XUUY7WSGQMO2P7YR4JY5","download_json":"https://pith.science/pith/POJYW6XUUY7WSGQMO2P7YR4JY5.json","view_paper":"https://pith.science/paper/POJYW6XU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2501.15397&json=true","fetch_graph":"https://pith.science/api/pith-number/POJYW6XUUY7WSGQMO2P7YR4JY5/graph.json","fetch_events":"https://pith.science/api/pith-number/POJYW6XUUY7WSGQMO2P7YR4JY5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/POJYW6XUUY7WSGQMO2P7YR4JY5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/POJYW6XUUY7WSGQMO2P7YR4JY5/action/storage_attestation","attest_author":"https://pith.science/pith/POJYW6XUUY7WSGQMO2P7YR4JY5/action/author_attestation","sign_citation":"https://pith.science/pith/POJYW6XUUY7WSGQMO2P7YR4JY5/action/citation_signature","submit_replication":"https://pith.science/pith/POJYW6XUUY7WSGQMO2P7YR4JY5/action/replication_record"}},"created_at":"2026-07-05T10:05:28.690809+00:00","updated_at":"2026-07-05T10:05:28.690809+00:00"}