AbstractThe characteristics of extensive air showers are sensitive to the details of hadronic interactions at energies and in kinematic regions beyond those tested by human-made accelerators. Uncertainties on extrapolations of the hadronic interaction models in these regions hamper the interpretation of the ultra high energy cosmic ray data in terms of primary mass composition. We report on how the Pierre Auger Observatory is able to constrain the hadronic interaction models by measuring the muon content and muon production depth of air showers and also by measuring the proton-air cross section for particle production at a center-of-mass energy per nucleon of 57 TeV
The surface detector array of the Pierre Auger Observatory provides information about the longitudin...
Published version. Added journal reference and DOI. Added Report NumberInternational audienceUltrahi...
The characteristics of an extensive air shower derive from both the mass of the primary ultra-high-e...
The characteristics of extensive air showers are sensitive to the details of hadronic interactions a...
AbstractThe characteristics of extensive air showers are sensitive to the details of hadronic intera...
The hybrid design of the Pierre Auger Observatory allows for the measurement of a number of properti...
Extensive air showers are complex objects, resulting of billions of particle reactions initiated by ...
Extensive air showers initiated by ultra-high energy cosmic rays are sensitive to the details of had...
International audienceThe development of an extensive air shower depends not only on the nature of t...
The muon content of extensive air showers produced by ultra-high energy cosmic rays is an observable...
The Pierre Auger Observatory is the largest detector of ultra-high energy cosmic rays (UHECR) in the...
Extensive air showers are the result of billions of particle reactions initiated by single cosmic ra...
The surface detector array of the Pierre Auger Observatory provides information about the longitudin...
Published version. Added journal reference and DOI. Added Report NumberInternational audienceUltrahi...
The characteristics of an extensive air shower derive from both the mass of the primary ultra-high-e...
The characteristics of extensive air showers are sensitive to the details of hadronic interactions a...
AbstractThe characteristics of extensive air showers are sensitive to the details of hadronic intera...
The hybrid design of the Pierre Auger Observatory allows for the measurement of a number of properti...
Extensive air showers are complex objects, resulting of billions of particle reactions initiated by ...
Extensive air showers initiated by ultra-high energy cosmic rays are sensitive to the details of had...
International audienceThe development of an extensive air shower depends not only on the nature of t...
The muon content of extensive air showers produced by ultra-high energy cosmic rays is an observable...
The Pierre Auger Observatory is the largest detector of ultra-high energy cosmic rays (UHECR) in the...
Extensive air showers are the result of billions of particle reactions initiated by single cosmic ra...
The surface detector array of the Pierre Auger Observatory provides information about the longitudin...
Published version. Added journal reference and DOI. Added Report NumberInternational audienceUltrahi...
The characteristics of an extensive air shower derive from both the mass of the primary ultra-high-e...