{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:3W23BKJUMELPW5GGONKWZHWAR2","short_pith_number":"pith:3W23BKJU","schema_version":"1.0","canonical_sha256":"ddb5b0a9346116fb74c673556c9ec08eb546aa05ed6930530c6980840f0b6b92","source":{"kind":"arxiv","id":"2508.14861","version":1},"attestation_state":"computed","paper":{"title":"Fermionic greybody factors and strong gravitational lensing by Lorentz-violating global monopole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"A. R. M. Oliveira, A. Yu. Petrov, F. M. Belchior, P. J. Porf\\'irio, R. V. Maluf","submitted_at":"2025-08-20T17:16:27Z","abstract_excerpt":"In this work, we study the greybody factors (GFs) of spin 1/2 and spin 3/2 fermions for a black hole with global monopole in self-interacting Kalb-Ramond gravity with Lorentz symmetry violation. For our purpose, we consider the Dirac and Rarita-Schwinger equations in curved spacetime by proceeding with separating these equations into sets of radial and angular equations. Using the analytical solution of the angular equation, the Schr\\\"{o}dinger-like wave equations with potentials are derived by decoupling the radial wave equations using the tortoise coordinate. Moreover, we calculate the angul"},"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":"2508.14861","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2025-08-20T17:16:27Z","cross_cats_sorted":[],"title_canon_sha256":"3f9c1461f90b04b7b9f023d7092964de572ee334df19a0f78088039469d5e77a","abstract_canon_sha256":"81ca00536cf9eab974e85cf6086356b087b226c3c4017139d68be97dbcafcff1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:56:45.622583Z","signature_b64":"PGqXWBTEqT10U1gkPwg24dnI+fouiQmAUH8KZ9Ch7MXrEiIU51mp+0Ab5s/O74Oa6Euewwomu+bywT7UFyGMBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ddb5b0a9346116fb74c673556c9ec08eb546aa05ed6930530c6980840f0b6b92","last_reissued_at":"2026-07-05T11:56:45.622002Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:56:45.622002Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fermionic greybody factors and strong gravitational lensing by Lorentz-violating global monopole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"A. R. M. Oliveira, A. Yu. Petrov, F. M. Belchior, P. J. Porf\\'irio, R. V. Maluf","submitted_at":"2025-08-20T17:16:27Z","abstract_excerpt":"In this work, we study the greybody factors (GFs) of spin 1/2 and spin 3/2 fermions for a black hole with global monopole in self-interacting Kalb-Ramond gravity with Lorentz symmetry violation. For our purpose, we consider the Dirac and Rarita-Schwinger equations in curved spacetime by proceeding with separating these equations into sets of radial and angular equations. Using the analytical solution of the angular equation, the Schr\\\"{o}dinger-like wave equations with potentials are derived by decoupling the radial wave equations using the tortoise coordinate. Moreover, we calculate the angul"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2508.14861","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/2508.14861/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":"2508.14861","created_at":"2026-07-05T11:56:45.622063+00:00"},{"alias_kind":"arxiv_version","alias_value":"2508.14861v1","created_at":"2026-07-05T11:56:45.622063+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2508.14861","created_at":"2026-07-05T11:56:45.622063+00:00"},{"alias_kind":"pith_short_12","alias_value":"3W23BKJUMELP","created_at":"2026-07-05T11:56:45.622063+00:00"},{"alias_kind":"pith_short_16","alias_value":"3W23BKJUMELPW5GG","created_at":"2026-07-05T11:56:45.622063+00:00"},{"alias_kind":"pith_short_8","alias_value":"3W23BKJU","created_at":"2026-07-05T11:56:45.622063+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2508.14859","citing_title":"Graph Structure Learning with Temporal Graph Information Bottleneck for Inductive Representation Learning","ref_index":1,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3W23BKJUMELPW5GGONKWZHWAR2","json":"https://pith.science/pith/3W23BKJUMELPW5GGONKWZHWAR2.json","graph_json":"https://pith.science/api/pith-number/3W23BKJUMELPW5GGONKWZHWAR2/graph.json","events_json":"https://pith.science/api/pith-number/3W23BKJUMELPW5GGONKWZHWAR2/events.json","paper":"https://pith.science/paper/3W23BKJU"},"agent_actions":{"view_html":"https://pith.science/pith/3W23BKJUMELPW5GGONKWZHWAR2","download_json":"https://pith.science/pith/3W23BKJUMELPW5GGONKWZHWAR2.json","view_paper":"https://pith.science/paper/3W23BKJU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2508.14861&json=true","fetch_graph":"https://pith.science/api/pith-number/3W23BKJUMELPW5GGONKWZHWAR2/graph.json","fetch_events":"https://pith.science/api/pith-number/3W23BKJUMELPW5GGONKWZHWAR2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3W23BKJUMELPW5GGONKWZHWAR2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3W23BKJUMELPW5GGONKWZHWAR2/action/storage_attestation","attest_author":"https://pith.science/pith/3W23BKJUMELPW5GGONKWZHWAR2/action/author_attestation","sign_citation":"https://pith.science/pith/3W23BKJUMELPW5GGONKWZHWAR2/action/citation_signature","submit_replication":"https://pith.science/pith/3W23BKJUMELPW5GGONKWZHWAR2/action/replication_record"}},"created_at":"2026-07-05T11:56:45.622063+00:00","updated_at":"2026-07-05T11:56:45.622063+00:00"}