{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:XC2FIF3BDCYSICOBA2MUSWBCYM","short_pith_number":"pith:XC2FIF3B","schema_version":"1.0","canonical_sha256":"b8b454176118b12409c10699495822c339d8f68023b8f5064fabfbd0ce240580","source":{"kind":"arxiv","id":"1907.10038","version":2},"attestation_state":"computed","paper":{"title":"Non-Linear Obstructions for Consistent New General Relativity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th","math-ph","math.MP"],"primary_cat":"gr-qc","authors_text":"Jose Beltr\\'an Jim\\'enez, Konstantinos F. Dialektopoulos","submitted_at":"2019-07-23T17:48:17Z","abstract_excerpt":"We revisit the field content and consistency of the New General Relativity family of theories. These theories are constructed in a geometrical framework with a flat and metric-compatible connection, so the affine structure is entirely determined by the torsion. The action is given by a local and parity-preserving quadratic form of the torsion with three free parameters. It is well-known that a special choice of parameters gives an equivalent to General Relativity and that the spectrum of the general linear theory around Minkowski contains an additional 2-form field. It has been suggested that "},"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":"1907.10038","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2019-07-23T17:48:17Z","cross_cats_sorted":["hep-th","math-ph","math.MP"],"title_canon_sha256":"bd87763b556b9fd85e128db7d9fb937452f29d5390bfcb7a5b1971b5050d4590","abstract_canon_sha256":"63e098e148e02f1d0afebbea144c540b1aabd9b6387e214a8aa57f2b2e93081d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:33:14.441688Z","signature_b64":"2fxSbjhO9+qDBKZ1yeggIa8ssBsCwvOKI3akLqekZLASYU883rhByHQer9irYDTI3f0jeQXq+x41f887iozGCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b8b454176118b12409c10699495822c339d8f68023b8f5064fabfbd0ce240580","last_reissued_at":"2026-07-05T00:33:14.441144Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:33:14.441144Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Non-Linear Obstructions for Consistent New General Relativity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th","math-ph","math.MP"],"primary_cat":"gr-qc","authors_text":"Jose Beltr\\'an Jim\\'enez, Konstantinos F. Dialektopoulos","submitted_at":"2019-07-23T17:48:17Z","abstract_excerpt":"We revisit the field content and consistency of the New General Relativity family of theories. These theories are constructed in a geometrical framework with a flat and metric-compatible connection, so the affine structure is entirely determined by the torsion. The action is given by a local and parity-preserving quadratic form of the torsion with three free parameters. It is well-known that a special choice of parameters gives an equivalent to General Relativity and that the spectrum of the general linear theory around Minkowski contains an additional 2-form field. It has been suggested that "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1907.10038","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/1907.10038/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":"1907.10038","created_at":"2026-07-05T00:33:14.441212+00:00"},{"alias_kind":"arxiv_version","alias_value":"1907.10038v2","created_at":"2026-07-05T00:33:14.441212+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1907.10038","created_at":"2026-07-05T00:33:14.441212+00:00"},{"alias_kind":"pith_short_12","alias_value":"XC2FIF3BDCYS","created_at":"2026-07-05T00:33:14.441212+00:00"},{"alias_kind":"pith_short_16","alias_value":"XC2FIF3BDCYSICOB","created_at":"2026-07-05T00:33:14.441212+00:00"},{"alias_kind":"pith_short_8","alias_value":"XC2FIF3B","created_at":"2026-07-05T00:33:14.441212+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.16869","citing_title":"Gauge-invariant cosmological perturbations in Type 3 New General Relativity and background-hierarchy bounds","ref_index":78,"is_internal_anchor":false},{"citing_arxiv_id":"2605.16869","citing_title":"Gauge-invariant cosmological perturbations in Type 3 New General Relativity and background-hierarchy bounds","ref_index":78,"is_internal_anchor":false},{"citing_arxiv_id":"2508.20314","citing_title":"On black holes in new general relativity","ref_index":24,"is_internal_anchor":false},{"citing_arxiv_id":"2602.12496","citing_title":"On non-vacuum black holes in new general relativity","ref_index":18,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XC2FIF3BDCYSICOBA2MUSWBCYM","json":"https://pith.science/pith/XC2FIF3BDCYSICOBA2MUSWBCYM.json","graph_json":"https://pith.science/api/pith-number/XC2FIF3BDCYSICOBA2MUSWBCYM/graph.json","events_json":"https://pith.science/api/pith-number/XC2FIF3BDCYSICOBA2MUSWBCYM/events.json","paper":"https://pith.science/paper/XC2FIF3B"},"agent_actions":{"view_html":"https://pith.science/pith/XC2FIF3BDCYSICOBA2MUSWBCYM","download_json":"https://pith.science/pith/XC2FIF3BDCYSICOBA2MUSWBCYM.json","view_paper":"https://pith.science/paper/XC2FIF3B","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1907.10038&json=true","fetch_graph":"https://pith.science/api/pith-number/XC2FIF3BDCYSICOBA2MUSWBCYM/graph.json","fetch_events":"https://pith.science/api/pith-number/XC2FIF3BDCYSICOBA2MUSWBCYM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XC2FIF3BDCYSICOBA2MUSWBCYM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XC2FIF3BDCYSICOBA2MUSWBCYM/action/storage_attestation","attest_author":"https://pith.science/pith/XC2FIF3BDCYSICOBA2MUSWBCYM/action/author_attestation","sign_citation":"https://pith.science/pith/XC2FIF3BDCYSICOBA2MUSWBCYM/action/citation_signature","submit_replication":"https://pith.science/pith/XC2FIF3BDCYSICOBA2MUSWBCYM/action/replication_record"}},"created_at":"2026-07-05T00:33:14.441212+00:00","updated_at":"2026-07-05T00:33:14.441212+00:00"}