13-16 February 2012
CERN
Europe/Zurich timezone
Home > Timetable > Contribution details
PDF | XML

Simulation of Ultra-High Energy Cosmic Ray Propagation

Presented by Dr. Peter SCHIFFER
Type: poster

Content

A future Ultra-High Energy Cosmic Ray (UHECR) Observatory will provide an unprecedented amount of high quality UHECR data. The astrophysical interpretation of this data requires a detailed Monte Carlo simulation of UHECR propagation. The publicly available code CRPropa allows such a simulation, taking into account all relevant energy losses in ambient photon fields and deflections in structured magnetic fields. In this talk the CRPropa software is introduced, recent developments like the extension to UHE nuclei propagation as well as future challenges are discussed.

Place

Location: CERN
Address: CERN, Geneva

Primary authors

More

Co-authors

More