{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:BHHQNT4IF2LO3HQ35JJMOSFMEQ","short_pith_number":"pith:BHHQNT4I","schema_version":"1.0","canonical_sha256":"09cf06cf882e96ed9e1bea52c748ac241e1683a070f95bb3483f9eee61b47574","source":{"kind":"arxiv","id":"1010.0029","version":1},"attestation_state":"computed","paper":{"title":"Study of solar and other unknown anti-neutrino fluxes with Borexino at LNGS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ex","authors_text":"Borexino collaboration, et al., G.Bellini","submitted_at":"2010-09-30T22:29:19Z","abstract_excerpt":"We report on the search for anti-neutrinos of yet unknown origin with the Borexino detector at the Laboratori Nazionali del Gran Sasso. In particular, a hypothetical anti-neutrino flux from the Sun is investigated. Anti-neutrinos are detected through the neutron inverse $\\beta$ decay reaction in a large liquid organic scintillator target. We set a new upper limit for a hypothetical solar $\\bar{\\nu}_e$ flux of 760 ${\\rm cm}^{-2}{\\rm s}^{-1}$, obtained assuming an undistorted solar $^8$B energy spectrum. This corresponds to a limit on the transition probability of solar neutrinos to anti-neutrin"},"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":"1010.0029","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ex","submitted_at":"2010-09-30T22:29:19Z","cross_cats_sorted":[],"title_canon_sha256":"9faea4b2f1e74c61eceb2635de6a6205867bf489d839e89f7aec4025932956cd","abstract_canon_sha256":"6fc9bdf405d7cb1903f21ce95365b2a3eecb6ad17130ff3a3895d138850a15f5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:31:32.171330Z","signature_b64":"RMK+vwxCOtIY5L2Sr3aYbdfgG2qO9+P1d0iACJ2P+zsHyIfW3SkZos+LWokqxS32hXId2R7LppcJPgkThO7zAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"09cf06cf882e96ed9e1bea52c748ac241e1683a070f95bb3483f9eee61b47574","last_reissued_at":"2026-05-18T04:31:32.170840Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:31:32.170840Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Study of solar and other unknown anti-neutrino fluxes with Borexino at LNGS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ex","authors_text":"Borexino collaboration, et al., G.Bellini","submitted_at":"2010-09-30T22:29:19Z","abstract_excerpt":"We report on the search for anti-neutrinos of yet unknown origin with the Borexino detector at the Laboratori Nazionali del Gran Sasso. In particular, a hypothetical anti-neutrino flux from the Sun is investigated. Anti-neutrinos are detected through the neutron inverse $\\beta$ decay reaction in a large liquid organic scintillator target. We set a new upper limit for a hypothetical solar $\\bar{\\nu}_e$ flux of 760 ${\\rm cm}^{-2}{\\rm s}^{-1}$, obtained assuming an undistorted solar $^8$B energy spectrum. This corresponds to a limit on the transition probability of solar neutrinos to anti-neutrin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1010.0029","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":"1010.0029","created_at":"2026-05-18T04:31:32.170915+00:00"},{"alias_kind":"arxiv_version","alias_value":"1010.0029v1","created_at":"2026-05-18T04:31:32.170915+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1010.0029","created_at":"2026-05-18T04:31:32.170915+00:00"},{"alias_kind":"pith_short_12","alias_value":"BHHQNT4IF2LO","created_at":"2026-05-18T12:26:05.355336+00:00"},{"alias_kind":"pith_short_16","alias_value":"BHHQNT4IF2LO3HQ3","created_at":"2026-05-18T12:26:05.355336+00:00"},{"alias_kind":"pith_short_8","alias_value":"BHHQNT4I","created_at":"2026-05-18T12:26:05.355336+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2506.23290","citing_title":"Type II Seesaw Leptogenesis in a Majoron background","ref_index":202,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BHHQNT4IF2LO3HQ35JJMOSFMEQ","json":"https://pith.science/pith/BHHQNT4IF2LO3HQ35JJMOSFMEQ.json","graph_json":"https://pith.science/api/pith-number/BHHQNT4IF2LO3HQ35JJMOSFMEQ/graph.json","events_json":"https://pith.science/api/pith-number/BHHQNT4IF2LO3HQ35JJMOSFMEQ/events.json","paper":"https://pith.science/paper/BHHQNT4I"},"agent_actions":{"view_html":"https://pith.science/pith/BHHQNT4IF2LO3HQ35JJMOSFMEQ","download_json":"https://pith.science/pith/BHHQNT4IF2LO3HQ35JJMOSFMEQ.json","view_paper":"https://pith.science/paper/BHHQNT4I","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1010.0029&json=true","fetch_graph":"https://pith.science/api/pith-number/BHHQNT4IF2LO3HQ35JJMOSFMEQ/graph.json","fetch_events":"https://pith.science/api/pith-number/BHHQNT4IF2LO3HQ35JJMOSFMEQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BHHQNT4IF2LO3HQ35JJMOSFMEQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BHHQNT4IF2LO3HQ35JJMOSFMEQ/action/storage_attestation","attest_author":"https://pith.science/pith/BHHQNT4IF2LO3HQ35JJMOSFMEQ/action/author_attestation","sign_citation":"https://pith.science/pith/BHHQNT4IF2LO3HQ35JJMOSFMEQ/action/citation_signature","submit_replication":"https://pith.science/pith/BHHQNT4IF2LO3HQ35JJMOSFMEQ/action/replication_record"}},"created_at":"2026-05-18T04:31:32.170915+00:00","updated_at":"2026-05-18T04:31:32.170915+00:00"}