{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:KVZCVRLVOMFBRLH4J6SKBJWELZ","short_pith_number":"pith:KVZCVRLV","canonical_record":{"source":{"id":"1604.01025","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2016-04-04T20:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"4f3a7986591ae696d174bb4eba7b924edd2d5ae0169566608db8d68cf49bf278","abstract_canon_sha256":"1637f83bd9d54a2ae318c87e3fcb0ada2caf7802338d8cdbcb38d6f6d78f6e7b"},"schema_version":"1.0"},"canonical_sha256":"55722ac575730a18acfc4fa4a0a6c45e63db3c223db74fe65414acc9cc8aa389","source":{"kind":"arxiv","id":"1604.01025","version":3},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1604.01025","created_at":"2026-05-18T01:11:12Z"},{"alias_kind":"arxiv_version","alias_value":"1604.01025v3","created_at":"2026-05-18T01:11:12Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1604.01025","created_at":"2026-05-18T01:11:12Z"},{"alias_kind":"pith_short_12","alias_value":"KVZCVRLVOMFB","created_at":"2026-05-18T12:30:29Z"},{"alias_kind":"pith_short_16","alias_value":"KVZCVRLVOMFBRLH4","created_at":"2026-05-18T12:30:29Z"},{"alias_kind":"pith_short_8","alias_value":"KVZCVRLV","created_at":"2026-05-18T12:30:29Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:KVZCVRLVOMFBRLH4J6SKBJWELZ","target":"record","payload":{"canonical_record":{"source":{"id":"1604.01025","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2016-04-04T20:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"4f3a7986591ae696d174bb4eba7b924edd2d5ae0169566608db8d68cf49bf278","abstract_canon_sha256":"1637f83bd9d54a2ae318c87e3fcb0ada2caf7802338d8cdbcb38d6f6d78f6e7b"},"schema_version":"1.0"},"canonical_sha256":"55722ac575730a18acfc4fa4a0a6c45e63db3c223db74fe65414acc9cc8aa389","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:11:12.266330Z","signature_b64":"QvIdws0Ozs4Y19VInkZKIowRmRbieaBcLORbpEZYDFysspM3VLsFuansb/B9ov4KXgh5aHFmrqEnvZBW7VA5BA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"55722ac575730a18acfc4fa4a0a6c45e63db3c223db74fe65414acc9cc8aa389","last_reissued_at":"2026-05-18T01:11:12.265858Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:11:12.265858Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1604.01025","source_version":3,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:11:12Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"u2zzOWE0IugIrw28vDVXD9fhpccSuhvdP40ADgxhg9e/Cu6Bj/GZcaKoLNasfB0+biZC0RHlw/doc1U3O2y2DQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-24T05:05:35.194415Z"},"content_sha256":"17d0f79d330a07f6f49d205b640eb40d374593a17e3e65ac47764008f927e451","schema_version":"1.0","event_id":"sha256:17d0f79d330a07f6f49d205b640eb40d374593a17e3e65ac47764008f927e451"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:KVZCVRLVOMFBRLH4J6SKBJWELZ","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Physics from solar neutrinos in dark matter direct detection experiments","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Aaron C. Vincent (IPPP, Annecy, Autonoma U.), Celine Boehm (IPPP, David G. Cerdeno (IPPP, Durham U., Durham U.), IFT, LAPTH), Madrid, Malcolm Fairbairn (King's Coll. London), Pedro A. N. Machado (Madrid, Thomas Jubb (IPPP","submitted_at":"2016-04-04T20:00:01Z","abstract_excerpt":"The next generation of dark matter direct detection experiments will be sensitive to both coherent neutrino-nucleus and neutrino-electron scattering. This will enable them to explore aspects of solar physics, perform the lowest energy measurement of the weak angle to date, and probe contributions from new theories with light mediators. In this article, we compute the projected nuclear and electron recoil rates expected in several dark matter direct detection experiments due to solar neutrinos, and use these estimates to quantify errors on future measurements of the neutrino fluxes, weak mixing"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1604.01025","kind":"arxiv","version":3},"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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:11:12Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"KoERl9Rwaf04PETT6gmcmxp8V1Z++qakc4cd4Zs7RtbO9r5jM+Pq+nTaUCOJJ+84FeHVaQTBXSB8Ae7dvNVkAA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-24T05:05:35.195072Z"},"content_sha256":"e2e8540658c759ef745562d99c24a40111b864eeca447eeedb529cbf534651d1","schema_version":"1.0","event_id":"sha256:e2e8540658c759ef745562d99c24a40111b864eeca447eeedb529cbf534651d1"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/KVZCVRLVOMFBRLH4J6SKBJWELZ/bundle.json","state_url":"https://pith.science/pith/KVZCVRLVOMFBRLH4J6SKBJWELZ/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/KVZCVRLVOMFBRLH4J6SKBJWELZ/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-24T05:05:35Z","links":{"resolver":"https://pith.science/pith/KVZCVRLVOMFBRLH4J6SKBJWELZ","bundle":"https://pith.science/pith/KVZCVRLVOMFBRLH4J6SKBJWELZ/bundle.json","state":"https://pith.science/pith/KVZCVRLVOMFBRLH4J6SKBJWELZ/state.json","well_known_bundle":"https://pith.science/.well-known/pith/KVZCVRLVOMFBRLH4J6SKBJWELZ/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:KVZCVRLVOMFBRLH4J6SKBJWELZ","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"1637f83bd9d54a2ae318c87e3fcb0ada2caf7802338d8cdbcb38d6f6d78f6e7b","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2016-04-04T20:00:01Z","title_canon_sha256":"4f3a7986591ae696d174bb4eba7b924edd2d5ae0169566608db8d68cf49bf278"},"schema_version":"1.0","source":{"id":"1604.01025","kind":"arxiv","version":3}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1604.01025","created_at":"2026-05-18T01:11:12Z"},{"alias_kind":"arxiv_version","alias_value":"1604.01025v3","created_at":"2026-05-18T01:11:12Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1604.01025","created_at":"2026-05-18T01:11:12Z"},{"alias_kind":"pith_short_12","alias_value":"KVZCVRLVOMFB","created_at":"2026-05-18T12:30:29Z"},{"alias_kind":"pith_short_16","alias_value":"KVZCVRLVOMFBRLH4","created_at":"2026-05-18T12:30:29Z"},{"alias_kind":"pith_short_8","alias_value":"KVZCVRLV","created_at":"2026-05-18T12:30:29Z"}],"graph_snapshots":[{"event_id":"sha256:e2e8540658c759ef745562d99c24a40111b864eeca447eeedb529cbf534651d1","target":"graph","created_at":"2026-05-18T01:11:12Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"The next generation of dark matter direct detection experiments will be sensitive to both coherent neutrino-nucleus and neutrino-electron scattering. This will enable them to explore aspects of solar physics, perform the lowest energy measurement of the weak angle to date, and probe contributions from new theories with light mediators. In this article, we compute the projected nuclear and electron recoil rates expected in several dark matter direct detection experiments due to solar neutrinos, and use these estimates to quantify errors on future measurements of the neutrino fluxes, weak mixing","authors_text":"Aaron C. Vincent (IPPP, Annecy, Autonoma U.), Celine Boehm (IPPP, David G. Cerdeno (IPPP, Durham U., Durham U.), IFT, LAPTH), Madrid, Malcolm Fairbairn (King's Coll. London), Pedro A. N. Machado (Madrid, Thomas Jubb (IPPP","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2016-04-04T20:00:01Z","title":"Physics from solar neutrinos in dark matter direct detection experiments"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1604.01025","kind":"arxiv","version":3},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:17d0f79d330a07f6f49d205b640eb40d374593a17e3e65ac47764008f927e451","target":"record","created_at":"2026-05-18T01:11:12Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"1637f83bd9d54a2ae318c87e3fcb0ada2caf7802338d8cdbcb38d6f6d78f6e7b","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2016-04-04T20:00:01Z","title_canon_sha256":"4f3a7986591ae696d174bb4eba7b924edd2d5ae0169566608db8d68cf49bf278"},"schema_version":"1.0","source":{"id":"1604.01025","kind":"arxiv","version":3}},"canonical_sha256":"55722ac575730a18acfc4fa4a0a6c45e63db3c223db74fe65414acc9cc8aa389","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"55722ac575730a18acfc4fa4a0a6c45e63db3c223db74fe65414acc9cc8aa389","first_computed_at":"2026-05-18T01:11:12.265858Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:11:12.265858Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"QvIdws0Ozs4Y19VInkZKIowRmRbieaBcLORbpEZYDFysspM3VLsFuansb/B9ov4KXgh5aHFmrqEnvZBW7VA5BA==","signature_status":"signed_v1","signed_at":"2026-05-18T01:11:12.266330Z","signed_message":"canonical_sha256_bytes"},"source_id":"1604.01025","source_kind":"arxiv","source_version":3}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:17d0f79d330a07f6f49d205b640eb40d374593a17e3e65ac47764008f927e451","sha256:e2e8540658c759ef745562d99c24a40111b864eeca447eeedb529cbf534651d1"],"state_sha256":"6eae7fa11147fe90e1359ad617f7c2bb89dacf773d1def39495944803bbd8106"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"SQmtPab3n8Wy7VyE+jirBAg2oDSIrLjIDDG6V6K7ZIY9oWdZarkbwEUtY/i1I7MWb34JPugcKseQgkAMbVcLBw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-24T05:05:35.198917Z","bundle_sha256":"a8a328fb9f3e0748a0a67fba6e343bf6f76a54af24042b6006023bd1a0482400"}}