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We study models in which neutrino masses are generated dynamically at cosmologically late times.
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Steen Hannestad: Structure formation with strongly interacting neutrinos - implications for the cosmological neutrino mass bound, JCAP 0502:011,2005, arXiv:astro-ph/0411475v3
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Antonio Enea Romano: Hubble trouble or Hubble bubble?, arXiv:1609.04081v5 [astro-ph.CO]
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