{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:PQ4MLFV6GSGCAHQSSXERCU62KF","short_pith_number":"pith:PQ4MLFV6","schema_version":"1.0","canonical_sha256":"7c38c596be348c201e1295c91153da51762cb749e31a9e5238abc667b2deef96","source":{"kind":"arxiv","id":"1001.1541","version":2},"attestation_state":"computed","paper":{"title":"Aspects of the BMS/CFT correspondence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Cedric Troessaert, Glenn Barnich","submitted_at":"2010-01-11T00:44:19Z","abstract_excerpt":"After a review of symmetries and classical solutions involved in the AdS3/CFT2 correspondence, we apply a similar analysis to asymptotically flat spacetimes at null infinity in 3 and 4 dimensions. In the spirit of two dimensional conformal field theory, the symmetry algebra of asymptotically flat spacetimes at null infinity in 4 dimensions is taken to be the semi-direct sum of supertranslations with infinitesimal local conformal transformations and not, as usually done, with the Lorentz algebra. As a first application, we derive how the symmetry algebra is realized on solution space. In partic"},"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":"1001.1541","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2010-01-11T00:44:19Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"58f1223be0e52b48a92bf92f2695b1eafb474d4e6f28f12d33094b3956ab93c2","abstract_canon_sha256":"ebee55274c6fb1870d669c00aaaef91b663eb77e3407a7ca20939043d90f4c32"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:34:00.445852Z","signature_b64":"DXF3pxWxOmuBw8o5IoW8Mu0ZIA7S4HTlH2G6AKibLIXg56MN3VZf53c92Lx/ZDHyMlvtAgZzqgIy8LOktT/FBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7c38c596be348c201e1295c91153da51762cb749e31a9e5238abc667b2deef96","last_reissued_at":"2026-05-18T04:34:00.445337Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:34:00.445337Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Aspects of the BMS/CFT correspondence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Cedric Troessaert, Glenn Barnich","submitted_at":"2010-01-11T00:44:19Z","abstract_excerpt":"After a review of symmetries and classical solutions involved in the AdS3/CFT2 correspondence, we apply a similar analysis to asymptotically flat spacetimes at null infinity in 3 and 4 dimensions. In the spirit of two dimensional conformal field theory, the symmetry algebra of asymptotically flat spacetimes at null infinity in 4 dimensions is taken to be the semi-direct sum of supertranslations with infinitesimal local conformal transformations and not, as usually done, with the Lorentz algebra. As a first application, we derive how the symmetry algebra is realized on solution space. In partic"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1001.1541","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":"1001.1541","created_at":"2026-05-18T04:34:00.445432+00:00"},{"alias_kind":"arxiv_version","alias_value":"1001.1541v2","created_at":"2026-05-18T04:34:00.445432+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1001.1541","created_at":"2026-05-18T04:34:00.445432+00:00"},{"alias_kind":"pith_short_12","alias_value":"PQ4MLFV6GSGC","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_16","alias_value":"PQ4MLFV6GSGCAHQS","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_8","alias_value":"PQ4MLFV6","created_at":"2026-05-18T12:26:12.377268+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":17,"internal_anchor_count":12,"sample":[{"citing_arxiv_id":"2202.04702","citing_title":"Carrollian Perspective on Celestial Holography","ref_index":56,"is_internal_anchor":true},{"citing_arxiv_id":"2503.15607","citing_title":"Operator Product Expansion in Carrollian CFT","ref_index":43,"is_internal_anchor":true},{"citing_arxiv_id":"2504.12521","citing_title":"Lectures on the Bondi--Metzner--Sachs group and related topics in infrared physics","ref_index":16,"is_internal_anchor":true},{"citing_arxiv_id":"2505.16436","citing_title":"QFT in Klein space","ref_index":15,"is_internal_anchor":true},{"citing_arxiv_id":"2510.25688","citing_title":"Conformal Blocks in 2d Carrollian/Galilean CFTs and Excited State Entanglement Entropy","ref_index":2,"is_internal_anchor":true},{"citing_arxiv_id":"2605.16641","citing_title":"On bulk reconstruction in Lorentzian AdS and its flat space limit","ref_index":34,"is_internal_anchor":true},{"citing_arxiv_id":"2506.16164","citing_title":"The Carrollian Kaleidoscope","ref_index":159,"is_internal_anchor":true},{"citing_arxiv_id":"2509.04974","citing_title":"Minkowski Space holography and Radon transform","ref_index":12,"is_internal_anchor":true},{"citing_arxiv_id":"2510.10519","citing_title":"Integrability in Three-Dimensional Gravity: Eigenfunction-Forced KdV Flows","ref_index":2,"is_internal_anchor":true},{"citing_arxiv_id":"2603.12670","citing_title":"Shaving off soft hairs and the black hole image memory effect","ref_index":15,"is_internal_anchor":true},{"citing_arxiv_id":"2603.11993","citing_title":"More on Bulk Local State Reconstruction in Flat/Carr CFT","ref_index":11,"is_internal_anchor":true},{"citing_arxiv_id":"2603.17045","citing_title":"The gravitational S-matrix from the path integral: asymptotic symmetries and soft theorems","ref_index":55,"is_internal_anchor":true},{"citing_arxiv_id":"2604.27068","citing_title":"Holographic realization of higher-spin Carrollian free fields","ref_index":59,"is_internal_anchor":false},{"citing_arxiv_id":"2604.22582","citing_title":"Carrollian ABJM: Fermions and Supersymmetry","ref_index":31,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11602","citing_title":"Celestial 1-form symmetries","ref_index":38,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13362","citing_title":"Quasi-Local Celestial Charges and Multipoles","ref_index":68,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14301","citing_title":"Carroll fermions, expansions and the lightcone","ref_index":71,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PQ4MLFV6GSGCAHQSSXERCU62KF","json":"https://pith.science/pith/PQ4MLFV6GSGCAHQSSXERCU62KF.json","graph_json":"https://pith.science/api/pith-number/PQ4MLFV6GSGCAHQSSXERCU62KF/graph.json","events_json":"https://pith.science/api/pith-number/PQ4MLFV6GSGCAHQSSXERCU62KF/events.json","paper":"https://pith.science/paper/PQ4MLFV6"},"agent_actions":{"view_html":"https://pith.science/pith/PQ4MLFV6GSGCAHQSSXERCU62KF","download_json":"https://pith.science/pith/PQ4MLFV6GSGCAHQSSXERCU62KF.json","view_paper":"https://pith.science/paper/PQ4MLFV6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1001.1541&json=true","fetch_graph":"https://pith.science/api/pith-number/PQ4MLFV6GSGCAHQSSXERCU62KF/graph.json","fetch_events":"https://pith.science/api/pith-number/PQ4MLFV6GSGCAHQSSXERCU62KF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PQ4MLFV6GSGCAHQSSXERCU62KF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PQ4MLFV6GSGCAHQSSXERCU62KF/action/storage_attestation","attest_author":"https://pith.science/pith/PQ4MLFV6GSGCAHQSSXERCU62KF/action/author_attestation","sign_citation":"https://pith.science/pith/PQ4MLFV6GSGCAHQSSXERCU62KF/action/citation_signature","submit_replication":"https://pith.science/pith/PQ4MLFV6GSGCAHQSSXERCU62KF/action/replication_record"}},"created_at":"2026-05-18T04:34:00.445432+00:00","updated_at":"2026-05-18T04:34:00.445432+00:00"}