{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:VYGGUSPU6FO775WSHTYLBOHCN4","short_pith_number":"pith:VYGGUSPU","schema_version":"1.0","canonical_sha256":"ae0c6a49f4f15dfff6d23cf0b0b8e26f19ae92e5e2d43b009077f35511c70922","source":{"kind":"arxiv","id":"1705.09455","version":2},"attestation_state":"computed","paper":{"title":"Fuzzy Dark Matter and Non-Standard Neutrino Interactions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ex"],"primary_cat":"hep-ph","authors_text":"Jia Liu, Joachim Kopp, Pascal Prass, Vedran Brdar, Xiao-Ping Wang (JGU Mainz)","submitted_at":"2017-05-26T07:04:23Z","abstract_excerpt":"We discuss novel ways in which neutrino oscillation experiments can probe dark matter. In particular, we focus on interactions between neutrinos and ultra-light (\"fuzzy\") dark matter particles with masses of order $10^{-22}$ eV. It has been shown previously that such dark matter candidates are phenomenologically successful and might help ameliorate the tension between predicted and observed small scale structures in the Universe. We argue that coherent forward scattering of neutrinos on fuzzy dark matter particles can significantly alter neutrino oscillation probabilities. These effects could "},"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":"1705.09455","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2017-05-26T07:04:23Z","cross_cats_sorted":["astro-ph.HE","hep-ex"],"title_canon_sha256":"b5aeafdcfce43aaee9087c4d332d91a511067dde0bad1e63d1d2ab7b8ddfc986","abstract_canon_sha256":"ca92cd7ccb9fcaf58562e7b65f7610b07723940e65b3176af16d4206aecdf259"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:24:35.351447Z","signature_b64":"BnzUeqkmPW63/SgKH/qKG1I+5Zsgtx3GapLi0i3N5hSX9cBXg9SL2Xy80ptQBbV8HbEwRm89n3hcX/u2jL7aBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ae0c6a49f4f15dfff6d23cf0b0b8e26f19ae92e5e2d43b009077f35511c70922","last_reissued_at":"2026-05-18T00:24:35.351021Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:24:35.351021Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fuzzy Dark Matter and Non-Standard Neutrino Interactions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ex"],"primary_cat":"hep-ph","authors_text":"Jia Liu, Joachim Kopp, Pascal Prass, Vedran Brdar, Xiao-Ping Wang (JGU Mainz)","submitted_at":"2017-05-26T07:04:23Z","abstract_excerpt":"We discuss novel ways in which neutrino oscillation experiments can probe dark matter. In particular, we focus on interactions between neutrinos and ultra-light (\"fuzzy\") dark matter particles with masses of order $10^{-22}$ eV. It has been shown previously that such dark matter candidates are phenomenologically successful and might help ameliorate the tension between predicted and observed small scale structures in the Universe. We argue that coherent forward scattering of neutrinos on fuzzy dark matter particles can significantly alter neutrino oscillation probabilities. These effects could "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.09455","kind":"arxiv","version":2},"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":"1705.09455","created_at":"2026-05-18T00:24:35.351089+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.09455v2","created_at":"2026-05-18T00:24:35.351089+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.09455","created_at":"2026-05-18T00:24:35.351089+00:00"},{"alias_kind":"pith_short_12","alias_value":"VYGGUSPU6FO7","created_at":"2026-05-18T12:31:49.984773+00:00"},{"alias_kind":"pith_short_16","alias_value":"VYGGUSPU6FO775WS","created_at":"2026-05-18T12:31:49.984773+00:00"},{"alias_kind":"pith_short_8","alias_value":"VYGGUSPU","created_at":"2026-05-18T12:31:49.984773+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.07176","citing_title":"Amplifying muon-to-positron conversion in nuclei with ultralight dark matter","ref_index":62,"is_internal_anchor":true},{"citing_arxiv_id":"2605.11071","citing_title":"Time-dependent signals of new physics at the LHC","ref_index":21,"is_internal_anchor":false},{"citing_arxiv_id":"2605.06777","citing_title":"Neutrino-Antineutrino Conversion from Ultralight Vector Dark Matter","ref_index":18,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VYGGUSPU6FO775WSHTYLBOHCN4","json":"https://pith.science/pith/VYGGUSPU6FO775WSHTYLBOHCN4.json","graph_json":"https://pith.science/api/pith-number/VYGGUSPU6FO775WSHTYLBOHCN4/graph.json","events_json":"https://pith.science/api/pith-number/VYGGUSPU6FO775WSHTYLBOHCN4/events.json","paper":"https://pith.science/paper/VYGGUSPU"},"agent_actions":{"view_html":"https://pith.science/pith/VYGGUSPU6FO775WSHTYLBOHCN4","download_json":"https://pith.science/pith/VYGGUSPU6FO775WSHTYLBOHCN4.json","view_paper":"https://pith.science/paper/VYGGUSPU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.09455&json=true","fetch_graph":"https://pith.science/api/pith-number/VYGGUSPU6FO775WSHTYLBOHCN4/graph.json","fetch_events":"https://pith.science/api/pith-number/VYGGUSPU6FO775WSHTYLBOHCN4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VYGGUSPU6FO775WSHTYLBOHCN4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VYGGUSPU6FO775WSHTYLBOHCN4/action/storage_attestation","attest_author":"https://pith.science/pith/VYGGUSPU6FO775WSHTYLBOHCN4/action/author_attestation","sign_citation":"https://pith.science/pith/VYGGUSPU6FO775WSHTYLBOHCN4/action/citation_signature","submit_replication":"https://pith.science/pith/VYGGUSPU6FO775WSHTYLBOHCN4/action/replication_record"}},"created_at":"2026-05-18T00:24:35.351089+00:00","updated_at":"2026-05-18T00:24:35.351089+00:00"}