PeV IceCube signals and $H_0$ tension in the framework of Non-Local Gravity
Salvatore Capozziello, Gaetano Lambiase

TL;DR
This paper explores how non-local gravity modifications could simultaneously explain high-energy PeV neutrino signals detected by IceCube, the abundance of dark matter, and potentially resolve the H_0 tension in cosmology.
Contribution
It introduces a framework where non-local gravity corrections account for IceCube neutrino flux, dark matter abundance, and the H_0 tension, linking particle physics and cosmology.
Findings
Non-local gravity can explain PeV neutrino flux.
The model accounts for dark matter abundance.
It offers a potential solution to the H_0 tension.
Abstract
We study possible effects of non-local gravity corrections on the recent discovery by the IceCube collaboration reporting high-energy neutrino flux detected at energies of order PeV. Considering the 4-dimensional operator , it is possible to explain both the IceCube neutrino rate and the abundance of Dark Matter, provided that non-local corrections are present in the cosmological background. Furthermore, the mechanism could constitute a natural way to address the tension issue.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Computational Physics and Python Applications · Cosmology and Gravitation Theories
