Measurement of the ionization response of amorphous selenium with 122keV $\gamma$ rays

TL;DR

This study measures the ionization response of amorphous selenium to 122 keV gamma rays, revealing how charge recombination affects energy resolution, with implications for neutrinoless double beta decay detection.

Contribution

It provides the first detailed measurement of charge yield and energy resolution in amorphous selenium under high electric fields relevant for neutrino physics.

Findings

Charge yield depends strongly on electric field and ionization density.

Energy resolution can reach 1% with charge yield correction.

Recombination dominates the energy resolution in amorphous selenium.

Abstract

We performed a measurement of the ionization response of 200 $\mu$m-thick amorphous selenium (aSe) layers under drift electric fields of up to 50 V/$\mu$m. The aSe target was exposed to ionizing radiation from a $^{57}$Co radioactive source and the ionization pulses were recorded with high resolution. Using the spectral line from the photoabsorption of 122 keV $\gamma$ rays, we measured the charge yield in aSe and the line width as a function of drift electric field. From a detailed microphysics simulation of charge generation and recombination in aSe, we conclude that the strong dependence of recombination on the ionization track density provides the dominant contribution to the energy resolution in aSe. These results provide valuable input to estimate the sensitivity of a proposed next-generation search for the neutrinoless $\beta\beta$ decay of $^{82}$Se that aims to employ imaging sensors with an active layer of aSe. We estimate the RMS line width of the integrated ionization signal from neutrinoless $\beta\beta$ decay events (of deposited energy 3 MeV) to be 2.0% for a drift field of 50 V/$\mu$m. The energy resolution can be improved to 1% by correcting for the charge yield as a function of ionization density along the imaged electron tracks.