Observations of diffuse fluxes of cosmic neutrinos
Christopher H. Wiebusch
TL;DR
This paper reviews current observational results on high-energy astrophysical neutrino diffuse fluxes, analyzing measurements across detection channels to understand their energy spectrum, flavor ratio, and anisotropy.
Contribution
It provides a comprehensive review of the latest observational data and compares results across different detection methods for high-energy neutrinos.
Findings
Measurements indicate a consistent diffuse flux across channels.
Energy spectrum analysis suggests a power-law behavior.
No significant large-scale anisotropy detected.
Abstract
In this contribution the current observational results for the diffuse flux of high-energy astrophysical neutrinos are reviewed. In order to understand the science implications, the measurements in different detection channels are discussed and results are compared. The discussion focuses is the energy spectrum, the flavor ratio and large scale anisotropy.
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