{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:5BTRFKDXQDALUXO457LSSS7CMT","short_pith_number":"pith:5BTRFKDX","schema_version":"1.0","canonical_sha256":"e86712a87780c0ba5ddcefd7294be264fd963a7f4a75a3c53454060a4d891b3d","source":{"kind":"arxiv","id":"1611.05865","version":2},"attestation_state":"computed","paper":{"title":"Dielectric Haloscopes: A New Way to Detect Axion Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE","hep-ex","hep-ph"],"primary_cat":"physics.ins-det","authors_text":"Alexander Millar, Bela Majorovits, Frank Simon, Frank Steffen, Georg Raffelt, Gia Dvali, Javier Redondo, Olaf Reimann, The MADMAX Working Group: Allen Caldwell","submitted_at":"2016-11-17T20:13:08Z","abstract_excerpt":"We propose a new strategy to search for dark matter axions in the mass range of 40--400 $\\mu$eV by introducing dielectric haloscopes, which consist of dielectric disks placed in a magnetic field. The changing dielectric media cause discontinuities in the axion-induced electric field, leading to the generation of propagating electromagnetic waves to satisfy the continuity requirements at the interfaces. Large-area disks with adjustable distances boost the microwave signal (10--100 GHz) to an observable level and allow one to scan over a broad axion mass range. A sensitivity to QCD axion models "},"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":"1611.05865","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.ins-det","submitted_at":"2016-11-17T20:13:08Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE","hep-ex","hep-ph"],"title_canon_sha256":"796d159e048b51c8038b1fa3fd6e0179b2f586bfb400c1fbdda429b7463b7d57","abstract_canon_sha256":"e91de09caebc06be997c99681e3add12fcc01bda50fef9e73b2d6d6a894deafb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:49:36.428366Z","signature_b64":"oF7taRIAwLE24NsZPsIgw+qoR2nMx9e0wPB4sfCCUUQgbG382wwqxTVyLtMyWM8ycYai8pNXWQtROX5/kYNaBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e86712a87780c0ba5ddcefd7294be264fd963a7f4a75a3c53454060a4d891b3d","last_reissued_at":"2026-05-18T00:49:36.427799Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:49:36.427799Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dielectric Haloscopes: A New Way to Detect Axion Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE","hep-ex","hep-ph"],"primary_cat":"physics.ins-det","authors_text":"Alexander Millar, Bela Majorovits, Frank Simon, Frank Steffen, Georg Raffelt, Gia Dvali, Javier Redondo, Olaf Reimann, The MADMAX Working Group: Allen Caldwell","submitted_at":"2016-11-17T20:13:08Z","abstract_excerpt":"We propose a new strategy to search for dark matter axions in the mass range of 40--400 $\\mu$eV by introducing dielectric haloscopes, which consist of dielectric disks placed in a magnetic field. The changing dielectric media cause discontinuities in the axion-induced electric field, leading to the generation of propagating electromagnetic waves to satisfy the continuity requirements at the interfaces. Large-area disks with adjustable distances boost the microwave signal (10--100 GHz) to an observable level and allow one to scan over a broad axion mass range. A sensitivity to QCD axion models "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.05865","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":""},"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":"1611.05865","created_at":"2026-05-18T00:49:36.427882+00:00"},{"alias_kind":"arxiv_version","alias_value":"1611.05865v2","created_at":"2026-05-18T00:49:36.427882+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1611.05865","created_at":"2026-05-18T00:49:36.427882+00:00"},{"alias_kind":"pith_short_12","alias_value":"5BTRFKDXQDAL","created_at":"2026-05-18T12:29:58.707656+00:00"},{"alias_kind":"pith_short_16","alias_value":"5BTRFKDXQDALUXO4","created_at":"2026-05-18T12:29:58.707656+00:00"},{"alias_kind":"pith_short_8","alias_value":"5BTRFKDX","created_at":"2026-05-18T12:29:58.707656+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"1907.04324","citing_title":"Dark Matter Energy Deposition and Production from the Table-Top to the Cosmos","ref_index":93,"is_internal_anchor":true},{"citing_arxiv_id":"1907.08010","citing_title":"Cosmological searches for the neutrino mass scale and mass ordering","ref_index":270,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5BTRFKDXQDALUXO457LSSS7CMT","json":"https://pith.science/pith/5BTRFKDXQDALUXO457LSSS7CMT.json","graph_json":"https://pith.science/api/pith-number/5BTRFKDXQDALUXO457LSSS7CMT/graph.json","events_json":"https://pith.science/api/pith-number/5BTRFKDXQDALUXO457LSSS7CMT/events.json","paper":"https://pith.science/paper/5BTRFKDX"},"agent_actions":{"view_html":"https://pith.science/pith/5BTRFKDXQDALUXO457LSSS7CMT","download_json":"https://pith.science/pith/5BTRFKDXQDALUXO457LSSS7CMT.json","view_paper":"https://pith.science/paper/5BTRFKDX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1611.05865&json=true","fetch_graph":"https://pith.science/api/pith-number/5BTRFKDXQDALUXO457LSSS7CMT/graph.json","fetch_events":"https://pith.science/api/pith-number/5BTRFKDXQDALUXO457LSSS7CMT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5BTRFKDXQDALUXO457LSSS7CMT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5BTRFKDXQDALUXO457LSSS7CMT/action/storage_attestation","attest_author":"https://pith.science/pith/5BTRFKDXQDALUXO457LSSS7CMT/action/author_attestation","sign_citation":"https://pith.science/pith/5BTRFKDXQDALUXO457LSSS7CMT/action/citation_signature","submit_replication":"https://pith.science/pith/5BTRFKDXQDALUXO457LSSS7CMT/action/replication_record"}},"created_at":"2026-05-18T00:49:36.427882+00:00","updated_at":"2026-05-18T00:49:36.427882+00:00"}