Constraining the Self-Interacting Neutrino Interpretation of the Hubble Tension

Blinov, Nikita; Kelly, Kevin J.; Krnjaic, Gordan; McDermott, Samuel D.

doi:10.1103/PhysRevLett.123.191102

Title: Constraining the Self-Interacting Neutrino Interpretation of the Hubble Tension

Journal Article · Thu Nov 07 00:00:00 EST 2019 · Physical Review Letters

DOI:https://doi.org/10.1103/PhysRevLett.123.191102· OSTI ID:1545086

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Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)

Large, nonstandard neutrino self-interactions have been shown to resolve the ~4σ tension in Hubble constant measurements and a milder tension in the amplitude of matter fluctuations. Herein 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 $$τ$$-flavored neutrinos. Furthermore, we find that the light neutrinos must be Majorana particles, and that a UV-complete model requires a nonminimal mechanism to simultaneously generate neutrino masses and appreciable self-interactions.

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Research Organization:: Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP)

Grant/Contract Number:: AC02-07CH11359

OSTI ID:: 1545086

Report Number(s):: arXiv:1905.02727; FERMILAB-PUB-19-175-A-T; arXiv:1905.02727v2; PRLTAO; oai:inspirehep.net:1733842

Journal Information:: Physical Review Letters, Vol. 123, Issue 19; ISSN 0031-9007

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 92 works

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