Ultrahigh energy cosmic ray air showers probe particle physics at energies beyond the reach of accelerators. Here we introduce a new method to test hadronic interaction models without relying on the absolute energy calibration, and apply it to events with primary energy 6-16 EeV (ECM=110-170 TeV), whose longitudinal development and lateral distribution were simultaneously measured by the Pierre Auger Observatory. The average hadronic shower is 1.33±0.16 (1.61±0.21) times larger than predicted using the leading LHC-tuned models EPOS-LHC (QGSJetII-04), with a corresponding excess of muons.La lista completa de autores que integran el documento puede consultarse en el archivoInstituto de Física La Plat
We measure the energy emitted by extensive air showers in the form of radio emission in the frequenc...
We present the first measurement of the fluctuations in the number of muons in extensive air showers...
We describe the method devised to reconstruct inclined cosmic-ray air showers with zenith angles gre...
Ultrahigh energy cosmic ray air showers probe particle physics at energies beyond the reach of accel...
We present the first measurement of the fluctuations in the number of muons in extensive air showers...
We have studied the structure of hadronic events with a hard, isolated photon in the final state (e+...
The observation of ultrahigh energy neutrinos (UHEs) has become a priority in experimental astropart...
We measure the energy emitted by extensive air showers in the form of radio emission in the frequenc...
In this paper we introduce the concept of Lateral Trigger Probability (LTP) function, i.e., the prob...
The determination of the primary energy of extensive air showers using the fluorescence detection te...
We present a new method for probing the hadronic interaction models at ultra-high energy and extract...
The intrinsic time structure of hadronic showers influences the timing capability and the required i...
We measure the energy emitted by extensive air showers in the form of radio emission in the frequenc...
We present the first measurement of the fluctuations in the number of muons in extensive air showers...
We describe the method devised to reconstruct inclined cosmic-ray air showers with zenith angles gre...
Ultrahigh energy cosmic ray air showers probe particle physics at energies beyond the reach of accel...
We present the first measurement of the fluctuations in the number of muons in extensive air showers...
We have studied the structure of hadronic events with a hard, isolated photon in the final state (e+...
The observation of ultrahigh energy neutrinos (UHEs) has become a priority in experimental astropart...
We measure the energy emitted by extensive air showers in the form of radio emission in the frequenc...
In this paper we introduce the concept of Lateral Trigger Probability (LTP) function, i.e., the prob...
The determination of the primary energy of extensive air showers using the fluorescence detection te...
We present a new method for probing the hadronic interaction models at ultra-high energy and extract...
The intrinsic time structure of hadronic showers influences the timing capability and the required i...
We measure the energy emitted by extensive air showers in the form of radio emission in the frequenc...
We present the first measurement of the fluctuations in the number of muons in extensive air showers...
We describe the method devised to reconstruct inclined cosmic-ray air showers with zenith angles gre...