560 research outputs found
Measurement of the energy spectrum of cosmic rays using the Pierre Auger Observatory
The flux of cosmic rays above 1018 eV has been measured with
unprecedented precision at the Pierre Auger Observatory. Two analysis techniques have been used to extend the spectrum downwards from 3×1018 eV, with the lower energies being explored using a unique technique that exploits the hybrid strengths of the instrument. The spectral features are also presented
Propagation of UHECRs in cosmological backgrounds: some results from SimProp
Ultra-High-Energy Cosmic Ray (UHECR) nuclei propagating in cosmological
radiation backgrounds produce secondary particles detectable at Earth. SimProp
is a one dimensional code for extragalactic propagation of UHECR nuclei,
inspired by the kinetic approach of Aloisio et al. As in this approach, only a
subset of nuclei and nuclear channels are used as representative. We discuss
the validation of the code and present applications to UHECR experimental
results. In particular we present the expected fluxes of neutrinos produced in
some astrophysical scenario.Comment: Poster presented by A. Di Matteo at the 33rd International Cosmic Ray
Conference, Rio De Janeiro (Brasil) July 2-9 201
Cosmogenic neutrinos and ultra-high energy cosmic ray models
We use an updated version of {\it SimProp}, a Monte Carlo simulation scheme
for the propagation of ultra-high energy cosmic rays, to compute cosmogenic
neutrino fluxes expected on Earth in various scenarios. These fluxes are
compared with the newly detected IceCube events at PeV energies and with recent
experimental limits at EeV energies of the Pierre Auger Observatory. This
comparison allows us to draw some interesting conclusions about the source
models for ultra-high energy cosmic rays. We will show how the available
experimental observations are almost at the level of constraining such models,
mainly in terms of the injected chemical composition and cosmological evolution
of sources. The results presented here will also be important in the evaluation
of the discovery capabilities of the future planned ultra-high energy cosmic
ray and neutrino observatories.Comment: 15 pages, 8 figures, some reference added, version accepted for
publication in JCA
Detection of GRB signals with Fluorescence Detectors
Gamma Ray Bursts are being searched in many ground based experiments
detecting the high energy component (GeV TeV energy range) of the photon
bursts. In this paper, Fluorescence Detectors are considered as possible
candidate devices for these searches. It is shown that the GRB photons induce
fluorescence emission of UV photons on a wide range of their spectrum. The
induced fluorescence flux is dominated by GRB photons from 0.1 to about 100 MeV
and, once the extinction through the atmosphere is taken into account, it is
distributed over a wide angular region. This flux can be detected through a
monitor of the diffuse photon flux, provided that its maximum value exceeds a
threshold value, that is primarily determined by the sky brightness above the
detector. The feasibility of this search and the expected rates are discussed
on the basis of the current GRB observations and the existing fluorescence
detectors.Comment: 16 pages 9 eps figure
Testing Lorentz invariance violation using cosmogenic neutrinos
Secondary messengers such as neutrinos and photons are expected to be
produced in interactions of ultra-high-energy cosmic rays (UHECRs) with
extragalactic background photons. Their propagation could be altered by the
effects of Lorentz invariance violation. In this work, we have developed an
extension of the SimProp code that includes some Lorentz-violating scenarios
affecting the propagation of neutrinos. We present the corresponding expected
cosmogenic neutrino fluxes for three different astrophysical scenarios for the
production of UHECRs. These results can be used to put constraints on the scale
of Lorentz violation in the neutrino sector.Comment: 8 pages. Proceedings for the 38th International Cosmic Ray Conference
(ICRC) 202
Ultra High Energy Cosmic Rays: Anisotropies and Spectrum
The recent results of the Pierre Auger Observatory on the possible
correlation of Ultra High Energy Cosmic Rays events and several nearby discrete
sources could be the starting point of a new era with charged particles
astronomy. In this paper we introduce a simple model to determine the effects
of any local distribution of sources on the expected flux. We consider two
populations of sources: faraway sources uniformly distributed and local point
sources. We study the effects on the expected flux of the local distribution of
sources, referring also to the set of astrophysical objects whose correlation
with the Auger events is experimentally claimed.Comment: 17 pages, 13 eps figures, version accepted for publication in
Astroparticle Physic
SimProp: a Simulation Code for Ultra High Energy Cosmic Ray Propagation
A new Monte Carlo simulation code for the propagation of Ultra High Energy
Cosmic Rays is presented. The results of this simulation scheme are tested by
comparison with results of another Monte Carlo computation as well as with the
results obtained by directly solving the kinetic equation for the propagation
of Ultra High Energy Cosmic Rays. A short comparison with the latest flux
published by the Pierre Auger collaboration is also presented.Comment: 19 pages, 12 eps figures, version accepted for publication in JCA
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