Letter

Nature 444, 1059-1062 (21 December 2006) | doi:10.1038/nature05390; Received 31 August 2006; Accepted 25 October 2006

Observation of the radiative decay mode of the free neutron

Jeffrey S. Nico1, Maynard S. Dewey1, Thomas R. Gentile1, H. Pieter Mumm1, Alan K. Thompson1, Brian M. Fisher2, Isaac Kremsky2, Fred E. Wietfeldt2, Timothy E. Chupp3, Robert L. Cooper3, Elizabeth J. Beise4, Kristin G. Kiriluk4, James Byrne5 & Kevin J. Coakley6

  1. Physics Laboratory, National Institute of Standards and Technology, Gaithersburg, Maryland 20899, USA
  2. Department of Physics, Tulane University, New Orleans, Louisiana 70118, USA
  3. FOCUS and Physics Department, University of Michigan, Ann Arbor, Michigan 48109, USA
  4. Department of Physics, University of Maryland, College Park, Maryland 20742, USA
  5. Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QH, UK
  6. Information Technology Laboratory, National Institute of Standards and Technology, Boulder, Colorado 80305, USA

Correspondence to: Jeffrey S. Nico1 Correspondence and requests for materials should be addressed to J.S.N. (Email: jnico@nist.gov).

The theory of quantum electrodynamics (QED) predicts that beta decay of the neutron into a proton, electron and antineutrino should be accompanied by a continuous spectrum of soft photons. While this inner bremsstrahlung branch has been previously measured in nuclear beta and electron capture decay, it has never been observed in free neutron decay. Recently, the photon energy spectrum and branching ratio for neutron radiative decay have been calculated using two approaches: a standard QED framework1, 2, 3 and heavy baryon chiral perturbation theory4 (an effective theory of hadrons based on the symmetries of quantum chromodynamics). The QED calculation treats the nucleons as point-like, whereas the latter approach includes the effect of nucleon structure in a systematic way. Here we observe the radiative decay mode of free neutrons, measuring photons in coincidence with both the emitted electron and proton. We determined a branching ratio of (3.13 plusminus 0.34) times 10-3 (68 per cent level of confidence) in the energy region between 15 and 340 keV, where the uncertainty is dominated by systematic effects. The value is consistent with the predictions of both theoretical approaches; the characteristic energy spectrum of the radiated photons, which differs from the uncorrelated background spectrum, is also consistent with the calculated spectrum. This result may provide opportunities for more detailed investigations of the weak interaction processes involved in neutron beta decay.

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