158 research outputs found
Neutrino oscillations from the splitting of Fermi points
As was shown previously, oscillations of massless neutrinos may be due to the
splitting of multiply degenerate Fermi points. In this Letter, we give the
details and propose a three-flavor model of Fermi point splittings and neutrino
mixings with only two free parameters. The model may explain recent
experimental results from the K2K and KamLAND collaborations. There is also
rough agreement with the data on atmospheric neutrinos (SuperK) and solar
neutrinos (SNO), but further analysis is required. Most importantly, the Ansatz
allows for relatively strong T-violating (CP-nonconserving) effects in the
neutrino sector.Comment: 6 pages with jetplFRK.cls, v4: published versio
The NuTeV Anomaly, Lepton Universality, and Non-Universal Neutrino-Gauge Couplings
In previous studies we found that models with flavor-universal suppression of
the neutrino-gauge couplings are compatible with NuTeV and Z-pole data. In this
paper we expand our analysis to obtain constraints on flavor-dependent coupling
suppression by including lepton universality data from W, tau, pi and K decays
in fits to model parameters. We find that the data are consistent with a
variety of patterns of coupling suppression. In particular, in scenarios in
which the suppression arises from the mixing of light neutrinos with heavy
gauge singlet states (neutrissimos), we find patterns of flavor-dependent
coupling suppression which are also consistent with constraints from mu -> e
gamma.Comment: REVTeX4, 25 pages, 10 postscript figures. Updated fits using the new
top mass. Updated figures. Extended discussion on the status of the
determination of B(tau->pi nu
Momentum-dependent contributions to the gravitational coupling of neutrinos in a medium
When neutrinos travel through a normal matter medium, the electron neutrinos
couple differently to gravity compared to the other neutrinos, due to the
presence of electrons in the medium and the absence of the other charged
leptons. We calculate the momentum-dependent part of the matter-induced
gravitational couplings of the neutrinos under such conditions, which arise at
order , and determine their contribution to the neutrino dispersion
relation in the presence of a gravitational potential .
These new contributions vanish for the muon and tau neutrinos. For electron
neutrinos with momentum , they are of the order of the usual Wolfenstein
term times the factor , for high energy
neutrinos. In environments where the gravitational potential is substantial,
such as those in the vicinity of Active Galactic Nuclei, they could be the
dominant term in the neutrino dispersion relation. They must also be taken into
account in the analysis of possible violations of the Equivalence Principle in
the neutrino sector, in experimental settings involving high energy neutrinos
traveling through a matter background.Comment: Minor corrections in the references; one reference adde
Violation of the Equivalence Principle in the light of the SNO and SK solar neutrino results
The SNO result on charged current deuteron disintegration, the
SuperKamiokande 1258-day data on electron scattering, and other solar neutrino
results are used to revisit the model of neutrino oscillations driven by a
violation of the equivalence principle. We use a chisq minimization technique
to examine oscillation between the nu(e) and another active neutrino, both
massless, and find that within the Standard Solar Model the fit to the SNO and
SuperKamiokande spectra are moderately good while a very good fit is obtained
when the absolute normalizations of the 8B and hep neutrino fluxes are allowed
to vary. The best fit prefers large, but not maximal, mixing, essentially no
hep neutrinos, and a 40% reduction in the 8B neutrino flux. The fit to the
total rates from the different experiments is not encouraging but when the
rates and spectra are considerd together the situation is much improved. We
remark on the expectations of the VEP model for the neutral current
measurements at SNO.Comment: Latex, 11 pages (incl. 1 postscript figure
Gravitational coupling of neutrinos in a medium
In a medium that contains electrons but not the other charged leptons, such
as normal matter, the gravitational interactions of neutrinos are not the same
for all the neutrino flavors. We calculate the leading order matter-induced
corrections to the neutrino gravitational interactions in such a medium and
consider some of their physical implications.Comment: 21 pages, Latex, uses axodraw.sty (typos corrected; two references
added. To appear in Phys. Rev. D
Interplay of gravitation and linear superposition of different mass eigenstates
The interplay of gravitation and the quantum-mechanical principle of linear
superposition induces a new set of neutrino oscillation phases. These ensure
that the flavor-oscillation clocks, inherent in the phenomenon of neutrino
oscillations, redshift precisely as required by Einstein's theory of
gravitation. The physical observability of these phases in the context of the
solar neutrino anomaly, type-II supernovae, and certain atomic systems is
briefly discussed
VEP oscillation solutions to the solar neutrino problem
We study the solar neutrino problem within the framework of a parametrized
post-Newtonian formulation for the gravitational interaction of the neutrinos,
which incorporates a violation to the equivalence principle (VEP). Using the
current data on the rates and the energy spectrum we find two possible
oscillation solutions, both for a large mixing angle. One of them involves the
MSW effect in matter and the other corresponds to vacuum oscillations. An
interesting characteristic of this mechanism is that it predicts a semi-annual
variation of the neutrino flux. Our analysis provides new constraints for some
VEP parameters.Comment: revtex, 18 pages, 11 figure
Photon-Neutrino Interactions in Magnetic Field through Neutrino Magnetic Moment
We study the neutrino-photon processes like in
the presence of uniform external magnetic field for the case when neutrinos can
couple to the electromagnetic field directly through their dipole magnetic
moment and obtain the stellar energy loss. The process would be of special
relevance in astrophysical situations where standard left-handed neutrinos are
trapped and the right handed neutrinos produced through the spin flip
interaction induced by neutrino magnetic moment alone can freely stream out.Comment: LaTex2e file, 9 page
Constraints on Exotic Mixing of Three Neutrinos
Exotic explanations are considered for atmospheric neutrino observations. Our
analysis includes matter effects and the mixing of all three neutrinos under
the simplifying assumption of only one relevant mixing scale. Constraints from
accelerator, reactor and solar neutrinos are included. We find that the
proposed mixing mechanisms based on violations of Lorentz invariance or on
violations of the equivalence principle cannot explain the recent observations
of atmospheric neutrino mixing. However the data still allow a wide range of
energy dependences for the vacuum mixing scale, and also allow large
electron-neutrino mixing of atmospheric neutrinos. Next generation long
baseline experiments will constrain these possibilities.Comment: 27 pages, 4 figure
Quantum field theoretic approach to neutrino oscillations in matter
We consider neutrino oscillations in non-uniform matter in a quantum field
theoretic (QFT) approach, in which neutrino production, propagation and
detection are considered as a single process. We find the conditions under
which the oscillation probability can be sensibly defined and demonstrate how
the properly normalized oscillation probability can be obtained in the QFT
framework. We derive the evolution equation for the oscillation amplitude and
discuss the conditions under which it reduces to the standard
Schr\"odinger-like evolution equation. It is shown that, contrary to the common
usage, the Schr\"odinger-like evolution equation is not applicable in certain
cases, such as oscillations of neutrinos produced in decays of free pions
provided that sterile neutrinos with eV exist.Comment: LaTeX, 24 pages + 16 pages of appendices, 1 figure. V2: typos
correcte
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