Ultrahigh energy cosmic rays and neutrino flux models
Marco Stein Muzio

TL;DR
This review discusses the motivation, production mechanisms, sources, and models of ultrahigh energy neutrino fluxes, emphasizing their connection to cosmic rays and exploring both model-independent benchmarks and model-dependent predictions.
Contribution
It provides a comprehensive overview of neutrino flux models, including benchmarks and specific examples, advancing understanding of ultrahigh energy neutrino predictions.
Findings
Identification of key neutrino production mechanisms
Discussion of model-independent flux benchmarks
Overview of model-dependent flux prediction approaches
Abstract
In this review we motivate ultrahigh energy neutrino searches and their connection to ultrahigh energy cosmic rays. We give an overview of neutrino production mechanisms and their potential sources. Several model-independent benchmarks of the ultrahigh energy neutrino flux are discussed. Finally, a brief discussion of approaches for model-dependent neutrino flux predictions are given, highlighting a few examples from the literature.
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