Skip to main content
U.S. flag

An official website of the United States government

Dot gov

The .gov means it’s official.
Federal government websites often end in .gov or .mil. Before sharing sensitive information, make sure you’re on a federal government site.

Https

The site is secure.
The https:// ensures that you are connecting to the official website and that any information you provide is encrypted and transmitted securely.

Summary

Quantum electrodynamics (QED) predicts that a neutron will decay into a proton, electron and anti-neutrino. A small fraction of the time, this beta-decay process will also produce a photon. NIST recently detected this rare radiative decay (RDK) mode for the first time. We are currently developing statistical methods for analysis of the second generation version of the experiment (RDKII). In the experiment, RDK photons deposit energy in scintillators than then produce light. With some quantum efficiency, the scintillation light produces photoelectrons at Avalanche Photodiodes. Current efforts focus on Monte Carlo modeling of the photon transport and systematic errors due to the fact that photons need not deposit all their energy in the scintillators and development of impulse response functions for observed data and nonlinear calibration models to relate the measured peak height of voltage pulse produced by point sources of photons to the energy deposited in a scintillator. The goal is to quantify the branching ratio for this rare decay mode and quantify systematic errors in the observed energy deposit spectrum so that we can test the consistency of QED.

Description

When a neutron decays by its radiative decay (RDK) mode, it produces a photon with a energy spectrum predicted by Quantum Electrodynamics. These RDK photons deposit energy in scintillators which produce voltage pulses in Avalanche Photo Diodes. We are developing nonlinear calibration models to predict the energy deposited in a scintillator by an event based on the observed pulse height of an event based on calibration data due a Cs137 point source (b) and Monte Carlo estimates of the energy deposit spectrum of this point source (a).
radiative decay of the neutron

Simulated energy deposit spectrum (a) and observed and predicted calibration data for a Cs137 point source

Major Accomplishments

(Selected Publications)

J.S. Nico, M.S. Dewey, T.R. Gentile, H.P. Mumm, A.K. Thompson, B.M. Fisher, I. Kremsky, F.E. Wietfeldt, T.E. Chupp, R.L. Cooper, E.J. Beise, K.G. Kiriluk, J. Byrne, K.J. Coakley, "Observation of the Radiative Decay of the Free Neutron" published in Nature 444, 1059-1062 (21 December 2006)

R.L. Cooper, C.D. Bass, E.J. Beise, H. Breuer, J. Byrne, T.E. Chupp, K.J. Coakley, M.S. Dewey, B.M. Fisher, C. Fu, T.R. Gentile, M. McGonagle, H.P. Mumm, J.S. Nico, A.K. Thompson, F.E. Wietfeldt. An experiment for the precision measurement of the radiative decay mode of the neutron Nuclear Instruments and Methods in Physics Research A, Vol. 611, Issues 2-3, pp. 219-223, Dec. 2009

R.L. Cooper, T.E. Chupp, M.S. Dewey,T.R. Gentile, H.P. Mumm, J.S. Nico, A.K. Thompson, B.M. Fisher, I. Kremsky, F.E. Wietfeldt, E.J. Biese, K.G. Kiriluk, J. Byrne, K.J. Coakley, C.Fu. Radiative beta-decay of the free neutron, Physical Review C, 81, 03550, 2010

Created September 1, 2010, Updated May 2, 2016