Frequency standards with breakthrough performance: engineering immunity to local oscillator instabilities using dynamical error suppression. This project aims to dramatically advance state-of-the-art performance of one of the most important technological systems in modern electronics - precision frequency standards. Our work will provide orders of magnitude gains in performance by translating new knowledge from quantum information to the precision metrology research community.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE180100042
Funder
Australian Research Council
Funding Amount
$621,834.00
Summary
Australian dark matter detector for high mass axions. This project aims to provide the necessary equipment to allow an Australian Dark Matter Axion Haloscope, with significantly increased sensitivity by providing a milliKelvin environment and a 14 T magnet to drive axion-to-photon conversions. Dark matter is a fundamental component of the universe yet the nature of its composition is still unknown. There is growing evidence that it is comprised of axions, a low energy, weakly interacting particl ....Australian dark matter detector for high mass axions. This project aims to provide the necessary equipment to allow an Australian Dark Matter Axion Haloscope, with significantly increased sensitivity by providing a milliKelvin environment and a 14 T magnet to drive axion-to-photon conversions. Dark matter is a fundamental component of the universe yet the nature of its composition is still unknown. There is growing evidence that it is comprised of axions, a low energy, weakly interacting particle. The precision measurement tools developed by this project will have the potential to contribute both to the economy, via commercialisation, and to national security, via future applications to radar, communication and the development of engineered quantum systems.Read moreRead less
Realisation of an ultra-stable local oscillator using an ultra-low vibration pulse-tube cryocooler. This project will complete the development of a new type of ultra-low-noise ultra-stable microwave oscillator cooled with an ultra-low vibration cryostat and cryocooler. The resulting oscillator will have wide application, but especially to atomic fountain clocks and to very high frequency Very Long Baseline Interferometry (VLBI) radio astronomy.