{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:GV74UGZQ7NBJQTIOKYM2FQG2N5","short_pith_number":"pith:GV74UGZQ","schema_version":"1.0","canonical_sha256":"357fca1b30fb42984d0e5619a2c0da6f68d8bcd121f4a1b18af9ebe4712e5c98","source":{"kind":"arxiv","id":"2010.10074","version":1},"attestation_state":"computed","paper":{"title":"Thick brane structures in generalized hybrid metric-Palatini gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Dionisio Bazeia, Douglas A. Ferreira, Francisco S. N. Lobo, Jo\\~ao Lu\\'is Rosa","submitted_at":"2020-10-20T07:03:39Z","abstract_excerpt":"In this work, we study 5-dimensional braneworld scenarios in the scalar-tensor representation of the generalized hybrid metric-Palatini gravitational theory. We start by considering a model for a brane supported purely by the gravitational scalar fields of the theory and then consider other distinct cases where the models are also supported by an additional matter scalar field. We investigate the stability of the gravity sector and show that the models are all robust against small fluctuations of the metric. In particular, in the presence of the additional scalar field, we find that the profil"},"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":"2010.10074","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2020-10-20T07:03:39Z","cross_cats_sorted":[],"title_canon_sha256":"ed491a2a11ba609217e8cc67fe8eced8bc62144b1a3cb7a647eb5b80e582d24c","abstract_canon_sha256":"83b273b770510c842751fa27fcd5e970cb2e83bb4f52c79c56c58594fc72e5f3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:07:31.755866Z","signature_b64":"ZdbPMsIKjffXwx+vRGAb+8ncLnZVPIW31TRqzAry4oWNA08AUahDjDG/nhQ4z87SXb4QTHbbdyxICPWSJXChAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"357fca1b30fb42984d0e5619a2c0da6f68d8bcd121f4a1b18af9ebe4712e5c98","last_reissued_at":"2026-07-05T02:07:31.755369Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:07:31.755369Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Thick brane structures in generalized hybrid metric-Palatini gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Dionisio Bazeia, Douglas A. Ferreira, Francisco S. N. Lobo, Jo\\~ao Lu\\'is Rosa","submitted_at":"2020-10-20T07:03:39Z","abstract_excerpt":"In this work, we study 5-dimensional braneworld scenarios in the scalar-tensor representation of the generalized hybrid metric-Palatini gravitational theory. We start by considering a model for a brane supported purely by the gravitational scalar fields of the theory and then consider other distinct cases where the models are also supported by an additional matter scalar field. We investigate the stability of the gravity sector and show that the models are all robust against small fluctuations of the metric. In particular, in the presence of the additional scalar field, we find that the profil"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2010.10074","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/2010.10074/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":"2010.10074","created_at":"2026-07-05T02:07:31.755428+00:00"},{"alias_kind":"arxiv_version","alias_value":"2010.10074v1","created_at":"2026-07-05T02:07:31.755428+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2010.10074","created_at":"2026-07-05T02:07:31.755428+00:00"},{"alias_kind":"pith_short_12","alias_value":"GV74UGZQ7NBJ","created_at":"2026-07-05T02:07:31.755428+00:00"},{"alias_kind":"pith_short_16","alias_value":"GV74UGZQ7NBJQTIO","created_at":"2026-07-05T02:07:31.755428+00:00"},{"alias_kind":"pith_short_8","alias_value":"GV74UGZQ","created_at":"2026-07-05T02:07:31.755428+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2412.10324","citing_title":"Novel electrically charged wormhole, black hole and black bounce exact solutions in hybrid metric-Palatini gravity","ref_index":85,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GV74UGZQ7NBJQTIOKYM2FQG2N5","json":"https://pith.science/pith/GV74UGZQ7NBJQTIOKYM2FQG2N5.json","graph_json":"https://pith.science/api/pith-number/GV74UGZQ7NBJQTIOKYM2FQG2N5/graph.json","events_json":"https://pith.science/api/pith-number/GV74UGZQ7NBJQTIOKYM2FQG2N5/events.json","paper":"https://pith.science/paper/GV74UGZQ"},"agent_actions":{"view_html":"https://pith.science/pith/GV74UGZQ7NBJQTIOKYM2FQG2N5","download_json":"https://pith.science/pith/GV74UGZQ7NBJQTIOKYM2FQG2N5.json","view_paper":"https://pith.science/paper/GV74UGZQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2010.10074&json=true","fetch_graph":"https://pith.science/api/pith-number/GV74UGZQ7NBJQTIOKYM2FQG2N5/graph.json","fetch_events":"https://pith.science/api/pith-number/GV74UGZQ7NBJQTIOKYM2FQG2N5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GV74UGZQ7NBJQTIOKYM2FQG2N5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GV74UGZQ7NBJQTIOKYM2FQG2N5/action/storage_attestation","attest_author":"https://pith.science/pith/GV74UGZQ7NBJQTIOKYM2FQG2N5/action/author_attestation","sign_citation":"https://pith.science/pith/GV74UGZQ7NBJQTIOKYM2FQG2N5/action/citation_signature","submit_replication":"https://pith.science/pith/GV74UGZQ7NBJQTIOKYM2FQG2N5/action/replication_record"}},"created_at":"2026-07-05T02:07:31.755428+00:00","updated_at":"2026-07-05T02:07:31.755428+00:00"}