{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:QNDNBUJVWQQB2OHEWAKBMEFCK3","short_pith_number":"pith:QNDNBUJV","schema_version":"1.0","canonical_sha256":"8346d0d135b4201d38e4b0141610a256c62491616c807f175b54775c1ca5dff2","source":{"kind":"arxiv","id":"2408.03861","version":1},"attestation_state":"computed","paper":{"title":"A tunable photonic band gap resonator for axion dark matter searches","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"physics.ins-det","authors_text":"Aarav M. Sindhwad, Alexander F. Leder, Dillon T. Goulart, Isabella Urdinaran, Karl van Bibber, Mirelys Carcana Barbosa, Samantha M. Lewis","submitted_at":"2024-08-07T16:10:13Z","abstract_excerpt":"Axions are a well-motivated dark matter candidate particle. Haloscopes aim to detect axions in the galactic halo by measuring the photon signal resulting from axions interacting with a strong magnetic field. Existing haloscopes are primarily targeting axion masses which produce microwave-range photons and rely on microwave resonators to enhance the signal power. Only a limited subset of resonator modes are useful for this process, and current cylindrical-style cavities suffer from mode mixing and crowding from other fundamental modes. The majority of these modes can be eliminated by using phot"},"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":"2408.03861","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"physics.ins-det","submitted_at":"2024-08-07T16:10:13Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"fa0fda9596a3592078bff37910f7d6ce829eca80792d7cf4d23415ea913d14a7","abstract_canon_sha256":"9194b9ee26088799671c1bf2759f0b617789175f5a5fc93a10c49b4631a34f57"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:53:12.092933Z","signature_b64":"YK/kHgSiHzD3fxiJCAdkg+EMOJHtX4yH1aTiKbuVdh26a/YmaXZ3hnwF6WY/mRwERj7Z+BSaiAqN4n28/u2sAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8346d0d135b4201d38e4b0141610a256c62491616c807f175b54775c1ca5dff2","last_reissued_at":"2026-07-05T08:53:12.092444Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:53:12.092444Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A tunable photonic band gap resonator for axion dark matter searches","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"physics.ins-det","authors_text":"Aarav M. Sindhwad, Alexander F. Leder, Dillon T. Goulart, Isabella Urdinaran, Karl van Bibber, Mirelys Carcana Barbosa, Samantha M. Lewis","submitted_at":"2024-08-07T16:10:13Z","abstract_excerpt":"Axions are a well-motivated dark matter candidate particle. Haloscopes aim to detect axions in the galactic halo by measuring the photon signal resulting from axions interacting with a strong magnetic field. Existing haloscopes are primarily targeting axion masses which produce microwave-range photons and rely on microwave resonators to enhance the signal power. Only a limited subset of resonator modes are useful for this process, and current cylindrical-style cavities suffer from mode mixing and crowding from other fundamental modes. The majority of these modes can be eliminated by using phot"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2408.03861","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/2408.03861/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":"2408.03861","created_at":"2026-07-05T08:53:12.092503+00:00"},{"alias_kind":"arxiv_version","alias_value":"2408.03861v1","created_at":"2026-07-05T08:53:12.092503+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2408.03861","created_at":"2026-07-05T08:53:12.092503+00:00"},{"alias_kind":"pith_short_12","alias_value":"QNDNBUJVWQQB","created_at":"2026-07-05T08:53:12.092503+00:00"},{"alias_kind":"pith_short_16","alias_value":"QNDNBUJVWQQB2OHE","created_at":"2026-07-05T08:53:12.092503+00:00"},{"alias_kind":"pith_short_8","alias_value":"QNDNBUJV","created_at":"2026-07-05T08:53:12.092503+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QNDNBUJVWQQB2OHEWAKBMEFCK3","json":"https://pith.science/pith/QNDNBUJVWQQB2OHEWAKBMEFCK3.json","graph_json":"https://pith.science/api/pith-number/QNDNBUJVWQQB2OHEWAKBMEFCK3/graph.json","events_json":"https://pith.science/api/pith-number/QNDNBUJVWQQB2OHEWAKBMEFCK3/events.json","paper":"https://pith.science/paper/QNDNBUJV"},"agent_actions":{"view_html":"https://pith.science/pith/QNDNBUJVWQQB2OHEWAKBMEFCK3","download_json":"https://pith.science/pith/QNDNBUJVWQQB2OHEWAKBMEFCK3.json","view_paper":"https://pith.science/paper/QNDNBUJV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2408.03861&json=true","fetch_graph":"https://pith.science/api/pith-number/QNDNBUJVWQQB2OHEWAKBMEFCK3/graph.json","fetch_events":"https://pith.science/api/pith-number/QNDNBUJVWQQB2OHEWAKBMEFCK3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QNDNBUJVWQQB2OHEWAKBMEFCK3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QNDNBUJVWQQB2OHEWAKBMEFCK3/action/storage_attestation","attest_author":"https://pith.science/pith/QNDNBUJVWQQB2OHEWAKBMEFCK3/action/author_attestation","sign_citation":"https://pith.science/pith/QNDNBUJVWQQB2OHEWAKBMEFCK3/action/citation_signature","submit_replication":"https://pith.science/pith/QNDNBUJVWQQB2OHEWAKBMEFCK3/action/replication_record"}},"created_at":"2026-07-05T08:53:12.092503+00:00","updated_at":"2026-07-05T08:53:12.092503+00:00"}