[PDF] Top 20 Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory
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Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory
... PN-II-RU-PD-2011-3-0062, the Minister of National Education, Programme Space Tech- nology and Advanced Research (STAR), Grant ...and The Grainger Foun- dation, USA; NAFOSTED, Vietnam; Marie Curie- ... See full document
9
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
... of the properties of the highest- energy cosmic rays has grown enormously over the last 12 years with the advent of data from the Pierre Auger Observatory ... See full document
21
Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above 1017.8 eV
... 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, ...describe the ... See full document
25
Ultrahigh-Energy Neutrino Follow-Up of Gravitational Wave Events GW150914 and GW151226 with the Pierre Auger Observatory
... With the surface detector (SD) of the Pierre Auger Ob- servatory [20] we can identify neutrino-induced air show- ers in the energy range above 100 PeV ...[21]. ... See full document
10
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 method in a full detector ... See full document
8
Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above $10^{17.8}$ eV
... on the discussion of the first two moments of the X max distribution, hX max i and σ(X max ), which are listed in ...together with their statistical and systematic uncertainties. The ... See full document
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High-energy interactions at the Pierre Auger Observatory
... (UHECRs) with the atoms of the atmosphere can occur at center-of-mass energies that surpass 100 TeV, while present human-made accelera- tors go up to 13 ...explore hadronic ... See full document
7
Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory
... to the shower energies under ...on the final result since the electromagnetic component of the shower, which is the most relevant part for neutrino iden- tification, is believed ... See full document
15
Constraints and measurements of hadronic interactions in extensive air showers with the Pierre Auger Observatory
... The Pierre Auger Observatory has unique capabilities to make measurements of the highest energy hadronic interactions and to constraint the models that attempt to ... See full document
9
Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory
... ( The Pierre Auger Collaboration 2017b ), since, otherwise, systematic modulations of the rates as a function of the hour of the day or of the season, and hence also as a ... See full document
16
Ultrahigh Energy Neutrinos at the Pierre Auger Observatory
... detected with a variety of techniques [13, ...observed with arrays of detectors at ground level that are currently being used to measure extensive showers produced by cosmic rays ... See full document
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Improved limit to the diffuse flux of ultrahigh energy neutrinos from the Pierre Auger Observatory
... PN-II-RU-PD-2011-3-0062, the Minister of National Education, Programme Space Technology and Advanced Research (STAR), Grant ...0450696, The Grainger Foundation, USA; NAFOSTED, Vietnam; Marie ... See full document
14
Highlights from the Pierre Auger Observatory
... that the cut-off region represents more a consequence of the source maximal acceleration energy (of the order of 4 EeV for proton) than a propagation effect as expected from the GZK ...account ... See full document
9
Depth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition implications
... eV measured by Auger [4] is used to determine whether it can be described satisfactorily by an evolution of compo- sition with ...of the two most stable types of particles, ... See full document
13
The Pierre Auger Cosmic Ray Observatory
... RU-PD-2011-3-0062, the Minister of National Education, Programme for research - Space Technology and Advanced Research - STAR, project number 83/2013, Roma- nia; Slovenian Research Agency, Slovenia; Comunidad de ... See full document
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Search for ultrarelativistic magnetic monopoles with the Pierre Auger Observatory
... good-quality showers. We required the zenith an- gle of the shower to be < 60 ◦ , and the distance of the shower core to the SD station with the highest signal ... See full document
12
Search for photons with energies above 10$^{18}$ eV using the hybrid detector of the Pierre Auger Observatory
... – the Australian Research Council; Brazil – Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq); Financiadora de Estudos e Projetos (FINEP); Fundação de Amparo à Pesquisa do Estado de Rio de ... See full document
23
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
... Mpc, the maximum propagation distance of the most en- ergetic particle in this ...to the continuous energy loss approximation the maximum distance is here a hard limit and these simulations ... See full document
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Upper limit on the diffuse flux of ultrahigh energy tau neutrinos from the pierre auger observatory
... of the Czech Republic; Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Re´gional Ile-de-France, De´partement Physique Nucle´aire et Corpusculaire (PNC-IN2P3/CNRS), ... See full document
7
A targeted search for point sources of EeV photons with the Pierre Auger Observatory
... accelerated at discrete sources within the Galaxy or its neighborhood. The null results reported here leave open the possibility that EeV pro- tons, as observed on Earth, are of extragalactic ... See full document
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