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The upcoming Karlsruhe Tritium Neutrino (KATRIN) experiment will put unprecedented constraints on the absolute mass of the electron neutrino, $\mnue$. In this paper we investigate how this information on $\mnue$ will affect our constraints…

Astrophysics · Physics 2010-12-09 Jostein R. Kristiansen , Oystein Elgaroy

Recently announced results from the KATRIN collaboration imply an upper bound on the effective electron anti-neutrino mass $m_{\nu_{e}}$, $m_{\nu_{e}}< 0.8~{\rm eV}/c^{2}$. Here we explore the implications of combining the KATRIN upper…

High Energy Physics - Phenomenology · Physics 2022-08-09 Ephraim Fischbach , Dennis E. Krause , Quan Le Thien , Carol Scarlett

With the compelling evidence for massive neutrinos from recent neutrino-oscillation experiments, one of the most fundamental tasks of particle physics over the next years will be the determination of the absolute mass scale of neutrinos.…

High Energy Physics - Experiment · Physics 2012-08-27 KATRIN collaboration

We reconstruct the neutrino mass as a function of redshift, z, from current cosmological data using both standard binned priors and linear spline priors with variable knots. Using cosmic microwave background temperature, polarization and…

Cosmology and Nongalactic Astrophysics · Physics 2021-12-22 Christiane S. Lorenz , Lena Funcke , Matthias Löffler , Erminia Calabrese

We present a short discussion of the Neutrino-4 experimental results and the results of other experiments searching for the sterile neutrino. We estimated the contribution of the sterile neutrino with parameters $\Delta m^2_{14} =…

High Energy Physics - Phenomenology · Physics 2023-02-15 A. P. Serebrov , R. M. Samoilov , M. E. Chaikovskii , O. M. Zherebtsov

Annihilation of extremely energetic cosmic neutrinos on the relic-neutrino background can give rise to absorption lines at energies corresponding to formation of the electroweak gauge boson $Z^{0}$. The positions of the absorption dips are…

High Energy Physics - Phenomenology · Physics 2008-11-26 Gabriela Barenboim , Olga Mena Requejo , Chris Quigg

Recent neutrino mass experiments at Mainz and Troitsk using tritium beta-decay have reached their sensitivity potential, yielding upper limits of about 2 eV/c^2 for the electron antineutrino mass. The KArlsruhe TRItium Neutrino experiment…

High Energy Physics - Experiment · Physics 2019-08-14 Kathrin Valerius

The KATRIN experiment in Karlsruhe Germany will monitor the decay of tritium, which produces an electron-antineutrino. While the present upper bound for its mass is 2 eV/$c^2$, KATRIN will search down to 0.2 eV$/c^2$. If the dark matter of…

Cosmology and Nongalactic Astrophysics · Physics 2011-04-01 Theo M. Nieuwenhuizen , Andrea Morandi

The fact that neutrinos carry a non-vanishing rest mass is evidence of physics beyond the Standard Model of elementary particles. Their absolute mass bears important relevance from particle physics to cosmology. In this work, we report on…

Nuclear Experiment · Physics 2025-09-19 M. Aker , D. Batzler , A. Beglarian , J. Behrens , J. Beisenkötter , M. Biassoni , B. Bieringer , Y. Biondi , F. Block , S. Bobien , M. Böttcher , B. Bornschein , L. Bornschein , T. S. Caldwell , M. Carminati , A. Chatrabhuti , S. Chilingaryan , B. A. Daniel , 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 , C. Fengler , C. Fiorini , J. A. Formaggio , C. Forstner , F. M. Fränkle , K. Gauda , A. S. Gavin , W. Gil , F. Glück , S. Grohmann , R. Grössle , R. Gumbsheimer , N. Gutknecht , V. Hannen , L. Hasselmann , N. Haußmann , K. Helbing , H. Henke , S. Heyns , S. Hickford , R. Hiller , D. Hillesheimer , D. Hinz , T. Höhn , A. Huber , A. Jansen , C. Karl , J. Kellerer , K. Khosonthongkee , M. Kleifges , M. Klein , J. Kohpeiß , C. Köhler , L. Köllenberger , A. Kopmann , N. Kovač , A. Kovalík , H. Krause , L. La Cascio , T. Lasserre , J. Lauer , T. Le , O. Lebeda , B. Lehnert , G. Li , A. Lokhov , M. Machatschek , M. Mark , A. Marsteller , E. L. Martin , C. Melzer , S. Mertens , S. Mohanty , J. Mostafa , K. Müller , A. Nava , H. Neumann , S. Niemes , A. Onillon , D. S. Parno , M. Pavan , U. Pinsook , A. W. P. Poon , J. M. Lopez Poyato , S. Pozzi , F. Priester , J. Ráliš , S. Ramachandran , R. G. H. Robertson , C. Rodenbeck , M. Röllig , C. Röttele , M. Ryšavý , R. Sack , A. Saenz , R. Salomon , P. Schäfer , M. Schlösser , K. Schlösser , L. Schlüter , S. Schneidewind , U. Schnurr , M. Schrank , J. Schürmann , A. Schütz , A. Schwemmer , A. Schwenck , M. Šefčík , D. Siegmann , F. Simon , F. Spanier , D. Spreng , W. Sreethawong , M. Steidl , J. Štorek , X. Stribl , M. Sturm , N. Suwonjandee , N. Tan Jerome , H. H. Telle , L. A. Thorne , T. Thümmler , S. Tirolf , N. Titov , I. Tkachev , K. Urban , K. Valerius , D. Vénos , C. Weinheimer , S. Welte , J. Wendel , C. Wiesinger , J. F. Wilkerson , J. Wolf , S. Wüstling , J. Wydra , W. Xu , S. Zadorozhny , G. Zeller

The existence of a cosmic neutrino background -- the analogue of the cosmic microwave background -- is a fundamental prediction of standard big bang cosmology. Up to now, the observational evidence for its existence is rather indirect and…

Cosmology and Nongalactic Astrophysics · Physics 2010-04-21 Andreas Ringwald

Relic neutrinos from the early universe are predicted to have a relatively large number density, but extremely low energies. Hence, the only possible interaction proceeds via neutrino capture on beta-decaying nuclei. In case relic neutrinos…

High Energy Physics - Phenomenology · Physics 2020-09-24 Tim Ruhe , Alexander Sandrock

We summarize a novel approach which has been recently proposed for direct detection of low energy neutrino backgrounds such as the cosmological relic neutrinos, exploiting neutrino/antineutrino capture on nuclei that spontaneously undergo…

Astrophysics · Physics 2008-11-26 Alfredo G. Cocco , Gianpiero Mangano , Marcello Messina

A range of experimental results point to the existence of a massive neutrino. The recent high precision measurements of the cosmic microwave background and the large scale surveys of galaxies can be used to place an upper bound on this…

Astrophysics · Physics 2009-06-12 C. Zunckel , P. G Ferreira

The spectrum of the Cosmic Microwave Background follows Planck's black body radiation formula and shows a remarkable constant temperature of T = 2.7. About 380 000 years after the Big Bang at a temperature of T = 3000 Kelvin in the matter…

Nuclear Theory · Physics 2013-12-13 Amand Faessler , Rastislav Hodak , Sergey Kovalenko , Fedor Simkovic

We perform a statistical analysis with the prospective results of future experiments on neutrino-less double beta decay, direct searches for neutrino mass (KATRIN) and cosmological observations. Realistic errors are used and the nuclear…

High Energy Physics - Phenomenology · Physics 2009-07-24 Werner Maneschg , Alexander Merle , Werner Rodejohann

Recently, a new non-Standard Model neutrino interaction mediated by a light scalar field was proposed, which renders the big-bang relic neutrinos of the cosmic neutrino background a natural dark energy candidate, the so-called Neutrino Dark…

Astrophysics · Physics 2009-11-11 Andreas Ringwald , Lily Schrempp

Existing and planned neutrino detectors, sensitive in the energy regime from 10^{17} eV to 10^{23} eV, offer opportunities for particle physics and cosmology. In this contribution, we discuss particularly the possibilities to infer…

High Energy Physics - Phenomenology · Physics 2009-11-10 A. Ringwald

The origin of highest energy cosmic rays is yet unknown. An appealing possibility is the so-called Z-burst scenario, in which a large fraction of these cosmic rays are decay products of Z bosons produced in the scattering of ultrahigh…

High Energy Physics - Phenomenology · Physics 2007-05-23 Z. Fodor , S. D. Katz , A. Ringwald

The precision measurement of the tritium $\beta$-decay spectrum performed by the KATRIN experiment provides a unique way to search for general neutrino interactions (GNI). All theoretical allowed GNI terms involving neutrinos are…

Nuclear Experiment · Physics 2025-09-19 M. Aker , D. Batzler , A. Beglarian , J. Beisenkötter , M. Biassoni , B. Bieringer , Y. Biondi , F. Block , B. Bornschein , L. Bornschein , M. Böttcher , M. Carminati , A. Chatrabhuti , S. Chilingaryan , B. A. Daniel , M. Descher , D. Díaz Barrero , P. J. Doe , O. Dragoun , G. Drexlin , F. Edzards , K. Eitel , E. Ellinger , R. Engel , S. Enomoto , 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 , N. Gutknecht , V. Hannen , L. Hasselmann , K. Helbing , H. Henke , S. Heyns , R. Hiller , D. Hillesheimer , D. Hinz , T. Höhn , A. Huber , A. Jansen , K. Khosonthongkee , C. Köhler , L. Köllenberger , A. Kopmann , N. Kovač , L. La Cascio , T. Lasserre , J. Lauer , T. L. Le , O. Lebeda , B. Lehnert , G. Li , A. Lokhov , M. Machatschek , M. Mark , A. Marsteller , K. McMichael , C. Melzer , S. Mertens , S. Mohanty , J. Mostafa , K. Müller , A. Nava , H. Neumann , S. Niemes , A. Onillon , D. S. Parno , M. Pavan , U. Pinsook , A. W. P. Poon , J. M. L. Poyato , F. Priester , J. Ráliš , S. Ramachandran , R. G. H. Robertson , C. Rodenbeck , M. Röllig , R. Sack , A. Saenz , R. Salomon , P. Schäfer , K. Schlösser , M. Schlösser , L. Schlüter , S. Schneidewind , M. Schrank , J. Schürmann , A. K. Schütz , A. Schwemmer , A. Schwenck , J. Seeyangnok , M. Šefčík , D. Siegmann , F. Simon , J. Songwadhana , F. Spanier , D. Spreng , W. Sreethawong , M. Steidl , J. Štorek , X. Stribl , M. Sturm , N. Suwonjandee , N. Tan Jerome , H. H. Telle , L. A. Thorne , T. Thümmler , N. Titov , I. Tkachev , K. Urban , K. Valerius , D. Vénos , C. Weinheimer , S. Welte , J. Wendel , M. Wetter , C. Wiesinger , J. F. Wilkerson , J. Wolf , S. Wüstling , J. Wydra , W. Xu , S. Zadorozhny , G. Zeller

Although the first results of the KATRIN neutrino mass experiment are consistent with a new improved upper limit of 1.1 eV for the effective mass of the electron neutrino, surprisingly they are also consistent with an exotic model of the…

High Energy Physics - Phenomenology · Physics 2021-08-11 Robert Ehrlich