{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:GYE5EU4VB2USROXUGGXM2L54OV","short_pith_number":"pith:GYE5EU4V","schema_version":"1.0","canonical_sha256":"3609d253950ea928baf431aecd2fbc75464998495f494efdd62392839ee7fa3f","source":{"kind":"arxiv","id":"2303.03997","version":6},"attestation_state":"computed","paper":{"title":"Discovery prospects with the Dark-photons & Axion-Like particles Interferometer","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ex"],"primary_cat":"hep-ph","authors_text":"Chiko Otani, Elvio Hern\\'andez-Su\\'arez, Enrique Joven-\\'Alvarez, J. Alberto Rubi\\~no-Mart\\'in (on behalf of the DALI Collaboration), Javier De Miguel, Juan F. Hern\\'andez-Cabrera","submitted_at":"2023-03-07T15:53:30Z","abstract_excerpt":"We discuss the discovery potential of the Dark-photons & Axion-Like particles Interferometer (DALI) in this letter. The apparatus, currently in a design and prototyping phase, will probe axion dark matter from the Teide Observatory, an environment protected from terrestrial microwave sources, reaching Dine--Fischler--Srednicki--Zhitnitsky-like axion sensitivity in the range 25--250 $\\mu$eV of mass. The experimental approach shows a potential to probe dark sector photons of kinetic mixing strength in excess of several $10^{-16}$, and to establish new constraints to a stochastic gravitational wa"},"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":"2303.03997","kind":"arxiv","version":6},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2023-03-07T15:53:30Z","cross_cats_sorted":["astro-ph.CO","hep-ex"],"title_canon_sha256":"7fb6c78fb7dbed2914161d7c7b2f93edf0e341360ceeaf0fe2d333fd70b28853","abstract_canon_sha256":"678f8fc41261fae18d18f065d8a5816a2f10452bea670ce13fead608f566e563"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:53:07.397877Z","signature_b64":"g6ZUBCchpX+n7ViuoOfWki+2MnBWeKkZL4h0av2gAwXaa32gehoHzAusubFmCfdOXbCKIQMp3FxGLxrF0Z8YCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3609d253950ea928baf431aecd2fbc75464998495f494efdd62392839ee7fa3f","last_reissued_at":"2026-07-05T07:53:07.397367Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:53:07.397367Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Discovery prospects with the Dark-photons & Axion-Like particles Interferometer","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ex"],"primary_cat":"hep-ph","authors_text":"Chiko Otani, Elvio Hern\\'andez-Su\\'arez, Enrique Joven-\\'Alvarez, J. Alberto Rubi\\~no-Mart\\'in (on behalf of the DALI Collaboration), Javier De Miguel, Juan F. Hern\\'andez-Cabrera","submitted_at":"2023-03-07T15:53:30Z","abstract_excerpt":"We discuss the discovery potential of the Dark-photons & Axion-Like particles Interferometer (DALI) in this letter. The apparatus, currently in a design and prototyping phase, will probe axion dark matter from the Teide Observatory, an environment protected from terrestrial microwave sources, reaching Dine--Fischler--Srednicki--Zhitnitsky-like axion sensitivity in the range 25--250 $\\mu$eV of mass. The experimental approach shows a potential to probe dark sector photons of kinetic mixing strength in excess of several $10^{-16}$, and to establish new constraints to a stochastic gravitational wa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2303.03997","kind":"arxiv","version":6},"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/2303.03997/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":"2303.03997","created_at":"2026-07-05T07:53:07.397428+00:00"},{"alias_kind":"arxiv_version","alias_value":"2303.03997v6","created_at":"2026-07-05T07:53:07.397428+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2303.03997","created_at":"2026-07-05T07:53:07.397428+00:00"},{"alias_kind":"pith_short_12","alias_value":"GYE5EU4VB2US","created_at":"2026-07-05T07:53:07.397428+00:00"},{"alias_kind":"pith_short_16","alias_value":"GYE5EU4VB2USROXU","created_at":"2026-07-05T07:53:07.397428+00:00"},{"alias_kind":"pith_short_8","alias_value":"GYE5EU4V","created_at":"2026-07-05T07:53:07.397428+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2404.13970","citing_title":"DALI sensitivity to streaming axion dark matter","ref_index":53,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GYE5EU4VB2USROXUGGXM2L54OV","json":"https://pith.science/pith/GYE5EU4VB2USROXUGGXM2L54OV.json","graph_json":"https://pith.science/api/pith-number/GYE5EU4VB2USROXUGGXM2L54OV/graph.json","events_json":"https://pith.science/api/pith-number/GYE5EU4VB2USROXUGGXM2L54OV/events.json","paper":"https://pith.science/paper/GYE5EU4V"},"agent_actions":{"view_html":"https://pith.science/pith/GYE5EU4VB2USROXUGGXM2L54OV","download_json":"https://pith.science/pith/GYE5EU4VB2USROXUGGXM2L54OV.json","view_paper":"https://pith.science/paper/GYE5EU4V","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2303.03997&json=true","fetch_graph":"https://pith.science/api/pith-number/GYE5EU4VB2USROXUGGXM2L54OV/graph.json","fetch_events":"https://pith.science/api/pith-number/GYE5EU4VB2USROXUGGXM2L54OV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GYE5EU4VB2USROXUGGXM2L54OV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GYE5EU4VB2USROXUGGXM2L54OV/action/storage_attestation","attest_author":"https://pith.science/pith/GYE5EU4VB2USROXUGGXM2L54OV/action/author_attestation","sign_citation":"https://pith.science/pith/GYE5EU4VB2USROXUGGXM2L54OV/action/citation_signature","submit_replication":"https://pith.science/pith/GYE5EU4VB2USROXUGGXM2L54OV/action/replication_record"}},"created_at":"2026-07-05T07:53:07.397428+00:00","updated_at":"2026-07-05T07:53:07.397428+00:00"}