{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:T5AAMSR653ULSDWMY4PVXVTB4M","short_pith_number":"pith:T5AAMSR6","schema_version":"1.0","canonical_sha256":"9f40064a3eeee8b90eccc71f5bd661e3213d79a209fdcbfa610a53820c7d7445","source":{"kind":"arxiv","id":"2306.01048","version":2},"attestation_state":"computed","paper":{"title":"Getting the most on supernova axions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Alessandro Lella, Alessandro Mirizzi, Giampaolo Co', Giuseppe Lucente, Maurizio Giannotti, Pierluca Carenza, Thomas Rauscher","submitted_at":"2023-06-01T18:00:05Z","abstract_excerpt":"Axion-like particles (ALPs) coupled to nucleons might be copiously emitted from a supernova (SN) core. We extend existing bounds on free-streaming ALPs to the case in which these are so strongly-interacting with the nuclear matter to be trapped in the SN core. For strongly-interacting ALPs, we also extend the bound from the absence of an ALP-induced signal in Kamiokande-II neutrino detector at the time of SN 1987A. We find that combining the different arguments, SNe exclude values of ALP-nucleon coupling $g_{aN}\\gtrsim10^{-9}$ for ALP masses $m_a\\lesssim 1\\,\\mathrm{MeV}$. Remarkably, in the ca"},"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":"2306.01048","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2023-06-01T18:00:05Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"4f441700bd4baebd92d31cc73f1eacd8767a9317407f32f6aecdc87453faabba","abstract_canon_sha256":"c90d607c4afa46d6d47b867991bd5e3e19a565b0f2e13aed2b325bbc74aeb889"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:29:38.836173Z","signature_b64":"Xnb9urk+q9YhSnDo+0+91Una+zcsJfc9GR/gyMeSbLcFPBaW+/C2a2goEIUATZYJtwGR4psWSN9HpKVvanbGBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9f40064a3eeee8b90eccc71f5bd661e3213d79a209fdcbfa610a53820c7d7445","last_reissued_at":"2026-07-05T07:29:38.835739Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:29:38.835739Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Getting the most on supernova axions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Alessandro Lella, Alessandro Mirizzi, Giampaolo Co', Giuseppe Lucente, Maurizio Giannotti, Pierluca Carenza, Thomas Rauscher","submitted_at":"2023-06-01T18:00:05Z","abstract_excerpt":"Axion-like particles (ALPs) coupled to nucleons might be copiously emitted from a supernova (SN) core. We extend existing bounds on free-streaming ALPs to the case in which these are so strongly-interacting with the nuclear matter to be trapped in the SN core. For strongly-interacting ALPs, we also extend the bound from the absence of an ALP-induced signal in Kamiokande-II neutrino detector at the time of SN 1987A. We find that combining the different arguments, SNe exclude values of ALP-nucleon coupling $g_{aN}\\gtrsim10^{-9}$ for ALP masses $m_a\\lesssim 1\\,\\mathrm{MeV}$. Remarkably, in the ca"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2306.01048","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/2306.01048/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":"2306.01048","created_at":"2026-07-05T07:29:38.835793+00:00"},{"alias_kind":"arxiv_version","alias_value":"2306.01048v2","created_at":"2026-07-05T07:29:38.835793+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2306.01048","created_at":"2026-07-05T07:29:38.835793+00:00"},{"alias_kind":"pith_short_12","alias_value":"T5AAMSR653UL","created_at":"2026-07-05T07:29:38.835793+00:00"},{"alias_kind":"pith_short_16","alias_value":"T5AAMSR653ULSDWM","created_at":"2026-07-05T07:29:38.835793+00:00"},{"alias_kind":"pith_short_8","alias_value":"T5AAMSR6","created_at":"2026-07-05T07:29:38.835793+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":11,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.20826","citing_title":"Counting axions with IAXO","ref_index":62,"is_internal_anchor":false},{"citing_arxiv_id":"2606.12298","citing_title":"The KSVZ Atlas: A Unified SMEFT-ALP Framework","ref_index":77,"is_internal_anchor":false},{"citing_arxiv_id":"2503.15630","citing_title":"Supernova production of axion-like particles coupling to electrons, reloaded","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2509.13322","citing_title":"Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities","ref_index":47,"is_internal_anchor":false},{"citing_arxiv_id":"2511.13815","citing_title":"Stripped-Envelope Supernovae for QCD Axion Detection","ref_index":17,"is_internal_anchor":false},{"citing_arxiv_id":"2512.13816","citing_title":"Stellar Superradiance and Low-Energy Absorption in Dense Nuclear Media","ref_index":20,"is_internal_anchor":false},{"citing_arxiv_id":"2512.20825","citing_title":"Irreducible Constraints on Hadronically Interacting Sub-GeV Dark Matter","ref_index":51,"is_internal_anchor":false},{"citing_arxiv_id":"2604.01277","citing_title":"Lights, Camera, Axion: Tracing Axions from Supernovae in the Diffuse $\\gamma$-ray Sky","ref_index":33,"is_internal_anchor":false},{"citing_arxiv_id":"2604.28062","citing_title":"Semi-analytic bounds on axion-like-particle supernovae emission","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2604.18397","citing_title":"Looking for Lights from the Darkness: Signals from MeV-scale Solar Axion-like Particles","ref_index":39,"is_internal_anchor":false},{"citing_arxiv_id":"2604.17840","citing_title":"Rotation-induced Relaxation of Supernova Constraints on Axionlike Particles","ref_index":26,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/T5AAMSR653ULSDWMY4PVXVTB4M","json":"https://pith.science/pith/T5AAMSR653ULSDWMY4PVXVTB4M.json","graph_json":"https://pith.science/api/pith-number/T5AAMSR653ULSDWMY4PVXVTB4M/graph.json","events_json":"https://pith.science/api/pith-number/T5AAMSR653ULSDWMY4PVXVTB4M/events.json","paper":"https://pith.science/paper/T5AAMSR6"},"agent_actions":{"view_html":"https://pith.science/pith/T5AAMSR653ULSDWMY4PVXVTB4M","download_json":"https://pith.science/pith/T5AAMSR653ULSDWMY4PVXVTB4M.json","view_paper":"https://pith.science/paper/T5AAMSR6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2306.01048&json=true","fetch_graph":"https://pith.science/api/pith-number/T5AAMSR653ULSDWMY4PVXVTB4M/graph.json","fetch_events":"https://pith.science/api/pith-number/T5AAMSR653ULSDWMY4PVXVTB4M/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/T5AAMSR653ULSDWMY4PVXVTB4M/action/timestamp_anchor","attest_storage":"https://pith.science/pith/T5AAMSR653ULSDWMY4PVXVTB4M/action/storage_attestation","attest_author":"https://pith.science/pith/T5AAMSR653ULSDWMY4PVXVTB4M/action/author_attestation","sign_citation":"https://pith.science/pith/T5AAMSR653ULSDWMY4PVXVTB4M/action/citation_signature","submit_replication":"https://pith.science/pith/T5AAMSR653ULSDWMY4PVXVTB4M/action/replication_record"}},"created_at":"2026-07-05T07:29:38.835793+00:00","updated_at":"2026-07-05T07:29:38.835793+00:00"}