{"record":{"author":{"account_ref":null,"orcid":null},"builds_on":[],"content_schema":"pubphys.content.topic/1","content_sha256":"05219168272fe3bd70c0d826cd5ce958d9ca0f2714491b28730d0db80e831aa3","created":"2026-10-03T07:17:52Z","files":[],"origin":{"assisted_by":[],"kind":"seed"},"parents":[],"salt":"23a1373450caaece0886045aa6e3726e9901921357d8763302b361ca2735cb49","schema":"pubphys.record/2","site":"pubphys.com","target":null,"type":"topic"},"content":{"external_id":"nuc.neutrino-nucleus","field":"nuc","n":"1","review_cite":"L. Alvarez-Ruso et al., NuSTEC White Paper: Status and challenges of neutrino-nucleus scattering, Progress in Particle and Nuclear Physics, 2018","review_link":"https://doi.org/10.1016/j.ppnp.2018.01.006","review_verified":"true","summary":"Experiments that measure how neutrinos change type detect them through collisions with nuclei, such as argon or the oxygen in water. To infer the neutrino energy and type from what comes out, they need a model of these collisions that is much better than current ones.","title":"Neutrino-nucleus interactions for oscillation experiments","topic_ref":null,"why":"Nuclear modelling errors are among the largest systematic uncertainties in the DUNE and Hyper-Kamiokande searches for matter-antimatter asymmetry in neutrinos."},"attested":{"attestation":{"batch":null,"client_id":null,"id_token_sha256":null,"kind":"platform"},"record_hash":"b26dbf879b3c8d9dff63a9d6b76e31cb28a6d3c51cf2e1a87d88d68d65a23459","schema":"pubphys.attested/1"},"envelope":{"attested_hash":"db8c7db10ef3d084da5c09696ab18dc6c5f55d546d4d0adaf0b5890ea7bacff1","platform_signature":{"key_id":"c6afc19b31429869751f06879c75cd64ea92654423d15b44be775bf1310a60da","sig":"UCzquoTg5OqhYqby85hiKTnvSMwkLUltb4ly3dqGvxIO-vnriAq1A7ARWTRZyjGKU2mcyQpTZ0MNzeA_sOEJDg"},"schema":"pubphys.envelope/1"},"record_hash":"b26dbf879b3c8d9dff63a9d6b76e31cb28a6d3c51cf2e1a87d88d68d65a23459","leaf_index":288}