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Related papers: Sterile neutrinos?

200 papers

We review theoretical ideas, problems and implications of neutrino masses and mixing angles. We give a general discussion of schemes with three light neutrinos. Several specific examples are analyzed in some detail, particularly those that…

High Energy Physics - Phenomenology · Physics 2009-11-10 Guido Altarelli , Ferruccio Feruglio

Evidences in favor of neutrino oscillations, obtained in the solar and atmospheric neutrino experiments, are discussed. Neutrino oscillations in the solar and atmospheric ranges of the neutrino mass-squared differences are considered in the…

High Energy Physics - Phenomenology · Physics 2007-05-23 S. M. Bilenky

The status of the problem of neutrino masses and mixing is shortly reviewed. Different schemes of mixing of (Dirac or Majorana) massive neutrinos are considered. The theory of neutrino oscillations in vacuum and in matter is presented.…

High Energy Physics - Phenomenology · Physics 2007-05-23 S. M. Bilenky

Neutrinos are one of the major puzzles in modern physics. Despite measurements of mass differences, the Standard Model of particle physics describes them as exactly massless. Additionally, recent measurements from both particle physics…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 Signe Riemer-Sørensen , David Parkinson , Tamara M. Davis

keV scale sterile neutrinos are excellent warm dark matter candidates. In the early Universe, these can be produced from oscillations and scatterings of active neutrinos. However, in the absence of any new physics, this mechanism is in…

High Energy Physics - Phenomenology · Physics 2022-03-02 Manibrata Sen

We present a comprehensive review of keV-scale sterile neutrino Dark Matter, collecting views and insights from all disciplines involved - cosmology, astrophysics, nuclear, and particle physics - in each case viewed from both theoretical…

High Energy Physics - Phenomenology · Physics 2017-02-10 R. Adhikari , M. Agostini , N. Anh Ky , T. Araki , M. Archidiacono , M. Bahr , J. Baur , J. Behrens , F. Bezrukov , P. S. Bhupal Dev , D. Borah , A. Boyarsky , A. de Gouvea , C. A. de S. Pires , H. J. de Vega , A. G. Dias , P. Di Bari , Z. Djurcic , K. Dolde , H. Dorrer , M. Durero , O. Dragoun , M. Drewes , G. Drexlin , Ch. E. Düllmann , K. Eberhardt , S. Eliseev , C. Enss , N. W. Evans , A. Faessler , P. Filianin , V. Fischer , A. Fleischmann , J. A. Formaggio , J. Franse , F. M. Fraenkle , C. S. Frenk , G. Fuller , L. Gastaldo , A. Garzilli , C. Giunti , F. Glück , M. C. Goodman , M. C. Gonzalez-Garcia , D. Gorbunov , J. Hamann , V. Hannen , S. Hannestad , S. H. Hansen , C. Hassel , J. Heeck , F. Hofmann , T. Houdy , A. Huber , D. Iakubovskyi , A. Ianni , A. Ibarra , R. Jacobsson , T. Jeltema , J. Jochum , S. Kempf , T. Kieck , M. Korzeczek , V. Kornoukhov , T. Lachenmaier , M. Laine , P. Langacker , T. Lasserre , J. Lesgourgues , D. Lhuillier , Y. F. Li , W. Liao , A. W. Long , M. Maltoni , G. Mangano , N. E. Mavromatos , N. Menci , A. Merle , S. Mertens , A. Mirizzi , B. Monreal , A. Nozik , A. Neronov , V. Niro , Y. Novikov , L. Oberauer , E. Otten , N. Palanque-Delabrouille , M. Pallavicini , V. S. Pantuev , E. Papastergis , S. Parke , S. Pascoli , S. Pastor , A. Patwardhan , A. Pilaftsis , D. C. Radford , P. C. -O. Ranitzsch , O. Rest , D. J. Robinson , P. S. Rodrigues da Silva , O. Ruchayskiy , N. G. Sanchez , M. Sasaki , N. Saviano , A. Schneider , F. Schneider , T. Schwetz , S. Schönert , S. Scholl , F. Shankar , R. Shrock , N. Steinbrink , L. Strigari , F. Suekane , B. Suerfu , R. Takahashi , N. Thi Hong Van , I. Tkachev , M. Totzauer , Y. Tsai , C. G. Tully , K. Valerius , J. W. F. Valle , D. Venos , M. Viel , M. Vivier , M. Y. Wang , C. Weinheimer , K. Wendt , L. Winslow , J. Wolf , M. Wurm , Z. Xing , S. Zhou , K. Zuber

Sterile neutrino dark matter, a popular alternative to the WIMP paradigm, has generally been studied in non-supersymmetric setups. If the underlying theory is supersymmetric, we find that several interesting and novel dark matter features…

High Energy Physics - Phenomenology · Physics 2017-08-23 Bibhushan Shakya , James D. Wells

The recent experimental results indicating the neutrino oscillations may strongly suggest that at least one more light neutrino species is required in order to reconcile the existing data. In the simple GUT frameworks, this fact seems…

High Energy Physics - Phenomenology · Physics 2009-10-31 Masako Bando , Koichi Yoshioka

Experimental work with solar neutrinos has illuminated the properties of neutrinos and tested models of how the sun produces its energy. Three experiments continue to take data, and at least seven are in various stages of planning or…

Nuclear Experiment · Physics 2009-11-11 R. G. H. Robertson

Sterile neutrinos at the eV scale have long been studied in the context of anomalies in short baseline neutrino experiments. Their cosmology can be made compatible with our understanding of the early Universe provided the sterile neutrino…

High Energy Physics - Phenomenology · Physics 2017-07-26 Francesco Capozzi , Ian M. Shoemaker , Luca Vecchi

A number of short baseline neutrino oscillation experiments have observed an anomalous excess of neutrinos in the low energy range. This may hint towards the existence of additional neutrino mass splittings. If true, additional sterile…

High Energy Physics - Experiment · Physics 2018-02-22 Alejandro Diaz

Sterile neutrinos may be one of the best Warm Dark Matter candidates we have today. Both lower and upper bounds on the mass of the sterile neutrino come from astronomical observations. We show that the proper inclusion of the neutrino…

Astrophysics · Physics 2008-11-26 Steen H. Hansen , Julien Lesgourgues , Sergio Pastor , Joseph Silk

We discuss a model in which three active and one sterile neutrino account for the solar, the atmospheric and the LSND neutrino anomalies. It is shown that if $N_\nu<4$ then these and other experiments and big bang nucleosynthesis constrain…

High Energy Physics - Phenomenology · Physics 2011-02-11 Nobuchika Okada , Osamu Yasuda

Possible explanations of solar neutrino and atmospheric neutrino anomalies are summarized and future tests discussed.

High Energy Physics - Phenomenology · Physics 2007-05-23 Sandip Pakvasa

The major steps in the development of our knowledge about neutrinos are reviewed. The basics of neutrino oscillation formalism is presented. Neutrino oscillations in the framework of three-neutrino mixing are considered. The evidence for…

High Energy Physics - Phenomenology · Physics 2007-05-23 S. M. Bilenky

In this talk I review what we know and don't know about neutrinos, neutrino masses and lepton mixing. I also discuss the importance of the discovery that neutrinos have nonzero masses, and illustrate how little is currently known about the…

High Energy Physics - Phenomenology · Physics 2009-02-27 Andre de Gouvea

In this letter we point out that in a class of models for spontaneous R-parity breaking based on gauged B-L, the spectrum for neutrinos is quite peculiar. We find that those models generally predict three layers of neutrinos: one heavy…

High Energy Physics - Phenomenology · Physics 2011-02-11 Vernon Barger , Pavel Fileviez Perez , Sogee Spinner

A simple model to accomodate light sterile neutrinos naturally with large mixing with the usual neutrinos has been proposed. The standard model gauge group is extended to include an $SU(2)_S$ gauge symmetry. Heavy triplet higgs scalars give…

High Energy Physics - Phenomenology · Physics 2009-12-30 Utpal Sarkar

Although the framework for oscillations of the three neutrino flavors in the Standard Model has been convincingly established, indications persist that it may be incomplete. Challenges are coming from the LSND and MiniBooNe short-baseline…

High Energy Physics - Phenomenology · Physics 2011-11-04 Francis Halzen

We discuss possibility of describing solar, atmospheric and LSND results with four neutrinos forming two quasi-degenerate pairs. The simplest versions of this 2+2 scheme with either $\nu_e$ or $\nu_\mu$ mixing exclusively with sterile…

High Energy Physics - Phenomenology · Physics 2009-11-07 Srubabati Goswami , Anjan S. Joshipura