{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:JJBK6NADAIBNRLH47LYH34HE7X","short_pith_number":"pith:JJBK6NAD","schema_version":"1.0","canonical_sha256":"4a42af34030202d8acfcfaf07df0e4fdcf8e4247777153bf6d4685233b4d0fb7","source":{"kind":"arxiv","id":"2002.07639","version":3},"attestation_state":"computed","paper":{"title":"Scalable haloscopes for axion dark matter detection in the 30$\\mu$eV range with RADES","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"hep-ex","authors_text":"A. \\'Alvarez Melc\\'on, A. D\\'iaz-Morcillo, A.J. Lozano-Guerrero, A. Millar, B. D\\\"obrich, B. Gimeno, C. Cogollos, C. Malbrunot, C. Pe\\~na Garay, I.G. Irastorza, J.D. Gallego, J. Golm, J.M. Garc\\'ia Barcel\\'o, J. Redondo, P. Navarro, S. Arguedas Cuendis, W. Wuensch","submitted_at":"2020-02-18T15:25:23Z","abstract_excerpt":"RADES (Relic Axion Detector Exploratory Setup) is a project with the goal of directly searching for axion dark matter above the $30 \\mu$eV scale employing custom-made microwave filters in magnetic dipole fields. Currently RADES is taking data at the LHC dipole of the CAST experiment. In the long term, the RADES cavities are envisioned to take data in the (baby)-IAXO magnet. In this article we report on the modelling, building and characterisation of an optimised microwave-filter design with alternating irises that exploits maximal coupling to axions while being scalable in length without suffe"},"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":"2002.07639","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ex","submitted_at":"2020-02-18T15:25:23Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"1be2f9b90719028cdd49896b0ccd290f89ee614bd3ac5008281de698f2d6f52f","abstract_canon_sha256":"65f5eb70103f8aa6d3d94a68e79593fba4e04f53a34a9b413ef153ee4e6e5337"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:12:02.569058Z","signature_b64":"WyKCBwtRb8vRDIkV7l8B2qWmP49s705SiH8FhenN3u9L4tiXS/Tx1s9HOULaRJ75CV+869u/SE7Kmwl9EHT4Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4a42af34030202d8acfcfaf07df0e4fdcf8e4247777153bf6d4685233b4d0fb7","last_reissued_at":"2026-07-05T01:12:02.568624Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:12:02.568624Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Scalable haloscopes for axion dark matter detection in the 30$\\mu$eV range with RADES","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"hep-ex","authors_text":"A. \\'Alvarez Melc\\'on, A. D\\'iaz-Morcillo, A.J. Lozano-Guerrero, A. Millar, B. D\\\"obrich, B. Gimeno, C. Cogollos, C. Malbrunot, C. Pe\\~na Garay, I.G. Irastorza, J.D. Gallego, J. Golm, J.M. Garc\\'ia Barcel\\'o, J. Redondo, P. Navarro, S. Arguedas Cuendis, W. Wuensch","submitted_at":"2020-02-18T15:25:23Z","abstract_excerpt":"RADES (Relic Axion Detector Exploratory Setup) is a project with the goal of directly searching for axion dark matter above the $30 \\mu$eV scale employing custom-made microwave filters in magnetic dipole fields. Currently RADES is taking data at the LHC dipole of the CAST experiment. In the long term, the RADES cavities are envisioned to take data in the (baby)-IAXO magnet. In this article we report on the modelling, building and characterisation of an optimised microwave-filter design with alternating irises that exploits maximal coupling to axions while being scalable in length without suffe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2002.07639","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/2002.07639/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":"2002.07639","created_at":"2026-07-05T01:12:02.568695+00:00"},{"alias_kind":"arxiv_version","alias_value":"2002.07639v3","created_at":"2026-07-05T01:12:02.568695+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2002.07639","created_at":"2026-07-05T01:12:02.568695+00:00"},{"alias_kind":"pith_short_12","alias_value":"JJBK6NADAIBN","created_at":"2026-07-05T01:12:02.568695+00:00"},{"alias_kind":"pith_short_16","alias_value":"JJBK6NADAIBNRLH4","created_at":"2026-07-05T01:12:02.568695+00:00"},{"alias_kind":"pith_short_8","alias_value":"JJBK6NAD","created_at":"2026-07-05T01:12:02.568695+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.20422","citing_title":"Resonant heterodyne conversion applied to a low-frequency haloscope for dark matter axion searches in the 1-35 MHz range","ref_index":17,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JJBK6NADAIBNRLH47LYH34HE7X","json":"https://pith.science/pith/JJBK6NADAIBNRLH47LYH34HE7X.json","graph_json":"https://pith.science/api/pith-number/JJBK6NADAIBNRLH47LYH34HE7X/graph.json","events_json":"https://pith.science/api/pith-number/JJBK6NADAIBNRLH47LYH34HE7X/events.json","paper":"https://pith.science/paper/JJBK6NAD"},"agent_actions":{"view_html":"https://pith.science/pith/JJBK6NADAIBNRLH47LYH34HE7X","download_json":"https://pith.science/pith/JJBK6NADAIBNRLH47LYH34HE7X.json","view_paper":"https://pith.science/paper/JJBK6NAD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2002.07639&json=true","fetch_graph":"https://pith.science/api/pith-number/JJBK6NADAIBNRLH47LYH34HE7X/graph.json","fetch_events":"https://pith.science/api/pith-number/JJBK6NADAIBNRLH47LYH34HE7X/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JJBK6NADAIBNRLH47LYH34HE7X/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JJBK6NADAIBNRLH47LYH34HE7X/action/storage_attestation","attest_author":"https://pith.science/pith/JJBK6NADAIBNRLH47LYH34HE7X/action/author_attestation","sign_citation":"https://pith.science/pith/JJBK6NADAIBNRLH47LYH34HE7X/action/citation_signature","submit_replication":"https://pith.science/pith/JJBK6NADAIBNRLH47LYH34HE7X/action/replication_record"}},"created_at":"2026-07-05T01:12:02.568695+00:00","updated_at":"2026-07-05T01:12:02.568695+00:00"}