{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:TX46O33YTA3WQJ6BFUKXMKF7HA","short_pith_number":"pith:TX46O33Y","schema_version":"1.0","canonical_sha256":"9df9e76f7898376827c12d157628bf3827ec308c0039535266db26a0a4689dba","source":{"kind":"arxiv","id":"1203.0969","version":1},"attestation_state":"computed","paper":{"title":"Neutrino Emission from Helium White Dwarfs with Condensed Cores","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"Aleksey Cherman, Evan Berkowitz, Paulo F. Bedaque","submitted_at":"2012-03-05T17:00:53Z","abstract_excerpt":"The possibility that ions in a helium white dwarf star are in a Bose-Einstein condensed state has been explored recently. In particular, it has been argued that the resulting novel quantum liquid has a new kind of quasiparticle excitation with a phonon-like dispersion relation. We investigate the neutrino emission rate due to this gapless state and the resulting impact on the total luminosity of helium white dwarf stars, as a possible observable way of detecting this exotic phase. If the condensation temperature for the quantum liquid state, which is currently not known very precisely, turns o"},"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":"1203.0969","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-03-05T17:00:53Z","cross_cats_sorted":["hep-ph","nucl-th"],"title_canon_sha256":"ef6cac76991e0c6d946db5b907eee890891547a99a7e8e742d9da9992e4561ea","abstract_canon_sha256":"51a092739b4fced6d9f8bafd35df7322b0ab1e0d28acd66c7770b811bc5fa6e9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:00:49.933886Z","signature_b64":"Fpya7ms4fJUqb5tc5xky6JiOsEdhruFw5PTVX2oCMtTuuqXUBbOq6i69pGSJPilnOCmEhQFq7UMp3ezv5IOtCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9df9e76f7898376827c12d157628bf3827ec308c0039535266db26a0a4689dba","last_reissued_at":"2026-05-18T04:00:49.933231Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:00:49.933231Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Neutrino Emission from Helium White Dwarfs with Condensed Cores","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"Aleksey Cherman, Evan Berkowitz, Paulo F. Bedaque","submitted_at":"2012-03-05T17:00:53Z","abstract_excerpt":"The possibility that ions in a helium white dwarf star are in a Bose-Einstein condensed state has been explored recently. In particular, it has been argued that the resulting novel quantum liquid has a new kind of quasiparticle excitation with a phonon-like dispersion relation. We investigate the neutrino emission rate due to this gapless state and the resulting impact on the total luminosity of helium white dwarf stars, as a possible observable way of detecting this exotic phase. If the condensation temperature for the quantum liquid state, which is currently not known very precisely, turns o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1203.0969","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":""},"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":"1203.0969","created_at":"2026-05-18T04:00:49.933335+00:00"},{"alias_kind":"arxiv_version","alias_value":"1203.0969v1","created_at":"2026-05-18T04:00:49.933335+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1203.0969","created_at":"2026-05-18T04:00:49.933335+00:00"},{"alias_kind":"pith_short_12","alias_value":"TX46O33YTA3W","created_at":"2026-05-18T12:27:23.164592+00:00"},{"alias_kind":"pith_short_16","alias_value":"TX46O33YTA3WQJ6B","created_at":"2026-05-18T12:27:23.164592+00:00"},{"alias_kind":"pith_short_8","alias_value":"TX46O33Y","created_at":"2026-05-18T12:27:23.164592+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TX46O33YTA3WQJ6BFUKXMKF7HA","json":"https://pith.science/pith/TX46O33YTA3WQJ6BFUKXMKF7HA.json","graph_json":"https://pith.science/api/pith-number/TX46O33YTA3WQJ6BFUKXMKF7HA/graph.json","events_json":"https://pith.science/api/pith-number/TX46O33YTA3WQJ6BFUKXMKF7HA/events.json","paper":"https://pith.science/paper/TX46O33Y"},"agent_actions":{"view_html":"https://pith.science/pith/TX46O33YTA3WQJ6BFUKXMKF7HA","download_json":"https://pith.science/pith/TX46O33YTA3WQJ6BFUKXMKF7HA.json","view_paper":"https://pith.science/paper/TX46O33Y","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1203.0969&json=true","fetch_graph":"https://pith.science/api/pith-number/TX46O33YTA3WQJ6BFUKXMKF7HA/graph.json","fetch_events":"https://pith.science/api/pith-number/TX46O33YTA3WQJ6BFUKXMKF7HA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TX46O33YTA3WQJ6BFUKXMKF7HA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TX46O33YTA3WQJ6BFUKXMKF7HA/action/storage_attestation","attest_author":"https://pith.science/pith/TX46O33YTA3WQJ6BFUKXMKF7HA/action/author_attestation","sign_citation":"https://pith.science/pith/TX46O33YTA3WQJ6BFUKXMKF7HA/action/citation_signature","submit_replication":"https://pith.science/pith/TX46O33YTA3WQJ6BFUKXMKF7HA/action/replication_record"}},"created_at":"2026-05-18T04:00:49.933335+00:00","updated_at":"2026-05-18T04:00:49.933335+00:00"}