Dirac neutrino mass from a neutrino dark matter model for the galaxy cluster Abell 1689

@article{Nieuwenhuizen2015DiracNM,
  title={Dirac neutrino mass from a neutrino dark matter model for the galaxy cluster Abell 1689},
  author={Theo M. Nieuwenhuizen},
  journal={arXiv: Cosmology and Nongalactic Astrophysics},
  year={2015}
}
  • T. Nieuwenhuizen
  • Published 2015
  • Physics
  • arXiv: Cosmology and Nongalactic Astrophysics
The dark matter in the galaxy cluster Abell 1689 is modelled as an isothermal sphere of neutrinos. New data on the $2d$ mass density allow an accurate description of its core and halo. The model has no "missing baryon problem" and beyond $2.1$ Mpc the baryons have the cosmic mass abundance. Combination of cluster data with the cosmic dark matter fraction -- here supposed to stem from the neutrinos -- leads to a solution of the dark matter riddle by left and right handed neutrinos with mass 1… Expand

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