769 research outputs found
Bilarge neutrino mixing from supersymmetry with high-scale nonrenormalizable interactions
We suggest a supersymmetric (SUSY) explanation of neutrino masses and mixing,
where nonrenormalizable interactions in the hidden sector generate lepton
number violating Majorana mass terms for both right-chiral sneutrinos and
neutrinos. It is found necessary to start with a superpotential including an
array of gauge singlet chiral superfields. This leads to nondiagonal mass terms and almost diagonal SUSY breaking -terms. As a result, the
observed pattern of bilarge mixing can be naturally explained by the
simultaneous existence of the seesaw mechanism and radiatively induced masses.
Allowed ranges of parameters in the gauge singlet sector are delineated,
corresponding to each of the cases of normal hierarchy, inverted hierarchy and
degenerate neutrinos.Comment: 19 pages, 5 figures. Minor modifications are made in the title and
the text, some new references are added. To appear in this form in Physical
Review
Solar neutrino spectrum, sterile neutrinos and additional radiation in the Universe
Recent results from the SNO, Super-Kamiokande and Borexino experiments do not
show the expected upturn of the energy spectrum of events (the ratio ) at low energies. At the same time, cosmological observations
testify for possible existence of additional relativistic degrees of freedom in
the early Universe: . These facts strengthen the case
of very light sterile neutrino, , with eV, which mixes weakly with the active neutrinos. The
mixing in the mass eigenstate characterized by can explain an absence of the upturn. The mixing of in
the eigenstate with leads to production of
via oscillations in the Universe and to additional contribution before the big bang nucleosynthesis and later. Such a
mixing can be tested in forthcoming experiments with the atmospheric neutrinos
as well as in future accelerator long baseline experiments. It has substantial
impact on conversion of the supernova neutrinos.Comment: 27 pages, LaTeX, 14 eps figures, 3 figures and additional
considerations adde
On in situ Determination of Earth Matter Density in Neutrino Factory
We point out that an accurate in situ determination of the earth matter
density \rho is possible in neutrino factory by placing a detector at the magic
baseline, L = \sqrt{2} \pi / G_{F} N_{e} where N_{e} denotes electron number
density. The accuracy of matter density determination is excellent in a region
of relatively large theta_{13} with fractional uncertainty \delta \rho / \rho
of about 0.43%, 1.3%, and \lsim 3% at 1 sigma CL at sin^2 2theta_{13}=0.1,
10^{-2}, and 3 x 10^{-3}, respectively. At smaller theta_{13} the uncertainty
depends upon the CP phase delta, but it remains small, 3%-7% in more than 3/4
of the entire region of delta at sin^2 2theta_{13} = 10^{-4}. The results would
allow us to solve the problem of obscured CP violation due to the uncertainty
of earth matter density in a wide range of theta_{13} and delta. It may provide
a test for the geophysical model of the earth, or it may serve as a method for
stringent test of the MSW theory of neutrino propagation in matter once an
accurate geophysical estimation of the matter density is available.Comment: 21 pages, 4 figures, version to appear in PR
Neutrino oscillations in low density medium
For the case of small matter effects: , where is the
matter potential, we develop the perturbation theory using as the expansion parameter. We derive simple and physically
transparent formulas for the oscillation probabilities in the lowest order in
which are valid for arbitrary density profile. The formulas can be
applied for propagation of the solar and supernova neutrinos in matter of the
Earth, substantially simplifying numerical calculations. Using these formulas
we study sensitivity of the oscillation effects to structures of the density
profile situated at different distances from the detector . We show that for
the mass-to-flavor state transitions, {\it e.g.}, , the
sensitivity is suppressed for remote structures: ,
where is the oscillation length and is the energy
resolution of detector.Comment: discussion simplified, clarifications adde
Test of Fermi Gas Model and Plane-Wave Impulse Approximation Against Electron-Nucleus Scattering Data
A widely used relativistic Fermi gas model and plane-wave impulse
approximation are tested against electron-nucleus scattering data. Inclusive
quasi-elastic cross section are calculated and compared with high-precision
data for C, O, and Ca. A dependence of agreement between calculated cross
section and data on a momentum transfer is shown. Results for the C(nu_mu,mu)
reaction are presented and compared with experimental data of the LSND
collaboration.Comment: 10 pages, 8 figure
Effects of CPT and Lorentz Invariance Violation on Pulsar Kicks
The breakdown of Lorentz's and CPT invariance, as described by the Extension
of the Standard Model, gives rise to a modification of the dispersion relation
of particles. Consequences of such a modification are reviewed in the framework
of pulsar kicks induced by neutrino oscillations (active-sterile conversion). A
peculiar feature of the modified energy-momentum relations is the occurrence of
terms of the form \delta {\bbox \Pi}\cdot {\bf {\hat p}}, where \delta
{\bbox \Pi} accounts for the difference of spatial components of flavor
depending coefficients which lead to the departure of the Lorentz symmetry, and
, being the neutrino momentum. Owing to the
relative orientation of with respect to \delta {\bbox \Pi}, the
{\it coupling} \delta {\bbox \Pi}\cdot {\bf {\hat p}} may induce the
mechanism to generate the observed pulsar velocities. Topics related to the
velocity distribution of pulsars are also discussed.Comment: 10 pages, 1 figur
Dark matter sterile neutrinos in stellar collapse: alteration of energy/lepton number transport and a mechanism for supernova explosion enhancement
We investigate matter-enhanced Mikheyev-Smirnov-Wolfenstein (MSW)
active-sterile neutrino conversion in the
channel in the collapse of the iron core of a pre-supernova star. For values of
sterile neutrino rest mass and vacuum mixing angle
(specifically, ) which include those required for viable sterile neutrino
dark matter, our one-zone in-fall phase collapse calculations show a
significant reduction in core lepton fraction. This would result in a smaller
homologous core and therefore a smaller initial shock energy, disfavoring
successful shock re-heating and the prospects for an explosion. However, these
calculations also suggest that the MSW resonance energy can exhibit a minimum
located between the center and surface of the core. In turn, this suggests a
post-core-bounce mechanism to enhance neutrino transport and neutrino
luminosities at the core surface and thereby augment shock re-heating: (1)
scattering-induced or coherent MSW conversion occurs deep in
the core, at the first MSW resonance, where energies are large ( MeV); (2) the high energy stream outward at near light speed; (3)
they deposit their energy when they encounter the second MSW resonance
just below the proto-neutron star surface.Comment: 13 pages, 9 figure
Simultaneous Flavor Transformation of Neutrinos and Antineutrinos with Dominant Potentials from Neutrino-Neutrino Forward Scattering
In astrophysical environments with intense neutrino fluxes, neutrino-neutrino
forward scattering contributes both diagonal and off-diagonal potentials to the
flavor-basis Hamiltonian that governs neutrino flavor evolution. We examine a
special case where adiabatic flavor evolution can produce an off-diagonal
potential from neutrino-neutrino forward scattering that dominates over both
the corresponding diagonal term and the potential from neutrino-matter forward
scattering. In this case, we find a solution that, unlike the ordinary
Mikeyhev-Smirnov-Wolfenstein scenario, has both neutrinos and antineutrinos
maximally mixed in medium over appreciable ranges of neutrino and antineutrino
energy. Employing the measured solar and atmospheric neutrino mass-squared
differences, we identify the conditions on neutrino fluxes that are required
for this solution to exist deep in the supernova environment, where it could
affect the neutrino signal, heavy-element nucleosynthesis, and even the revival
of the supernova shock. We speculate on how this solution might or might not be
attained in realistic supernova evolution. Though this solution is ephemeral in
time and/or space in supernovae, it may signal the onset of subsequent
appreciable flavor mixing for both neutrinos and antineutrinos. A similar
solution may also exist in an early universe with significant net
neutrino-lepton numbers.Comment: 16 pages; 4 figures; RevTe
Genes associated with ant social behavior show distinct transcriptional and evolutionary patterns
Studies of the genetic basis and evolution of complex social behavior emphasize either conserved or novel genes. To begin to reconcile these perspectives, we studied how the evolutionary conservation of genes associated with social behavior depends on regulatory context, and whether genes associated with social behavior exist in distinct regulatory and evolutionary contexts. We identified modules of co-expressed genes associated with age-based division of labor between nurses and foragers in the ant Monomorium pharaonis, and we studied the relationship between molecular evolution, connectivity, and expression. Highly connected and expressed genes were more evolutionarily conserved, as expected. However, compared to the rest of the genome, forager-upregulated genes were much more highly connected and conserved, while nurse-upregulated genes were less connected and more evolutionarily labile. Our results indicate that the genetic architecture of social behavior includes both highly connected and conserved components as well as loosely connected and evolutionarily labile components.It was funded by University of Pennsylvania with grant name: University Research Foundation
grant
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