{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:PHGUOS7WCIUM3DZ5KQN3OI3WBE","short_pith_number":"pith:PHGUOS7W","schema_version":"1.0","canonical_sha256":"79cd474bf61228cd8f3d541bb72376092d09ef1e6f05d3af1bf8bc7fb8668b0b","source":{"kind":"arxiv","id":"2508.06602","version":1},"attestation_state":"computed","paper":{"title":"On Carrollian and Celestial Correlators in General Dimensions","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Akshay Yelleshpur Srikant, Harshal Kulkarni, Romain Ruzziconi","submitted_at":"2025-08-08T18:00:00Z","abstract_excerpt":"Carrollian holography is a framework for flat space holography, suggesting that gravity in asymptotically flat spacetime in $D$ dimensions is dual to a conformal Carrollian field theory in $D - 1$ dimensions living at null infinity. In this work, we elaborate on the definition of Carrollian amplitudes for massless scalar fields in general dimensions and provide explicit expressions for the two-, three-, and four-point functions. We show that these amplitudes naturally arise from Lorentzian holographic correlators in AdS/CFT through a correspondence between the flat space limit in the bulk and "},"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":"2508.06602","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2025-08-08T18:00:00Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"305412941e4e2aed85c4663a2238bf2a93a0d0c3afa3a424596e6fb60b3ae17b","abstract_canon_sha256":"507c7b30badb23533124206853e64a3404baf4590d7a110a706c9617a973612e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:51:03.356219Z","signature_b64":"kMyJWV8SdOLMvOMk2vCl00l5p5Vu0jhVPUPg91NodETpkqniUNJRZM/r5JNSDypBeSwAduMuuwDkd5OT6p0EBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"79cd474bf61228cd8f3d541bb72376092d09ef1e6f05d3af1bf8bc7fb8668b0b","last_reissued_at":"2026-07-05T11:51:03.355779Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:51:03.355779Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On Carrollian and Celestial Correlators in General Dimensions","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Akshay Yelleshpur Srikant, Harshal Kulkarni, Romain Ruzziconi","submitted_at":"2025-08-08T18:00:00Z","abstract_excerpt":"Carrollian holography is a framework for flat space holography, suggesting that gravity in asymptotically flat spacetime in $D$ dimensions is dual to a conformal Carrollian field theory in $D - 1$ dimensions living at null infinity. In this work, we elaborate on the definition of Carrollian amplitudes for massless scalar fields in general dimensions and provide explicit expressions for the two-, three-, and four-point functions. We show that these amplitudes naturally arise from Lorentzian holographic correlators in AdS/CFT through a correspondence between the flat space limit in the bulk and "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2508.06602","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/2508.06602/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":"2508.06602","created_at":"2026-07-05T11:51:03.355839+00:00"},{"alias_kind":"arxiv_version","alias_value":"2508.06602v1","created_at":"2026-07-05T11:51:03.355839+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2508.06602","created_at":"2026-07-05T11:51:03.355839+00:00"},{"alias_kind":"pith_short_12","alias_value":"PHGUOS7WCIUM","created_at":"2026-07-05T11:51:03.355839+00:00"},{"alias_kind":"pith_short_16","alias_value":"PHGUOS7WCIUM3DZ5","created_at":"2026-07-05T11:51:03.355839+00:00"},{"alias_kind":"pith_short_8","alias_value":"PHGUOS7W","created_at":"2026-07-05T11:51:03.355839+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":11,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.24285","citing_title":"Topics in Celestial holography: A bottom-up perspective","ref_index":49,"is_internal_anchor":false},{"citing_arxiv_id":"2606.26163","citing_title":"Large-$N$ Carrollian Thermodynamics from AdS Black-Hole Phase-Space Contractions","ref_index":106,"is_internal_anchor":false},{"citing_arxiv_id":"2606.19112","citing_title":"Post-Carroll Algebra, Conformal Extensions, and Field Theories","ref_index":26,"is_internal_anchor":false},{"citing_arxiv_id":"2606.24285","citing_title":"Topics in Celestial holography: A bottom-up perspective","ref_index":50,"is_internal_anchor":false},{"citing_arxiv_id":"2606.19112","citing_title":"Post-Carroll Algebra, Conformal Extensions, and Field Theories","ref_index":26,"is_internal_anchor":false},{"citing_arxiv_id":"2606.06326","citing_title":"Spinning bulk-to-boundary correlators in the massless theories with Poincar\\'e symmetry","ref_index":57,"is_internal_anchor":false},{"citing_arxiv_id":"2606.03955","citing_title":"Flat from AdS: in any dimension and for any spin","ref_index":24,"is_internal_anchor":false},{"citing_arxiv_id":"2606.27421","citing_title":"Observing Massive Scattering from Null Infinity","ref_index":26,"is_internal_anchor":false},{"citing_arxiv_id":"2606.26163","citing_title":"Large-$N$ Carrollian Thermodynamics from AdS Black-Hole Phase-Space Contractions","ref_index":107,"is_internal_anchor":false},{"citing_arxiv_id":"2604.08498","citing_title":"On Carrollian Loop Amplitudes for Gauge Theory and Gravity","ref_index":42,"is_internal_anchor":false},{"citing_arxiv_id":"2604.08498","citing_title":"On Carrollian Loop Amplitudes for Gauge Theory and Gravity","ref_index":42,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PHGUOS7WCIUM3DZ5KQN3OI3WBE","json":"https://pith.science/pith/PHGUOS7WCIUM3DZ5KQN3OI3WBE.json","graph_json":"https://pith.science/api/pith-number/PHGUOS7WCIUM3DZ5KQN3OI3WBE/graph.json","events_json":"https://pith.science/api/pith-number/PHGUOS7WCIUM3DZ5KQN3OI3WBE/events.json","paper":"https://pith.science/paper/PHGUOS7W"},"agent_actions":{"view_html":"https://pith.science/pith/PHGUOS7WCIUM3DZ5KQN3OI3WBE","download_json":"https://pith.science/pith/PHGUOS7WCIUM3DZ5KQN3OI3WBE.json","view_paper":"https://pith.science/paper/PHGUOS7W","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2508.06602&json=true","fetch_graph":"https://pith.science/api/pith-number/PHGUOS7WCIUM3DZ5KQN3OI3WBE/graph.json","fetch_events":"https://pith.science/api/pith-number/PHGUOS7WCIUM3DZ5KQN3OI3WBE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PHGUOS7WCIUM3DZ5KQN3OI3WBE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PHGUOS7WCIUM3DZ5KQN3OI3WBE/action/storage_attestation","attest_author":"https://pith.science/pith/PHGUOS7WCIUM3DZ5KQN3OI3WBE/action/author_attestation","sign_citation":"https://pith.science/pith/PHGUOS7WCIUM3DZ5KQN3OI3WBE/action/citation_signature","submit_replication":"https://pith.science/pith/PHGUOS7WCIUM3DZ5KQN3OI3WBE/action/replication_record"}},"created_at":"2026-07-05T11:51:03.355839+00:00","updated_at":"2026-07-05T11:51:03.355839+00:00"}