{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:GCOH4YCGFM2X3ERSNUSBKAL2P4","short_pith_number":"pith:GCOH4YCG","schema_version":"1.0","canonical_sha256":"309c7e60462b357d92326d2415017a7f0019f7bd5ec1b71eabb476161cd02877","source":{"kind":"arxiv","id":"2505.20450","version":1},"attestation_state":"computed","paper":{"title":"Searching for Axion Dark Matter Near Relaxing Magnetars","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Anirudh Prabhu, Carlos Blanco, Christopher Thompson, Jonathan Zhang, Samuel J. Witte, Sandip Roy","submitted_at":"2025-05-26T18:43:50Z","abstract_excerpt":"Axion dark matter passing through the magnetospheres of magnetars can undergo hyper-efficient resonant mixing with low-energy photons, leading to the production of narrow spectral lines that could be detectable on Earth. Since this is a resonant process triggered by the spatial variation in the photon dispersion relation, the luminosity and spectral properties of the emission are highly sensitive to the charge and current densities permeating the magnetosphere. To date, a majority of the studies investigating this phenomenon have assumed a perfectly dipolar magnetic field structure with a near"},"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":"2505.20450","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/publicdomain/zero/1.0/","primary_cat":"hep-ph","submitted_at":"2025-05-26T18:43:50Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"e4f14a99cfa799bb7a6c4ccb443211ac05353e055d92acc6e16c0620588833ac","abstract_canon_sha256":"189781a3bd0fa85d6be2de5b29a3c9e2bfe8169d2758b1cb1c8b2d736d474801"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:10:12.646374Z","signature_b64":"RPTHcBp1qVASTIt+Tnm5du0xFIGxtq0h9D7sABrHapFQ85f5fDEGYdGwBoU0O1NTR0wDxL1PE0nUK2uiu/H1Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"309c7e60462b357d92326d2415017a7f0019f7bd5ec1b71eabb476161cd02877","last_reissued_at":"2026-07-05T11:10:12.645875Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:10:12.645875Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Searching for Axion Dark Matter Near Relaxing Magnetars","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Anirudh Prabhu, Carlos Blanco, Christopher Thompson, Jonathan Zhang, Samuel J. Witte, Sandip Roy","submitted_at":"2025-05-26T18:43:50Z","abstract_excerpt":"Axion dark matter passing through the magnetospheres of magnetars can undergo hyper-efficient resonant mixing with low-energy photons, leading to the production of narrow spectral lines that could be detectable on Earth. Since this is a resonant process triggered by the spatial variation in the photon dispersion relation, the luminosity and spectral properties of the emission are highly sensitive to the charge and current densities permeating the magnetosphere. To date, a majority of the studies investigating this phenomenon have assumed a perfectly dipolar magnetic field structure with a near"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2505.20450","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/2505.20450/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":"2505.20450","created_at":"2026-07-05T11:10:12.645932+00:00"},{"alias_kind":"arxiv_version","alias_value":"2505.20450v1","created_at":"2026-07-05T11:10:12.645932+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2505.20450","created_at":"2026-07-05T11:10:12.645932+00:00"},{"alias_kind":"pith_short_12","alias_value":"GCOH4YCGFM2X","created_at":"2026-07-05T11:10:12.645932+00:00"},{"alias_kind":"pith_short_16","alias_value":"GCOH4YCGFM2X3ERS","created_at":"2026-07-05T11:10:12.645932+00:00"},{"alias_kind":"pith_short_8","alias_value":"GCOH4YCG","created_at":"2026-07-05T11:10:12.645932+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.31476","citing_title":"Landau-Zener formula and resonant axion conversion in neutron star magnetospheres","ref_index":49,"is_internal_anchor":false},{"citing_arxiv_id":"2507.13432","citing_title":"INTEGRAL, eROSITA and Voyager Constraints on Light Bosonic Dark Matter: ALPs, Dark Photons, Scalars, $B-L$ and $L_{i}-L_{j}$ Vectors","ref_index":54,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GCOH4YCGFM2X3ERSNUSBKAL2P4","json":"https://pith.science/pith/GCOH4YCGFM2X3ERSNUSBKAL2P4.json","graph_json":"https://pith.science/api/pith-number/GCOH4YCGFM2X3ERSNUSBKAL2P4/graph.json","events_json":"https://pith.science/api/pith-number/GCOH4YCGFM2X3ERSNUSBKAL2P4/events.json","paper":"https://pith.science/paper/GCOH4YCG"},"agent_actions":{"view_html":"https://pith.science/pith/GCOH4YCGFM2X3ERSNUSBKAL2P4","download_json":"https://pith.science/pith/GCOH4YCGFM2X3ERSNUSBKAL2P4.json","view_paper":"https://pith.science/paper/GCOH4YCG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2505.20450&json=true","fetch_graph":"https://pith.science/api/pith-number/GCOH4YCGFM2X3ERSNUSBKAL2P4/graph.json","fetch_events":"https://pith.science/api/pith-number/GCOH4YCGFM2X3ERSNUSBKAL2P4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GCOH4YCGFM2X3ERSNUSBKAL2P4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GCOH4YCGFM2X3ERSNUSBKAL2P4/action/storage_attestation","attest_author":"https://pith.science/pith/GCOH4YCGFM2X3ERSNUSBKAL2P4/action/author_attestation","sign_citation":"https://pith.science/pith/GCOH4YCGFM2X3ERSNUSBKAL2P4/action/citation_signature","submit_replication":"https://pith.science/pith/GCOH4YCGFM2X3ERSNUSBKAL2P4/action/replication_record"}},"created_at":"2026-07-05T11:10:12.645932+00:00","updated_at":"2026-07-05T11:10:12.645932+00:00"}