94 research outputs found
Energy and Flux Measurements of Ultra-High Energy Cosmic Rays Observed During the First ANITA Flight
The first flight of the Antarctic Impulsive Transient Antenna (ANITA)
experiment recorded 16 radio signals that were emitted by cosmic-ray induced
air showers. For 14 of these events, this radiation was reflected from the ice.
The dominant contribution to the radiation from the deflection of positrons and
electrons in the geomagnetic field, which is beamed in the direction of motion
of the air shower. This radiation is reflected from the ice and subsequently
detected by the ANITA experiment at a flight altitude of 36km. In this paper,
we estimate the energy of the 14 individual events and find that the mean
energy of the cosmic-ray sample is 2.9 EeV. By simulating the ANITA flight, we
calculate its exposure for ultra-high energy cosmic rays. We estimate for the
first time the cosmic-ray flux derived only from radio observations. In
addition, we find that the Monte Carlo simulation of the ANITA data set is in
agreement with the total number of observed events and with the properties of
those events.Comment: Added more explanation of the experimental setup and textual
improvement
The Antarctic Impulsive Transient Antenna Ultra-high Energy Neutrino Detector Design, Performance, and Sensitivity for 2006-2007 Balloon Flight
We present a detailed report on the experimental details of the Antarctic
Impulsive Transient Antenna (ANITA) long duration balloon payload, including
the design philosophy and realization, physics simulations, performance of the
instrument during its first Antarctic flight completed in January of 2007, and
expectations for the limiting neutrino detection sensitivity. Neutrino physics
results will be reported separately.Comment: 50 pages, 49 figures, in preparation for PR
Ab initio calculations of optical properties of silver clusters: cross-over from molecular to nanoscale behavior
Electronic and optical properties of silver clusters were calculated using
two different \textit{ab initio} approaches: 1) based on all-electron
full-potential linearized-augmented plane-wave method and 2) local basis
function pseudopotential approach. Agreement is found between the two methods
for small and intermediate sized clusters for which the former method is
limited due to its all-electron formulation. The latter, due to non-periodic
boundary conditions, is the more natural approach to simulate small clusters.
The effect of cluster size is then explored using the local basis function
approach. We find that as the cluster size increases, the electronic structure
undergoes a transition from molecular behavior to nanoparticle behavior at a
cluster size of 140 atoms (diameter \,nm). Above this cluster size
the step-like electronic structure, evident as several features in the
imaginary part of the polarizability of all clusters smaller than
Ag, gives way to a dominant plasmon peak localized at
wavelengths 350\,nm 600\,nm. It is, thus, at this length-scale
that the conduction electrons' collective oscillations that are responsible for
plasmonic resonances begin to dominate the opto-electronic properties of silver
nanoclusters
Tumours and Tumour-Like Lesions of the Hip in the Paediatric Age: A Review of the Rizzoli Experience
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