Beliebiger Eintrag,

Constraining the Self-Interacting Neutrino Interpretation of the Hubble Tension

, , , und .
(2019)cite arxiv:1905.02727Comment: 10 pages, 2 figures, 3 appendices.

Zusammenfassung

Large, non-standard neutrino self-interactions have been shown to resolve the $4\sigma$ tension in Hubble constant measurements and a milder tension in the amplitude of matter fluctuations. We demonstrate that interactions of the necessary size imply the existence of a force-carrier with a large neutrino coupling ($> 10^-4$) and mass in the keV -- 100 MeV range. This mediator is subject to stringent cosmological and laboratory bounds, and we find that nearly all realizations of such a particle are excluded by existing data unless it carries spin 0 and couples almost exclusively to $\tau$-flavored neutrinos. Furthermore, we find that the light neutrinos must be Majorana, and that a UV-complete model requires a non-minimal mechanism to simultaneously generate neutrino masses and appreciable self-interactions.

Tags

Nutzer

  • @citekhatri

Kommentare und Rezensionen