[PDF] Top 20 Hadronic physics with the Pierre Auger Observatory
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Hadronic physics with the Pierre Auger Observatory
... which the number of charged particles reaches its maximum in the air shower, X max , is sensi- tive to the mass composition of the primaries through the depth of the first ... See full document
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Ultrahigh-Energy Neutrino Follow-Up of Gravitational Wave Events GW150914 and GW151226 with the Pierre Auger Observatory
... is the total search pe- riod interval. Here it is assumed that the sources of GW events emit UHE neutrinos continuously during the search ...period. The constraints on spectral fluence are ... See full document
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Azimuthal Asymmetry in the Risetime of the Surface Detector Signals of the Pierre Auger Observatory
... showers with a duty cycle of nearly ...water. The water volume is viewed by three 9” photomultiplier tubes ...(from the an- ode and from the amplified dynode) from each of PMTs are digitized ... See full document
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Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory
... while the electromagnetic compo- nent develops, the time spread of the particles in the shower front is large ( ...When the shower becomes old, most of the particles in ... See full document
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Combined fit of spectrum and composition data as measured by the Pierre Auger Observatory
... 0450696; The Grainger Foundation; Marie Curie-IRSES/EPLANET; European Particle Physics Latin American Network; European Union 7th Framework Pro- gram, Grant ... 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
... – the Australian Research Coun- cil; Brazil – Conselho Nacional de Desenvolvimento Cient´ıfico e Tecnol ´ogico (CNPq); Financiadora de Es- tudos e Projetos (FINEP); Fundac¸˜ao de Amparo `a Pesquisa do Estado de ... See full document
21
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 ...showers with a hybrid detection ...grid, with a distance of ... See full document
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Measurement of the proton-air cross-section at $\sqrt{s}=57$ TeV with the Pierre Auger Observatory
... for the inelastic and total cross-sections include contributions from the elastic slope parameter, from λ, from the description of the nuclear density profile, and from cross-checking these ... See full document
9
Search for photons with energies above 10$^{18}$ eV using the hybrid detector of the Pierre Auger Observatory
... 0450696; The Grainger Foundation; Marie Curie-IRSES/EPLANET; European Particle Physics Latin American Network; European Union 7th Framework Pro- gram, Grant ... See full document
23
Techniques for Measuring Aerosol Attenuation using the Central Laser Facility at the Pierre Auger Observatory
... : The Pierre Auger Observatory in Malargüe, Argentina, is designed to study the prop- erties of ultra-high energy cosmic rays with energies above 10 18 ...from the FD, ... See full document
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Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory
... quantify the distinctive features of hadronic and deeply penetrating showers induced by neutrinos at large zenith angle, improve the separation between the samples and enhance the ... See full document
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Improved limit to the diffuse flux of ultrahigh energy neutrinos from the Pierre Auger Observatory
... Argentina; the Australian Research Coun- cil; Conselho Nacional de Desenvolvimento Cient´ıfico e Tecnol´ ogico (CNPq), Financiadora de Estudos e Pro- jetos (FINEP), Funda¸ c˜ ao de Amparo ` a Pesquisa do Estado de ... See full document
14
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
... estimate the uncertainty on the measurement, we repeatedly vary the energy and arrival directions of all events detected with the Pierre Auger Observatory above E = ... See full document
16
Multi-resolution anisotropy studies of ultrahigh-energy cosmic rays detected at the Pierre Auger Observatory
... 0450696; The Grainger Foundation; Marie Curie-IRSES/EPLANET; European Particle Physics Latin American Network; European Union 7th Framework Program, Grant ... See full document
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Muons in air showers at the Pierre Auger Observatory: Mean number in highly inclined events
... and the Czech Science Founda- tion grant 14-17501S, Czech Republic; Centre de Cal- cul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil R´egional Ile-de-France, D´epartement Physique ... See full document
12
Upper limit on the diffuse flux of ultrahigh energy tau neutrinos from the pierre auger observatory
... in the relevant energy range, namely, the interaction cross-section, the energy loss, and the ...polarization. The main uncertainty in these comes from the QCD structure ... See full document
7
Depth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition implications
... improves the fits for all hadronic interaction ...of the energy ...brings the models into remarkable agreement in their predictions of the protons and iron nuclei contributions despite ... See full document
13
Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory
... that the propagation of particles was performed under the assump- tion that UHECRs are ...fact, the propagation for iron nuclei and its secondaries, mainly determined by nuclear photodisintegration ... See full document
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Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth
... in the atmosphere, the trans- verse momentum of secondary particles makes them deviate from the shower axis on their way to the ...Unlike the electromagnetic component of the ... See full document
15
Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory
... DGAPA-UNAM; The Netherlands – Ministry of Edu- cation, Culture and Science; Netherlands Organisation for Scientific Research (NWO); Dutch national e-infrastructure with the support of SURF ... See full document
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