24 research outputs found
Neutrino Mixing and Neutrino Telescopes
Measuring flux ratios of ultra-high energy neutrinos is an alternative method
to determine the neutrino mixing angles and the CP phase delta. We conduct a
systematic analysis of the neutrino mixing probabilities and of various flux
ratios measurable at neutrino telescopes. The considered cases are neutrinos
from pion, neutron and muon-damped sources. Explicit formulae in case of mu-tau
symmetry and its special case tri-bimaximal mixing are obtained, and the
leading corrections due to non-zero theta_{13} and non-maximal theta_{23} are
given. The first order correction is universal as it appears in basically all
ratios. We study in detail its dependence on theta_{13}, theta_{23} and the CP
phase, finding that the dependence on theta_{23} is strongest. The flavor
compositions for the considered neutrino sources are evaluated in terms of this
correction. A measurement of a flux ratio is a clean measurement of the
universal correction (and therefore of theta_{13}, theta_{23} and delta) if the
zeroth order ratio does not depend on theta_{12}. This favors pion sources over
the other cases, which in turn are good candidates to probe theta_{12}. The
only situations in which the universal correction does not appear are certain
ratios in case of a neutron and muon-damped source, which depend mainly on
theta_{12} and receive only quadratic corrections from the other parameters. We
further show that there are only two independent neutrino oscillation
probabilities, give the allowed ranges of the considered flux ratios and of all
probabilities, and show that none of the latter can be zero or one.Comment: 29 pages, 8 figures. Minor changes, to appear in JCA
The Inert Doublet Model: an Archetype for Dark Matter
The Inert Doublet Model (IDM), a two Higgs extension of the Standard Model
with an unbroken symmetry, is a simple and yet rich model of dark matter.
We present a systematic analysis of the dark matter abundance and investigate
the potentialities for direct and gamma indirect detection. We show that the
model should be within the range of future experiments, like GLAST and ZEPLIN.
The lightest stable scalar in the IDM is a perfect example, or archetype of a
weakly interacting massive particle.Comment: 12 pages, 7 figures, references added and typos correcte
Physics Potential of the ICAL detector at the India-based Neutrino Observatory (INO)
The upcoming 50 kt magnetized iron calorimeter (ICAL) detector at the
India-based Neutrino Observatory (INO) is designed to study the atmospheric
neutrinos and antineutrinos separately over a wide range of energies and path
lengths. The primary focus of this experiment is to explore the Earth matter
effects by observing the energy and zenith angle dependence of the atmospheric
neutrinos in the multi-GeV range. This study will be crucial to address some of
the outstanding issues in neutrino oscillation physics, including the
fundamental issue of neutrino mass hierarchy. In this document, we present the
physics potential of the detector as obtained from realistic detector
simulations. We describe the simulation framework, the neutrino interactions in
the detector, and the expected response of the detector to particles traversing
it. The ICAL detector can determine the energy and direction of the muons to a
high precision, and in addition, its sensitivity to multi-GeV hadrons increases
its physics reach substantially. Its charge identification capability, and
hence its ability to distinguish neutrinos from antineutrinos, makes it an
efficient detector for determining the neutrino mass hierarchy. In this report,
we outline the analyses carried out for the determination of neutrino mass
hierarchy and precision measurements of atmospheric neutrino mixing parameters
at ICAL, and give the expected physics reach of the detector with 10 years of
runtime. We also explore the potential of ICAL for probing new physics
scenarios like CPT violation and the presence of magnetic monopoles.Comment: 139 pages, Physics White Paper of the ICAL (INO) Collaboration,
Contents identical with the version published in Pramana - J. Physic
WIMP dark matter, Higgs exchange and DAMA
In the WIMP scenario, there is a one-to-one relation between the dark matter
(DM) relic density and spin independent direct detection rate if both the
annihilation of DM and its elastic scattering on nuclei go dominantly through
Higgs exchange. In particular, for DM masses much smaller than the Higgs boson
mass, the ratio of the relevant cross sections depends only on the DM mass.
Assuming DM mass and direct detection rate within the ranges allowed by the
recent DAMA collaboration results -taking account of the channelling effect on
energy threshold and the null results of the other direct detection
experiments- gives a definite range for the relic density. For scalar DM
models, like the Higgs portal models or the inert doublet model, the relic
density range turns out to be in agreement with WMAP. This scenario implies
that the Higgs boson has a large branching ratio to pairs of DM particles, a
prediction which might challenge its search at the LHC.Comment: 5 pages, 5 figures. Matches the published version. One figure
modified. Conclusions unchange