Inverse Seesaw, dark matter and the Hubble tension

Author:

Fernandez-Martinez E.,Pierre M.,Pinsard E.,Rosauro-Alcaraz S.

Abstract

AbstractWe consider the inverse Seesaw scenario for neutrino masses with the approximate Lepton number symmetry broken dynamically by a scalar with Lepton number two. We show that the Majoron associated to the spontaneous symmetry breaking can alleviate the Hubble tension through its contribution to $$\Delta N_\text {eff}$$ Δ N eff and late decays to neutrinos. Among the additional fermionic states required for realizing the inverse Seesaw mechanism, sterile neutrinos at the keV-MeV scale can account for all the dark matter component of the Universe if produced via freeze-in from the decays of heavier degrees of freedom.

Publisher

Springer Science and Business Media LLC

Subject

Physics and Astronomy (miscellaneous),Engineering (miscellaneous)

Cited by 20 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. A cosmological sandwiched window for lepton-number breaking scale;Journal of Cosmology and Astroparticle Physics;2024-04-01

2. Particle Physics and Cosmology Intertwined;Entropy;2024-01-25

3. Diraxiogenesis;Journal of High Energy Physics;2024-01-11

4. Majoron dark matter from a type II seesaw model;Physical Review D;2023-12-05

5. Thermal effects in freeze-in neutrino dark mater production;Journal of High Energy Physics;2023-11-24

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