Search for the Neutron Decay nX+γ , Where X is a Dark Matter Particle

Abstract
Fornal and Grinstein recently proposed that the discrepancy between two different methods of neutron lifetime measurements, the beam and bottle methods, can be explained by a previously unobserved dark matter decay mode, nX+γ. We perform a search for this decay mode over the allowed range of energies of the monoenergetic γ ray for X to be dark matter. A Compton-suppressed high-purity germanium detector is used to identify γ rays from neutron decay in a nickel-phosphorous-coated stainless-steel bottle. A combination of Monte Carlo and radioactive source calibrations is used to determine the absolute efficiency for detecting γ rays arising from the dark matter decay mode. We exclude the possibility of a sufficiently strong branch to explain the lifetime discrepancy with 97% confidence.
Funding Information
  • Laboratory Directed Research and Development (20140568DR)
  • National Science Foundation (130692, 1307426, 161454, 1506459, 1553861)
  • U.S. Department of Energy (DE-FG02-97ER41042, DE-SC0014622, DE-AC05-00OR22725)
  • LLC (8215)
  • IU Center for Space Time Symmetries (IUCSS)