[PDF] Top 20 Constraints and measurements of hadronic interactions in extensive air showers with the Pierre Auger Observatory
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Constraints and measurements of hadronic interactions in extensive air showers with the Pierre Auger Observatory
... goal of the Pierre Auger Observatory is to unveil the origin and nature of ...number of breakthroughs and some very important steps towards this goal ... See full document
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Inferences on mass composition and tests of hadronic interactions from 0.3 to 100 EeV using the water-Cherenkov detectors of the Pierre Auger Observatory
... following the procedure discussed in section V. The evolution of h ln A i as a function of energy is shown in ...18. In the energy range where the FD ... See full document
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High-energy interactions at the Pierre Auger Observatory
... interaction of Ultra High Energy Cosmic Rays (UHECRs) with the atoms of the atmosphere can occur at center-of-mass energies that surpass 100 TeV, while present human-made ... See full document
7
Particle physics measurements at the highest energies with the Pierre Auger Observatory
... limited in statistics and the SD can be used to extend the available beam energies even further, giving also independent measurements in the overlap ...region. Of ... See full document
7
Measurement of the Proton-Air Cross Section at s√=57 TeV with the Pierre Auger Observatory
... , and EPOS are 523.7, 502.9, 496.7, and 497.7 mb, respectively, with the statistical uncertainty for each of these values being 22 ...mb. The difference of these cross ... See full document
9
Measurement of the Muon Content of EAS With the Pierre Auger Observatory
... The Pierre Auger Observatory is a hybrid detector with the aim of studying the characteristics of the longitudinal and lateral profiles ... See full document
6
Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above 1017.8 eV
... tail of the X max distribution at large values is related to the distribution of the first interactions of the primary particles in the atmosphere ... See full document
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Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above $10^{17.8}$ eV
... tail of the X max distribution at large values is re- lated to the distribution of the first interactions of the pri- mary particles in the atmosphere ... See full document
25
Results of a Self-Triggered Prototype System for Radio-Detection of Extensive Air Showers at the Pierre Auger Observatory
... describe the experimental setup and the results of RAuger, a small radio-antenna array, consisting of three fully autonomous and self-triggered radio-detection stations, ... See full document
28
Ultrahigh Energy Neutrinos at the Pierre Auger Observatory
... detected with a variety of techniques [13, 14]. In particular they can be observed with arrays of detectors at ground level that are currently being used to measure extensive ... See full document
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Probing the radio emission from air showers with polarization measurements
... studied with two different radio-detection setups deployed at the Pierre Auger Observatory the emission around 50 MHz of radio waves from air ...sample of 37 ... See full document
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Azimuthal Asymmetry in the Risetime of the Surface Detector Signals of the Pierre Auger Observatory
... comparison in Fig. 11 of mass values (in terms of hln Ai) obtained from the measurements of (sec θ) max for the two distance ranges to previous mass estimates from ... See full document
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Muon counting using silicon photomultipliers in the AMIGA detector of the Pierre Auger observatory
... The Pierre Auger Obsevatory [ 1 ] is located in the province of Mendoza, Argentina and has an area of 3000 km 2 ...ray showers with a hybrid detection ... See full document
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Measurement of the Depth of Maximum of Extensive Air Showers above 1018 eV
... measurement of both hX max i and rms ðX max Þ using high quality and high statistics data col- lected with the southern site of the Pierre Auger ... See full document
7
Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory
... Center of Excellence, Ministero degli Affari Esteri (MAE), Italy; Consejo Nacional de Ciencia y Tecnolog´ıa (CONACYT) ...Research and Development, Grants ...funds and FEDER funds within Programa ... See full document
9
Reconstruction of inclined air showers detected with the Pierre Auger Observatory
... upon the particular choice of composition and hadronic model made for the reference ...distribution. The proton showers obtained with the QGSJetII-03 model ... See full document
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Hadronic physics with the Pierre Auger Observatory
... is the composition-averaged shower-to-shower ...on the details of hadronic interactions, and in practice is parametrized from the interaction models ...discussion ... See full document
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Interpretation of the Depths of Maximum of Extensive Air Showers Measured by the Pierre Auger Observatory
... for the study of the composition of Ultra High Energy Cosmic Rays (UHECR) are the mean value of the depth of shower maximum, hX max i, and its dispersion, ... See full document
22
Measurement of the average electromagnetic longitudinal shower profile at the Pierre Auger Observatory
... work, the average shape of the longitudinal profile of the air showers in the Pierre Auger Observatory was ...validated the ... See full document
8
Spectral Calibration of the Fluorescence Telescopes of the Pierre Auger Observatory
... convolution of separate reflection or transmission measurements of each optical component used in the first Los Leones telescopes ...[11]. The first end- to-end spectral ... See full document
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