Abstract

We 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 ΔNeff 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.

Details

Title
Inverse Seesaw, dark matter and the Hubble tension
Author
Fernandez-Martinez, E 1 ; Pierre, M 1 ; Pinsard, E 2 ; Rosauro-Alcaraz, S 1 

 Universidad Autónoma de Madrid, Departamento de Física Teórica and Instituto de Física Teórica, IFT-UAM/CSIC, Madrid, Spain (GRID:grid.5515.4) (ISNI:0000000119578126) 
 CNRS/IN2P3, Univ. Clermont Auvergne, Laboratoire de Physique de Clermont (UMR 6533), Aubière Cedex, France (GRID:grid.5515.4) 
Publication year
2021
Publication date
Oct 2021
Publisher
Springer Nature B.V.
ISSN
14346044
e-ISSN
14346052
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2588185260
Copyright
© The Author(s) 2021. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.