Ultrahigh energy cosmic rays and new particle physics

The current status of the UltraHigh Energy Cosmic Ray (UHE: CR) enigma and several proposed solutions involving particle physics beyond the standard model are discussed. Emphasis is given to top-down models, and as a main example, supermassive dark matter as galactic source for UHE CR and the status of its experimental signatures (galactic anisotropy, chemical composition and clustering) is reviewed. Then different approaches to calculate fragmentation spectra of supermassive particles are discussed. Finally, it is argued that UHE neutrinos cannot be - neither directly or indirectly - responsible for the observed UHE CR events.