{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:TH3YD5B2BDV3QN7K5BLF2GPQ4O","short_pith_number":"pith:TH3YD5B2","schema_version":"1.0","canonical_sha256":"99f781f43a08ebb837eae8565d19f0e3892e449334470c077e422cc83087fb66","source":{"kind":"arxiv","id":"2306.13473","version":1},"attestation_state":"computed","paper":{"title":"Cosmological Perturbations in the Teleparallel analog of Horndeski gravity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Abdurakhmon Nosirov, Bobomurat Ahmedov, Jackson Levi Said, Konstantinos F. Dialektopoulos, Odil Yunusov, Zinovia Oikonomopoulou","submitted_at":"2023-06-23T12:29:28Z","abstract_excerpt":"In this work we study the cosmological perturbations in Bahamonde-Dialektopoulos-Levi Said (BDLS) theory, i.e. the teleparallel analog of Horndeski gravity. In order to understand the evolution of structure in a cosmological model, it is necessary to study its cosmology not only in the background but also perturbatively. Both Horndeski and its teleparallel analog have been analyzed a lot in the literature, but in order to study them quantitatively, we need to know their cosmological perturbations. That is why, we study here the scalar-vector-tensor decomposition of the theory and we also expre"},"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":"2306.13473","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2023-06-23T12:29:28Z","cross_cats_sorted":[],"title_canon_sha256":"66e926f9b134c30f883e363a80ca5738c17fea67704d50f2eeebb91d46d2a2c9","abstract_canon_sha256":"418195fc0a9ff15056cd35aa86a2efa98242b709672a5476a2632d2187589440"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:24:05.827065Z","signature_b64":"jdgpLJFKWfasU48nbWpqpGwZEDzXPW+b/4Sxi/F+C+yo7cVX4aGX+SSVI41mClQTnEwsmXcay/N+rstJWMJwCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"99f781f43a08ebb837eae8565d19f0e3892e449334470c077e422cc83087fb66","last_reissued_at":"2026-07-05T06:24:05.826637Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:24:05.826637Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmological Perturbations in the Teleparallel analog of Horndeski gravity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Abdurakhmon Nosirov, Bobomurat Ahmedov, Jackson Levi Said, Konstantinos F. Dialektopoulos, Odil Yunusov, Zinovia Oikonomopoulou","submitted_at":"2023-06-23T12:29:28Z","abstract_excerpt":"In this work we study the cosmological perturbations in Bahamonde-Dialektopoulos-Levi Said (BDLS) theory, i.e. the teleparallel analog of Horndeski gravity. In order to understand the evolution of structure in a cosmological model, it is necessary to study its cosmology not only in the background but also perturbatively. Both Horndeski and its teleparallel analog have been analyzed a lot in the literature, but in order to study them quantitatively, we need to know their cosmological perturbations. That is why, we study here the scalar-vector-tensor decomposition of the theory and we also expre"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2306.13473","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/2306.13473/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":"2306.13473","created_at":"2026-07-05T06:24:05.826703+00:00"},{"alias_kind":"arxiv_version","alias_value":"2306.13473v1","created_at":"2026-07-05T06:24:05.826703+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2306.13473","created_at":"2026-07-05T06:24:05.826703+00:00"},{"alias_kind":"pith_short_12","alias_value":"TH3YD5B2BDV3","created_at":"2026-07-05T06:24:05.826703+00:00"},{"alias_kind":"pith_short_16","alias_value":"TH3YD5B2BDV3QN7K","created_at":"2026-07-05T06:24:05.826703+00:00"},{"alias_kind":"pith_short_8","alias_value":"TH3YD5B2","created_at":"2026-07-05T06:24:05.826703+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.04524","citing_title":"Cosmological scalar perturbations in Horndeski-like gravity","ref_index":13,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TH3YD5B2BDV3QN7K5BLF2GPQ4O","json":"https://pith.science/pith/TH3YD5B2BDV3QN7K5BLF2GPQ4O.json","graph_json":"https://pith.science/api/pith-number/TH3YD5B2BDV3QN7K5BLF2GPQ4O/graph.json","events_json":"https://pith.science/api/pith-number/TH3YD5B2BDV3QN7K5BLF2GPQ4O/events.json","paper":"https://pith.science/paper/TH3YD5B2"},"agent_actions":{"view_html":"https://pith.science/pith/TH3YD5B2BDV3QN7K5BLF2GPQ4O","download_json":"https://pith.science/pith/TH3YD5B2BDV3QN7K5BLF2GPQ4O.json","view_paper":"https://pith.science/paper/TH3YD5B2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2306.13473&json=true","fetch_graph":"https://pith.science/api/pith-number/TH3YD5B2BDV3QN7K5BLF2GPQ4O/graph.json","fetch_events":"https://pith.science/api/pith-number/TH3YD5B2BDV3QN7K5BLF2GPQ4O/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TH3YD5B2BDV3QN7K5BLF2GPQ4O/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TH3YD5B2BDV3QN7K5BLF2GPQ4O/action/storage_attestation","attest_author":"https://pith.science/pith/TH3YD5B2BDV3QN7K5BLF2GPQ4O/action/author_attestation","sign_citation":"https://pith.science/pith/TH3YD5B2BDV3QN7K5BLF2GPQ4O/action/citation_signature","submit_replication":"https://pith.science/pith/TH3YD5B2BDV3QN7K5BLF2GPQ4O/action/replication_record"}},"created_at":"2026-07-05T06:24:05.826703+00:00","updated_at":"2026-07-05T06:24:05.826703+00:00"}