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KATRIN: Status and Prospects for the Neutrino Mass and Beyond

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arxiv 2203.08059 v3 pith:2P7I63YI submitted 2022-03-15 nucl-ex astro-ph.COhep-exphysics.ins-det

M. Aker , M. Balzer , D. Batzler , A. Beglarian , J. Behrens , A. Berlev , U. Besserer , M. Biassoni
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B. Bieringer F. Block S. Bobien L. Bombelli D. Bormann B. Bornschein L. Bornschein M. Böttcher C. Brofferio C. Bruch T. Brunst T. S. Caldwell M. 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. Hau{ss}mann 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 E. Weiss S. Welte J. Wendel C. Wiesinger J. F. Wilkerson J. Wolf L. Wunderl S. Wüstling J. Wydra W. Xu S. Zadoroghny G. Zeller
This is my paper · ORCID
classification nucl-exastro-ph.COhep-exphysics.ins-det
keywords katrinneutrinomasssensitivityexperimentfirstotherprospects
verification ladder T0 review T1 audit T2 compute T3 formal
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The Karlsruhe Tritium Neutrino (KATRIN) experiment is designed to measure a high-precision integral spectrum of the endpoint region of T2 beta 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.

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Cited by 4 Pith papers

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  1. Neutrino mass and leptogenesis in the non-SUSY modular $A^\prime_5$ inverse seesaw model

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  3. Thermal leptogenesis in minimal unified models

    hep-ph 2025-06 conditional novelty 4.0 of 10

    Thermal leptogenesis in minimal flipped SU(5) and SO(10) models tightly constrains their flavour parameters, yielding a lightest-neutrino mass below 0.03 eV and a B-L breaking scale near 10^12.5 GeV.

  4. Baryogenesis through leptogenesis in the minimal flipped $SU(5)$ with radiative seesaw

    hep-ph 2025-06 conditional novelty 2.0 of 10

    In the minimal flipped SU(5) model with radiative seesaw, successful thermal leptogenesis implies an upper limit on the lightest neutrino mass of about 3 x 10^-2 eV, testable at KATRIN.

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