In these three lectures I discuss the present status of high-energy astroparticle physics including Ultra-High-Energy Cosmic Rays (UHECR), high-energy gamma rays, and neutrinos. The first lecture is devoted to ultra-high-energy cosmic rays. After a brief introduction to UHECR I discuss the acceleration of charged particles to highest energies in the astrophysical objects, their propagation in the intergalactic space, recent observational results by the Auger and HiRes experiments, anisotropies of UHECR arrival directions, and secondary gamma rays produced by UHECR. In the second lecture I review recent results on TeV gamma rays. After a short introduction to detection techniques, I discuss recent exciting results of the H.E.S.S., MAGIC, and...
It is an exciting time to be working at the interface between physics and astron-omy. Experiments bu...
This is a written version of a series of lectures aimed at graduate students in astrophysics/particl...
We briefly review the main channels of gamma ray and neutrino production due to the propagation of ul...
29 pages, Lectures given at the 5th CERN-Latin-American School of High-Energy Physics, Recinto Quira...
The origin of the highest energy cosmic rays (UHECR) with energies above 1000 TeV, is still unknown....
The propagation of UHECR nuclei for A = 1 (protons) to A = 56 (iron) from cosmological sources thr...
The origin of the ultra high energy cosmic rays (UHECR) with energies above E > 10 17 eV, is still u...
The origin of the highest energy cosmic rays (UHECR) with energies above 1000 TeV, is still unknown....
We review the physics of the highest energy cosmic rays, i.e. those astrophysical particles with ene...
44 latex pages, 8 postscript figures included; based on lectures given at summer schools in Kopenhag...
We outline the current situation in ultrahigh energy (UHE) cosmic ray physics, pointing out the rema...
The construction of large volume detectors of high energy, >1 TeV, neutrinos is mainly driven by the...
Presents three complementary lectures on very-high-energy astrophysics given by worldwide leaders in...
In the last century, astronomy evolved from optical observation to the multi-wavelength study of cel...
Summary. — High-energy photons are a powerful probe for astrophysics and for fundamental physics und...
It is an exciting time to be working at the interface between physics and astron-omy. Experiments bu...
This is a written version of a series of lectures aimed at graduate students in astrophysics/particl...
We briefly review the main channels of gamma ray and neutrino production due to the propagation of ul...
29 pages, Lectures given at the 5th CERN-Latin-American School of High-Energy Physics, Recinto Quira...
The origin of the highest energy cosmic rays (UHECR) with energies above 1000 TeV, is still unknown....
The propagation of UHECR nuclei for A = 1 (protons) to A = 56 (iron) from cosmological sources thr...
The origin of the ultra high energy cosmic rays (UHECR) with energies above E > 10 17 eV, is still u...
The origin of the highest energy cosmic rays (UHECR) with energies above 1000 TeV, is still unknown....
We review the physics of the highest energy cosmic rays, i.e. those astrophysical particles with ene...
44 latex pages, 8 postscript figures included; based on lectures given at summer schools in Kopenhag...
We outline the current situation in ultrahigh energy (UHE) cosmic ray physics, pointing out the rema...
The construction of large volume detectors of high energy, >1 TeV, neutrinos is mainly driven by the...
Presents three complementary lectures on very-high-energy astrophysics given by worldwide leaders in...
In the last century, astronomy evolved from optical observation to the multi-wavelength study of cel...
Summary. — High-energy photons are a powerful probe for astrophysics and for fundamental physics und...
It is an exciting time to be working at the interface between physics and astron-omy. Experiments bu...
This is a written version of a series of lectures aimed at graduate students in astrophysics/particl...
We briefly review the main channels of gamma ray and neutrino production due to the propagation of ul...