Published January 23, 2024
| Version v1
Conference paper
Investigation of Radiation Effects on Low Noise Photoreceivers for Laser Interferometric Space applications such as LISA
Contributors
Others:
- Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS) ; Université Nice Sophia Antipolis (1965 - 2019) (UNS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur ; Université Côte d'Azur (UniCA)-Université Côte d'Azur (UniCA)-Centre National de la Recherche Scientifique (CNRS)
- DPHY, ONERA, Université de Toulouse [Toulouse] ; ONERA-PRES Université de Toulouse
- Centre de Lutte contre le Cancer Antoine Lacassagne [Nice] (UNICANCER/CAL) ; UNICANCER-Université Côte d'Azur (UniCA)
- National Institute for Subatomic Physics [Amsterdam] (NIKHEF)
- Japan Aerospace Exploration Agency [Tokyo] (JAXA)
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute) (AEI) ; Max-Planck-Gesellschaft
- SRON Netherlands Institute for Space Research (SRON)
Description
This study assesses the impact of space environmental radiation on low-noise Quadrant Photoreceivers (QPRs) for use in high-precision interferometric systems like the Laser Interferometer Space Antenna (LISA). InGaAs Quadrant Photodiodes (QPDs) of 1.0 mm, 1.5 mm, and 2.0 mm sizes were irradiated with 20 and 60 MeV protons, 0.5 and 1 MeV electrons, and Co60 gamma rays, receiving a Displacement Damage Equivalent Fluence (DDEF) of 1.0×10+12 p/cm² and a Total Ionising Dose (TID) of 237 krad, five times LISA's requirement. These QPDs, integrated with a low-noise DC-coupled Transimpedance Amplifier (TIA) to form the QPR, were tested for phase and amplitude response to signals akin to LISA's interferometric signal. Additional measurements on the QPDs covered dark current, capacitance, Quantum Efficiency (QE), and QPR's input equivalent current noise. These findings indicate a predictable pattern of QPR performance degradation, based on the irradiated QPD parameters and suggest the QPDs' suitability for LISA and comparable space missions.
Abstract
International audienceAdditional details
Identifiers
- URL
- https://hal.science/hal-04894540
- URN
- urn:oai:HAL:hal-04894540v1
Origin repository
- Origin repository
- UNICA