Observation of Time-Dependent Internal Charge Amplification in a Planar Germanium Detector at Cryogenic Temperature
arXiv:2211.16256 · doi:10.1140/epjc/s10052-023-11432-y
Abstract
For the first time, time-dependent internal charge amplification through impact ionization has been observed in a planar germanium (Ge) detector operated at cryogenic temperature. In a time period of 30 and 45 minutes after applying a bias voltage, the charge energy corresponding to a baseline of the 59.54 keV rays from a Am source is amplified for a short period of time and then decreases back to the baseline. The amplification of charge energy depends strongly on the applied positive bias voltage with drifting holes across the detector. No such phenomenon is visible with drifting electrons across the detector. We find that the observed charge amplification is dictated by the impact ionization of charged states, which has a strong correlation with impurity level and applied electric field. We analyze the dominant physics mechanisms that are responsible for the creation and the impact ionization of charged states. Our analysis suggests that the appropriate level of impurity in a Ge detector can enhance charge yield through the impact ionization of charged states to achieve extremely low-energy detection threshold ( 10 meV) for MeV-scale dark matter searches if the charge amplification can be stabilized.
arXiv comment7 pages and 9 figures
References in corpus (16)
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
- Supersymmetric Dark Matter
- New results from DAMA/LIBRA
- Results from 730 kg days of the CRESST-II Dark Matter Search
- A SQUID-based microwave cavity search for dark-matter axions
- Direct Detection of Sub-GeV Dark Matter
- First dark matter search results from a 4-kg CFI bubble chamber operated in a deep underground site
- Direct Search for Low Mass Dark Matter Particles with CCDs
- First dark matter search results from the PandaX-I experiment
- Equivalent Neutrinos, Light WIMPs, and the Chimera of Dark Radiation
- Limits on MeV Dark Matter from the Effective Number of Neutrinos
- On the Existence of Low-Mass Dark Matter and its Direct Detection
- Direct Detection of MeV-Scale Dark Matter Utilizing Germanium Internal Amplification for the Charge Created by the Ionization of Impurities
- Supersymmetry and Cosmology
- Germanium Detector with Internal Amplification for Investigation of Rare Processes
- Evidence of cluster dipole states in germanium detectors operating at temperatures below 10 K