KATRIN: status and prospects for the neutrino mass and beyond

M. Aker, M. Balzer, D. Batzler, A. Beglarian, J. Behrens, A. Berlev, U. Besserer, M. Biassoni, B. Bieringer, F. Block, S. Bobien, L. Bombelli, D. Bormann, B. Bornschein, L. Bornschein, M. Böttcher, C. Brofferio, C. Bruch, T. Brunst, T. S. CaldwellM. Carminati, R. M.D. Carney, S. Chilingaryan, W. Choi, O. Cremonesi, K. Debowski, M. Descher, D. Díaz Barrero, P. J. Doe, O. Dragoun, G. Drexlin, F. Edzards, K. Eitel, E. Ellinger, R. Engel, S. Enomoto, A. Felden, D. Fink, C. Fiorini, J. A. Formaggio, C. Forstner, F. M. Fränkle, G. B. Franklin, F. Friedel, A. Fulst, K. Gauda, A. S. Gavin, W. Gil, F. Glück, A. Grande, R. Grössle, M. Gugiatti, R. Gumbsheimer, V. Hannen, J. Hartmann, N. Haußmann, K. Helbing, S. Hickford, R. Hiller, D. Hillesheimer, D. Hinz, T. Höhn, T. Houdy, A. Huber, A. Jansen, C. Karl, J. Kellerer, P. King, M. Kleifges, M. Klein, C. Köhler, L. Köllenberger, A. Kopmann, M. Korzeczek, A. Kovalík, B. Krasch, H. Krause, T. Lasserre, L. La Cascio, O. Lebeda, P. Lechner, B. Lehnert, T. L. Le, A. Lokhov, M. Machatschek, E. Malcherek, D. Manfrin, M. Mark, A. Marsteller, E. L. Martin, E. Mazzola, C. Melzer, S. Mertens, J. Mostafa, K. Müller, A. Nava, H. Neumann, S. Niemes, P. Oelpmann, A. Onillon, D. S. Parno, M. Pavan, A. Pigliafreddo, A. W.P. Poon, J. M.L. Poyato, S. Pozzi, F. Priester, M. Puritscher, D. C. Radford, J. Ráliš, S. Ramachandran, R. G.H. Robertson, W. Rodejohann, C. Rodenbeck, M. Röllig, C. Röttele, M. Ryšavý, R. Sack, A. Saenz, R. W.J. Salomon, P. Schäfer, L. Schimpf, K. Schlösser, M. Schlösser, L. Schlüter, S. Schneidewind, M. Schrank, A. K. Schütz, A. Schwemmer, A. Sedlak, M. Šefčík, V. Sibille, D. Siegmann, M. Slezák, F. Spanier, D. Spreng, M. Steidl, M. Sturm, H. H. Telle, L. A. Thorne, T. Thümmler, N. Titov, I. Tkachev, P. Trigilio, K. Urban, K. Valerius, D. Vénos, A. P. Vizcaya Hernández, P. Voigt, C. Weinheimer, S. Welte, J. Wendel, C. Wiesinger, J. F. Wilkerson, J. Wolf, L. Wunderl, S. Wüstling, J. Wydra, W. Xu, S. Zadoroghny, G. Zeller

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Abstract

The Karlsruhe Tritium Neutrino (KATRIN) experiment is designed to measure a high-precision integral spectrum of the endpoint region of T2 β decay, with the primary goal of probing the absolute mass scale of the neutrino. After a first tritium commissioning campaign in 2018, the experiment has been regularly running since 2019, and in its first two measurement campaigns has already achieved a sub-eV sensitivity. After 1000 days of data-taking, KATRIN’s design sensitivity is 0.2 eV at the 90% confidence level. In this white paper we describe the current status of KATRIN; explore prospects for measuring the neutrino mass and other physics observables, including sterile neutrinos and other beyond-Standard-Model hypotheses; and discuss research-and-development projects that may further improve the KATRIN sensitivity.

Original languageEnglish
Article number100501
JournalJournal of Physics G: Nuclear and Particle Physics
Volume49
Issue number10
DOIs
StatePublished - Oct 2022

Funding

We acknowledge the support of Helmholtz Association (HGF), Ministry for Education and Research BMBF (05A20PMA, 05A20PX3, 05A20VK3), Helmholtz Alliance for Astroparticle Physics (HAP), the doctoral school KSETA at KIT, and Helmholtz Young Investigator Group (VH-NG-1055), Max Planck Research Group (MaxPlanck@TUM), and Deutsche Forschungsgemeinschaft DFG (Research Training Groups Grant Nos. GRK 1694 and GRK 2149, Graduate School Grant Nos. GSC 1085-KSETA, and SFB-1258) in Germany; Ministry of Education, Youth and Sport (CANAM-LM2015056, LTT19005) in the Czech Republic; and the Department of Energy through Grants DE-FG02-97ER41020, DE-FG02-94ER40818, DE-SC0004036, DE-FG02-97ER41033, DE-FG02-97ER41041, DE-SC0011091 and DE-SC0019304 and the Federal Prime Agreement DE-AC02-05CH11231 in the United States. This project has received funding from the European Research Council (ERC) under the European Union Horizon 2020 research and innovation programme (Grant Agreement No. 852845). The development of the TRISTAN detector has received funding from Istituto Nazionale di Fisica Nucleare (Italy) CSN2. We thank the computing cluster support at the Institute for Astroparticle Physics at Karlsruhe Institute of Technology, Max Planck Computing and Data Facility (MPCDF), and National Energy Research Scientific Computing Center (NERSC) at Lawrence Berkeley National Laboratory. We acknowledge the support of Helmholtz Association (HGF), Ministry for Education and Research BMBF (05A20PMA, 05A20PX3, 05A20VK3), Helmholtz Alliance for Astroparticle Physics (HAP), the doctoral school KSETA at KIT, and Helmholtz Young Investigator Group (VH-NG-1055), Max Planck Research Group (MaxPlanck@TUM), and Deutsche Forschungsgemeinschaft DFG (Research Training Groups Grant Nos. GRK 1694 and GRK 2149, Graduate School Grant Nos. GSC 1085-KSETA, and SFB-1258) in Germany; Ministry of Education, Youth and Sport (CANAM-LM2015056, LTT19005) in the Czech Republic; and the Department of Energy through Grants DE-FG02-97ER41020, DE-FG02-94ER40818, DE-SC0004036, DE-FG02-97ER41033, DE-FG02-97ER41041, DE-SC0011091 and DE-SC0019304 and the Federal Prime Agreement DE-AC02-05CH11231 in the United States. This project has received funding from the European Research Council (ERC) under the European Union Horizon 2020 research and innovation programme (Grant Agreement No. 852845). The development of the TRISTAN detector has received funding from Istituto Nazionale di Fisica Nucleare (Italy) CSN2. We thank the computing cluster support at the Institute for Astroparticle Physics at Karlsruhe Institute of Technology, Max Planck Computing and Data Facility (MPCDF), and National Energy Research Scientific Computing Center (NERSC) at Lawrence Berkeley National Laboratory.

Keywords

  • beyond standard model
  • krypton
  • neutrino
  • neutrino mass
  • sterile neutrino
  • tritium beta decay

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