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Related papers: Supernova Neutrino Oscillations

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We discuss the possibility for matter effects in the three-neutrino oscillations of the atmospheric nu_e (bar{nu}_e) and nu_mu (bar{nu}_mu), driven by one neutrino mass squared difference, |Delta m2_{31}| >> Delta m2_{21}, to be observable…

High Energy Physics - Phenomenology · Physics 2007-05-23 Jose Bernabeu , Sergio Palomares-Ruiz

The field of neutrino physics is currently very exciting, with several recent results pointing to new physics. I will give an overview of the current experimental situation, focusing primarily on neutrino oscillation results. The data are…

High Energy Physics - Experiment · Physics 2007-05-23 Kate Scholberg

Massive neutrinos open up the possibility for a variety of new physical phenomena. Among them are oscillations and double beta decay. Furthermore they influence several fields from particle physics to cosmology. In this article the concept…

High Energy Physics - Phenomenology · Physics 2009-09-25 K. Zuber

Supernova neutrinos are of considerable importance for ongoing research in astrophysics, nuclear and particle physics. Existing simulations of this complex event are increasingly sophisticated, but the accuracy with which they describe the…

High Energy Physics - Phenomenology · Physics 2025-01-16 Veronica Oliviero , Riccardo Maria Bozza , Vigilante di Risi , Giuseppe Matteucci , Giulia Ricciardi , Francesco Vissani

I review the status of neutrino masses and mixings in the light of the solar and atmospheric neutrino data in the framework of two--, three-- and four neutrino mixing.

High Energy Physics - Phenomenology · Physics 2009-10-31 M. C. Gonzalez-Garcia

In this note we investigate the impact of new physics in the form of general four-fermion interactions on neutrino oscillation signals. We develop a field theoretic description of the overall oscillation process which includes the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Matthew Garbutt , Bruce H. J. McKellar

I summarize the status of three--neutrino oscillations that follow from combining the relevant world's data. The discussion includes the small parameters Delta_m-sol/Delta_m-atm and \sin^2\theta_{13}, which characterize the strength of CP…

High Energy Physics - Phenomenology · Physics 2016-09-06 J. W. F. Valle

The aim of these notes is to provide a brief review of the topic of neutrino astronomy and in particular of neutrinos from core collapse supernovae. They are addressed to a curious reader, beginning to work in a multidisciplinary area that…

Astrophysics · Physics 2009-11-10 Flavio Cavanna , Maria Laura Costantini , Ornella Palamara , Francesco Vissani

We explain the physics of neutrino oscillation in vacuum and in matter. We attempt to clarify several features of oscillation that can be puzzling when neutrinos are their own antiparticles.

High Energy Physics - Phenomenology · Physics 2009-09-29 Boris Kayser

In this review, the effect of flavor oscillations on the neutrinos released during supernova explosion after core collapse is described. In some scenarios there are large enhancement of the number of events compared to the no oscillation…

High Energy Physics - Phenomenology · Physics 2007-05-23 Sandhya Choubey , Kamales Kar

Matter effects on neutrino oscillations in both, a supernova and the Earth, change the observed supernova neutrino spectra. We calculate the expected number of supernova neutrino interactions for ICARUS, SK and SNO detectors as a function…

High Energy Physics - Phenomenology · Physics 2007-05-23 B. Bekman , J. Holeczek , J. Kisiel

We briefly review the recent activity on neutrino masses and mixings which was prompted by the confirmation of neutrino oscillations by the Superkamiokande experiment.

High Energy Physics - Phenomenology · Physics 2009-10-31 Guido Altarelli , Ferruccio Feruglio

In this talk, we will demonstrate some concepts of a simultaneous treatment of neutrino decays and neutrino oscillations in an illustrative manner. This includes topics such as phase coherence discussions and time delay effects of massive…

High Energy Physics - Phenomenology · Physics 2007-05-23 Walter Winter

Neutrino oscillation is the new physics beyond standard model. In this paper we have revisited the issue of neutrino oscillation in simple and delicate manner. Starting from the fundamental quantum mechanical treatment for the neutrinos, we…

High Energy Physics - Phenomenology · Physics 2013-02-15 A. Upadhyay , M. Batra

Nonstandard neutrino properties (masses, mixing, sterile states, electromagnetic interactions, and so forth) can have far-reaching ramifications in astrophysics and cosmology. We look at the most interesting cases in the light of the…

High Energy Physics - Phenomenology · Physics 2007-05-23 G. Raffelt

We present a short review of the present status of the problem of neutrino masses and mixing including a survey of theoretical motivations and models, experimental searches and implications of recently appeared solar and atmospheric…

High Energy Physics - Phenomenology · Physics 2007-05-23 E. Torrente-Lujan

We discuss an Ansatz for the neutrino mixing matrix and speculate on the form and origin of the neutrino mass matrix.

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

In solar neutrino oscillations, if $\nu_e$ has a significant third massive component, the allowed parameter space in $\Delta m^2$ and $\sin^2 2 \theta$ for the first two components is shown to be greatly increased. This third component may…

High Energy Physics - Phenomenology · Physics 2007-05-23 Ernest Ma

I review some theoretical aspects of neutrino oscillations in the case when more than two neutrino flavours are involved. These include: approximate analytic solutions for 3-flavour (3f) oscillations in matter; matter effects in nu_mu -…

High Energy Physics - Phenomenology · Physics 2008-11-26 E. Kh. Akhmedov

The theoretical schemes on neutrino oscillations are considered. The experimental data on neutrino oscillations from Super-Kamiokande (Japan) and SNO (Kanada) are given. Comparison of these data with theoretical schemes is done. Conclusion…

High Energy Physics - Phenomenology · Physics 2007-05-23 Kh. M. Beshtoev
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