{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:SM5HATSB2L4GEHMZH7EOAT5PIE","short_pith_number":"pith:SM5HATSB","schema_version":"1.0","canonical_sha256":"933a704e41d2f8621d993fc8e04faf4134d781265a0990c7d67f65b5e59cc5db","source":{"kind":"arxiv","id":"2405.08059","version":2},"attestation_state":"computed","paper":{"title":"Axion-Induced Patchy Screening of the Cosmic Microwave Background","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Cristina Mondino, Dalila P\\^irvu, Junwu Huang, Matthew C. Johnson","submitted_at":"2024-05-13T18:00:00Z","abstract_excerpt":"Cosmic Microwave Background (CMB) photons can undergo resonant conversion into axions in the presence of magnetized plasma distributed inside non-linear large-scale structure (LSS). This process leads to axion-induced patchy screening: secondary temperature and polarization anisotropies with a characteristic non-blackbody frequency dependence that are strongly correlated with the distribution of LSS along our past light cone. We compute the axion-induced patchy screening contribution to two- and three- point correlation functions that include CMB anisotropies and tracers of LSS within the halo"},"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":"2405.08059","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2024-05-13T18:00:00Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"10e80ecf85bd2eecf89ce87446c994999df850712b9ef03bad328df13ae52558","abstract_canon_sha256":"a78786ccbbfeab243abe47d17e030e0c7f825a1a4c7e5e7cf604b732e649f0e4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:33:31.617745Z","signature_b64":"+Orx2FfRL9VyJeSlOVvhY2jCg9pq87Yjq87vTp4nSwfRiScxM8EoeIgFEjjCSo8a3PaHx8zbmeyPa2tpqA3VCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"933a704e41d2f8621d993fc8e04faf4134d781265a0990c7d67f65b5e59cc5db","last_reissued_at":"2026-07-05T09:33:31.617247Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:33:31.617247Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Axion-Induced Patchy Screening of the Cosmic Microwave Background","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Cristina Mondino, Dalila P\\^irvu, Junwu Huang, Matthew C. Johnson","submitted_at":"2024-05-13T18:00:00Z","abstract_excerpt":"Cosmic Microwave Background (CMB) photons can undergo resonant conversion into axions in the presence of magnetized plasma distributed inside non-linear large-scale structure (LSS). This process leads to axion-induced patchy screening: secondary temperature and polarization anisotropies with a characteristic non-blackbody frequency dependence that are strongly correlated with the distribution of LSS along our past light cone. We compute the axion-induced patchy screening contribution to two- and three- point correlation functions that include CMB anisotropies and tracers of LSS within the halo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.08059","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2405.08059/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":"2405.08059","created_at":"2026-07-05T09:33:31.617300+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.08059v2","created_at":"2026-07-05T09:33:31.617300+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.08059","created_at":"2026-07-05T09:33:31.617300+00:00"},{"alias_kind":"pith_short_12","alias_value":"SM5HATSB2L4G","created_at":"2026-07-05T09:33:31.617300+00:00"},{"alias_kind":"pith_short_16","alias_value":"SM5HATSB2L4GEHMZ","created_at":"2026-07-05T09:33:31.617300+00:00"},{"alias_kind":"pith_short_8","alias_value":"SM5HATSB","created_at":"2026-07-05T09:33:31.617300+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2509.23123","citing_title":"Constraining Inflationary Particle Production with CMB Polarization","ref_index":43,"is_internal_anchor":false},{"citing_arxiv_id":"2604.20768","citing_title":"Primordial Magnetogenesis and Gravitational Waves from ALP-assisted Phase Transition","ref_index":184,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SM5HATSB2L4GEHMZH7EOAT5PIE","json":"https://pith.science/pith/SM5HATSB2L4GEHMZH7EOAT5PIE.json","graph_json":"https://pith.science/api/pith-number/SM5HATSB2L4GEHMZH7EOAT5PIE/graph.json","events_json":"https://pith.science/api/pith-number/SM5HATSB2L4GEHMZH7EOAT5PIE/events.json","paper":"https://pith.science/paper/SM5HATSB"},"agent_actions":{"view_html":"https://pith.science/pith/SM5HATSB2L4GEHMZH7EOAT5PIE","download_json":"https://pith.science/pith/SM5HATSB2L4GEHMZH7EOAT5PIE.json","view_paper":"https://pith.science/paper/SM5HATSB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.08059&json=true","fetch_graph":"https://pith.science/api/pith-number/SM5HATSB2L4GEHMZH7EOAT5PIE/graph.json","fetch_events":"https://pith.science/api/pith-number/SM5HATSB2L4GEHMZH7EOAT5PIE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SM5HATSB2L4GEHMZH7EOAT5PIE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SM5HATSB2L4GEHMZH7EOAT5PIE/action/storage_attestation","attest_author":"https://pith.science/pith/SM5HATSB2L4GEHMZH7EOAT5PIE/action/author_attestation","sign_citation":"https://pith.science/pith/SM5HATSB2L4GEHMZH7EOAT5PIE/action/citation_signature","submit_replication":"https://pith.science/pith/SM5HATSB2L4GEHMZH7EOAT5PIE/action/replication_record"}},"created_at":"2026-07-05T09:33:31.617300+00:00","updated_at":"2026-07-05T09:33:31.617300+00:00"}