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Methods: We calculate the neutrino flux from $\\beta$ processes using nuclear statistical equilibrium abundances convoluted with approximate neutrino spectra of the individual nuclei and the thermal neutrino spectrum (pair+plasma). Results: Although the two considered thermonuclear supernova explosion scenarios are expected to produce almost identical electromagnetic output, their neutrino signatures appear vastly different, which all"},"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":"1006.0490","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-06-02T20:07:15Z","cross_cats_sorted":["hep-ex","hep-ph","nucl-ex","nucl-th"],"title_canon_sha256":"5e8a3bbb100010f1e3c5264557fa37178033b3a32f5ff139247281c18d28a921","abstract_canon_sha256":"32b0bde20fa4f40ced5056fabc500daf890d574c94f404a5f9570f296e38c0cc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:25:39.161844Z","signature_b64":"HWJHlc90WZ9LzTTYgqlaSffSRJ2NieHSZ9n9jZhqxPj5jHmfaEU+5RzZdLHjX9iU1Gd1Z2wqy+beMAh0SZMiDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0d9149b932dbd272c4dbb4142d521f99dced0d0243f7cca0c7b8a864fd1792c9","last_reissued_at":"2026-05-18T04:25:39.161311Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:25:39.161311Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Probing thermonuclear supernova explosions with neutrinos","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex","hep-ph","nucl-ex","nucl-th"],"primary_cat":"astro-ph.SR","authors_text":"A. 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