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Related papers: A supernova constraint on bulk majorons

200 papers

We show that in the presence of sufficiently strong tau neutrino annihilations into majorons, the primordial nucleosynthesis constraints can not rule out tau neutrino masses in the MeV range.

High Energy Physics - Phenomenology · Physics 2007-05-23 J. C. Romao

We propose a model with one large submm size extra dimension in which the gravity and right-handed (RH) neutrino propagate, but the three Standard Model (SM) families are confined to fat branes of TeV^(-1) size or smaller. The charged…

High Energy Physics - Phenomenology · Physics 2008-11-26 S. Nandi , C. M. Rujoiu

We study neutrino masses and mixing in Supersymmetric Models without $R$ parity and with generic soft Supersymmetry breaking terms. Neutrinos acquire mass from various sources: tree level neutrino--neutralino mixing, loop effects and…

High Energy Physics - Phenomenology · Physics 2009-10-28 Francesca M. Borzumati , Yuval Grossman , Enrico Nardi , Yosef Nir

The case for small neutrino mass differences from atmospheric and solar neutrino oscillation experiments has become compelling, but leaves the overall neutrino mass scale m_nu undetermined. The most restrictive limit of m_nu < 0.8 eV arises…

Astrophysics · Physics 2009-11-07 G. G. Raffelt

Ultra-high energy cosmic neutrinos are incisive probes of both astrophysical sources and new TeV-scale physics. Such neutrinos would create extensive air showers deep in the atmosphere. The absence of such showers implies upper limits on…

High Energy Physics - Phenomenology · Physics 2008-11-26 Luis A. Anchordoqui , Jonathan L. Feng , Haim Goldberg , Alfred D. Shapere

Particle physics models where there are large hidden extra dimensions are currently on the focus of an intense activity. The main reason is that these large extra dimensions may come with a TeV scale for quantum gravity (or string theory)…

High Energy Physics - Phenomenology · Physics 2009-10-31 A. Pérez-Lorenzana

We address the issue of whether extra dimensions could have an infinite volume and yet reproduce the effects of observable four-dimensional gravity on a brane. There is no normalizable zero-mode graviton in this case, nevertheless correct…

High Energy Physics - Theory · Physics 2009-10-31 G. Dvali , G. Gabadadze , M. Porrati

We propose a model of neutrino mass generation in extra dimension. Allowing a large lepton number violation on a distant brane spatially separated from the standard model brane, a small neutrino mass is naturally generated due to an…

High Energy Physics - Phenomenology · Physics 2010-03-02 Seong Chan Park , Kai Wang , Tsutomu T. Yanagida

The presence of the triplet $\Delta_{L}$ in left-right symmetric theories leads to type-II see-saw mechanism for the neutrino masses. In these models, assuming a normal mass hierarchy for the heavy Majorana neutrinos, we derive a lower…

High Energy Physics - Phenomenology · Physics 2014-11-17 Narendra Sahu , S. Uma Sankar

We study a multi-localization model for charged leptons and neutrinos, including the possibility of a see-saw mechanism. This framework offers the opportunity to allow for realistic solutions in a consistent model without fine-tuning of…

High Energy Physics - Phenomenology · Physics 2009-11-10 J. -M. Frere , G. Moreau , E. Nezri

Recently there has been a lot of interest in models in which gravity becomes strong at the TeV scale. The observed weakness of gravitational interactions is then explained by the existence of extra compact dimensions of space, which are…

High Energy Physics - Phenomenology · Physics 2009-10-31 Schuyler Cullen , Maxim Perelstein

General classes of mechanisms for generating small neutrino masses are surveyed from a top-down (superstring) perspective. In particular, string constructions have motivated various possibilities involving higher-dimensional operators,…

High Energy Physics - Phenomenology · Physics 2015-06-03 Paul Langacker

We extend the recently proposed gluino axion model to include neutrino masses. We discuss how the canonical seesaw model and the Higgs triplet model may be realized in this framework. In the former case, the heavy singlet neutrinos are…

High Energy Physics - Phenomenology · Physics 2009-10-31 D. A. Demir , Ernest Ma , Utpal Sarkar

We show that the see-saw neutrino mass mechanism can coexist naturally with an extended gauge symmetry (i.e. without any gauge heirarchy problem) provided that the gauge symmetry contains gauged lepton number differences. The simplest such…

High Energy Physics - Phenomenology · Physics 2009-11-11 R. Foot

The constraints on the radion evolution in the Universal Extra Dimension (UED) model from Cosmic Microwave Background (CMB) and Type Ia supernovae (SNe Ia) data are studied. In the UED model, where both the gravity and standard model fields…

Astrophysics · Physics 2008-12-18 K. C. Chan , M. -C. Chu

We investigate the nature (Dirac vs. Majorana) and size of left-handed neutrino masses in a supersymmetric five-dimensional model compactified in the interval [0,\pi R], where quarks and leptons are localized on the boundaries while the…

High Energy Physics - Phenomenology · Physics 2008-11-26 D. Diego , M. Quiros

Recent advances in cosmic observations have brought us to the verge of discovery of the absolute scale of neutrino masses. Nonzero neutrino masses are known evidence of new physics beyond the Standard Model. Our understanding of the…

We construct extensions of the Standard Model in which the gauge symmetries and supersymmetry prevent the dangerously large effects that may potentially be induced in a supersymmetric standard model by Planck scale physics. These include…

High Energy Physics - Phenomenology · Physics 2008-11-26 Hsin-Chia Cheng , Bogdan A. Dobrescu , Konstantin T. Matchev

We propose the inverse seesaw mechanism as a way to understand small Majorana masses for neutrinos in warped extra dimension models with seesaw scale in the TeV range. The ultra-small lepton number violation needed in implementing inverse…

High Energy Physics - Phenomenology · Physics 2012-08-13 Chee Sheng Fong , Rabindra N. Mohapatra , Ilmo Sung

A large fraction of massive stars are found in higher order systems where the presence of a tertiary may significantly modify the system's evolution. In particular, it can lead to increased numbers of compact object binaries and accelerate…

Solar and Stellar Astrophysics · Physics 2024-04-11 Karina Barboza , Christopher S. Kochanek