Radioluminescence yield of alpha particles in air

Abstract

Alpha particles can be detected by measuring the radioluminescence light which they induce when absorbed in air. The light is emitted in the near ultraviolet region by nitrogen molecules excited by secondary electrons. The accurate knowledge of the radioluminescence yield is of utmost importance for novel radiation detection applications utilizing this secondary effect. Here, the radioluminescence yield of an alpha particle is investigated as a function of energy loss in air for the first time. Also, the total radioluminescence yield of the particle is measured with a carefully calibrated $^{239}$ Pu emitter used in the experiments. The obtained results consistently indicate that alpha particles generate $19\pm 3$ photons per one MeV of energy released in air at normal pressure (temperature $22{{\;}^{{}^\circ }}$ C, relative humidity 43%) and the dependence is found to be linear in the studied energy range from 0.3 MeV to 5.1 MeV. The determined radioluminescence yield is higher than previously reported for alpha particles and similar to the radioluminescence yield of electrons at comparable energies. This strengthens the evidence that the luminescence induced by charged particles is mostly proportional to the energy loss in the media and not very sensitive to the type of primary particle.

Keywords

• radioluminescence
• air fluorescence
• alpha particles
• optical detection
• 23.60.+e
• 34.50.Gb