English

Consequences of Modified Cosmologies in DM abundance and PeV IceCube signals

Cosmology and Nongalactic Astrophysics 2019-03-26 v1

Abstract

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

Keywords

Cite

@article{arxiv.1903.10038,
  title  = {Consequences of Modified Cosmologies in DM abundance and PeV IceCube signals},
  author = {G. Lambiase},
  journal= {arXiv preprint arXiv:1903.10038},
  year   = {2019}
}

Comments

Talk presented at NuPhys2018 (London, 19-21 December 2018). 4 pages, LaTeX, 1 figure