Scintillation detectors for gamma rays transfer the energy of a gamma-ray
photon to an electron within a crystal, via the photoelectric effect or
Compton scattering. The electron transfers its energy to atoms in the crystal,
which re-emit it as a light flash detected by a photomultiplier tube. The
charge pulse produced by the photomultiplier tube is proportional to the
energy originally deposited in the crystal; this can be measured so an energy
spectrum can be displayed. Gamma rays absorbed by the photoelectric effect are
recorded as a photopeak in the spectrum, at the full energy of the gammas. The
Compton-scattered electrons are also recorded, at a range of lower energies
known as the Compton plateau. The highest-energy of these form the Compton
edge of the plateau. Gamma-ray photons scattered \(180 .^{\circ}\) by the
Compton effect appear as a backscatter peak in the spectrum. For gamma-ray
photons of energy \(511 \mathrm{KeV}\) calculate the energies of the Compton
edge and the backscatter peak in the spectrum.