Ultra High Energy Cosmic Rays in Our Universe
W-Y. Pauchy Hwang, Bo-Qiang Ma

TL;DR
This paper discusses the propagation of ultra high energy cosmic rays within the universe, emphasizing the roles of the Cosmic Microwave Background and cosmic background neutrinos, and explores phenomena like the knee, ankle, and potential ultra-high-energy bursts.
Contribution
It provides a comprehensive analysis of UHECR propagation considering the Standard Model and cosmic backgrounds, offering explanations for observed spectral features and potential ultra-high-energy phenomena.
Findings
CMB influences the spectral features of UHECRs such as the knee and ankle.
Neutrino halos around celestial objects affect cosmic ray interactions.
Potential observation of $W^ ext{±}$ and $Z^0$ bursts at ultra-high energies.
Abstract
Our Universe is described jointly by Einstein's relativity principle and the quantum principle; there the existence of the smallest units of matter, such as electrons, neutrinos, quarks, and photons, is well established and the smallest units of matter are described by the Standard Model. Based on these, we have a clear picture for the propagation of ultra high energy cosmic rays (UHECR's), for energies greater than but less than , in the cosmic medium of the Cosmic Microwave Background (CMB) and of the cosmic background neutrinos (CB's). We find that the CMB plays a pivot role in this energy range, so that the observed "knee(s)" and the "ankle" could be understood in reasonable terms. What we might observe at the energy near ', the so-called " bursts" or " bursts", is briefly discussed. Meanwhile, in the early Universe,…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Dark Matter and Cosmic Phenomena · Neutrino Physics Research
