{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:UOCOWUPK74OIK6TXL6ZYN7N6UG","short_pith_number":"pith:UOCOWUPK","schema_version":"1.0","canonical_sha256":"a384eb51eaff1c857a775fb386fdbea1932dbfa1b2a108d9fb686ed3b78169f7","source":{"kind":"arxiv","id":"1810.07153","version":1},"attestation_state":"computed","paper":{"title":"The time spectra in the neutron radiative decay experiment","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ins-det"],"primary_cat":"nucl-ex","authors_text":"G. M. Trifonov, I. A. Kolesnikov, I. V. Konorov, M. R. Kolkhidashvili, M. V. Nikolenko, R. U. Khafizov, S. A. Tarnovitsky, S. V. Tolokonnikov, V. A. Solovei, V. D. Torokhov","submitted_at":"2018-10-16T17:28:14Z","abstract_excerpt":"To measure the main characteristics of radiative neutron decay, namely its relative intensity BR (branching ratio), it is necessary to measure the spectra of double coincidences between beta-electron and proton as well as the spectra of triple coincidences of electron, proton and radiative gamma-quantum. Analysis of double coincidences spectra requires one to distinguish events of ordinary neutron beta decay from the background; analysis of triple coincidences relies on distinguishing radiative neutron decay from background events. As demonstrated in our first experiment, these spectra present"},"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":"1810.07153","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-ex","submitted_at":"2018-10-16T17:28:14Z","cross_cats_sorted":["physics.ins-det"],"title_canon_sha256":"f09c75dd55a108deda8b08cefcfc25c294755d8f2983547b86d05910fc002df0","abstract_canon_sha256":"7a44bf075c24f108b1e587a3b454fd7ba706d35ea9265ec3b696b64092ceb032"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:03:10.269739Z","signature_b64":"KL+sEsYpONI4MDenAIcPCxZezUKyKl3Fq7Ne+iD1FKC0ouwzlNWrnH5AhBDF9ffbFNqrJeE0ezUhG2fGYTkzBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a384eb51eaff1c857a775fb386fdbea1932dbfa1b2a108d9fb686ed3b78169f7","last_reissued_at":"2026-05-18T00:03:10.269036Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:03:10.269036Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The time spectra in the neutron radiative decay experiment","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ins-det"],"primary_cat":"nucl-ex","authors_text":"G. M. Trifonov, I. A. Kolesnikov, I. V. Konorov, M. R. Kolkhidashvili, M. V. Nikolenko, R. U. Khafizov, S. A. Tarnovitsky, S. V. Tolokonnikov, V. A. Solovei, V. D. Torokhov","submitted_at":"2018-10-16T17:28:14Z","abstract_excerpt":"To measure the main characteristics of radiative neutron decay, namely its relative intensity BR (branching ratio), it is necessary to measure the spectra of double coincidences between beta-electron and proton as well as the spectra of triple coincidences of electron, proton and radiative gamma-quantum. Analysis of double coincidences spectra requires one to distinguish events of ordinary neutron beta decay from the background; analysis of triple coincidences relies on distinguishing radiative neutron decay from background events. As demonstrated in our first experiment, these spectra present"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1810.07153","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":"1810.07153","created_at":"2026-05-18T00:03:10.269151+00:00"},{"alias_kind":"arxiv_version","alias_value":"1810.07153v1","created_at":"2026-05-18T00:03:10.269151+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1810.07153","created_at":"2026-05-18T00:03:10.269151+00:00"},{"alias_kind":"pith_short_12","alias_value":"UOCOWUPK74OI","created_at":"2026-05-18T12:32:56.356000+00:00"},{"alias_kind":"pith_short_16","alias_value":"UOCOWUPK74OIK6TX","created_at":"2026-05-18T12:32:56.356000+00:00"},{"alias_kind":"pith_short_8","alias_value":"UOCOWUPK","created_at":"2026-05-18T12:32:56.356000+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/UOCOWUPK74OIK6TXL6ZYN7N6UG","json":"https://pith.science/pith/UOCOWUPK74OIK6TXL6ZYN7N6UG.json","graph_json":"https://pith.science/api/pith-number/UOCOWUPK74OIK6TXL6ZYN7N6UG/graph.json","events_json":"https://pith.science/api/pith-number/UOCOWUPK74OIK6TXL6ZYN7N6UG/events.json","paper":"https://pith.science/paper/UOCOWUPK"},"agent_actions":{"view_html":"https://pith.science/pith/UOCOWUPK74OIK6TXL6ZYN7N6UG","download_json":"https://pith.science/pith/UOCOWUPK74OIK6TXL6ZYN7N6UG.json","view_paper":"https://pith.science/paper/UOCOWUPK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1810.07153&json=true","fetch_graph":"https://pith.science/api/pith-number/UOCOWUPK74OIK6TXL6ZYN7N6UG/graph.json","fetch_events":"https://pith.science/api/pith-number/UOCOWUPK74OIK6TXL6ZYN7N6UG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UOCOWUPK74OIK6TXL6ZYN7N6UG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UOCOWUPK74OIK6TXL6ZYN7N6UG/action/storage_attestation","attest_author":"https://pith.science/pith/UOCOWUPK74OIK6TXL6ZYN7N6UG/action/author_attestation","sign_citation":"https://pith.science/pith/UOCOWUPK74OIK6TXL6ZYN7N6UG/action/citation_signature","submit_replication":"https://pith.science/pith/UOCOWUPK74OIK6TXL6ZYN7N6UG/action/replication_record"}},"created_at":"2026-05-18T00:03:10.269151+00:00","updated_at":"2026-05-18T00:03:10.269151+00:00"}