117 research outputs found
Detection of Supernova Neutrinos
Matter effects on neutrino oscillations in both, a supernova and the Earth,
change the observed supernova neutrino spectra. We calculate the expected
number of supernova neutrino interactions for ICARUS, SK and SNO detectors as a
function of the distance which they traveled in the Earth. Calculations are
performed for supernova type II at 10kpc from the Earth, using standard
supernova neutrino fluxes described by thermal Fermi--Dirac distributions and
the PREM I Earth matter density profile.Comment: Postscript file: 7 pages, 2 figures; tar-compressed file: tex source
code, eps figures. To appear in Acta. Phys. Pol. B. Talk given at the XXVIII
Mazurian Lakes School of Physics, Krzyze, Poland, August 31 - September 7,
200
Impact of massive neutrinos on the Higgs self-coupling and electroweak vacuum stability
The presence of right-handed neutrinos in the type I seesaw mechanism may
lead to significant corrections to the RG evolution of the Higgs self-coupling.
Compared to the Standard Model case, the Higgs mass window can become narrower,
and the cutoff scale become lower. Naively, these effects decrease with
decreasing right-handed neutrino mass. However, we point out that the unknown
Dirac Yukawa matrix may impact the vacuum stability constraints even in the low
scale seesaw case not far away from the electroweak scale, hence much below the
canonical seesaw scale of 10^15 GeV. This includes situations in which
production of right-handed neutrinos at colliders is possible. We illustrate
this within a particular parametrization of the Dirac Yukawas and with explicit
low scale seesaw models. We also note the effect of massive neutrinos on the
top quark Yukawa coupling, whose high energy value can be increased with
respect to the Standard Model case.Comment: 17 pages, 7 figures, minor revisions, version to appear in JHE
Matter effects and CP violating neutrino oscillations with non-decoupling heavy neutrinos
The evolution equation for active and sterile neutrinos propagating in
general anisotropic or polarized background environment is found and solved for
a special case when heavy neutrinos do not decouple, resulting in non-unitary
mixing among light neutrino states. Then new CP violating neutrino oscillation
effects appear. In contrast to the standard unitary neutrino oscillations these
effects can be visible even for two flavour neutrino transitions and even if
one of the elements of the neutrino mixing matrix is equal to zero. They do not
necessarily vanish with and they are different for various
pairs of flavour neutrino transitions (), (), (). Neutrino oscillations in vacuum and Earth's
matter are calculated for some fixed baseline experiments and a comparison
between unitary and non-unitary oscillations are presented. It is shown, taking
into account the present experimental constraints, that heavy neutrino states
can affect CP and T asymmetries. This is especially true in the case of
oscillations.Comment: 18 pages, 6 fig
Non-unitary Leptonic Mixing and Leptogenesis
We investigate the relation between non-unitarity of the leptonic mixing
matrix and leptogenesis. We discuss how all parameters of the canonical type-I
seesaw mechanism can, in principle, be reconstructed from the neutrino mass
matrix and the deviation of the effective low-energy leptonic mixing matrix
from unitary. When the mass M' of the lightest right-handed neutrino is much
lighter than the masses of the others, we show that its decay asymmetries
within flavour-dependent leptogenesis can be expressed in terms of two
contributions, one depending on the unique dimension five (d=5) operator
generating neutrino masses and one depending on the dimension six (d=6)
operator associated with non-unitarity. In low-energy seesaw scenarios where
small lepton number violation explains the smallness of neutrino masses, the
lepton number conserving d=6 operator contribution generically dominates over
the d=5 operator contribution which results in a strong enhancement of the
flavour-dependent decay asymmetries without any resonance effects. To calculate
the produced final baryon asymmetry, the flavour equilibration effects directly
related to non-unitarity have to be taken into account. In a simple realization
of this non-unitarity driven leptogenesis, the lower bound on M' is found to be
about 10^8 GeV at the onset of the strong washout regime, more than one order
of magnitude below the bound in "standard" thermal leptogenesis.Comment: 19 pages, REVTeX4, 2 eps and 2 axodraw figure
Non-standard Hamiltonian effects on neutrino oscillations
We investigate non-standard Hamiltonian effects on neutrino oscillations,
which are effective additional contributions to the vacuum or matter
Hamiltonian. Since these effects can enter in either flavor or mass basis, we
develop an understanding of the difference between these bases representing the
underlying theoretical model. In particular, the simplest of these effects are
classified as ``pure'' flavor or mass effects, where the appearance of such a
``pure'' effect can be quite plausible as a leading non-standard contribution
from theoretical models. Compared to earlier studies investigating particular
effects, we aim for a top-down classification of a possible ``new physics''
signature at future long-baseline neutrino oscillation precision experiments.
We develop a general framework for such effects with two neutrino flavors and
discuss the extension to three neutrino flavors, as well as we demonstrate the
challenges for a neutrino factory to distinguish the theoretical origin of
these effects with a numerical example. We find how the precision measurement
of neutrino oscillation parameters can be altered by non-standard effects alone
(not including non-standard interactions in the creation and detection
processes) and that the non-standard effects on Hamiltonian level can be
distinguished from other non-standard effects (such as neutrino decoherence and
decay) if we consider specific imprint of the effects on the energy spectra of
several different oscillation channels at a neutrino factory.Comment: 30 pages, 6 figures, LaTeX, final version, published in Eur.Phys.J.
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