<p>Neutrinos are the most abundant fundamental matter particles in the Universe and play a crucial part in particle physics and cosmology. Neutrino oscillation, discovered about 25 years ago, shows that the three known species mix with each other. Anomalous results from reactor and radioactive-source experiments<sup><CitationRef CitationID="CR1">1</CitationRef></sup> suggest a possible fourth neutrino state, the sterile neutrino, which does not interact through the weak force. The Karlsruhe Tritium Neutrino (KATRIN) experiment<sup><CitationRef CitationID="CR2">2</CitationRef></sup>, primarily designed to measure the neutrino mass using tritium β-decay, also searches for sterile neutrinos suggested by these anomalies. A sterile-neutrino signal would appear as a distortion in the β-decay energy spectrum, characterized by a discontinuity in curvature (kink) related to the sterile-neutrino mass. This signature, which depends only on the shape of the spectrum rather than its absolute normalization, offers a robust, complementary approach to reactor experiments. Here we report the analysis of the energy spectrum of 36 million tritium β-decay electrons recorded in 259 measurement days within the last 40 eV below the endpoint. The results exclude a substantial part of the parameter space suggested by the gallium anomaly and challenge the Neutrino-4 claim. Together with other neutrino-disappearance experiments, KATRIN probes sterile-to-active mass splittings from a fraction of an eV<sup>2</sup> to several hundred eV<sup>2</sup>, excluding light sterile neutrinos with mixing angles above a few per cent.</p>

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Sterile-neutrino search based on 259 days of KATRIN data

  • H. Acharya,
  • M. Aker,
  • D. Batzler,
  • A. Beglarian,
  • J. Beisenkötter,
  • M. Biassoni,
  • B. Bieringer,
  • Y. Biondi,
  • M. Böttcher,
  • B. Bornschein,
  • L. Bornschein,
  • M. Carminati,
  • A. Chatrabhuti,
  • S. Chilingaryan,
  • D. Díaz Barrero,
  • B. A. Daniel,
  • M. Descher,
  • O. Dragoun,
  • G. Drexlin,
  • F. Edzards,
  • K. Eitel,
  • E. Ellinger,
  • R. Engel,
  • S. Enomoto,
  • L. Fallböhmer,
  • A. Felden,
  • C. Fengler,
  • C. Fiorini,
  • J. A. Formaggio,
  • C. Forstner,
  • F. M. Fränkle,
  • G. Gagliardi,
  • K. Gauda,
  • A. S. Gavin,
  • W. Gil,
  • F. Glück,
  • R. Grössle,
  • T. Höhn,
  • K. Habib,
  • V. Hannen,
  • L. Haßelmann,
  • K. Helbing,
  • H. Henke,
  • S. Heyns,
  • R. Hiller,
  • D. Hillesheimer,
  • D. Hinz,
  • A. Jansen,
  • C. Köhler,
  • K. Khosonthongkee,
  • J. Kohpeiß,
  • L. Köllenberger,
  • A. Kopmann,
  • N. Kovač,
  • L. La Cascio,
  • L. Laschinger,
  • T. Lasserre,
  • J. Lauer,
  • T.-L. Le,
  • O. Lebeda,
  • B. Lehnert,
  • A. Lokhov,
  • M. Machatschek,
  • A. Marsteller,
  • E. L. Martin,
  • K. McMichael,
  • C. Melzer,
  • L. E. Mettler,
  • S. Mertens,
  • S. Mohanty,
  • J. Mostafa,
  • I. Müller,
  • A. Nava,
  • H. Neumann,
  • S. Niemes,
  • I. Nutini,
  • A. Onillon,
  • D. S. Parno,
  • M. Pavan,
  • U. Pinsook,
  • J. Plößner,
  • A. W. P. Poon,
  • J. M. L. Poyato,
  • F. Priester,
  • J. Ráliš,
  • M. Röllig,
  • S. Ramachandran,
  • R. G. H. Robertson,
  • C. Rodenbeck,
  • R. Sack,
  • A. Saenz,
  • R. Salomon,
  • J. Schürmann,
  • P. Schäfer,
  • A.-K. Schütz,
  • M. Schlösser,
  • L. Schlüter,
  • S. Schneidewind,
  • U. Schnurr,
  • A. Schwemmer,
  • A. Schwenck,
  • M. Šefčík,
  • J. Seeyangnok,
  • D. Siegmann,
  • F. Simon,
  • J. Songwadhana,
  • F. Spanier,
  • D. Spreng,
  • W. Sreethawong,
  • M. Steidl,
  • J. Štorek,
  • X. Stribl,
  • M. Sturm,
  • N. Suwonjandee,
  • N. T. Jerome,
  • H. H. H. Telle,
  • T. Thümmler,
  • L. A. Thorne,
  • N. Titov,
  • I. Tkachev,
  • K. Trost,
  • K. Urban,
  • D. Vénos,
  • K. Valerius,
  • S. Wüstling,
  • C. Weinheimer,
  • S. Welte,
  • J. Wendel,
  • C. Wiesinger,
  • J. F. Wilkerson,
  • J. Wolf,
  • J. Wydra,
  • W. Xu,
  • S. Zadorozhny,
  • G. Zeller

摘要

Neutrinos are the most abundant fundamental matter particles in the Universe and play a crucial part in particle physics and cosmology. Neutrino oscillation, discovered about 25 years ago, shows that the three known species mix with each other. Anomalous results from reactor and radioactive-source experiments1 suggest a possible fourth neutrino state, the sterile neutrino, which does not interact through the weak force. The Karlsruhe Tritium Neutrino (KATRIN) experiment2, primarily designed to measure the neutrino mass using tritium β-decay, also searches for sterile neutrinos suggested by these anomalies. A sterile-neutrino signal would appear as a distortion in the β-decay energy spectrum, characterized by a discontinuity in curvature (kink) related to the sterile-neutrino mass. This signature, which depends only on the shape of the spectrum rather than its absolute normalization, offers a robust, complementary approach to reactor experiments. Here we report the analysis of the energy spectrum of 36 million tritium β-decay electrons recorded in 259 measurement days within the last 40 eV below the endpoint. The results exclude a substantial part of the parameter space suggested by the gallium anomaly and challenge the Neutrino-4 claim. Together with other neutrino-disappearance experiments, KATRIN probes sterile-to-active mass splittings from a fraction of an eV2 to several hundred eV2, excluding light sterile neutrinos with mixing angles above a few per cent.