{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:L7LQGFW5PAMN3NPTKXTF5Z3Y6U","short_pith_number":"pith:L7LQGFW5","schema_version":"1.0","canonical_sha256":"5fd70316dd7818ddb5f355e65ee778f53b0d2fa7b31d474fdbc8eebbd4475d5c","source":{"kind":"arxiv","id":"2605.24046","version":1},"attestation_state":"computed","paper":{"title":"Geodesics and Thermodynamics of a Schwarzschild Black Hole with Hernquist Dark Matter","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"A. Bouzenada, A. R. P. Moreira, F. C. E. Lima, F. M. Belchior","submitted_at":"2026-05-21T21:15:24Z","abstract_excerpt":"In this work, we investigate the physical and geometrical properties of a Schwarzschild black hole (BH) immersed in a Hernquist dark matter halo. To accomplish our purpose, one builds the BH metric by incorporating the Hernquist dark matter profile into the Schwarzschild geometry. In addition, we verify the null geodesic solutions and the Halo effect on photon dynamics. Within this framework, one examines the corresponding light trajectories to determine the deformation of photon paths generated by the dark matter distribution. Furthermore, the thermodynamic properties of the system are studie"},"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":"2605.24046","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2026-05-21T21:15:24Z","cross_cats_sorted":[],"title_canon_sha256":"fa796cf2975ca5254bdfe2282d70213de2655a9fd6a513206732089da0505875","abstract_canon_sha256":"99b78a780cf4b5634e9886c4b3fcefb31caeebf579ea09b6b6852010dd82f2f2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-26T01:02:42.708510Z","signature_b64":"Q1+Xg4lL4LBjFYsEoArO9WvewanwjKlvgvLdeurEb85gDRdlM+tD77W43i4ealIEBgzyyixbBm00dQt6tSapBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5fd70316dd7818ddb5f355e65ee778f53b0d2fa7b31d474fdbc8eebbd4475d5c","last_reissued_at":"2026-05-26T01:02:42.707630Z","signature_status":"signed_v1","first_computed_at":"2026-05-26T01:02:42.707630Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Geodesics and Thermodynamics of a Schwarzschild Black Hole with Hernquist Dark Matter","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"A. Bouzenada, A. R. P. Moreira, F. C. E. Lima, F. M. Belchior","submitted_at":"2026-05-21T21:15:24Z","abstract_excerpt":"In this work, we investigate the physical and geometrical properties of a Schwarzschild black hole (BH) immersed in a Hernquist dark matter halo. To accomplish our purpose, one builds the BH metric by incorporating the Hernquist dark matter profile into the Schwarzschild geometry. In addition, we verify the null geodesic solutions and the Halo effect on photon dynamics. Within this framework, one examines the corresponding light trajectories to determine the deformation of photon paths generated by the dark matter distribution. Furthermore, the thermodynamic properties of the system are studie"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2605.24046","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/2605.24046/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":"2605.24046","created_at":"2026-05-26T01:02:42.707740+00:00"},{"alias_kind":"arxiv_version","alias_value":"2605.24046v1","created_at":"2026-05-26T01:02:42.707740+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.24046","created_at":"2026-05-26T01:02:42.707740+00:00"},{"alias_kind":"pith_short_12","alias_value":"L7LQGFW5PAMN","created_at":"2026-05-26T01:02:42.707740+00:00"},{"alias_kind":"pith_short_16","alias_value":"L7LQGFW5PAMN3NPT","created_at":"2026-05-26T01:02:42.707740+00:00"},{"alias_kind":"pith_short_8","alias_value":"L7LQGFW5","created_at":"2026-05-26T01:02:42.707740+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/L7LQGFW5PAMN3NPTKXTF5Z3Y6U","json":"https://pith.science/pith/L7LQGFW5PAMN3NPTKXTF5Z3Y6U.json","graph_json":"https://pith.science/api/pith-number/L7LQGFW5PAMN3NPTKXTF5Z3Y6U/graph.json","events_json":"https://pith.science/api/pith-number/L7LQGFW5PAMN3NPTKXTF5Z3Y6U/events.json","paper":"https://pith.science/paper/L7LQGFW5"},"agent_actions":{"view_html":"https://pith.science/pith/L7LQGFW5PAMN3NPTKXTF5Z3Y6U","download_json":"https://pith.science/pith/L7LQGFW5PAMN3NPTKXTF5Z3Y6U.json","view_paper":"https://pith.science/paper/L7LQGFW5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2605.24046&json=true","fetch_graph":"https://pith.science/api/pith-number/L7LQGFW5PAMN3NPTKXTF5Z3Y6U/graph.json","fetch_events":"https://pith.science/api/pith-number/L7LQGFW5PAMN3NPTKXTF5Z3Y6U/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/L7LQGFW5PAMN3NPTKXTF5Z3Y6U/action/timestamp_anchor","attest_storage":"https://pith.science/pith/L7LQGFW5PAMN3NPTKXTF5Z3Y6U/action/storage_attestation","attest_author":"https://pith.science/pith/L7LQGFW5PAMN3NPTKXTF5Z3Y6U/action/author_attestation","sign_citation":"https://pith.science/pith/L7LQGFW5PAMN3NPTKXTF5Z3Y6U/action/citation_signature","submit_replication":"https://pith.science/pith/L7LQGFW5PAMN3NPTKXTF5Z3Y6U/action/replication_record"}},"created_at":"2026-05-26T01:02:42.707740+00:00","updated_at":"2026-05-26T01:02:42.707740+00:00"}