[PDF] Top 20 Experimental Summary: Very High Energy Cosmic Rays and their Interactions
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Experimental Summary: Very High Energy Cosmic Rays and their Interactions
... by high statistics measurements from ARGO-YBJ and from IceTop in the southern ...with energy and appears to persist to beyond PeV ...Galactic cosmic-ray distribution, which must be incorpo- rated ... See full document
10
Recent results from the Pierre Auger Observatory on the mass composition and hadronic interactions of ultra-high energy cosmic rays
... Abstract. Recent results on the mass composition and hadronic interactions of ultra-high energy cosmic rays (UHECR) obtained at the Pierre Auger Observatory are reviewed. Different ... See full document
8
Measurement of ultra-high energy cosmic rays: An experimental summary and prospects
... this energy range, has not associated the observed spectral features with a particular physics ...Auger’s high statistics spectrum data, and measurements of X max and RMS(X max ...the high ... See full document
18
High energy cosmic ray interactions and UHECR composition problem
... of high energy collisions of hadrons and nuclei, which describe interactions of both primary CRs and of the produced secondary hadrons with nuclei of the ...ultra-high energy ... See full document
10
The GRAND project and GRANDProto300 experiment
... decades-long experimental e ff orts. Ultra-high energy neutrinos could be an extremely valuable tool to answer this question: thanks to their very low interaction probabil- ity and neutral ... See full document
7
TeV Blazars as the Sources of Ultra High Energy Cosmic Rays
... low energy peak, BL Lacertae objects are fur- ther subdivided into low-, intermediate- and high-frequency peaked BL Lac objects, and they are abbreviated as LBL, IBL and HBL, ...The high ... See full document
12
LHCf and connection to high energy cosmic rays
... ultra high energy cosmic ...hadron interactions at such high ...hadron interactions relevant for air ...at very forward region in LHC to verify the forward energy ... See full document
6
The ATLAS Hadronic Physics Program and High Energy Cosmic Rays
... strong interactions at low ...on high-pT phenomena due to underlying events and event pileup effects and are therefore of growing importance for future LHC ... See full document
7
Ultra High Energy Cosmic Rays: Origin, Composition and Spectrum
... is very important a detailed modelling of UHECR propagation in the intergalactic medium, which is mainly conditioned by the interaction with astrophysical photon backgrounds and intergalac- tic magnetic fields, ... See full document
6
Ultra-high energy cosmic rays: 40 years retrospective of continuous observations at the Yakutsk array: Part 2. Mass composition of cosmic rays at ultra high energies
... In this review, we used the work of the Yakutsk group in which was introduced an estimation of the mass composition of cosmic rays at ultrahigh energies [1–5]. In these studies we analyzed the ... See full document
5
Neutrinos from colliding wind binaries: future prospects for PINGU and ORCA
... ray energy spectra from stellar environments are believed to be of too low energy in order to explain the total flux of cosmic rays up to the knee: the observed cosmic ray energy ... See full document
5
Observation of ultra-high energy cosmic rays with the Telescope Array experiment
... m) [18]. The left panel of figure 5 shows the ratio of the SD signal of the experimental data to the MC prediction as a function of a lateral distance R [18]. The result on the high muon purity condition ... See full document
9
Cosmic rays in the knee energy range
... the cosmic ray spectrum ex- pected: (i) A knee of the heavy component which is either expected (depending on the model) at the position of the first knee scaled with Z (the charge) or alternatively with A (the ... See full document
7
Very-high-energy astrophysical neutrinos with IceCube
... a very-high-energy neutrino telescope in operation at the South ...in very transparent Antarctic ...the very low neutrino-matter interaction cross-section, the instrumented volume is ... See full document
8
Nucleus-nucleus interactions in very-high-energy cosmic ray experiments
... the experimental points are in a good agreement with calculations for normal energy spectrum and composition of cosmic rays, and even the knee in the interval 1-10 PeV is ...at very ... See full document
13
Observation of high-energy cosmic rays by very inclined muon bundles in the NEVOD-DECOR experiment
... 5, experimental LMDS reconstructed from DECOR data are compared with CORSIKA-based calculations for 4 different zenith angles (35 ◦ , 50 ◦ , 65 ◦ , and 78 ◦ ...type energy spectrum with differential slope ... See full document
5
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
10
Ankle Phenomenon in the Cosmic Ray Energy Spectrum
... knee energy range (at 3 PeV) may not be stable, as in the case of the standard ...knee energy phenomenon is observed when cosmic rays are emitted from ... See full document
5
Status and perspectives of the radio detection of highenergy cosmic rays
... incoming cosmic rays, namely their arrival direction, energy and particle type (nuclear ...the cosmic ray is obtained through a precise measurement of the arrival time of the wavefront at the ... See full document
7
INFN - LNS
... Radio detection of ultra high energy cosmic rays with the Auger Engineering Radio Array. 10:00 - 10:30 Abigail Vieregg[r] ... See full document
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