{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:B3O7RHLJNNNNS4TJDLSRW37B3K","short_pith_number":"pith:B3O7RHLJ","schema_version":"1.0","canonical_sha256":"0eddf89d696b5ad972691ae51b6fe1dab3ec69b60a98ce64e65b09026450c9d2","source":{"kind":"arxiv","id":"2008.03924","version":1},"attestation_state":"computed","paper":{"title":"Supernova-scope for the Direct Search of Supernova Axions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ex"],"primary_cat":"hep-ph","authors_text":"Jiaming Zheng, Koichi Hamaguchi, Koichi Ichimura, Koji Ishidoshiro, Natsumi Nagata, Shao-Feng Ge, Yasuhiro Kishimoto, Yoshiki Kanazawa","submitted_at":"2020-08-10T07:12:36Z","abstract_excerpt":"If a supernova explosion occurs within a few hundred parsecs from the Earth, a huge number of axions, in addition to neutrinos, may arrive at the Earth. In this paper, we discuss in detail the prospect of detecting those supernova axions by an axion helioscope. With the help of a pre-supernova neutrino alert system, it is possible to point a helioscope at an exploding supernova in advance. The supernova axions can then be detected by a gamma-ray detector installed at the end of the helioscope. We call such a detection system an axion supernova-scope (SNscope). We propose a conceptual design fo"},"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":"2008.03924","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2020-08-10T07:12:36Z","cross_cats_sorted":["astro-ph.HE","hep-ex"],"title_canon_sha256":"b69db4e6dcdc998352ec4bc505eb89cac7641922e681430b4799ff35d6707aa8","abstract_canon_sha256":"4413f054ff58527c095b5ef642f6a97fa03a07c1bea7406f134591059e62ac13"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:57:53.279334Z","signature_b64":"lrPEdBGrqkNL7nIfdyl5jYCQiGlOPfkjrsVo6pQ4qiYFaS30EmJXdn3Wb4rqOB0fGYGyvWGBckWSvSdhGQiMAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0eddf89d696b5ad972691ae51b6fe1dab3ec69b60a98ce64e65b09026450c9d2","last_reissued_at":"2026-07-05T01:57:53.278877Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:57:53.278877Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Supernova-scope for the Direct Search of Supernova Axions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ex"],"primary_cat":"hep-ph","authors_text":"Jiaming Zheng, Koichi Hamaguchi, Koichi Ichimura, Koji Ishidoshiro, Natsumi Nagata, Shao-Feng Ge, Yasuhiro Kishimoto, Yoshiki Kanazawa","submitted_at":"2020-08-10T07:12:36Z","abstract_excerpt":"If a supernova explosion occurs within a few hundred parsecs from the Earth, a huge number of axions, in addition to neutrinos, may arrive at the Earth. In this paper, we discuss in detail the prospect of detecting those supernova axions by an axion helioscope. With the help of a pre-supernova neutrino alert system, it is possible to point a helioscope at an exploding supernova in advance. The supernova axions can then be detected by a gamma-ray detector installed at the end of the helioscope. We call such a detection system an axion supernova-scope (SNscope). We propose a conceptual design fo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2008.03924","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/2008.03924/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":"2008.03924","created_at":"2026-07-05T01:57:53.278934+00:00"},{"alias_kind":"arxiv_version","alias_value":"2008.03924v1","created_at":"2026-07-05T01:57:53.278934+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2008.03924","created_at":"2026-07-05T01:57:53.278934+00:00"},{"alias_kind":"pith_short_12","alias_value":"B3O7RHLJNNNN","created_at":"2026-07-05T01:57:53.278934+00:00"},{"alias_kind":"pith_short_16","alias_value":"B3O7RHLJNNNNS4TJ","created_at":"2026-07-05T01:57:53.278934+00:00"},{"alias_kind":"pith_short_8","alias_value":"B3O7RHLJ","created_at":"2026-07-05T01:57:53.278934+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2505.17007","citing_title":"Broadband Search for Axion Dark Matter via Shift Current","ref_index":56,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/B3O7RHLJNNNNS4TJDLSRW37B3K","json":"https://pith.science/pith/B3O7RHLJNNNNS4TJDLSRW37B3K.json","graph_json":"https://pith.science/api/pith-number/B3O7RHLJNNNNS4TJDLSRW37B3K/graph.json","events_json":"https://pith.science/api/pith-number/B3O7RHLJNNNNS4TJDLSRW37B3K/events.json","paper":"https://pith.science/paper/B3O7RHLJ"},"agent_actions":{"view_html":"https://pith.science/pith/B3O7RHLJNNNNS4TJDLSRW37B3K","download_json":"https://pith.science/pith/B3O7RHLJNNNNS4TJDLSRW37B3K.json","view_paper":"https://pith.science/paper/B3O7RHLJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2008.03924&json=true","fetch_graph":"https://pith.science/api/pith-number/B3O7RHLJNNNNS4TJDLSRW37B3K/graph.json","fetch_events":"https://pith.science/api/pith-number/B3O7RHLJNNNNS4TJDLSRW37B3K/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/B3O7RHLJNNNNS4TJDLSRW37B3K/action/timestamp_anchor","attest_storage":"https://pith.science/pith/B3O7RHLJNNNNS4TJDLSRW37B3K/action/storage_attestation","attest_author":"https://pith.science/pith/B3O7RHLJNNNNS4TJDLSRW37B3K/action/author_attestation","sign_citation":"https://pith.science/pith/B3O7RHLJNNNNS4TJDLSRW37B3K/action/citation_signature","submit_replication":"https://pith.science/pith/B3O7RHLJNNNNS4TJDLSRW37B3K/action/replication_record"}},"created_at":"2026-07-05T01:57:53.278934+00:00","updated_at":"2026-07-05T01:57:53.278934+00:00"}