A brief overview of what we mean by “precision metrology” in the context of the Centre’s search for dark matter.
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US funding extends the ADMX search for axions
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Celebrate the search for Dark Matter!
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SUPL excavation reaches major milestone
Read MoreBefore we get started, it should be pointed out that what is meant here by “small-scale” is something on the scale of our galaxy’s dark matter halo.
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ARC CoE funding announced in August 2019
Read MoreOccasional updates on the progress of the SABRE South experiment.
Read MoreWhat makes us think we need dark matter?
Read MoreAn axion-detection experiment at the University of Western Australia.
Read MoreHow does one detect an axion?
Read MoreLighter than a WIMP, but more of them…
Read MoreWhy we would expect an annual variation in the dark matter count rate.
Read MoreAn overview of how the SABRE dark matter detector works.
Read MoreSUPL will be the home of the SABRE South dark matter detector.
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The SABRE experiment has two sites - one in Italy, and the other to be in Victoria.
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Dr. Richard Garrett (ANSTO) is Senior Advisor, Strategic Projects, and Manager, Industry and External Engagement at the Australian Nuclear Science and Technology Organisation.
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Dr Maxim Goryachev is an established physicist with vast experience in low-temperature and condensed-matter physics, frequency measurement and control, low-noise and precision measurements, photonic and phononic low-loss systems, and paramagnetic and ferrimagnetic spin systems at low temperatures.
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Associate Professor Gary Hill is an accomplished astrophysicist in the area of high-energy neutrino detection, with expertise in low-signal/high-background data analysis.
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Dr. Michael Hotchkis (ANSTO) is Principal Research Scientist at the Australian Nuclear Science and Technology Organisation.
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Professor Paul Jackson is an experimental particle physicist specialising in searches for beyond the Standard Model physics, primarily using detectors situated at particle colliders.
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