[PDF] Top 20 Preditores de percepção de saúde em adolescentes escolares
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Ultra-high energy cosmic rays and the strongest AGN flares
... the AGN engine, or in the magnetized intracluster ...of cosmic rays is generated by large number of flares with only small fraction of them pointing at ... See full document
13
Ultra-high energy cosmic rays: Setting the stage
... the cosmic ray flux beyond the GZK cutoff in addition to confirming the ankle ...highest energy event at 2 × 10 20 eV ...and energy of 3 × 10 20 eV ...and cosmic strings to violation of ... See full document
17
TeV Blazars as the Sources of Ultra High Energy Cosmic Rays
... to high energy gamma rays, and they show variability in flux at all wavelengths as well as spectral shape on time scales ranging from months to a few ...gamma rays from Mkn 421 with the ... See full document
11
Experimental Summary: Very High Energy Cosmic Rays and their Interactions
... A comprehensive review of direct measurements of cos- mic rays was presented by R. Sparvoli [1]. Clearly, data from recent experiments have reached a new level of qual- ity and quantity, with PAMELA taking the ... See full document
29
ATLAS and ultra high energy cosmic ray physics
... In particular, multi-muon events where the muon tracks were parallel and grouped together, called muon bundles, were first highlighted by the Cosmo-LEP activity. They found that muon bundles with very large muon ... See full document
47
The ATLAS Hadronic Physics Program and High Energy Cosmic Rays
... A fast timing system that can precisely measure the time difference between outgoing scattered protons is a key component of the AFP detector. The time difference is equivalent to a constraint on the event vertex, thus ... See full document
5
Particle spectra and mass composition in the ultra-high energy region in the framework of the Galactic origin of cosmic rays
... probability of reaching the observer at a distance, r, from the source for a particle with a certain energy and atomic number without scattering. This factor has a power-law asymptotic with respect to r (the L´evy ... See full document
23
Effects of Mobile Radiations and its Prevention
... These high amounts of cortisol suppress the immune system, blood sugar levels rise and insomnia can ...rage, high blood pressure, loss of blood sugar control, decreased thyroid function and weight gain can ... See full document
14
Ultra-high-energy cosmic rays mass composition studies with the Telescope Array Surface Detector data
... Figure 1 shows ξ parameter distribution histograms for all the energy bins. In the Figure 2 the average atomic mass ln A is shown in comparison with the Telescope array hybrid re- sults [13]. In the Figure 3 the ... See full document
33
Neutrino Sources from a Multi-Messenger Perspective
... On September 22nd, 2017 IceCube observed a high-energy muon that entered the detector from a direction a few degrees below the Horizon (see left panel of Fig. 2). These rare type of events trigger alerts ... See full document
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Neutrinos from colliding wind binaries: future prospects for PINGU and ORCA
... hadronic cosmic rays interact with a matter target lo- cally at the cosmic ray acceleration site, neutral particles like gamma-rays and neutrinos are produced via pion- and kaon decay from the ... See full document
6
Recent results from the Pierre Auger Observatory on the mass composition and hadronic interactions of ultra-high energy cosmic rays
... the energy of the primary particle are based on the detection of fluorescence light emitted by the molecules of atmospheric nitrogen due to their interactions with the shower ... See full document
6
Recent results from ANTARES
... Abstract. Operating 40 km off the coast of France since 2007, the ANTARES detector is the largest deep-sea neutrino telescope in the Northern Hemisphere with an instrumented volume of more than 0.01 cubic kilometers. It ... See full document
6
Cosmic rays in the knee energy range
... the cosmic ray spectra obtained by direct measurements for the different ...galactic cosmic rays originated from a single acceleration and propagation process within our Milky Way which is valid up ... See full document
80
Study of muons in extensive air showers from ultra-high energy cosmic rays measured with the Telescope Array experiment
... of ultra-high energy cosmic rays (UHECRs) has been a long-standing mystery of ...the energy spectrum, anisotropy and mass composition of cosmic ... See full document
8
Detecting ultra-high energy cosmic rays from space with unprecedented acceptance: objectives and design of the JEM-EUSO mission
... Fig. 7. Data Reduction scheme. Each of the ' 6000 Multi-Anode Photo Multiplier (MAPMT) of the focal surface is read by an ASIC digitizing the photoelectron signal. A 6*6 array of MAPMT is present and read by each of the ... See full document
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FAMOUS – A prototype silicon photomultiplier telescope for the fluorescence detection of ultra-high-energy cosmic rays
... a high number of cells on a certain area, but smaller cell pitches lead to more dead space between the individual ...a high dynamic range and the demand for a high PDE are ... See full document
22
Ultra High Energy Cosmic Rays: Origin, Composition and Spectrum
... the redshift of the first stars (pop III). Once produced at these cosmological distances neutrinos travel toward the observer almost freely, except for the adiabatic energy losses and flavour oscillations, the ... See full document
21
Observation of ultra-high energy cosmic rays with the Telescope Array experiment
... of cosmic rays follows power law distribution, and due to low flux, the origin of UHECR is ...primary cosmic rays with atmo- spheric particles, which are called air ...the energy and ... See full document
78
Measurement of ultra-high energy cosmic rays: An experimental summary and prospects
... ln A is statistically not consistent with a constant value of ln A, whereas the same plots by other experiments are statistically consistent with both constant and changing values of ln A with respect to log(E) (see Fig. ... See full document
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