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arXiv · 1903.10038

Consequences of Modified Cosmologies in DM abundance and PeV IceCube signals

G. Lambiase
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Abstract

To explain the high-energy astrophysical neutrino flux with energies $\sim PeV$ recently observed by IceCube collaboration and the relic abundance of DM in the Universe, we consider the minimal 4-dimensional operator $\sim y_{αχ}\overline{L_{L_α}}\, H\, χ$. The cosmological background is assumed to evolve according to $f({\cal T})$ cosmology, where ${\cal T}$ is the scalar torsion.

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G. Lambiase. 2019-03-24. Consequences of Modified Cosmologies in DM abundance and PeV IceCube signals. https://arxiv.org/abs/1903.10038

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