{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:LLZIV7M4OHIEUGT23SOGXTQNYG","short_pith_number":"pith:LLZIV7M4","schema_version":"1.0","canonical_sha256":"5af28afd9c71d04a1a7adc9c6bce0dc18fd3587c04e3f3312f684fdae2a7bda4","source":{"kind":"arxiv","id":"1603.02243","version":2},"attestation_state":"computed","paper":{"title":"On CMB B-Mode Non-Gaussianity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alex van Engelen (CITA), Joel Meyers, P. Daniel Meerburg, Yacine Ali-Ha\\\"imoud (JHU)","submitted_at":"2016-03-07T20:30:11Z","abstract_excerpt":"We study the degree to which the cosmic microwave background (CMB) can be used to constrain primordial non-Gaussianity involving one tensor and two scalar fluctuations, focusing on the correlation of one polarization $B$ mode with two temperature modes. In the simplest models of inflation, the tensor-scalar-scalar primordial bispectrum is non-vanishing and is of the same order in slow-roll parameters as the scalar-scalar-scalar bispectrum. We calculate the $\\langle BTT\\rangle$ correlation arising from a primordial tensor-scalar-scalar bispectrum, and show that constraints from an experiment li"},"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":"1603.02243","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-03-07T20:30:11Z","cross_cats_sorted":[],"title_canon_sha256":"f577c7c73689687731db7e5854c5cb8ef714b8c98dd71c685975250f7924df94","abstract_canon_sha256":"de5b8092df1c95d410dc0ea9fdb5326e4e21a2bf863038b5b71f71e488e1c83c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:12:29.855898Z","signature_b64":"X7+Zc7jALm/RI60/Wdnuds5oqBhZv1SOqnPaLO07QjuZMqybtIUkHlm6HJWt8rgkvcvMMOvcv5wn96rDuiXDDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5af28afd9c71d04a1a7adc9c6bce0dc18fd3587c04e3f3312f684fdae2a7bda4","last_reissued_at":"2026-05-18T01:12:29.855580Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:12:29.855580Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On CMB B-Mode Non-Gaussianity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alex van Engelen (CITA), Joel Meyers, P. Daniel Meerburg, Yacine Ali-Ha\\\"imoud (JHU)","submitted_at":"2016-03-07T20:30:11Z","abstract_excerpt":"We study the degree to which the cosmic microwave background (CMB) can be used to constrain primordial non-Gaussianity involving one tensor and two scalar fluctuations, focusing on the correlation of one polarization $B$ mode with two temperature modes. In the simplest models of inflation, the tensor-scalar-scalar primordial bispectrum is non-vanishing and is of the same order in slow-roll parameters as the scalar-scalar-scalar bispectrum. We calculate the $\\langle BTT\\rangle$ correlation arising from a primordial tensor-scalar-scalar bispectrum, and show that constraints from an experiment li"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.02243","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":"1603.02243","created_at":"2026-05-18T01:12:29.855629+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.02243v2","created_at":"2026-05-18T01:12:29.855629+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.02243","created_at":"2026-05-18T01:12:29.855629+00:00"},{"alias_kind":"pith_short_12","alias_value":"LLZIV7M4OHIE","created_at":"2026-05-18T12:30:29.479603+00:00"},{"alias_kind":"pith_short_16","alias_value":"LLZIV7M4OHIEUGT2","created_at":"2026-05-18T12:30:29.479603+00:00"},{"alias_kind":"pith_short_8","alias_value":"LLZIV7M4","created_at":"2026-05-18T12:30:29.479603+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1907.04473","citing_title":"CMB-S4 Science Case, Reference Design, and Project Plan","ref_index":24,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LLZIV7M4OHIEUGT23SOGXTQNYG","json":"https://pith.science/pith/LLZIV7M4OHIEUGT23SOGXTQNYG.json","graph_json":"https://pith.science/api/pith-number/LLZIV7M4OHIEUGT23SOGXTQNYG/graph.json","events_json":"https://pith.science/api/pith-number/LLZIV7M4OHIEUGT23SOGXTQNYG/events.json","paper":"https://pith.science/paper/LLZIV7M4"},"agent_actions":{"view_html":"https://pith.science/pith/LLZIV7M4OHIEUGT23SOGXTQNYG","download_json":"https://pith.science/pith/LLZIV7M4OHIEUGT23SOGXTQNYG.json","view_paper":"https://pith.science/paper/LLZIV7M4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.02243&json=true","fetch_graph":"https://pith.science/api/pith-number/LLZIV7M4OHIEUGT23SOGXTQNYG/graph.json","fetch_events":"https://pith.science/api/pith-number/LLZIV7M4OHIEUGT23SOGXTQNYG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LLZIV7M4OHIEUGT23SOGXTQNYG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LLZIV7M4OHIEUGT23SOGXTQNYG/action/storage_attestation","attest_author":"https://pith.science/pith/LLZIV7M4OHIEUGT23SOGXTQNYG/action/author_attestation","sign_citation":"https://pith.science/pith/LLZIV7M4OHIEUGT23SOGXTQNYG/action/citation_signature","submit_replication":"https://pith.science/pith/LLZIV7M4OHIEUGT23SOGXTQNYG/action/replication_record"}},"created_at":"2026-05-18T01:12:29.855629+00:00","updated_at":"2026-05-18T01:12:29.855629+00:00"}