87 research outputs found
A Fresh Look at keV Sterile Neutrino Dark Matter from Frozen-In Scalars
Sterile neutrinos with a mass of a few keV can serve as cosmological warm
dark matter. We study the production of keV sterile neutrinos in the early
universe from the decay of a frozen-in scalar. Previous studies focused on
heavy frozen-in scalars with masses above the Higgs mass leading to a hot
spectrum for sterile neutrinos with masses below 8-10 keV. Motivated by the
recent hints for an X-ray line at 3.55 keV, we extend the analysis to lighter
frozen-in scalars, which allow for a cooler spectrum. Below the electroweak
phase transition, several qualitatively new channels start contributing. The
most important ones are annihilation into electroweak vector bosons,
particularly W-bosons as well as Higgs decay into pairs of frozen-in scalars
when kinematically allowed.Comment: 19 pages, 4 figures, model section (sec. 2) splits in effective
description (sec. 2) and UV completion (sec. 5), minor changes, references
added, matches published versio
Non-Abelian Discrete Groups from the Breaking of Continuous Flavor Symmetries
We discuss the possibility of obtaining a non-abelian discrete flavor
symmetry from an underlying continuous, possibly gauged, flavor symmetry SU(2)
or SU(3) through spontaneous symmetry breaking. We consider all possible cases,
where the continuous symmetry is broken by small representations. "Small"
representations are these which couple at leading order to the Standard Model
fermions transforming as two- or three-dimensional representations of the
flavor group. We find that, given this limited representation content, the only
non-abelian discrete group which can arise as a residual symmetry is the
quaternion group D_2'.Comment: 15 page
Non-Abelian Discrete Flavor Symmetries from T^2/Z_N Orbifolds
In [1] it was shown how the flavor symmetry A4 (or S4) can arise if the three
fermion generations are taken to live on the fixed points of a specific
2-dimensional orbifold. The flavor symmetry is a remnant of the 6-dimensional
Poincare symmetry, after it is broken down to the 4-dimensional Poincare
symmetry through compactification via orbifolding. This raises the question if
there are further non-abelian discrete symmetries that can arise in a similar
setup. To this end, we generalize the discussion by considering all possible
2-dimensional orbifolds and the flavor symmetries that arise from them. The
symmetries we obtain from these orbifolds are, in addition to S4 and A4, the
groups D3, D4 and D6 \simeq D3 x Z2 which are all popular groups for flavored
model building.Comment: 12 pages, 4 figure
Non-Abelian Discrete Flavor Symmetries on Orbifolds
We study non-Abelian flavor symmetries on orbifolds, and .
Our extra dimensional models realize , , and
including and . In addition, one can also realize
their subgroups such as , , etc. The flavor symmetry can be
realized on both and orbifolds.Comment: 16 page
Golden Ratio Prediction for Solar Neutrino Mixing
It has recently been speculated that the solar neutrino mixing angle is
connected to the golden ratio phi. Two such proposals have been made, cot
theta_{12} = phi and cos theta_{12} = phi/2. We compare these Ansatze and
discuss a model leading to cos theta_{12} = phi/2 based on the dihedral group
D_{10}. This symmetry is a natural candidate because the angle in the
expression cos theta_{12} = phi/2 is simply pi/5, or 36 degrees. This is the
exterior angle of a decagon and D_{10} is its rotational symmetry group. We
also estimate radiative corrections to the golden ratio predictions.Comment: 15 pages, 1 figure. Matches published versio
A Supersymmetric D4 Model for mu-tau Symmetry
We construct a supersymmeterized version of the model presented by Grimus and
Lavoura (GL) in [1] which predicts theta_{23} maximal and theta_{13}=0 in the
lepton sector. For this purpose, we extend the flavor group, which is D4 x
Z2^{(aux)} in the original model, to D4 x Z5. An additional difference is the
absence of right-handed neutrinos. Despite these changes the model is the same
as the GL model, since theta_{23} maximal and theta_{13}=0 arise through the
same mismatch of D4 subgroups, D2 in the charged lepton and Z2 in the neutrino
sector. In our setup D4 is solely broken by gauge singlets, the flavons. We
show that their vacuum structure, which leads to the prediction of theta_{13}
and theta_{23}, is a natural result of the scalar potential. We find that the
neutrino mass matrix only allows for inverted hierarchy, if we assume a certain
form of spontaneous CP violation. The quantity |m_{ee}|, measured in
neutrinoless double beta decay, is nearly equal to the lightest neutrino mass
m3. The Majorana phases phi1 and phi2 are restricted to a certain range for m3
< 0.06 eV. We discuss the next-to-leading order corrections which give rise to
shifts in the vacuum expectation values of the flavons. These induce deviations
from maximal atmospheric mixing and vanishing theta_{13}. It turns out that
these deviations are smaller for theta_{23} than for theta_{13}.Comment: 19 pages, 4 figure
Z_2 Symmetry Prediction for the Leptonic Dirac CP Phase
Model-independent consequences of applying a generalized hidden horizontal
Z_2 symmetry to the neutrino mass matrix are explored. The Dirac CP phase
delta_D can be expressed in terms of the three mixing angles as 4 c_a s_a c_s
s_s s_x cos delta_D = (s^2_s - c^2_s s^2_x) (c^2_a - s^2_a) where the s_i, c_i
are sines and cosines of the atmospheric, solar, and reactor angles. This
relation is independent of neutrino masses and whether neutrinos are Dirac- or
Majorana-type. Given the present constraints on the angles, delta_D is
constrained to be almost maximal, a result which can be explored in experiments
such as NOvA and T2K. The Majorana CP phases do not receive any constraint and
are thus model-dependent. Also a distribution of theta_x with a lower limit is
obtained without specifying delta_D.Comment: 5 pages, 4 figures; Condensed version or PLB with references added;
for more details see the previous versio
Discrete symmetries and models of flavor mixing
Evidences of a discrete symmetry behind the pattern of lepton mixing are
analyzed. The program of "symmetry building" is outlined. Generic features and
problems of realization of this program in consistent gauge models are
formulated. The key issues include the flavor symmetry breaking, connection of
mixing and masses, {\it ad hoc} prescription of flavor charges, "missing"
representations, existence of new particles, possible accidental character of
the TBM mixing. Various ways are considered to extend the leptonic symmetries
to the quark sector and to reconcile them with Grand Unification. In this
connection the quark-lepton complementarity could be a viable alternative to
TBM. Observational consequences of the symmetries and future experimental tests
of their existence are discussed.Comment: 14 pages, 5 figures. Talk given at the Symposium "DISCRETE 2010", 6 -
11 December 2010, La Sapienza, Rome, Ital
A4 Flavor Models in Split Seesaw Mechanism
A seesaw mechanism in an extra-dimension, known as the split seesaw
mechanism, provides a natural way to realize a splitting mass spectrum of
right-handed neutrinos. It leads to one keV sterile neutrino as a dark matter
candidate and two heavy right-handed neutrinos being responsible for
leptogenesis to explain the observed baryon asymmetry of the Universe. We study
models based on flavor symmetry in the context of the split seesaw
mechanism. It is pointed out that most of known flavor models with three
right-handed neutrinos being triplet suffer from a degeneracy problem for
the bulk mass terms, which disturbs the split mechanism for right-handed
neutrino mass spectrum. Then we construct a new flavor model to work in
the split seesaw mechanism. In the model, the experimentally observed neutrino
masses and mixing angles can be realized from both type I+II seesaw
contributions. The model predicts the symmetry in the neutrino mass
matrix at the leading order, resulting in the vanishing and
maximal . The flavor symmetry is broken via the flavon
vacuum alignment which can be obtained from the orbifold compactification. The
model can be consistent with all data of neutrino oscillation experiments,
cosmological discussions of dark matter abundance, leptogenesis, and recent
astrophysical data.Comment: 21 pages, 1 figure, version to appear in JHE
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