Converging on new particles and fundamental symmetries. The goal of this project is to test theories for new particles and fundamental symmetries. By using advanced computational and statistical methods to combine all relevant data from many different experiments with a large number of different theoretical predictions, it expects to reveal just how well different theories actually describe reality. This will help us to understand what new particles and fundamental symmetries exist beyond thos ....Converging on new particles and fundamental symmetries. The goal of this project is to test theories for new particles and fundamental symmetries. By using advanced computational and statistical methods to combine all relevant data from many different experiments with a large number of different theoretical predictions, it expects to reveal just how well different theories actually describe reality. This will help us to understand what new particles and fundamental symmetries exist beyond those we already know. It will lead to new algorithms and computational methods in machine learning and statistical sampling, and will train a cohort of graduates highly skilled in statistical data science and research computing.Read moreRead less
Utilising artificial intelligence to elucidate the physics of galaxies. For decades astronomers have puzzled over the connection between the structure and evolution of galaxies and the role played by host environments. This project aims to resolve this problem by combining multi-wavelength observations, multi-component simulations, and pioneering data analysis using artificial intelligence. In particular, we target the nearby Fornax galaxy cluster as a laboratory for studying galaxy formation in ....Utilising artificial intelligence to elucidate the physics of galaxies. For decades astronomers have puzzled over the connection between the structure and evolution of galaxies and the role played by host environments. This project aims to resolve this problem by combining multi-wavelength observations, multi-component simulations, and pioneering data analysis using artificial intelligence. In particular, we target the nearby Fornax galaxy cluster as a laboratory for studying galaxy formation in dense environments. Using our novel machine learning techniques, we will elucidate the physical mechanisms that drive the rapid evolution of star formation, galactic nuclei, and gas and dust content within Fornax. Our predictions will benefit ongoing and future surveys at the national and international level. Read moreRead less
A Space Odyssey: Exploring the Universe with Gravitational-Wave Sirens. How fast is the Universe expanding? This project aims to produce the most precise measurement to date of the present day expansion rate of the Universe using gravitational waves and thus resolve current tensions plaguing existing measurements. We plan to develop the most comprehensive catalogue of gravitational waves and their hosts using the largest galaxy surveys in the world and use innovative statistical techniques to ex ....A Space Odyssey: Exploring the Universe with Gravitational-Wave Sirens. How fast is the Universe expanding? This project aims to produce the most precise measurement to date of the present day expansion rate of the Universe using gravitational waves and thus resolve current tensions plaguing existing measurements. We plan to develop the most comprehensive catalogue of gravitational waves and their hosts using the largest galaxy surveys in the world and use innovative statistical techniques to extract cosmological measurements from them. Expected outcomes include new knowledge of what the Universe is made of and how it has evolved, and enhanced international collaboration between Australia and other survey member countries. Anticipated benefits include new software and methods for the analysis of big data.Read moreRead less
Discovery Early Career Researcher Award - Grant ID: DE220100003
Funder
Australian Research Council
Funding Amount
$450,675.00
Summary
Understanding diversity: chemical and kinematic tracers of galaxy evolution. Understanding how galaxies form and evolve throughout the Universe is one of the biggest outstanding challenges in astrophysics. The project aims to develop an innovative method for understanding the fundamental properties of angular momentum and chemical content of all kinds of galaxies. This project expects to generate new knowledge in the field of galaxy evolution, for the first time enabling astronomers to robustly ....Understanding diversity: chemical and kinematic tracers of galaxy evolution. Understanding how galaxies form and evolve throughout the Universe is one of the biggest outstanding challenges in astrophysics. The project aims to develop an innovative method for understanding the fundamental properties of angular momentum and chemical content of all kinds of galaxies. This project expects to generate new knowledge in the field of galaxy evolution, for the first time enabling astronomers to robustly compare distant, long-ago galaxies with those in the nearby, present-day Universe. Expected outcomes include a novel framework for determining galaxy morphology, based on fundamental physics. The framework will be highly beneficial to understanding the evolution of diverse types of galaxies, including our own Milky Way.Read moreRead less
Australian Laureate Fellowships - Grant ID: FL180100168
Funder
Australian Research Council
Funding Amount
$2,899,722.00
Summary
Illuminating the dark universe. This project aims to measure and explain the dark side of the universe, by performing new theoretical analyses of two groundbreaking surveys. Dark energy and dark matter are amongst the most profound puzzles facing fundamental physics. The Dark Energy Survey expects to discover approximately 3000 supernovae, and using The Dark Energy Spectroscopic Instrument will measure distances to 30 million galaxies. This project will combine these findings to determine whethe ....Illuminating the dark universe. This project aims to measure and explain the dark side of the universe, by performing new theoretical analyses of two groundbreaking surveys. Dark energy and dark matter are amongst the most profound puzzles facing fundamental physics. The Dark Energy Survey expects to discover approximately 3000 supernovae, and using The Dark Energy Spectroscopic Instrument will measure distances to 30 million galaxies. This project will combine these findings to determine whether dark energy changes with time, narrow the search for a quantum theory of gravity, and complete the standard model of particle physics by measuring the mass of the neutrino, a subatomic particle. This will substantially advance our understanding of the physics of our Universe, inspiring the next generation of innovators.Read moreRead less