Physics of extreme brightness temperatures in radioastronomical sources. Pulsars and some quasars are so very bright that the conventional explanation for radioastronomical emission from other sources either does not apply to them, or presents unsolved problems. We see (in radio waves) these sources through the interstellar medium which acts like a wrinkled pane of glass in distorting the image. New scientific ideas and methodologies are proposed here and will be explored in the project, with th ....Physics of extreme brightness temperatures in radioastronomical sources. Pulsars and some quasars are so very bright that the conventional explanation for radioastronomical emission from other sources either does not apply to them, or presents unsolved problems. We see (in radio waves) these sources through the interstellar medium which acts like a wrinkled pane of glass in distorting the image. New scientific ideas and methodologies are proposed here and will be explored in the project, with the objective to understand these sources and to extract information on their propreties and those of the interstellar medium. Read moreRead less
Interstellar Gas Dynamics. The conversion of interstellar gas into stars is a key process in the life-history of galaxies and the formation of planetary systems. Star formation takes place within a heterogeneous, dynamic cloud, and entails a million-fold contraction controlled by a complex interplay between gravity, magnetic forces, ionisation balance, chemical reactions and particles of interstellar dust. Previous modelling has adopted inappropriate approximations for the evolution of the mag ....Interstellar Gas Dynamics. The conversion of interstellar gas into stars is a key process in the life-history of galaxies and the formation of planetary systems. Star formation takes place within a heterogeneous, dynamic cloud, and entails a million-fold contraction controlled by a complex interplay between gravity, magnetic forces, ionisation balance, chemical reactions and particles of interstellar dust. Previous modelling has adopted inappropriate approximations for the evolution of the magnetic field. This research will bring a rigorous treatment of magnetic diffusion to bear on the theory of cloud evolution, shock waves, star formation and protoplanetary discs.
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Complex plasmas: self-organized dusty matter from nanotechnology to astrophysics. The importance of complex plasmas is based on their intricate self-organized behaviour, on their rich variety in nature and extensive use in the laboratory and advanced technologies. This project aims at breakthrough results advancing the fundamental knowledge and contributing to frontier technologies such as nanoelectronics and nanotechnology as well as reliability of space technological systems and communication ....Complex plasmas: self-organized dusty matter from nanotechnology to astrophysics. The importance of complex plasmas is based on their intricate self-organized behaviour, on their rich variety in nature and extensive use in the laboratory and advanced technologies. This project aims at breakthrough results advancing the fundamental knowledge and contributing to frontier technologies such as nanoelectronics and nanotechnology as well as reliability of space technological systems and communications. The project will boost fundamental and applied aspects of the Australian science as well as international collaborative links of Australian research and technology by allowing access and involvement to advanced multi-national programs and high-profile experiments such as those on board the International Space Station.Read moreRead less
Feedback Processes in Galaxy Formation. We have an opportunity to combine the best Australian theory with the best local and international telescopes, to probe the murky story of how galaxies form and why they look they way they do today. By looking back to a time when the Universe was only 1 billion years old, and comparing what we see with cutting edge supercomputer simulations plus pure theory, we will gain insight into the birth of entire galaxies. The results will form part of the study o ....Feedback Processes in Galaxy Formation. We have an opportunity to combine the best Australian theory with the best local and international telescopes, to probe the murky story of how galaxies form and why they look they way they do today. By looking back to a time when the Universe was only 1 billion years old, and comparing what we see with cutting edge supercomputer simulations plus pure theory, we will gain insight into the birth of entire galaxies. The results will form part of the study of how the universe works - that is driving astrophysics today, and represents pure research for the sake of advancing knowledge and showing us where we fit into the Universe. In doing so we will also advance Australia's base of theoretical and computational expertise.Read moreRead less
Field Statistics of Space and Astrophysical Phenomena. Waves and radiation typically occur in bursts and persist, with their driving particle distributions, for unexpectedly long distances in space and astrophysical sources. These features cannot be accounted for with older plasma theory but are explained naturally with stochastic growth theory (SGT). Recent observations show SGT to be widely applicable in space and for pulsars. We propose to make SGT into a quantitative dynamic theory tested on ....Field Statistics of Space and Astrophysical Phenomena. Waves and radiation typically occur in bursts and persist, with their driving particle distributions, for unexpectedly long distances in space and astrophysical sources. These features cannot be accounted for with older plasma theory but are explained naturally with stochastic growth theory (SGT). Recent observations show SGT to be widely applicable in space and for pulsars. We propose to make SGT into a quantitative dynamic theory tested on known SGT systems, to discover and interpret field statistics of natural radio emissions, and to develop and test observationally theories based on SGT and associated wave/radiation processes for key space and astrophysical phenomena.Read moreRead less