Impact of Warm Dark Matter on the Cosmic Neutrino Background Anisotropies

@article{Tully2022ImpactOW,
  title={Impact of Warm Dark Matter on the Cosmic Neutrino Background Anisotropies},
  author={Christopher G. Tully and Gemma Zhang},
  journal={Universe},
  year={2022}
}
The Cosmic Neutrino Background (CνB) anisotropies for massive neutrinos are a unique probe of large-scale structure formation. The redshift-distance measure is completely different for massive neutrinos as compared to electromagnetic radiation. The CνB anisotropies in massive neutrinos grow in response to non-relativistic motion in gravitational potentials seeded by relatively high k-modes. Differences in the early phases of large-scale structure formation in warm dark matter (WDM) versus cold… 
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