{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:IDELSQM23FCZHHPRVAVVP2W4X4","short_pith_number":"pith:IDELSQM2","schema_version":"1.0","canonical_sha256":"40c8b9419ad945939df1a82b57eadcbf1e1acf3e346154e5ec36c5cbb31bd6d8","source":{"kind":"arxiv","id":"0810.2388","version":5},"attestation_state":"computed","paper":{"title":"Symmetric Teleparallel Gravity: Some exact solutions and spinor couplings","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Mestan Kalay, Murat Sar{\\i}, Muzaffer Adak, \\\"Ozcan Sert","submitted_at":"2008-10-14T08:39:13Z","abstract_excerpt":"In this paper we elaborate on the symmetric teleparallel gravity (STPG) written in a non-Riemannian spacetime with nonzero nonmetricity, but zero torsion and zero curvature. Firstly we give a prescription for obtaining the nonmetricity from the metric in a peculiar gauge. Then we state that under a novel prescription of parallel transportation of a tangent vector in this non-Riemannian geometry the autoparallel curves coincides with those of the Riemannian spacetimes. Subsequently we represent the symmetric teleparallel theory of gravity by the most general quadratic and parity conserving lagr"},"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":"0810.2388","kind":"arxiv","version":5},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2008-10-14T08:39:13Z","cross_cats_sorted":[],"title_canon_sha256":"c392a99a0514e9b28913cb9680ba9d8e9c248abc88ee6937eafcce99cb2bdd74","abstract_canon_sha256":"6985f6e7fa4bb5a244dcce0ffc6d83adb0633b8e950073cce9e0bc4ece265fae"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:09:24.396917Z","signature_b64":"GkgssnkznY1lZJpL3yHP1MBGcVf0ndfwBMYTsdE01lUk1Njpd1g92DAC7btm2c3K8/rVVYGDmADdni/DgdWJAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"40c8b9419ad945939df1a82b57eadcbf1e1acf3e346154e5ec36c5cbb31bd6d8","last_reissued_at":"2026-05-18T01:09:24.396476Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:09:24.396476Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Symmetric Teleparallel Gravity: Some exact solutions and spinor couplings","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Mestan Kalay, Murat Sar{\\i}, Muzaffer Adak, \\\"Ozcan Sert","submitted_at":"2008-10-14T08:39:13Z","abstract_excerpt":"In this paper we elaborate on the symmetric teleparallel gravity (STPG) written in a non-Riemannian spacetime with nonzero nonmetricity, but zero torsion and zero curvature. Firstly we give a prescription for obtaining the nonmetricity from the metric in a peculiar gauge. Then we state that under a novel prescription of parallel transportation of a tangent vector in this non-Riemannian geometry the autoparallel curves coincides with those of the Riemannian spacetimes. Subsequently we represent the symmetric teleparallel theory of gravity by the most general quadratic and parity conserving lagr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0810.2388","kind":"arxiv","version":5},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"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":"0810.2388","created_at":"2026-05-18T01:09:24.396540+00:00"},{"alias_kind":"arxiv_version","alias_value":"0810.2388v5","created_at":"2026-05-18T01:09:24.396540+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0810.2388","created_at":"2026-05-18T01:09:24.396540+00:00"},{"alias_kind":"pith_short_12","alias_value":"IDELSQM23FCZ","created_at":"2026-05-18T12:25:57.157939+00:00"},{"alias_kind":"pith_short_16","alias_value":"IDELSQM23FCZHHPR","created_at":"2026-05-18T12:25:57.157939+00:00"},{"alias_kind":"pith_short_8","alias_value":"IDELSQM2","created_at":"2026-05-18T12:25:57.157939+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2512.19207","citing_title":"Static plane symmetric solutions in $f(Q)$ gravity","ref_index":7,"is_internal_anchor":true},{"citing_arxiv_id":"2604.19310","citing_title":"Extrinsic geometry and Hamiltonian analysis of symmetric teleparallel gravity","ref_index":16,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IDELSQM23FCZHHPRVAVVP2W4X4","json":"https://pith.science/pith/IDELSQM23FCZHHPRVAVVP2W4X4.json","graph_json":"https://pith.science/api/pith-number/IDELSQM23FCZHHPRVAVVP2W4X4/graph.json","events_json":"https://pith.science/api/pith-number/IDELSQM23FCZHHPRVAVVP2W4X4/events.json","paper":"https://pith.science/paper/IDELSQM2"},"agent_actions":{"view_html":"https://pith.science/pith/IDELSQM23FCZHHPRVAVVP2W4X4","download_json":"https://pith.science/pith/IDELSQM23FCZHHPRVAVVP2W4X4.json","view_paper":"https://pith.science/paper/IDELSQM2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0810.2388&json=true","fetch_graph":"https://pith.science/api/pith-number/IDELSQM23FCZHHPRVAVVP2W4X4/graph.json","fetch_events":"https://pith.science/api/pith-number/IDELSQM23FCZHHPRVAVVP2W4X4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IDELSQM23FCZHHPRVAVVP2W4X4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IDELSQM23FCZHHPRVAVVP2W4X4/action/storage_attestation","attest_author":"https://pith.science/pith/IDELSQM23FCZHHPRVAVVP2W4X4/action/author_attestation","sign_citation":"https://pith.science/pith/IDELSQM23FCZHHPRVAVVP2W4X4/action/citation_signature","submit_replication":"https://pith.science/pith/IDELSQM23FCZHHPRVAVVP2W4X4/action/replication_record"}},"created_at":"2026-05-18T01:09:24.396540+00:00","updated_at":"2026-05-18T01:09:24.396540+00:00"}