Published 2024 | D. Ferlewicz, P. Urquijo et al. (Belle)
Our group is involved in a broad and diverse scope of research areas, including dark matter searches, collider physics, matter-antimatter asymmetry, neutrino oscillations, and exploring physics beyond the Standard Model.
The group is part of the head node of the ARC Centre of Excellence for Dark Matter.
The School of Physics is also a key proponent of the Stawell Underground Physics Laboratory (SUPL) which will house SABRE – the first-ever direct-detection dark matter experiment in the southern hemisphere.
| Name | Supervisor | Degree | Research Project |
|---|---|---|---|
| Isabel Carr | Geoffrey Taylor | PhD | LHC/ATLAS |
| Sen Sam Chhun | Phillip Urquijo / Florian Bernlochner | PhD | SABRE, FASER |
| Guangyong Fu | Phillip Urquijo | PhD | SABRE |
| Daniel Marcantonio | Phillip Urquijo | PhD | Belle/Belle II |
| Mike Mews | Phillip Urquijo | PhD | SABRE |
| Lachlan Milligan | Phillip Urquijo | PhD | SABRE |
| Wi Han Ng | Phillip Urquijo | PhD | Hyper-K |
| Isabelle Ostrowski | Phillip Urquijo | PhD | Belle II |
| Sai Pemmaraju | Phillip Urquijo | PhD | Hyper-K, SABRE |
| Ananthakrishnan Ravindran | Elisabetta Barberio | PhD | XLZD, XENON |
| Paolo Rocchetti | Phillip Urquijo | PhD | Belle II |
| Kieran Rule | Elisabetta Barberio | PhD | SABRE |
| Owen Stanley | Elisabetta Barberio / Phillip Urquijo | PhD | SABRE, XLZD |
| Christian Albrecht | Martin Sevior | MSc | Belle II |
| Aspen Anderson | Geoffrey Taylor | MSc | HL-LHC/ATLAS |
| Adrian Babic | Martin Sevior | MSc | TPC/Micromegas |
| Yona Jessica Leony Detaq | Elisabetta Barberio | MSc | SABRE |
| Jackson Dun | Phillip Urquijo | MSc | SABRE |
| Shayne Earle | Phillip Urquijo | MSc | Hyper-K |
| Daniel Goldberg | Phillip Urquijo | MSc | Hyper-K |
| Georgia Juler | Elisabetta Barberio | MSc | SABRE |
| Akshayan Manivannan | Elisabetta Barberio | MSc | SABRE |
| Gohel Samarth Paraskumar | Elisabetta Barberio | MSc | SABRE |
| Rithik Rakesh | Phillip Urquijo | MSc | Hyper-K |
| Name | Primary Supervisor | Degree | Current Position |
|---|---|---|---|
| Marcel Hohmann | Phillip Urquijo | PhD 2025 | Postdoc at DESY |
| Daniel Ferlewicz | Phillip Urquijo | PhD 2023 | JSPS Fellow U Tokyo, Marie Curie Fellow at LPNHE Sorbonne |
| William Melbourne | Phillip Urquijo | PhD 2023 | R&D Engineer |
| Madeleine Zurowski | Elisabetta Barberio | PhD 2023 | Postdoc at U Toronto |
| Jo-Frederik Krohn | Phillip Urquijo | PhD 2022 | IBM Solutions Architect |
| Justin Tan | Phillip Urquijo | MPhil 2020 | PhD at U Cambridge |
| Giacomo Caria | Phillip Urquijo | PhD 2019 | Postdoc Sorbonne, Climate scientist |
| Eiasha Waheed | Phillip Urquijo | PhD 2018 | JSPS Fellow KEK, Postdoc U Melbourne |
| Luis Pesantez | Phillip Urquijo (Joint/Bonn) | PhD 2017 | Software Engineer |
| Name | Period of Employment | Current Position |
|---|---|---|
| Yajing Xing | 2024 | Research staff at LPNHE Sorbonne |
| William Melbourne | 2023 - 2024 | R&D Engineer |
| Marco Milesi | 2018 – 2023 | Data Science Manager |
| Matthew Gerathy | 2022 – 2023 | Data Scientist |
| Federico Scutti | 2016 – 2021 | Postdoc Swinburne |
| Francesco Tenchini | 2015 – 2017 | Postdoc DESY, Marie Curie Fellow U Pisa |
| Chunhua Li | 2014 – 2017 | Faculty at Liaoning Normal U |
SABRE
The aim of the SABRE experiment is to search for one possible dark matter candidate, Weakly Interacting Massive Particles (WIMPS). SABRE will look for WIMPS via direct detection in Sodium-Iodide crystals, surrounded by a large volume of liquid scintillator, which will act as a veto to eliminate unwanted background signals.
SABRE is located approximately 1 km underground in the Stawell Underground Physics Laboratory.
XLZD
A collaboration of experiments - XENON, LUX-ZEPLIN, and DARWIN - XLZD are all liquid xenon detectors designed for low-energy particle detection. XLZD searches for WIMP Dark Matter particles, exotic Dark Matter candidates, solar and supernova neutrinos, and cosmic rays.
Belle II
Belle II observes asymmetric, electron-positron collisions from the SuperKEKB accelerator. The detector has been designed to make precise measurements of weak interaction parameters, study exotic hadrons, and explore potential new phenomena beyond the Standard Model of particle physics.
Hyper-Kamiokande
The successor of Kamiokande and Super-Kamiokande, Hyper-Kamiokande (Hyper-K) will be the largest water Cherenkov neutrino detector in the world, with a detectable volume of 190 kton of ultra-purified water. The goal of Hyper-K is to measure Charge-Parity Violation in neutrino oscillations, investigate the neutrino mass hierarchy, and search for proton decay.
ATLAS
The ATLAS detector collects particles from over a billion collisions per second from the LHC. The large, 7000-tonne detector investigates a large scope of physics phenomena, from studying the Higgs boson to Beyond Standard Model searches.
Published 2024 | D. Ferlewicz, P. Urquijo et al. (Belle)
Published April 8, 2025 | E. Barberio et al. (SABRE South)
The SABRE South detector is designed to test the long-standing DAMA/LIBRA signal of an annually modulating rate consistent with dark matter by using the same target material. Located in the Southern Hemisphere, the detector is uniquely positioned to disentangle modulating seasonal effects.
| Name | Position | Conference |
|---|---|---|
| Kieran Rule | PhD Student | Kashiwa-no-ha Dark Matter and Cosmology Symposium, Tokyo 2024 |
| Name | Position | Award / Scholarship |
|---|---|---|
| Shayne Earle | MSc Student |
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| Wi Han Ng | PhD Student |
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| Isabelle Ostrowski | PhD Student |
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| Kieran Rule | PhD Student |
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| Owen Stanley | PhD Student |
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