Joint measurement of the ultra-high-energy neutrino spectrum and cross section
Victor B. Valera, Mauricio Bustamante, Olga Mena

TL;DR
This paper proposes a joint measurement approach for ultra-high-energy neutrino flux and cross section, emphasizing flexible spectral parametrizations and forecasting capabilities for upcoming neutrino telescopes like IceCube-Gen2.
Contribution
It introduces a method for simultaneous measurement of UHE neutrino spectrum and cross section without prior assumptions, using flexible spectral models for improved accuracy.
Findings
Flexible spectral parametrizations improve measurement accuracy.
Joint measurement reduces uncertainties in flux and cross section.
Forecasts demonstrate feasibility for IceCube-Gen2.
Abstract
Soon, a new generation of neutrino telescopes, presently under planning, will target the discovery of ultra-high-energy (UHE) neutrinos of cosmic origin, with energies higher than 100 PeV, that promise unique insight into astrophysics and particle physics. Yet, predictions of the UHE neutrino flux and interaction cross section -- whose measurement is co-dependent -- are laden with significant uncertainty that, if unaddressed, could misrepresent the capabilities to measure one or the other. To address this, we advocate for the joint measurement of the UHE neutrino spectrum and neutrino-nucleon cross section, including of their energy dependence, without assuming prior knowledge of either. We illustrate our methods by adopting empirical parametrizations of the neutrino spectrum, in forecasts geared to the planned radio array of the IceCube-Gen2 neutrino telescope. We warn against using…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Neutrino Physics Research · Radio Astronomy Observations and Technology
