Cosmogenic Neutrinos from Ultra-High Energy Nuclei

Maximo Ave; N. Busca; A. V. Olinto; A. A. Watson; T. Yamamoto

doi:10.1016/j.astropartphys.2004.11.001

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arXiv · astro-ph/0409316

Cosmogenic Neutrinos from Ultra-High Energy Nuclei

Maximo Ave·N. Busca·A. V. Olinto·A. A. Watson·T. Yamamoto

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Abstract

We calculate the flux of neutrinos generated by the propagation of ultra-high energy iron over cosmological distances and show that even if ultra-high energy cosmic rays are composed of heavy nuclei, a significant flux of high-energy neutrinos should be present throughout the universe. The resulting neutrino flux has a new peak at $\sim 10^{14} eV$ generated by neutron decay and reproduces the double peak structure due to photopion production at higher energies ($\sim 10^{18}$ eV). Depending on the maximum energy and cosmological evolution of extremely high energy cosmic accelerators the generated neutrino flux can be detected by future experiments.

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BibTeX RIS

Maximo Ave, N. Busca, A. V. Olinto, A. A. Watson, T. Yamamoto. 2004-11-06. Cosmogenic Neutrinos from Ultra-High Energy Nuclei. https://doi.org/10.1016/j.astropartphys.2004.11.001

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