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We discuss some of the signatures associated with extensions of the Standard Model related to the neutrino and electroweak symmetry breaking sectors, with and without supersymmetry. The topics include a basic discussion of the theory of…

High Energy Physics - Phenomenology · Physics 2015-06-25 J. W. F. Valle

In spite of enormous experimental progress in determination of the neutrino parameters, theory of neutrino mass and mixing is still on the cross-roads. Guidelines could be (i) the connection between zero neutrino charges (and therefore a…

High Energy Physics - Phenomenology · Physics 2022-03-02 Alexei Yu. Smirnov

The sensitivity of the differential cross section of the interaction between neutrino-electron with dense matter to the possibly nonzero neutrino electromagnetic properties has been investigated. Here, the relativistic mean field model…

Nuclear Theory · Physics 2008-11-26 A. Sulaksono , C. K. Williams , P. T. P. Hutauruk , T. Mart

Recently it has been shown that one of the basic parameters of the neutrino sector, so called theta13 angle is very small, but quite probably non-zero. We argue that the small value of theta13 can still be reproduced easily by a wide…

High Energy Physics - Phenomenology · Physics 2013-05-30 Janusz Gluza , Robert Szafron

Neutrinos allow for a test of the hypothesis that the fermions of the Standard Model have Fermi-point splitting, analogous to the fermionic quasi-particles of certain condensed-matter systems. If present, the corresponding Lorentz-violating…

High Energy Physics - Phenomenology · Physics 2007-05-23 F. R. Klinkhamer

Neutrino mass generation may affect the basic structure of the electroweak symmetry breaking sector. We consider a broad class of elementary particle theories where neutrinos get mass at a low mass scale. We show how these can be made…

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

We discuss the profile of neutrino masses and mixings in models with large extra dimensions when right handed neutrinos are present in the branes along with the usual standard model particles. In these models, string scale must be bigger…

High Energy Physics - Phenomenology · Physics 2008-11-26 R. N. Mohapatra , S. Nandi , A. Pérez-Lorenzana

We evaluate semi-inclusive neutral-current quasielastic differential neutrino and antineutrino cross sections within the framework of the relativistic impulse approximation. The results of the relativistic mean field and of the relativistic…

In practically all extentions of the standard model, the neutrinos naturally acquire a mass. The neutrino mass matrix, however, contains many parameters which can neither be predicted by the prevailing models nor can be fitted to the data.…

High Energy Physics - Phenomenology · Physics 2007-05-23 G. K. Leontaris , J. D. Vergados

Neutrinos are the most elusive particles in our universe. They have masses at least one million times smaller than the electron mass, carry no electric charge, and very weakly interact with other particles, meaning they are rarely captured…

High Energy Physics - Phenomenology · Physics 2015-04-20 Tommy Ohlsson , Shun Zhou

The helicity evolution of a neutrino interacting with randomly moving and polarized matter is studied. We derive the equation for the averaged neutrino helicity. The type of the neutrino interaction with background fermions is not fixed. In…

High Energy Physics - Phenomenology · Physics 2008-07-31 Maxim Dvornikov

In this talk we explore the possibility that the smallness of the observed neutrino masses is naturally understood in a modified version of the standard model with N extra generations of fermions and N right-handed neutrinos, in which light…

High Energy Physics - Phenomenology · Physics 2014-10-15 A. Aparici , J. Herrero-Garcia , N. Rius , A. Santamaria

We discuss neutrino oscillations in the framework of the quantum field theory without introducing the concept of neutrino weak eigenstates. The external particles are described by wave packets and the different mass eigenstate neutrinos…

High Energy Physics - Phenomenology · Physics 2009-10-22 C. Giunti , C. W. Kim , J. A. Lee

The fact that neutrinos are massive suggests that the minimal supersymmetric standard model (MSSM) might be extended in order to include three gauge-singlet neutrino superfields with Yukawa couplings of the type $H_2 L \nu^c$. We propose to…

High Energy Physics - Phenomenology · Physics 2009-11-11 D. E. Lopez-Fogliani , C. Munoz

The study of neutrino interactions has recently experienced a renaissance, motivated by the fact that neutrino oscillation experiments depend critically on an accurate models of neutrino interactions. These models have to predict not only…

High Energy Physics - Experiment · Physics 2015-06-10 Deborah A. Harris

Neutrino masses are zero in the minimal supersymmetric standard model. I discuss how they may become nonzero with new interactions which may or may not violate R-parity conservation.

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

The evidence for non-vanishing neutrino masses from solar and atmospheric neutrinos provides the first solid hint towards physics beyond the standard model. A full reconstruction of the neutrino spectrum may well provide a key to the…

High Energy Physics - Phenomenology · Physics 2017-09-27 Heinrich Päs

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

Massive neutrinos can be accommodated into the noncommutative geometry reinterpretation of the Standard Model. The constrained Standard Model Lagrangian is computed anew under the assumption of nonzero neutrino masses. This gives the…

High Energy Physics - Theory · Physics 2009-10-28 Jose M. Gracia-Bondia

A cubic kilometer scale experiment has been proposed to detect cosmic neutrinos of energy from tens of GeV up to the highest energies observed for cosmic rays, around 10**20 eV, or possibly even beyond. Detection efficiencies depend…

High Energy Physics - Phenomenology · Physics 2009-10-30 Guenter Sigl