{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:VLCI4IRPT73FLFTLJJIRZ6NFIC","short_pith_number":"pith:VLCI4IRP","schema_version":"1.0","canonical_sha256":"aac48e222f9ff655966b4a511cf9a54093c8fb6ca4b41004dfc35296db38b558","source":{"kind":"arxiv","id":"2412.07814","version":1},"attestation_state":"computed","paper":{"title":"Accretion onto a Charged Black Hole in Consistent 4D Einstein-Gauss-Bonnet Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"gr-qc","authors_text":"Kourosh Nozari, Mohammad Hassani, Sara Saghafi","submitted_at":"2024-12-10T08:55:30Z","abstract_excerpt":"In astrophysics, accretion is the process by which a massive object acquires matter. The infall leads to the extraction of gravitational energy. Accretion onto dark compact objects such as black holes, neutron stars, and white dwarfs is a crucial process in astrophysics as it turns gravitational energy into radiation. The accretion process is an effective technique to investigate the properties of other theories of gravity by examining the behavior of their solutions with compact objects. In this paper, we investigate the behavior of test particles around a charged four dimensional Einstein Ga"},"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":"2412.07814","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2024-12-10T08:55:30Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"720acc27646ae5ff10906256164336b7d331fb33b32f9062b82b6c92b2289a33","abstract_canon_sha256":"21d809a920deabba6f4b7fda714dbbe0fcc1a4f1e4d7d61306d4aba226a86ab3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:50:55.293886Z","signature_b64":"qv/TiH7qWpCxiId/n2ZdvaiihMq0WEXNgzBkidCS39B67yPl3kGFGpZxZntaNQERERAk5lwBn/7yGsvK7NqQBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"aac48e222f9ff655966b4a511cf9a54093c8fb6ca4b41004dfc35296db38b558","last_reissued_at":"2026-07-05T09:50:55.293399Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:50:55.293399Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Accretion onto a Charged Black Hole in Consistent 4D Einstein-Gauss-Bonnet Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"gr-qc","authors_text":"Kourosh Nozari, Mohammad Hassani, Sara Saghafi","submitted_at":"2024-12-10T08:55:30Z","abstract_excerpt":"In astrophysics, accretion is the process by which a massive object acquires matter. The infall leads to the extraction of gravitational energy. Accretion onto dark compact objects such as black holes, neutron stars, and white dwarfs is a crucial process in astrophysics as it turns gravitational energy into radiation. The accretion process is an effective technique to investigate the properties of other theories of gravity by examining the behavior of their solutions with compact objects. In this paper, we investigate the behavior of test particles around a charged four dimensional Einstein Ga"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2412.07814","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/2412.07814/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":"2412.07814","created_at":"2026-07-05T09:50:55.293461+00:00"},{"alias_kind":"arxiv_version","alias_value":"2412.07814v1","created_at":"2026-07-05T09:50:55.293461+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2412.07814","created_at":"2026-07-05T09:50:55.293461+00:00"},{"alias_kind":"pith_short_12","alias_value":"VLCI4IRPT73F","created_at":"2026-07-05T09:50:55.293461+00:00"},{"alias_kind":"pith_short_16","alias_value":"VLCI4IRPT73FLFTL","created_at":"2026-07-05T09:50:55.293461+00:00"},{"alias_kind":"pith_short_8","alias_value":"VLCI4IRP","created_at":"2026-07-05T09:50:55.293461+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.08431","citing_title":"Null geodesics, causal structure, and matter accretion in Lorentzian-Euclidean black holes","ref_index":123,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VLCI4IRPT73FLFTLJJIRZ6NFIC","json":"https://pith.science/pith/VLCI4IRPT73FLFTLJJIRZ6NFIC.json","graph_json":"https://pith.science/api/pith-number/VLCI4IRPT73FLFTLJJIRZ6NFIC/graph.json","events_json":"https://pith.science/api/pith-number/VLCI4IRPT73FLFTLJJIRZ6NFIC/events.json","paper":"https://pith.science/paper/VLCI4IRP"},"agent_actions":{"view_html":"https://pith.science/pith/VLCI4IRPT73FLFTLJJIRZ6NFIC","download_json":"https://pith.science/pith/VLCI4IRPT73FLFTLJJIRZ6NFIC.json","view_paper":"https://pith.science/paper/VLCI4IRP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2412.07814&json=true","fetch_graph":"https://pith.science/api/pith-number/VLCI4IRPT73FLFTLJJIRZ6NFIC/graph.json","fetch_events":"https://pith.science/api/pith-number/VLCI4IRPT73FLFTLJJIRZ6NFIC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VLCI4IRPT73FLFTLJJIRZ6NFIC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VLCI4IRPT73FLFTLJJIRZ6NFIC/action/storage_attestation","attest_author":"https://pith.science/pith/VLCI4IRPT73FLFTLJJIRZ6NFIC/action/author_attestation","sign_citation":"https://pith.science/pith/VLCI4IRPT73FLFTLJJIRZ6NFIC/action/citation_signature","submit_replication":"https://pith.science/pith/VLCI4IRPT73FLFTLJJIRZ6NFIC/action/replication_record"}},"created_at":"2026-07-05T09:50:55.293461+00:00","updated_at":"2026-07-05T09:50:55.293461+00:00"}