{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:IVZQH27Y7CQQVDDXCKBSZHSNMV","short_pith_number":"pith:IVZQH27Y","schema_version":"1.0","canonical_sha256":"457303ebf8f8a10a8c7712832c9e4d657f08752a681de9a74efe41d53d1c5e2e","source":{"kind":"arxiv","id":"2212.00257","version":1},"attestation_state":"computed","paper":{"title":"Revisiting the Shadow Stress Tensor in Celestial CFT","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Sabrina Pasterski, Shamik Banerjee","submitted_at":"2022-12-01T03:49:42Z","abstract_excerpt":"We revisit the standard construction of the celestial stress tensor as a shadow of the subleading conformally soft graviton. In its original formulation there is an obstruction to reproducing the expected TT OPE in the double soft limit. We propose a modification to the definition which circumvents this obstruction and then extend this change of basis beyond the conformally soft and single helicity sectors. In the process we investigate how (non)-commutativity of double soft limits is tied to the decoupling of primary descendants, and how our choice of celestial basis determines which symmetri"},"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":"2212.00257","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2022-12-01T03:49:42Z","cross_cats_sorted":[],"title_canon_sha256":"17dbf7c5b3dd865fa524254d1c53638774f73bf1ab4ebe1800d2c9b9786c9517","abstract_canon_sha256":"1cce0d6aec0bc8948239d1585441926fae6171c4d4226e9afee985007048f7fb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:08:14.873537Z","signature_b64":"bve1l687m2Cq8ajvvuRA7qRHyXXbYS4bboTmEOgDveXPXi0SEliIhb3GIe4BHTEJ6HvGFOHFN9sw9Q2nmFRZBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"457303ebf8f8a10a8c7712832c9e4d657f08752a681de9a74efe41d53d1c5e2e","last_reissued_at":"2026-07-05T06:08:14.873074Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:08:14.873074Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Revisiting the Shadow Stress Tensor in Celestial CFT","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Sabrina Pasterski, Shamik Banerjee","submitted_at":"2022-12-01T03:49:42Z","abstract_excerpt":"We revisit the standard construction of the celestial stress tensor as a shadow of the subleading conformally soft graviton. In its original formulation there is an obstruction to reproducing the expected TT OPE in the double soft limit. We propose a modification to the definition which circumvents this obstruction and then extend this change of basis beyond the conformally soft and single helicity sectors. In the process we investigate how (non)-commutativity of double soft limits is tied to the decoupling of primary descendants, and how our choice of celestial basis determines which symmetri"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2212.00257","kind":"arxiv","version":1},"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/2212.00257/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":"2212.00257","created_at":"2026-07-05T06:08:14.873130+00:00"},{"alias_kind":"arxiv_version","alias_value":"2212.00257v1","created_at":"2026-07-05T06:08:14.873130+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2212.00257","created_at":"2026-07-05T06:08:14.873130+00:00"},{"alias_kind":"pith_short_12","alias_value":"IVZQH27Y7CQQ","created_at":"2026-07-05T06:08:14.873130+00:00"},{"alias_kind":"pith_short_16","alias_value":"IVZQH27Y7CQQVDDX","created_at":"2026-07-05T06:08:14.873130+00:00"},{"alias_kind":"pith_short_8","alias_value":"IVZQH27Y","created_at":"2026-07-05T06:08:14.873130+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.26163","citing_title":"Large-$N$ Carrollian Thermodynamics from AdS Black-Hole Phase-Space Contractions","ref_index":104,"is_internal_anchor":false},{"citing_arxiv_id":"2606.26163","citing_title":"Large-$N$ Carrollian Thermodynamics from AdS Black-Hole Phase-Space Contractions","ref_index":105,"is_internal_anchor":false},{"citing_arxiv_id":"2605.16641","citing_title":"On bulk reconstruction in Lorentzian AdS and its flat space limit","ref_index":128,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IVZQH27Y7CQQVDDXCKBSZHSNMV","json":"https://pith.science/pith/IVZQH27Y7CQQVDDXCKBSZHSNMV.json","graph_json":"https://pith.science/api/pith-number/IVZQH27Y7CQQVDDXCKBSZHSNMV/graph.json","events_json":"https://pith.science/api/pith-number/IVZQH27Y7CQQVDDXCKBSZHSNMV/events.json","paper":"https://pith.science/paper/IVZQH27Y"},"agent_actions":{"view_html":"https://pith.science/pith/IVZQH27Y7CQQVDDXCKBSZHSNMV","download_json":"https://pith.science/pith/IVZQH27Y7CQQVDDXCKBSZHSNMV.json","view_paper":"https://pith.science/paper/IVZQH27Y","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2212.00257&json=true","fetch_graph":"https://pith.science/api/pith-number/IVZQH27Y7CQQVDDXCKBSZHSNMV/graph.json","fetch_events":"https://pith.science/api/pith-number/IVZQH27Y7CQQVDDXCKBSZHSNMV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IVZQH27Y7CQQVDDXCKBSZHSNMV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IVZQH27Y7CQQVDDXCKBSZHSNMV/action/storage_attestation","attest_author":"https://pith.science/pith/IVZQH27Y7CQQVDDXCKBSZHSNMV/action/author_attestation","sign_citation":"https://pith.science/pith/IVZQH27Y7CQQVDDXCKBSZHSNMV/action/citation_signature","submit_replication":"https://pith.science/pith/IVZQH27Y7CQQVDDXCKBSZHSNMV/action/replication_record"}},"created_at":"2026-07-05T06:08:14.873130+00:00","updated_at":"2026-07-05T06:08:14.873130+00:00"}