Cosmic powerhouses: The birth, death, and legacy of black hole jets. This project targets relativistic jets powered by supermassive black holes - the most powerful systems in the Universe. Theoretically, the enormous energies released have a profound influence on how galaxies evolve; empirically, observations reveal signatures of their impact across cosmic time. However, fundamental questions remain about how these jets are triggered and what impact they have on galaxies. The project will addres ....Cosmic powerhouses: The birth, death, and legacy of black hole jets. This project targets relativistic jets powered by supermassive black holes - the most powerful systems in the Universe. Theoretically, the enormous energies released have a profound influence on how galaxies evolve; empirically, observations reveal signatures of their impact across cosmic time. However, fundamental questions remain about how these jets are triggered and what impact they have on galaxies. The project will address these questions using novel supercomputer models of black hole jets in realistic cosmological environments, then confront these predictions with new data from Square Kilometre Array (SKA) pathfinding radio telescopes. This will substantially enhance Australia’s leadership capacity in a strategically important area.Read moreRead less
Relativistic Particles in Star-Forming Galaxies. This project aims to understand how galactic evolution is shaped by the relativistic particles known as cosmic rays that fill interstellar space. We understand only poorly how cosmic rays interact with non-relativistic interstellar matter, which in turn limits our understanding of how they affect galaxies. The project seeks to resolve this question by calculating how cosmic ray-matter interaction gives rise to light and neutrinos that we can obser ....Relativistic Particles in Star-Forming Galaxies. This project aims to understand how galactic evolution is shaped by the relativistic particles known as cosmic rays that fill interstellar space. We understand only poorly how cosmic rays interact with non-relativistic interstellar matter, which in turn limits our understanding of how they affect galaxies. The project seeks to resolve this question by calculating how cosmic ray-matter interaction gives rise to light and neutrinos that we can observe using current and future telescopes, enabling us to use observations from these telescopes to solve the problem of cosmic ray-matter interaction. This would resolve the question of how cosmic rays shape galaxy evolution, and thus represent a substantial advance in the theory of galaxy formation.Read moreRead less
Discovery Early Career Researcher Award - Grant ID: DE240100433
Funder
Australian Research Council
Funding Amount
$390,627.00
Summary
Origins and implications of cosmic explosions . This project aims to solve the origin of Fast Radio Bursts (FRBs) by conducting a study of a large sample (>100) of localised bursts detected with a new coherent FRB detection system called CRACO deployed at the Australia Square Kilometre Array Pathfinder (ASKAP). Such a rich sample will enable novel studies of the structure of the Universe. The powerful and sensitive CRACO system will also search for transients that last for hundreds of millisecon ....Origins and implications of cosmic explosions . This project aims to solve the origin of Fast Radio Bursts (FRBs) by conducting a study of a large sample (>100) of localised bursts detected with a new coherent FRB detection system called CRACO deployed at the Australia Square Kilometre Array Pathfinder (ASKAP). Such a rich sample will enable novel studies of the structure of the Universe. The powerful and sensitive CRACO system will also search for transients that last for hundreds of milliseconds, exploring new types of astrophysical phenomena that give insight into the Universe's extremes. These discoveries will have a significant impact on science, establishing Australia as a key player in the international FRB community.
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On the origin of very massive back holes. This project aims to investigate the origin of massive black holes observed in recent years by gravitational wave detectors. This project expects to generate new knowledge in the area of very massive stars utilising stellar evolution models, hydrodynamic simulations, light curve calculations and supernova observations, in order to explain the unexpected absence of a gap in the black hole mass distribution. Expected outcomes of this project include a bett ....On the origin of very massive back holes. This project aims to investigate the origin of massive black holes observed in recent years by gravitational wave detectors. This project expects to generate new knowledge in the area of very massive stars utilising stellar evolution models, hydrodynamic simulations, light curve calculations and supernova observations, in order to explain the unexpected absence of a gap in the black hole mass distribution. Expected outcomes of this project include a better understanding of mass loss and the collapse of very massive stars as key factors for the observed black hole mass distribution.This should provide significant benefits for gravitational wave astronomy, but also for observations of stellar explosions by informing future survey strategies.
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