7–11 Dec 2026
The University of Sydney
Australia/Sydney timezone
AIP Congress 2026

The ORGAN Experiment: Results, Status, and Future Plans

Not scheduled
20m
Belinda Hutchinson Building (The University of Sydney )

Belinda Hutchinson Building

The University of Sydney

Abercrombie St & Codrington St NSW 2008
Invited talk AIP | Nuclear and Particle Physics (NUPP)

Description

We present the status and plans of The Oscillating Resonant Group AxioN (ORGAN) Collaboration, which develops microwave cavity axion haloscopes to search for dark matter. ORGAN is a nation wide collaboration, with the main experiment hosted at The University of Western Australia.

Axions are a leading dark matter candidate. Axion haloscopes are a class of experiments which search for axion dark matter using electromagnetic resonant cavities submerged in magnetic fields.

The main ORGAN Experiment is a high mass haloscope (~60-200 micro-eV) broken down into various phases, having commenced data-taking in 2021. Phase 1 recently concluded, excluding ALP Cogenesis models of dark matter in the relevant mass ranges along with scalar dark matter and dark photon limits. Phase 2 is in research and development, expected to commence in late 2026 and achieve deeper sensitivity. Active avenues of research and development for ORGAN Phase 2 include novel high frequency cavity design, superconducting materials, and single photon counting – we will report on the status of R&D in these areas.

ORGAN-Q is a pathfinder experiment (~25 micro-eV), designed as a testbed for various techniques to be integrated into the main ORGAN Experiment in Phase 2, such as quantum enhances amplification, and other improvements. The first ORGAN-Q run concluded in 2024, and we are currently in preparation for the next run which plans to implement various design improvements, including squeezed state receiving.

ORGAN-Low Frequency is a lower-mass experiment designed to utilise an MRI magnet, and novel re-entrant cavities to push into the low frequency regime, and search for different models of dark matter. It completed its path-finding run in 2026, and is currently in development for full-scale deployment.

We will summarize each experiment in terms of the relevant experimental details, current status, run plans, and projected reach.

I am the presenting author Yes

Authors

Aaron Quiskamp (The University of Western Australia) Ben McAllister (Swinburne University of Technology) Geoffrey Brooks (Swinburne University of Technology) Dr Graeme Flower (The University of Western Australia) Michael E. Tobar Paige Taylor (Swinburne University of Technology) Raj Aryan Singh (Swinburne University of Technology)

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