4.8 Article

Direct neutrino-mass measurement with sub-electronvolt sensitivity

期刊

NATURE PHYSICS
卷 18, 期 2, 页码 160-+

出版社

NATURE PORTFOLIO
DOI: 10.1038/s41567-021-01463-1

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资金

  1. Helmholtz Association (HGF)
  2. Ministry for Education and Research BMBF [05A17PM3, 05A17PX3, 05A17VK2, 05A17PDA, 05A17WO3, 05A20VK3, 05A20PMA, 05A20PX3]
  3. Helmholtz Alliance for Astroparticle Physics (HAP)
  4. doctoral school KSETA at KIT
  5. Max Planck Research Group [VH-NG-1055]
  6. Max Planck Research Group (MaxPlanck@TUM)
  7. Deutsche Forschungsgemeinschaft DFG [GRK 1694, GRK 2149]
  8. Graduate School in Germany [GSC 1085-KSETA, SFB-1258]
  9. Ministry of Education, Youth and Sport in the Czech Republic [CANAM-LM2015056, LTT19005]
  10. Ministry of Science and Higher Education of the Russian Federation [075-15-2020-778]
  11. Department of Energy [DE-FG02-97ER41020, DE-FG02-94ER40818, DE-SC0004036, DE-FG02-97ER41033, DE-FG02-97ER41041, DE-SC0011091, DE-SC0019304]
  12. Federal Prime Agreement in the USA [DE-AC0205CH11231]
  13. European Research Council (ERC) under the European Union Horizon 2020 research and innovation programme [852845]
  14. U.S. Department of Energy (DOE) [DE-SC0004036, DE-SC0011091, DE-SC0019304] Funding Source: U.S. Department of Energy (DOE)

向作者/读者索取更多资源

This article reports on the upper limits of the effective electron anti-neutrino mass from the second physics run of the Karlsruhe Tritium Neutrino experiment. Using a high-precision measurement of the tritium beta-decay spectrum, independent of cosmological models and particle assumptions, the sensitivity and upper limit of the neutrino mass were determined.
Since the discovery of neutrino oscillations, we know that neutrinos have non-zero mass. However, the absolute neutrino-mass scale remains unknown. Here we report the upper limits on effective electron anti-neutrino mass, m(nu), from the second physics run of the Karlsruhe Tritium Neutrino experiment. In this experiment, m(nu) is probed via a high-precision measurement of the tritium beta-decay spectrum close to its endpoint. This method is independent of any cosmological model and does not rely on assumptions whether the neutrino is a Dirac or Majorana particle. By increasing the source activity and reducing the background with respect to the first physics campaign, we reached a sensitivity on m(nu) of 0.7 eV c(-2) at a 90% confidence level (CL). The best fit to the spectral data yields m(nu)(2) = (0.26 +/- 0.34) eV(2) c(-4), resulting in an upper limit of m(nu) < 0.9 eV c(-2) at 90% CL. By combining this result with the first neutrino-mass campaign, we find an upper limit of m(nu) < 0.8 eV c(-2) at 90% CL.

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