{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:CQLRXAIARPQ5UG6JNW64MDVAYZ","short_pith_number":"pith:CQLRXAIA","schema_version":"1.0","canonical_sha256":"14171b81008be1da1bc96dbdc60ea0c675e839dcb1546e12cdc5d4183f72741f","source":{"kind":"arxiv","id":"2104.00116","version":2},"attestation_state":"computed","paper":{"title":"Static spherically symmetric black holes in weak f(T)-gravity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Christian Pfeifer (Universit\\\"at Bremen), Sebastian Schuster (Univerzita Karlova)","submitted_at":"2021-03-31T21:03:00Z","abstract_excerpt":"With the advent of gravitational wave astronomy and first pictures of the \"shadow\" of the central black hole of our milky way, theoretical analyses of black holes (and compact objects mimicking them sufficiently closely) have become more important than ever. The near future promises more and more detailed information about the observable black holes and black hole candidates. This information could lead to important advances on constraints on or evidence for modifications of general relativity. More precisely, we are studying the influence of weak teleparallel perturbations on general relativi"},"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":"2104.00116","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2021-03-31T21:03:00Z","cross_cats_sorted":[],"title_canon_sha256":"5d42297f94141fc86a4cdc0af0a9ec62f2172ee1d490236d91ed7140a90ff7ea","abstract_canon_sha256":"b06691774a1c1e357c4b0b2013d7b9a2fc0ec92055eeb39e8813de6b4617fdf0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:41:50.549592Z","signature_b64":"Lia1fvrC8ufohYcMa53u4jMVFGJdTI3GtZddr3e6Zm7nQqEHUJdzQvjK/5O2vQ6sk5sbKgjOC62D2s2f1egUDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"14171b81008be1da1bc96dbdc60ea0c675e839dcb1546e12cdc5d4183f72741f","last_reissued_at":"2026-07-05T02:41:50.548925Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:41:50.548925Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Static spherically symmetric black holes in weak f(T)-gravity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Christian Pfeifer (Universit\\\"at Bremen), Sebastian Schuster (Univerzita Karlova)","submitted_at":"2021-03-31T21:03:00Z","abstract_excerpt":"With the advent of gravitational wave astronomy and first pictures of the \"shadow\" of the central black hole of our milky way, theoretical analyses of black holes (and compact objects mimicking them sufficiently closely) have become more important than ever. The near future promises more and more detailed information about the observable black holes and black hole candidates. This information could lead to important advances on constraints on or evidence for modifications of general relativity. More precisely, we are studying the influence of weak teleparallel perturbations on general relativi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2104.00116","kind":"arxiv","version":2},"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/2104.00116/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":"2104.00116","created_at":"2026-07-05T02:41:50.549046+00:00"},{"alias_kind":"arxiv_version","alias_value":"2104.00116v2","created_at":"2026-07-05T02:41:50.549046+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2104.00116","created_at":"2026-07-05T02:41:50.549046+00:00"},{"alias_kind":"pith_short_12","alias_value":"CQLRXAIARPQ5","created_at":"2026-07-05T02:41:50.549046+00:00"},{"alias_kind":"pith_short_16","alias_value":"CQLRXAIARPQ5UG6J","created_at":"2026-07-05T02:41:50.549046+00:00"},{"alias_kind":"pith_short_8","alias_value":"CQLRXAIA","created_at":"2026-07-05T02:41:50.549046+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2508.20314","citing_title":"On black holes in new general relativity","ref_index":8,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CQLRXAIARPQ5UG6JNW64MDVAYZ","json":"https://pith.science/pith/CQLRXAIARPQ5UG6JNW64MDVAYZ.json","graph_json":"https://pith.science/api/pith-number/CQLRXAIARPQ5UG6JNW64MDVAYZ/graph.json","events_json":"https://pith.science/api/pith-number/CQLRXAIARPQ5UG6JNW64MDVAYZ/events.json","paper":"https://pith.science/paper/CQLRXAIA"},"agent_actions":{"view_html":"https://pith.science/pith/CQLRXAIARPQ5UG6JNW64MDVAYZ","download_json":"https://pith.science/pith/CQLRXAIARPQ5UG6JNW64MDVAYZ.json","view_paper":"https://pith.science/paper/CQLRXAIA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2104.00116&json=true","fetch_graph":"https://pith.science/api/pith-number/CQLRXAIARPQ5UG6JNW64MDVAYZ/graph.json","fetch_events":"https://pith.science/api/pith-number/CQLRXAIARPQ5UG6JNW64MDVAYZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CQLRXAIARPQ5UG6JNW64MDVAYZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CQLRXAIARPQ5UG6JNW64MDVAYZ/action/storage_attestation","attest_author":"https://pith.science/pith/CQLRXAIARPQ5UG6JNW64MDVAYZ/action/author_attestation","sign_citation":"https://pith.science/pith/CQLRXAIARPQ5UG6JNW64MDVAYZ/action/citation_signature","submit_replication":"https://pith.science/pith/CQLRXAIARPQ5UG6JNW64MDVAYZ/action/replication_record"}},"created_at":"2026-07-05T02:41:50.549046+00:00","updated_at":"2026-07-05T02:41:50.549046+00:00"}