Dark Matter Centre physicists enjoyed talking to Channel 7 about the Partner Schools Program, which has expanded into New South Wales.
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Laura Manenti is a Lecturer at the University of Sydney. Her research focuses on rare event searches and experiments aimed at detecting dark matter particles
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Kooringal High School students learnt about physics from scientists involved in world-leading dark matter projects today.
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Michael is a PhD student at the University of Melbourne working under the supervision of Prof. Nicole Bell. His area of research is in dark matter phenomenology.
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Robert Crew is a PhD student at the University of Western Australia working under the supervision of Professor Michael Tobar. He has also been a CDM summer student during his undergraduate studies.
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Steven Samuels is a PhD student at the University of Western Australia working under the supervision of Professor Michael Tobar.
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Emma Paterson is a PhD student at the University of Western Australia working under the supervision of Dr Jeremy Bourhill.
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Michael Mews is a PhD student at the University of Melbourne.
He works on the SABRE South experiment.
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Dr Peter McNamara is an experimental particle physicist.
He was a postdoctoral researcher at the ANU node involved with the CYGNUS and SABRE South collaborations. He is now based at the University of Toronto.
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University of Massachusetts Amherst
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Lachlan Milligan is a PhD student at the University of Melbourne. He participates in the SABRE South experiment and has also worked with DSTG developing a GEANT4 simulation modelling a new neutron spectrometer.
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Dr Robert James is a postdoctoral fellow at the University of Melbourne. He leads statistical inference for the world-leading LUX-ZEPLIN (LZ) experiment, which utilises a deep underground dual-phase liquid xenon time projection chamber. In Australia he is currently leading physics and simulation work for the SABRE South experiment, as it prepares for initial commissioning and data taking. He is also involved in R&D efforts through the XLZD consortium to optimise the design of a next-generation liquid xenon detector to maximise its physics reach.
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