245 research outputs found
Renormalization Group Analysis of Neutrino Mass Parameters
Tools for calculating the Renormalization Group Equations for renormalizable
and non-renormalizable operators in various theories are reviewed, which are
essential for comparing experimental results with predictions from models
beyond the Standard Model. Numerical examples for the running of the lepton
mixing angles in models with non-degenerate see-saw scales are shown, in which
the best-fit values of the experimentally favored LMA solution are produced
from maximal or from vanishing solar neutrino mixing at the GUT scale.Comment: 6 pages, 17 figures; to appear in the proceedings of the 10th
International Conference on Supersymmetry and Unification of Fundamental
Interactions (SUSY02), June 17 - 23, DESY Hambur
Sneutrino Hybrid Inflation
We review the scenario of sneutrino hybrid inflation, where one of the
singlet sneutrinos, the superpartners of the right-handed neutrinos, plays the
role of the inflaton. In a minimal model of sneutrino hybrid inflation, the
spectral index is given by . With constrained by WMAP, a running spectral index and a tensor-to-scalar ratio are predicted. Small
neutrino masses arise from the seesaw mechanism, with heavy masses for the
singlet (s)neutrinos generated by the vacuum expectation value of the waterfall
field after inflation. The baryon asymmetry of the universe can be explained by
non-thermal leptogenesis via sneutrino inflaton decay, with low reheat
temperature GeV.Comment: 7 pages, 2 figures; talk presented at the International Workshop on
The Dark Side of the Universe (DSU2006), Madrid, Spain, June 20-24, 200
Implications of Running Neutrino Parameters for Leptogenesis and for Testing Model Predictions
The running of neutrino parameters in see-saw models and its implications for
leptogenesis and for testing predictions of mass models with future precision
experiments are discussed using analytical approximations as well as numerical
results.Comment: 5 pages, 2 figures; talk presented at 10th International Symposium on
Particles, Strings and Cosmology (Pascos04), Northeastern University, Boston,
August 16-22, 2004; references adde
Searches for Sterile Neutrinos at Future Electron-Proton Colliders
Sterile neutrinos are an attractive extension of the Standard Model of
elementary particles towards including a mechanism for generating the observed
light neutrino masses. We discuss that when an approximate protective "lepton
number"-like symmetry is present, the sterile neutrinos can have masses around
the electroweak scale and potentially large neutrino Yukawa couplings, which
makes them well testable at planned future particle colliders. We
systematically discuss the production and decay channels for sterile neutrinos
at electron-proton colliders and give a complete list of the leading order
signatures for sterile neutrino searches. We highlight several novel search
channels and present a first look at the possible sensitivities for the
active-sterile mixing parameters and the heavy neutrino masses. We also compare
the performance of electron-proton colliders with the ones of proton-proton and
electron-positron colliders, and discuss the complementarity of the different
collider types.Comment: Conference proceedings for the DIS 2017 in Birmingham, 13 pages, 8
figures, 2 table
Impact of other scalar fields on oscillons after hilltop inflation
Oscillons are spatially localized and relatively stable field fluctuations
which can form after inflation under suitable conditions. In order to reheat
the universe, the fields which dominate the energy density after inflation have
to couple to other degrees of freedom and finally produce the matter particles
present in the universe today. In this study, we use lattice simulations in 2+1
dimensions to investigate how such couplings can affect the formation and
stability of oscillons. We focus on models of hilltop inflation, where we have
recently shown that hill crossing oscillons generically form, and consider the
coupling to an additional scalar field which, depending on the value of the
coupling parameter, can get resonantly enhanced from the inhomogeneous inflaton
field. We find that three cases are realized: without a parametric resonance,
the additional scalar field has no effects on the oscillons. For a fast and
strong parametric resonance of the other scalar field, oscillons are strongly
suppressed. For a delayed parametric resonance, on the other hand, the
oscillons get imprinted on the other scalar field and their stability is even
enhanced compared to the single-field oscillons.Comment: 15 pages, 6 figures, version published in JCA
GUT predictions for quark and lepton mass ratios
Group theoretical factors from GUT symmetry breaking can lead to predictions
for the ratios of quark and lepton masses at the unification scale. Due to
supersymmetric (SUSY) threshold corrections the viability of such predictions
can depend strongly on the SUSY parameters. We derive possible new predictions
for the GUT scale ratios m_\mu/m_s, y_\tau/y_b and y_t/y_b and compare them
with the experimentally allowed ranges for three common SUSY breaking
scenarios.Comment: Based on a talk given at SUSY 09; 5 pages, 1 figure, 2 table
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