10,491 research outputs found
Flavor Physics in SO(10) GUTs with Suppressed Proton decay Due to Gauged Discrete Symmetry
Generic SO(10) GUT models suffer from the problem that Planck scale induced
non-renormalizable proton decay operators require extreme suppression of their
couplings to be compatible with present experimental upper limits. One way to
resolve this problem is to supplement SO(10) by simple gauged discrete
symmetries which can also simultaneously suppress the renormalizable R-parity
violating ones when they occur and make the theory "more natural". Here we
discuss the phenomenological viability of such models. We first show that for
both classes of models, e.g the ones that use or to
break B-L symmetry, the minimal Higgs content which is sufficient for proton
decay suppression is inadequate for explaining fermion masses despite the
presence of all apparently needed couplings. We then present an extended model, with three {\bf 10} and three {\bf 45}-Higgs, where is free of
this problem. We propose this as a realistic and "natural" model for fermion
unification and discuss the phenomenology of this model e.g. its predictions
for neutrino mixings and lepton flavor violation.Comment: 21 pages, 2 figure
Baryon Asymmetry, Supersymmetry and Gravitational Anomalies
We discuss two independent issues about the baryon asymmetry of the universe.
First, assuming that it is generated by an unspecified source at high
temperatures, we study the effects of non-perturbative dynamics above
the electroweak scale, in the context of supersymmetric models. We find that
there is a substantial difference with the nonsupersymmetric case with the net
effect of relaxing previous bounds on B and L violating interactions. In
particular supersymmetry allows neutrino masses as large as 10 eV (preferred by
solar neutrino and COBE data and measurable at future neutrino oscillation
experiments). Second, we argue that the existence of a mixed lepton
number-gravitational anomaly in the standard model will induce B-L violating
interactions. These transitions would be catalized by Einstein-Yang-Mills
instantons or sphalerons and could create a primordial B-L asymmetry at Planck
temperatures or lower. Gravity (and the anomaly structure of the standard
model) could then be the ultimate source of the baryon asymmetry. We analyze
the viability of the presently known gravitational instantons and sphalerons to
realize this scenario. (Talk presented by FQ at the Texas/Pascos Conference,
Berkeley Dec.1992.)Comment: 8 pages,FTUAM-93-07 NEIP93-001, harvma
A Supersymmetric Contribution to the Neutrino Mass Matrix and Breaking of mu-tau Symmetry
Supersymmetry broken by anomaly mediation suffers from tachyonic slepton
masses. A possible solution to this problem results in "decoupling", i.e., the
first two generations of sfermions are much heavier than the third one. We note
that in this scenario a sizable loop-induced contribution to the neutrino mass
matrix results. As an application of this scenario we take advantage of the
fact that the decoupling evidently not obeys 2-3 generation exchange symmetry.
In the neutrino sector, this 2-3 symmetry (or mu-tau symmetry) is a useful
Ansatz to generate zero theta_{13} and maximal theta_{23}. The induced
deviations from these values are given for some examples, thereby linking SUSY
breaking to the small parameters (including possibly the solar mass splitting)
of the neutrino sector.Comment: 5 pages, 1 figur
Seesaw Right Handed Neutrino as the Sterile Neutrino for LSND
We show that a double seesaw framework for neutrino masses with
exchange symmetry can lead to one of the righthanded seesaw partners of the
light neutrinos being massless. This can play the role of a light sterile
neutrino, giving a model that explains the LSND results. We get a very
economical scheme, which makes it possible to predict the full
neutrino mass matrix if CP is conserved. Once CP violation is included, effect
of the LSND mass range sterile neutrino is to eliminate the lower bound on
neutrinoless double beta decay rate which exists for the three neutrino case
with inverted mass hierarchy. The same strategy can also be used to generate a
natural model for LSND, which is also equally predictive for the CP
conserving case in the limit of exact symmetry.Comment: 13 pages and one figure; model extended to 3+2 cas
Cosmology of Brane-Bulk Models in Five Dimensions
We study the cosmology of models with four space and one time dimension where
our universe is a 3-brane and report a few results which extend existing work
in several directions. Assuming a stable fifth dimension, we obtain a solution
for the metric, which does not depend on any arbitrary parameters. We discuss
some implications of this result.Comment: Minor changes: brane energy conservation law and some typos
corrected. All main results unchanged. 11 pages, no figures, LaTeX fil
Minimal Seesaw as an Ultraviolet Insensitive Cure for the Problems of Anomaly Mediation
We show that an intermediate scale supersymmetric left-right seesaw scenario
with automatic R-parity conservation can cure the problem of tachyonic slepton
masses that arises when supersymmetry is broken by anomaly mediation, while
preserving ultraviolet insensitivity. The reason for this is the existence of
light B - L = 2 higgses with yukawa couplings to the charged leptons. We find
these theories to have distinct predictions compared to the usual mSUGRA and
gauge mediated models as well as the minimal AMSB models. Such predictions
include a condensed gaugino mass spectrum and possibly a correspondingly
condensed sfermion spectrum.Comment: 19 pages, 1 figur
Searching for Strongly Interacting Massive Particles (SIMPs)
We consider laboratory experiments that can detect stable, neutral strongly
interacting massive particles (SIMPs). We explore the SIMP annihilation cross
section from its minimum value (restricted by cosmological bounds) to the barn
range, and vary the mass values from a GeV to a TeV. We calculate, as a
function of the SIMP-nucleon cross section, the minimum nucleon number A for
which there should be binding in a nucleus. We consider accelerator mass
spectrometry with a gold (A=200) target, and compute the likely abundance of
anomalous gold nuclei if stable neutral SIMPs exist. We also consider the
prospects and problems of detecting such particles at the Tevatron. We estimate
optimistically that such detection might be possible for SIMPs with
SIMP-nucleon cross sections larger than 0.1 millibarn and masses between 25 and
50 GeV.Comment: RevTeX, 10 pages, 3 figures; Minor updates to match published versio
Phenomenological Consequences of sub-leading Terms in See-Saw Formulas
Several aspects of next-to-leading (NLO) order corrections to see-saw
formulas are discussed and phenomenologically relevant situations are
identified. We generalize the formalism to calculate the NLO terms developed
for the type I see-saw to variants like the inverse, double or linear see-saw,
i.e., to cases in which more than two mass scales are present. In the standard
type I case with very heavy fermion singlets the sub-leading terms are
negligible. However, effects in the percent regime are possible when
sub-matrices of the complete neutral fermion mass matrix obey a moderate
hierarchy, e.g. weak scale and TeV scale. Examples are cancellations of large
terms leading to small neutrino masses, or inverse see-saw scenarios. We
furthermore identify situations in which no NLO corrections to certain
observables arise, namely for mu-tau symmetry and cases with a vanishing
neutrino mass. Finally, we emphasize that the unavoidable unitarity violation
in see-saw scenarios with extra fermions can be calculated with the formalism
in a straightforward manner.Comment: 22 pages, matches published versio
Two Categories of Approximately mu-tau Symmetric Neutrino Mass Textures
Our approximately \mu-\tau symmetric neutrino mass textures fall into two
different categories, whose behaviors in the \mu-\tau symmetric limit are
characterized by either \sin(theta_{13})->0 (referred to as C1)), or
\sin(theta_{12})->0 (referred to as C2)). We present ten phenomenologically
viable neutrino mass textures: two for the normal mass hierarchy, three for the
inverted mass hierarchy, and five for the quasi degenerate mass pattern. Tiny
\mu-\tau symmetry breaking ensures that \sin^2(theta_{13}) << 1 for C1), and
\Delta m^2_\odot/\Delta m^2_{atm} (\equiv R) << 1 for C2). A correlation among
small quantities is provided by \cos 2(theta_{23}) \sim \sin(theta_{13}) for
C1), and by either \cos(2theta_{23}) \sim R, or
\cos(2theta_{23})\sin(theta_{13}) \sim R for C2). It is further shown that
\tan(2theta_{12}) \sim \cos(2theta_{23})/\sin(theta_{13}) is satisfied for C2).
We find specific properties for each mass ordering, which are discussed in this
article.Comment: 31 pages, 15 figures (High-resolution figures can be downloaded from
http://www.sp.u-tokai.ac.jp/~yasue/two_categories_of.pdf.tar.gz
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