Jade is the Database Administrator for the Centre and the SABRE South Experiment
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World leading researchers with more than twenty years of sucessfully building liquid xenon Dark Matter detectors unite XLZD Consortium. DARWIN, LZ and XENONnT have the same scientific goals but differ in technical details. XLZD are able to explore and select the best options from both worlds, strengthening R&D efforts by combining ideas and resources.
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Centre researchers Elisabetta Barberio and Madeleine Zurowski participated in the ABC Catalyst The Dark Side of the Universe episode.
Read MoreM. Tobar, C. Thomson, A. Quiskamp, B. McAllister, M. Goryachev, G. Rybka
Read MoreCentre Authors: McAllister, Ben, Tobar, Michael, Goryachev, Maxim, Thomson, Catriona
Read MoreC. O’Hare
Read MoreCentre Authors: Tobar, Michael
Read MoreCentre Authors: Quiskamp, Aaron, McAllister, Ben, Rybka, Gray, Tobar, Michael, Goryachev, Maxim, Thomson, Catriona
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Members of the CYGNUS-Oz collaboration have received a funding injection of more than $90,000 that will enable the Australian team to play a pivotal role in the international quest to develop directional dark matter detectors.
Read MoreF. Scutti
Read MoreCentre Authors: Tobar, Michael, Goryachev, Maxim
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CYGNUS is a grouping of international researchers who have an interest in directional detection using gaseous Time Projection Chambers (TPCs).
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Centre Director Elisabetta Barberio will provide an update on the SABRE South experiment, which will be located in the Stawell Underground Physics Laboratory.
Read MoreCentre Authors: Duffy, A., Mould, J., Flynn, C., Dixon, M., Taylor, E.
Read MoreCentre Authors: Tobar, M., Goryachev, M., McAllister, B., Quiskamp, A., Campbell, W., Thomson, C., Ivanov, E., Bourhill, J.
Read MoreCentre Authors: Tobar, M., McAllister, B.
Read MoreCentre Authors: Bell, N., Barberio, E. L., Newstead, J., O'Hare, C., Boehm, C., Urquijo, P.
Read MoreCentre Authors: Duffy, A., Lawrence, G., Hopkins, P.
Read MoreCentre Authors: Tobar, M., Goryachev, M.
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Grace Lawrence’s area of research is direct detection, using simulations to study galaxy-scale dark matter distribution.
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