{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:ZXU4LJHOCTZ25KYJMG6UBSPVD5","short_pith_number":"pith:ZXU4LJHO","schema_version":"1.0","canonical_sha256":"cde9c5a4ee14f3aeab0961bd40c9f51f41600800d0086af7f7861177e473aba0","source":{"kind":"arxiv","id":"2105.06476","version":2},"attestation_state":"computed","paper":{"title":"Supernova constraints on an axion-photon-dark photon interaction","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Anson Hook, Clayton Ristow, Gustavo Marques-Tavares","submitted_at":"2021-05-13T18:00:01Z","abstract_excerpt":"We present the supernova constraints on an axion-photon-dark photon coupling, which can be the leading coupling to dark sector models and can also lead to dramatic changes to axion cosmology. We show that the supernova bound on this coupling has two unusual features. One occurs because the scattering that leads to the trapping regime converts axions and dark photons into each other. Thus, if one of the two new particles is sufficiently massive, both production and scattering become suppressed and the bounds from bulk emission and trapped (area) emission both weaken exponentially and do not int"},"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":"2105.06476","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2021-05-13T18:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"35ac92180c466d8fc76a11a6979b80696e6d4c4a27b2d3afd30c490492c12261","abstract_canon_sha256":"f51247e0d051ef1ef9be633c761a214bf2cfe15c42e142b27017cbe2767dc26f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:57:20.989093Z","signature_b64":"ERxTpkZDUfs1J0T9hUNDj1gvpZ6Dhrl5gjZBgo+AYBqD1plueVW939ek8bPi8+ao6IklczU5ATrWXOGFWTABBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cde9c5a4ee14f3aeab0961bd40c9f51f41600800d0086af7f7861177e473aba0","last_reissued_at":"2026-07-05T02:57:20.988628Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:57:20.988628Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Supernova constraints on an axion-photon-dark photon interaction","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Anson Hook, Clayton Ristow, Gustavo Marques-Tavares","submitted_at":"2021-05-13T18:00:01Z","abstract_excerpt":"We present the supernova constraints on an axion-photon-dark photon coupling, which can be the leading coupling to dark sector models and can also lead to dramatic changes to axion cosmology. We show that the supernova bound on this coupling has two unusual features. One occurs because the scattering that leads to the trapping regime converts axions and dark photons into each other. Thus, if one of the two new particles is sufficiently massive, both production and scattering become suppressed and the bounds from bulk emission and trapped (area) emission both weaken exponentially and do not int"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2105.06476","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2105.06476/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":"2105.06476","created_at":"2026-07-05T02:57:20.988680+00:00"},{"alias_kind":"arxiv_version","alias_value":"2105.06476v2","created_at":"2026-07-05T02:57:20.988680+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2105.06476","created_at":"2026-07-05T02:57:20.988680+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZXU4LJHOCTZ2","created_at":"2026-07-05T02:57:20.988680+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZXU4LJHOCTZ25KYJ","created_at":"2026-07-05T02:57:20.988680+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZXU4LJHO","created_at":"2026-07-05T02:57:20.988680+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.23769","citing_title":"SN1987A Constraints of Light $\\boldsymbol{Z'}$ with Non-Mixing Polarisations","ref_index":18,"is_internal_anchor":false},{"citing_arxiv_id":"2606.01791","citing_title":"Probing the dark axion portal via $J/\\psi$ decays at BESIII and STCF","ref_index":35,"is_internal_anchor":false},{"citing_arxiv_id":"2604.28064","citing_title":"3D Reconstruction Techniques in the Manufacturing Domain: Applications, Research Opportunities and Use Cases","ref_index":32,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25090","citing_title":"Can LLP detectors probe the reheating temperature? A case study of vector dark matter","ref_index":19,"is_internal_anchor":false},{"citing_arxiv_id":"2605.08010","citing_title":"Producing the GeV Galactic Center Excess via Cosmic Ray-Dark Matter Scattering","ref_index":65,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZXU4LJHOCTZ25KYJMG6UBSPVD5","json":"https://pith.science/pith/ZXU4LJHOCTZ25KYJMG6UBSPVD5.json","graph_json":"https://pith.science/api/pith-number/ZXU4LJHOCTZ25KYJMG6UBSPVD5/graph.json","events_json":"https://pith.science/api/pith-number/ZXU4LJHOCTZ25KYJMG6UBSPVD5/events.json","paper":"https://pith.science/paper/ZXU4LJHO"},"agent_actions":{"view_html":"https://pith.science/pith/ZXU4LJHOCTZ25KYJMG6UBSPVD5","download_json":"https://pith.science/pith/ZXU4LJHOCTZ25KYJMG6UBSPVD5.json","view_paper":"https://pith.science/paper/ZXU4LJHO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2105.06476&json=true","fetch_graph":"https://pith.science/api/pith-number/ZXU4LJHOCTZ25KYJMG6UBSPVD5/graph.json","fetch_events":"https://pith.science/api/pith-number/ZXU4LJHOCTZ25KYJMG6UBSPVD5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZXU4LJHOCTZ25KYJMG6UBSPVD5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZXU4LJHOCTZ25KYJMG6UBSPVD5/action/storage_attestation","attest_author":"https://pith.science/pith/ZXU4LJHOCTZ25KYJMG6UBSPVD5/action/author_attestation","sign_citation":"https://pith.science/pith/ZXU4LJHOCTZ25KYJMG6UBSPVD5/action/citation_signature","submit_replication":"https://pith.science/pith/ZXU4LJHOCTZ25KYJMG6UBSPVD5/action/replication_record"}},"created_at":"2026-07-05T02:57:20.988680+00:00","updated_at":"2026-07-05T02:57:20.988680+00:00"}