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Academic

Research profile of Swinburne astronomer Professor Alan Duffy, Pro Vice Chancellor of Flagship Initiatives and established the Space Technology and Industry Institute at Swinburne as its inaugural Director (2021-2023). Alan has published articles on dark matter, dark energy, galaxy formation, muon technologies, and cosmology, view at ADS or Google Scholar. He is an experienced public speaker, science communicator and leading expert in space science and astrophysics.

Pro Vice Chancellor of Flagship Initiatives at Swinburne University Of Technology, driving large and ambitious transdisciplinary research across our flagship research areas (Space/Aerospace, MedTech Health, Hydrogen and Renewables) by actively engaging with external organisations (including government, industry, NGOs) to identify large-scale opportunities that require university-wide collaboration and the formation of coalitions of universities and partners.

From 2021 - 2023, was the founding Director of the Space Technology and Industry Institute and continue as a Professor of Astrophysics @ Swinburne University.

Until 2023 I was the Swinburne Node Leader, and remain an active Chief Investigator, in the ARC Centre of Excellence for Dark Matter Particle Physics (CDMPP) from 2020 - 2027, attempting to detect the dark matter particle itself. One of the experiments is SABRE, of which I am also a Chief Investigator, the world's first dark matter detector in the Southern Hemisphere at the bottom of the Stawell gold mine at SUPL (Stawell Underground Physics Laboratory) in Victoria, Australia.

Along with experimental dark matter detector physics I also study the formation galaxies within dark matter halos using supercomputer simulations. Most notably the First Galaxies and their impact on the Epoch of Reionisation as part of the DRAGONS team led by Professor Stuart Wyithe. This uses a (SPH) hydrodynamical simulation series Smaug and a larger volume N-body (i.e. dark matter) simulation Tiamat with a new semi-analytic model Meraxes to predict what telescopes will see reionisation. 

From 2017 - 2024 I was also an Associate Investigator in the ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO3D) and the ARC Centre of Excellence for Gravitational Wave Discovery (OzGRav).

As a member of two leading surveys on the next-generation Australia Square Kilometre Array Pathfinder telescope I create local universe simulations that can be used to test our galaxy formation and dark matter theories when compared with observations from the WALLABY and DINGO surveys.

This CV contains all my various activities.

 

A dwarf galaxy forming when the Universe was half its current age. The Dark Matter is in red, the stars in yellow and the gas in blue. Galaxy formation occurs along Dark Matter filaments, and is a violent process of merging of gas clouds, spawning stars deep within their sheltered cores. Credit: Bourke, Crain and Duffy

The Dark Matter in a simulation 600 million lightyears across. The Dark Matter forms filaments spanning the Universe, known as the Cosmic Web. Galaxies form in the intersection of these filaments, seen as spherical clumps or haloes. Credit: Bourke and Duffy

My Research