Semantic Scholar Open Access 2005

Strongly interacting astrophysical neutrinos

M. Ahlers

Abstrak

Abstract The origin and chemical composition of ultrahigh energy cosmic rays is still an open question in astroparticle physics. The observed large-scale isotropy and also direct composition measurements can be interpreted as an extragalactic proton dominance above the ankle at about 10 10  GeV. Photopion production of extragalactic protons in the cosmic microwave background predicts a cut-off at about 5×10 10 GeV in conflict with excesses reported by some experiments. In this report we will outline a recent statistical analysis [M. Ahlers, A. Ringwald, H. Tu, Astropart. Phys. (in press). Preprint astro-ph/0506698 ] of cosmic ray data using strongly interacting neutrinos as primaries for these excesses.

Topik & Kata Kunci

Penulis (1)

M

M. Ahlers

Format Sitasi

Ahlers, M. (2005). Strongly interacting astrophysical neutrinos. https://doi.org/10.1016/j.ppnp.2005.11.026

Akses Cepat

Lihat di Sumber doi.org/10.1016/j.ppnp.2005.11.026
Informasi Jurnal
Tahun Terbit
2005
Bahasa
en
Sumber Database
Semantic Scholar
DOI
10.1016/j.ppnp.2005.11.026
Akses
Open Access ✓