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

Zhoawen Tang, Marie Blatnik, Leah J. Broussard, J. H. Choi, Stephen M. Clayton, Christopher Cude-Woods, Scott Currie, D. E. Fellers, E. M. Fries, Peter Geltenbort, F. Gonzalez, Kevin P. Hickerson, Takeyasu M. Ito, Chen Y. Liu, S. W. T. MacDonald, Mark Makela, Christopher L. Morris, C. M. O'Shaughnessy, Robert W. Pattie, Bradley R. PlasterD. J. Salvat, Alexander Saunders, Zhehui Wang, Albert R. Young, B. A. Zeck

Research output: Contribution to journalArticlepeer-review

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,  n X + 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.
Original languageAmerican English
JournalPhysical Review Letters
Volume121
DOIs
StatePublished - Jul 13 2018
Externally publishedYes

Keywords

  • Dark Matter Particle
  • Neutron Decay

Disciplines

  • Atomic, Molecular and Optical Physics
  • Physics
  • Nuclear

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