#### Filter Results:

- Full text PDF available (27)

#### Publication Year

2001

2018

- This year (1)
- Last 5 years (19)
- Last 10 years (34)

#### Publication Type

#### Co-author

#### Journals and Conferences

Learn More

- Alar Aab, Fernando Arqueros Martínez, +481 authors Francesca A. Zuccarello
- 2014

We report a study of the distributions of the depth of maximum, X-max, of extensive air-shower profiles with energies above 10(17.8) eV as observed with the fluorescence telescopes of the Pierre… (More)

- Fernando Arqueros Martínez, Massimo Aglietta, +497 authors B. Zamorano Garcia
- 2012

The Pierre Auger Observatory is exploring the potential of the radio detection technique to study extensive air showers induced by ultra-high energy cosmic rays. The Auger Engineering Radio Array… (More)

The Pierre Auger Observatory has begun a major Upgrade of its already impressive capabilities, with an emphasis on improved mass composition determination using the surface detectors of the… (More)

We consider a nonlinear Schrodinger equation with a nonlinearity of the form V (x)g(u). Assuming that V (x) behaves like |x|−b at infinity and g(s) like |s|p around 0, we prove the existence and… (More)

- Alar Aab, Fernando Arqueros Martínez, +481 authors Francesca A. Zuccarello
- 2014

Using the data taken at the Pierre Auger Observatory between December 2004 and December 2012, we have examined the implications of the distributions of depths of atmospheric shower maximum (X-max),… (More)

Abstract We consider the nonlinear Schrodinger equation in R d i ∂ t u + Δ u + f ( u ) = 0 . For d ⩾ 2 , this equation admits traveling wave solutions of the form e i ω t Φ ( x ) (up to a Galilean… (More)

- The Pierre Auger Collaboration P. Abreu, Massimo Aglietta, +497 authors B. Zamorano Garcia
- 2012

The Pierre Auger Observatory is a facility built to detect air showers produced by cosmic rays above 10^17 eV. During clear nights with a low illuminated moon fraction, the UV fluorescence light… (More)

- Stefan Le Coz
- 2007

In this note we give an alternative, shorter proof of the classical result of Berestycki and Cazenave on the instability by blow-up for the standing waves of some nonlinear Schr\"odinger equations.

A flux of neutrons from an astrophysical source in the Galaxy can be detected in the Pierre Auger Observatory as an excess of cosmic-ray air showers arriving from the direction of the source. To… (More)

AMIGA (Auger Muons and Infill for the Ground Array) is an upgrade of the Pierre Auger Observatory to extend its range of detection and to directly measure the muon content of the particle showers. It… (More)