{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:7A37IAYPJKYGOVV3TQVLIDOTLW","short_pith_number":"pith:7A37IAYP","schema_version":"1.0","canonical_sha256":"f837f4030f4ab06756bb9c2ab40dd35dbd6fe8372c6f99c692b549ea6dff471e","source":{"kind":"arxiv","id":"2111.05490","version":3},"attestation_state":"computed","paper":{"title":"Nonmetricity theories and aspects of gauge symmetry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"gr-qc","authors_text":"Israel Quiros","submitted_at":"2021-11-10T02:30:35Z","abstract_excerpt":"In this paper we discuss on the phenomenological viability of nonmetricity theories of gravity which are based in the class of generalized Weyl spacetimes -- denoted by $W_4$ -- where arbitrary nonmetricity is allowed. This class of geometry includes the so called teleparallel spaces $Z_4$, which are the geometric basement of the symmetric teleparallel theories (STTs). The guiding principle in our discussion is Weyl gauge symmetry (WGS), which is a manifest symmetry of $W_4$ spaces. Here we derive the master equation that drives the gauge invariant variations of the length of vectors during pa"},"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":"2111.05490","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2021-11-10T02:30:35Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"031ea71eeb4c548222e7f74908001177bcdb58f21fbe858a2da4a264a7c86767","abstract_canon_sha256":"8be505f6bfdeac6c015446ff6a4c66b70751712147f1e7e16ad5841a26b25d2f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:29:51.876167Z","signature_b64":"qfMVxdg8GsDFX/R7w5ntZPDQmokT13mboXKq9jirElZvaP2JxMoYjmJDRZlMDCesT5Q5mkLHEb+EYYrom8xrAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f837f4030f4ab06756bb9c2ab40dd35dbd6fe8372c6f99c692b549ea6dff471e","last_reissued_at":"2026-07-05T04:29:51.875746Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:29:51.875746Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Nonmetricity theories and aspects of gauge symmetry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"gr-qc","authors_text":"Israel Quiros","submitted_at":"2021-11-10T02:30:35Z","abstract_excerpt":"In this paper we discuss on the phenomenological viability of nonmetricity theories of gravity which are based in the class of generalized Weyl spacetimes -- denoted by $W_4$ -- where arbitrary nonmetricity is allowed. This class of geometry includes the so called teleparallel spaces $Z_4$, which are the geometric basement of the symmetric teleparallel theories (STTs). The guiding principle in our discussion is Weyl gauge symmetry (WGS), which is a manifest symmetry of $W_4$ spaces. Here we derive the master equation that drives the gauge invariant variations of the length of vectors during pa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2111.05490","kind":"arxiv","version":3},"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/2111.05490/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":"2111.05490","created_at":"2026-07-05T04:29:51.875807+00:00"},{"alias_kind":"arxiv_version","alias_value":"2111.05490v3","created_at":"2026-07-05T04:29:51.875807+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2111.05490","created_at":"2026-07-05T04:29:51.875807+00:00"},{"alias_kind":"pith_short_12","alias_value":"7A37IAYPJKYG","created_at":"2026-07-05T04:29:51.875807+00:00"},{"alias_kind":"pith_short_16","alias_value":"7A37IAYPJKYGOVV3","created_at":"2026-07-05T04:29:51.875807+00:00"},{"alias_kind":"pith_short_8","alias_value":"7A37IAYP","created_at":"2026-07-05T04:29:51.875807+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2506.10046","citing_title":"3-dimensional charged black holes in $f({Q})$ gravity","ref_index":53,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7A37IAYPJKYGOVV3TQVLIDOTLW","json":"https://pith.science/pith/7A37IAYPJKYGOVV3TQVLIDOTLW.json","graph_json":"https://pith.science/api/pith-number/7A37IAYPJKYGOVV3TQVLIDOTLW/graph.json","events_json":"https://pith.science/api/pith-number/7A37IAYPJKYGOVV3TQVLIDOTLW/events.json","paper":"https://pith.science/paper/7A37IAYP"},"agent_actions":{"view_html":"https://pith.science/pith/7A37IAYPJKYGOVV3TQVLIDOTLW","download_json":"https://pith.science/pith/7A37IAYPJKYGOVV3TQVLIDOTLW.json","view_paper":"https://pith.science/paper/7A37IAYP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2111.05490&json=true","fetch_graph":"https://pith.science/api/pith-number/7A37IAYPJKYGOVV3TQVLIDOTLW/graph.json","fetch_events":"https://pith.science/api/pith-number/7A37IAYPJKYGOVV3TQVLIDOTLW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7A37IAYPJKYGOVV3TQVLIDOTLW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7A37IAYPJKYGOVV3TQVLIDOTLW/action/storage_attestation","attest_author":"https://pith.science/pith/7A37IAYPJKYGOVV3TQVLIDOTLW/action/author_attestation","sign_citation":"https://pith.science/pith/7A37IAYPJKYGOVV3TQVLIDOTLW/action/citation_signature","submit_replication":"https://pith.science/pith/7A37IAYPJKYGOVV3TQVLIDOTLW/action/replication_record"}},"created_at":"2026-07-05T04:29:51.875807+00:00","updated_at":"2026-07-05T04:29:51.875807+00:00"}