{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:D7CK5C45G3CF7AOINMBX7SW6KN","short_pith_number":"pith:D7CK5C45","schema_version":"1.0","canonical_sha256":"1fc4ae8b9d36c45f81c86b037fcade53435c07e5e9d40e5bc183d2eb3fe8c96b","source":{"kind":"arxiv","id":"2405.08879","version":3},"attestation_state":"computed","paper":{"title":"A Diffused Background from Axion-like Particles in the Microwave Sky","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Harsh Mehta, Suvodip Mukherjee","submitted_at":"2024-05-14T18:00:39Z","abstract_excerpt":"The nature of dark matter is an unsolved cosmological problem and axions are one of the weakly interacting cold dark matter candidates. Axions or ALPs (Axion-like particles) are pseudo-scalar bosons predicted by beyond-standard model theories. The weak coupling of ALPs with photons leads to the conversion of CMB photons to ALPs in the presence of a transverse magnetic field. If they have the same mass as the effective mass of a photon in a plasma, the resonant conversion would cause a polarized spectral distortion leading to temperature fluctuations with the distortion spectrum. The probabilit"},"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":"2405.08879","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-05-14T18:00:39Z","cross_cats_sorted":["hep-ph","hep-th"],"title_canon_sha256":"b9ea6d480ab2615e7d7cb85744b30710590942f75f4456ac02ee7ec1011ad9b1","abstract_canon_sha256":"bc3a03fc3f1f8c3c548e2996c4d99da6c21540228858e4c133f32c259a1e0831"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:50:12.406617Z","signature_b64":"wUVn+SwGsvMoSTDO3xpdp3SGtsYxRMae/e7+u5cwrKuCb29ahzn8ilYBzkm6Szl7wrqDVj8Qehib+vxnlmHGDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1fc4ae8b9d36c45f81c86b037fcade53435c07e5e9d40e5bc183d2eb3fe8c96b","last_reissued_at":"2026-07-05T08:50:12.406162Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:50:12.406162Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Diffused Background from Axion-like Particles in the Microwave Sky","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Harsh Mehta, Suvodip Mukherjee","submitted_at":"2024-05-14T18:00:39Z","abstract_excerpt":"The nature of dark matter is an unsolved cosmological problem and axions are one of the weakly interacting cold dark matter candidates. Axions or ALPs (Axion-like particles) are pseudo-scalar bosons predicted by beyond-standard model theories. The weak coupling of ALPs with photons leads to the conversion of CMB photons to ALPs in the presence of a transverse magnetic field. If they have the same mass as the effective mass of a photon in a plasma, the resonant conversion would cause a polarized spectral distortion leading to temperature fluctuations with the distortion spectrum. The probabilit"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.08879","kind":"arxiv","version":3},"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/2405.08879/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":"2405.08879","created_at":"2026-07-05T08:50:12.406225+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.08879v3","created_at":"2026-07-05T08:50:12.406225+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.08879","created_at":"2026-07-05T08:50:12.406225+00:00"},{"alias_kind":"pith_short_12","alias_value":"D7CK5C45G3CF","created_at":"2026-07-05T08:50:12.406225+00:00"},{"alias_kind":"pith_short_16","alias_value":"D7CK5C45G3CF7AOI","created_at":"2026-07-05T08:50:12.406225+00:00"},{"alias_kind":"pith_short_8","alias_value":"D7CK5C45","created_at":"2026-07-05T08:50:12.406225+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2505.11592","citing_title":"The Prospect from the Upcoming CMB Experiment LiteBIRD to Discover Axion-like Particles Using Milky Way","ref_index":58,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/D7CK5C45G3CF7AOINMBX7SW6KN","json":"https://pith.science/pith/D7CK5C45G3CF7AOINMBX7SW6KN.json","graph_json":"https://pith.science/api/pith-number/D7CK5C45G3CF7AOINMBX7SW6KN/graph.json","events_json":"https://pith.science/api/pith-number/D7CK5C45G3CF7AOINMBX7SW6KN/events.json","paper":"https://pith.science/paper/D7CK5C45"},"agent_actions":{"view_html":"https://pith.science/pith/D7CK5C45G3CF7AOINMBX7SW6KN","download_json":"https://pith.science/pith/D7CK5C45G3CF7AOINMBX7SW6KN.json","view_paper":"https://pith.science/paper/D7CK5C45","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.08879&json=true","fetch_graph":"https://pith.science/api/pith-number/D7CK5C45G3CF7AOINMBX7SW6KN/graph.json","fetch_events":"https://pith.science/api/pith-number/D7CK5C45G3CF7AOINMBX7SW6KN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/D7CK5C45G3CF7AOINMBX7SW6KN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/D7CK5C45G3CF7AOINMBX7SW6KN/action/storage_attestation","attest_author":"https://pith.science/pith/D7CK5C45G3CF7AOINMBX7SW6KN/action/author_attestation","sign_citation":"https://pith.science/pith/D7CK5C45G3CF7AOINMBX7SW6KN/action/citation_signature","submit_replication":"https://pith.science/pith/D7CK5C45G3CF7AOINMBX7SW6KN/action/replication_record"}},"created_at":"2026-07-05T08:50:12.406225+00:00","updated_at":"2026-07-05T08:50:12.406225+00:00"}