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arxiv: 1903.10038 · v1 · submitted 2019-03-24 · 🌌 astro-ph.CO

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Consequences of Modified Cosmologies in DM abundance and PeV IceCube signals

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classification 🌌 astro-ph.CO
keywords abundancealphaicecubeaccordingassumedastrophysicalbackgroundcollaboration
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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 $\sim y_{\alpha \chi}\overline{{L_{L_{\alpha}}}}\, H\, \chi$. The cosmological background is assumed to evolve according to $f({\cal T})$ cosmology, where ${\cal T}$ is the scalar torsion.

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