{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:BCE3TYIOFP3WUSS5JEN3VKYI4Z","short_pith_number":"pith:BCE3TYIO","schema_version":"1.0","canonical_sha256":"0889b9e10e2bf76a4a5d491bbaab08e65da9854a504e0f01caee739a64a57f22","source":{"kind":"arxiv","id":"1604.08054","version":2},"attestation_state":"computed","paper":{"title":"Non-Relativistic Chern-Simons Theories and Three-Dimensional Horava-Lifshitz Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Jelle Hartong, Niels A. Obers, Yang Lei","submitted_at":"2016-04-27T13:08:08Z","abstract_excerpt":"We show that certain three-dimensional Horava-Lifshitz gravity theories can be written as Chern-Simons gauge theories on various non-relativistic algebras. The algebras are specific extensions of the Bargmann, Newton-Hooke and Schroedinger algebra each of which has the Galilean algebra as a subalgebra. To show this we employ the fact that Horava-Lifshitz gravity corresponds to dynamical Newton-Cartan geometry. In particular, the extended Bargmann (Newton-Hooke) Chern-Simons theory corresponds to projectable Horava-Lifshitz gravity with a local U(1) gauge symmetry without (with) a cosmological "},"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":"1604.08054","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2016-04-27T13:08:08Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"563311c457d6fd9d104a92f55768914c21a090f39c211281b9789b3a696dcb1f","abstract_canon_sha256":"c632827733bdf9a209acce977977bbd4cba005349e67b5eef13433c7253b1d16"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:03:49.981700Z","signature_b64":"Q0bebspVAJZ/oz6yN1NSGdohWatKLjQlpjgSDC8eq1b3FYiSovK8PCilMIr+1jAHcmNd/JNxvVHZD+lz0B5TAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0889b9e10e2bf76a4a5d491bbaab08e65da9854a504e0f01caee739a64a57f22","last_reissued_at":"2026-05-18T01:03:49.981048Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:03:49.981048Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Non-Relativistic Chern-Simons Theories and Three-Dimensional Horava-Lifshitz Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Jelle Hartong, Niels A. Obers, Yang Lei","submitted_at":"2016-04-27T13:08:08Z","abstract_excerpt":"We show that certain three-dimensional Horava-Lifshitz gravity theories can be written as Chern-Simons gauge theories on various non-relativistic algebras. The algebras are specific extensions of the Bargmann, Newton-Hooke and Schroedinger algebra each of which has the Galilean algebra as a subalgebra. To show this we employ the fact that Horava-Lifshitz gravity corresponds to dynamical Newton-Cartan geometry. In particular, the extended Bargmann (Newton-Hooke) Chern-Simons theory corresponds to projectable Horava-Lifshitz gravity with a local U(1) gauge symmetry without (with) a cosmological "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1604.08054","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":""},"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":"1604.08054","created_at":"2026-05-18T01:03:49.981148+00:00"},{"alias_kind":"arxiv_version","alias_value":"1604.08054v2","created_at":"2026-05-18T01:03:49.981148+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1604.08054","created_at":"2026-05-18T01:03:49.981148+00:00"},{"alias_kind":"pith_short_12","alias_value":"BCE3TYIOFP3W","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_16","alias_value":"BCE3TYIOFP3WUSS5","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_8","alias_value":"BCE3TYIO","created_at":"2026-05-18T12:30:07.202191+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.24615","citing_title":"Non-Relativistic Chern-Simons Supergravity with Torsion","ref_index":38,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BCE3TYIOFP3WUSS5JEN3VKYI4Z","json":"https://pith.science/pith/BCE3TYIOFP3WUSS5JEN3VKYI4Z.json","graph_json":"https://pith.science/api/pith-number/BCE3TYIOFP3WUSS5JEN3VKYI4Z/graph.json","events_json":"https://pith.science/api/pith-number/BCE3TYIOFP3WUSS5JEN3VKYI4Z/events.json","paper":"https://pith.science/paper/BCE3TYIO"},"agent_actions":{"view_html":"https://pith.science/pith/BCE3TYIOFP3WUSS5JEN3VKYI4Z","download_json":"https://pith.science/pith/BCE3TYIOFP3WUSS5JEN3VKYI4Z.json","view_paper":"https://pith.science/paper/BCE3TYIO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1604.08054&json=true","fetch_graph":"https://pith.science/api/pith-number/BCE3TYIOFP3WUSS5JEN3VKYI4Z/graph.json","fetch_events":"https://pith.science/api/pith-number/BCE3TYIOFP3WUSS5JEN3VKYI4Z/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BCE3TYIOFP3WUSS5JEN3VKYI4Z/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BCE3TYIOFP3WUSS5JEN3VKYI4Z/action/storage_attestation","attest_author":"https://pith.science/pith/BCE3TYIOFP3WUSS5JEN3VKYI4Z/action/author_attestation","sign_citation":"https://pith.science/pith/BCE3TYIOFP3WUSS5JEN3VKYI4Z/action/citation_signature","submit_replication":"https://pith.science/pith/BCE3TYIOFP3WUSS5JEN3VKYI4Z/action/replication_record"}},"created_at":"2026-05-18T01:03:49.981148+00:00","updated_at":"2026-05-18T01:03:49.981148+00:00"}