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We consider an Supersymmetric extension of the Standard Model with some extra Higgs doublets and a global $(B - L)$, where $B$ and $L$ are the usual baryonic and lepton number respectivelly, and ${\cal Z}_{3} \otimes {\cal Z}^{\prime}_{3}$…

High Energy Physics - Phenomenology · Physics 2021-02-24 M. C. Rodriguez

R-parity can be violated through either bilinear and/or trilinear terms in the superpotential. The decay properties of sneutrinos can be used to obtain information about the relative importance of these couplings provided sneutrinos are the…

High Energy Physics - Phenomenology · Physics 2010-02-03 D. Aristizabal Sierra , M. Hirsch , W. Porod

The discovery of neutrino mass establishes the need for physics beyond the Standard Model. I summarize the status of two- and three-neutrino oscillation parameters from current solar, atmospheric, reactor and accelerator data. Future…

High Energy Physics - Phenomenology · Physics 2007-05-23 J. W. F. Valle

We review theoretical ideas, problems and implications of different models for neutrino masses and mixing angles. We give a general discussion of schemes with three or more light neutrinos. Several specific examples are analyzed in some…

High Energy Physics - Phenomenology · Physics 2009-07-09 Guido Altarelli , Ferruccio Feruglio

If all indications for neutrino oscillations observed in the solar, atmospheric neutrino data as well as in the LSND experiments are borne out by the ongoing and future experiments, then they severely constrain the neutrino mass texture. In…

High Energy Physics - Phenomenology · Physics 2007-05-23 R. N. Mohapatra

In this letter we consider that assuming: a) that the only left-handed neutral fermions are the active neutrinos, b) that $B-L$ is a gauge symmetry, and c) that the $L$ assignment is restricted to the integer numbers, the anomaly…

High Energy Physics - Phenomenology · Physics 2009-05-29 J. C. Montero , V. Pleitez

MACRO can detect three topologies of neutrino induced events, corresponding to different parent neutrino energies. The most numerous sample is made of upward throughgoing muons induced by atmospheric neutrinos of average energy 100 GeV. We…

High Energy Physics - Experiment · Physics 2019-08-14 T. Montaruli

Ongoing developments in theory and phenomenology are related to the measured large value of 1-3 mixing and indications of significant deviation of the 2-3 mixing from maximal one. "Race" for the mass hierarchy has started and there is good…

High Energy Physics - Phenomenology · Physics 2015-06-11 A. Yu. Smirnov

Preliminary remarks, theoretical scenarios, cosmological constraints, couplings of very heavy neutrinos, production mechanisms and detection, summary.

High Energy Physics - Phenomenology · Physics 2016-09-01 Probir Roy

In theories with three light neutrinos, a complete list of five zeroth-order textures for lepton mass matrices is found, which naturally yield: m_e = m_mu=0, m_tau \neq 0, Delta m^2_sun = 0, together with theta_{e tau} = 0, theta_{mu tau}…

High Energy Physics - Phenomenology · Physics 2009-10-09 Riccardo Barbieri , Lawrence J. Hall , Alessandro Strumia

A scheme is described in which the light gravitino in low energy SUSY breaking models mixes with neutrinos. The mixing between gravitino and neutrinos arises through the standard model symmetry breaking and an R-parity and lepton number…

High Energy Physics - Phenomenology · Physics 2007-05-23 Taekoon Lee

This part offers a survey of models proposed to cope with the symmetry-breaking challenge. Among them are the two-component neutrinos, the neutrino twins, the universal Fermi interaction, etc. Moreover, the broken discrete symmetries in…

History and Philosophy of Physics · Physics 2008-11-21 Mladen Georgiev

The observation of the neutrinos arrived from Supernova LMC-'87A shows, with a good confidence level, the existence of two massive neutrinos. For the unobserved third neutrino mass, could speculate two possibilities either that this mass is…

High Energy Physics - Phenomenology · Physics 2007-05-23 Humiaki Huzita

We update the hints of the existence of sterile neutrinos.

High Energy Physics - Phenomenology · Physics 2015-06-18 Boris Kayser

The simplest type III seesaw model as originally proposed introduces one lepton triplet. It thus contains four active neutrinos, two massive and two massless at tree level. We determine the radiative masses that the latter receive first at…

High Energy Physics - Phenomenology · Physics 2009-04-22 Yi Liao , Ji-Yuan Liu , Guo-Zhu Ning

Even the elusive neutrinos are trapped in matter, albeit transiently, in several astrophysical circumstances. Their interactions with the ambient matter not only reveal the properties of such exotic matter itself, but also shed light on the…

Astrophysics · Physics 2009-11-06 M. Prakash , J. M. Lattimer , R. F. Sawyer , R. R. Volkas

In view of the observation by IceCube of high-energy astrophysical neutrinos, it is important to quantify the uncertainty in the background of atmospheric neutrinos. There are two sources of uncertainty, the imperfect knowledge of the…

High Energy Astrophysical Phenomena · Physics 2016-06-22 Thomas K. Gaisser

Neutrino masses and mixing are generated in a supersymmetric standard model when R-parity is violated in bilinear mass terms. The mixing matrix among the neutrinos takes a restrictive form if the lepton flavor universality holds in the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Fumihiro Takayama , Masahiro Yamaguchi

In addition to three active neutrinos, one or more light sterile neutrinos have been conjectured to account for the LSND, MiniBooNE and reactor antineutrino anomalies (at the sub-eV mass scale) or for warm dark matter in the Universe (at…

High Energy Physics - Phenomenology · Physics 2013-05-30 Zhi-zhong Xing

The elastic scattering of longitudinal and transversal neutrinos on a spinless nucleus have been discussed taking into account the charge, magnetic, anapole and electric dipole moments of fermions and their weak neutral currents. Compound…

High Energy Physics - Phenomenology · Physics 2021-01-29 R. B. Begzhanov , R. S. Sharafiddinov
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