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  • Letter
  • Open Access

Minimal sterile neutrino dark matter

Torsten Bringmann1,2,*, Paul Frederik Depta3,†, Marco Hufnagel4,‡, Jörn Kersten5,6,§, Joshua T. Ruderman7,∥, and Kai Schmidt-Hoberg8,¶

  • 1Department of Physics, University of Oslo, Box 1048, N-0316 Oslo, Norway
  • 2Theoretical Physics Department, CERN, 1211 Geneva 23, Switzerland
  • 3Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany
  • 4Service de Physique Théorique, Université Libre de Bruxelles, Boulevard du Triomphe, CP225, B-1050 Brussels, Belgium
  • 5Korea Institute for Advanced Study, Seoul 02455, Republic of Korea
  • 6Department of Physics and Technology, University of Bergen, 5020 Bergen, Norway
  • 7Center for Cosmology and Particle Physics, Department of Physics, New York University, New York, New York 10003, USA
  • 8Deutsches Elektronen-Synchrotron DESY, Notkestr. 85, 22607 Hamburg, Germany

  • *torsten.bringmann@fys.uio.no
  • †frederik.depta@mpi-hd.mpg.de
  • ‡marco.hufnagel@ulb.be
  • §joern.kersten@uib.no
  • ∥ruderman@nyu.edu
  • kai.schmidt-hoberg@desy.de

Phys. Rev. D 107, L071702 – Published 24 April, 2023

DOI: https://doi.org/10.1103/PhysRevD.107.L071702

Abstract

We propose a novel mechanism to generate sterile neutrinos νs in the early Universe, by converting ordinary neutrinos να in scattering processes νsνα→νsνs. After initial production by oscillations, this leads to an exponential growth in the νs abundance. We show that such a production regime naturally occurs for self-interacting νs, and that this opens up significant new parameter space where νs make up all of the observed dark matter. Our results provide strong motivation to further push the sensitivity of X-ray line searches, and to improve on constraints from structure formation.

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