Building the future of theoretical astrophysics: Views of the virtual Universe. The virtual observatory (VO) is a major international initiative to
maximise scientific returns from astrophysical databases by providing
enhanced network access to data and analysis procedures, but it
lacks a vital theoretical complement. This project presents a unified
forward modelling approach to three key problems in: 1. gravitational
lens reconstruction; 2. solar coronal magnetic fields; and 3.
interpreta ....Building the future of theoretical astrophysics: Views of the virtual Universe. The virtual observatory (VO) is a major international initiative to
maximise scientific returns from astrophysical databases by providing
enhanced network access to data and analysis procedures, but it
lacks a vital theoretical complement. This project presents a unified
forward modelling approach to three key problems in: 1. gravitational
lens reconstruction; 2. solar coronal magnetic fields; and 3.
interpretation of stellar oscillations. The goal is the development of
a `virtual telescope' for visualising synthetic datasets, designed to
provide the necessary theoretical complement to the VO.
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Relativistic Plasma Astrophysics: Pulsars, IDVs and transients. We will tackle four fundamental problems in theoretical astrophysics. How do small, dead stars known as pulsars produce radio emission? Why do quasars, the most distant objects in the universe, twinkle at radio wavelengths? What is the relationship between violent bursts of gamma-ray emission and other astrophysical explosions? Why are strongly magnetized pulsars so efficient at radiating high energy photons? We will attack these qu ....Relativistic Plasma Astrophysics: Pulsars, IDVs and transients. We will tackle four fundamental problems in theoretical astrophysics. How do small, dead stars known as pulsars produce radio emission? Why do quasars, the most distant objects in the universe, twinkle at radio wavelengths? What is the relationship between violent bursts of gamma-ray emission and other astrophysical explosions? Why are strongly magnetized pulsars so efficient at radiating high energy photons? We will attack these questions by developing new theories for coherent emission, scintillation, particle acceleration and processes in superstrong magnetic fields, and testing them against observationsRead moreRead less
Development and study of a new theory of gravity. Gravity is thought to be an understood physical phenomena. But recently dramatic discoveries have revealed that major aspects of this phenomenon have been completely missed. This research project will develop and explore implications of these discoveries. At one level this project is about major breakthroughs in fundamental science, but discoveries are revealing space to be a complex dynamic system, and new technologies to detect and exp ....Development and study of a new theory of gravity. Gravity is thought to be an understood physical phenomena. But recently dramatic discoveries have revealed that major aspects of this phenomenon have been completely missed. This research project will develop and explore implications of these discoveries. At one level this project is about major breakthroughs in fundamental science, but discoveries are revealing space to be a complex dynamic system, and new technologies to detect and exploit this are foreseen. There is some evidence that space is a self-organising information system of a totally new kind, and this will also have applications. At a scientific level these developments will attract considerable international attention and will enthuse younger researchersRead moreRead less
Super-AGB Stars: the Missing Link? By being the first to investigate a specific class of stars, Australia will also be the first to reap the scientific rewards from the many applications that will follow - including the chemical history of
the Galaxy and how globular clusters form. We will also develop large-scale computing tools using the latest in cluster computing technology to study the multi-dimensional character of a special class
of supernova explosion. We extend a fruitful collaboratio ....Super-AGB Stars: the Missing Link? By being the first to investigate a specific class of stars, Australia will also be the first to reap the scientific rewards from the many applications that will follow - including the chemical history of
the Galaxy and how globular clusters form. We will also develop large-scale computing tools using the latest in cluster computing technology to study the multi-dimensional character of a special class
of supernova explosion. We extend a fruitful collaboration with a super-computer centre in the US and also train graduate students in advanced computing techniques for Australia's future, in both science and other applications and technologies.Read moreRead less
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
Plasma Astrophysics under Extreme Conditions. A new branch of theoretical physics, quantum plasmadynamics (QPD), will be applied to plasmas under extreme conditions of magnetic field and density, to plasma-neutrino effects and nonlinear radiation.
Magnetic energy dissipation in solar flares will be attributed to a large number of coupled, local, transient, anomalously resistive regions excited by current filamentation. The model will include nonlocal energy release at Alfvenic fronts, 3D reconn ....Plasma Astrophysics under Extreme Conditions. A new branch of theoretical physics, quantum plasmadynamics (QPD), will be applied to plasmas under extreme conditions of magnetic field and density, to plasma-neutrino effects and nonlinear radiation.
Magnetic energy dissipation in solar flares will be attributed to a large number of coupled, local, transient, anomalously resistive regions excited by current filamentation. The model will include nonlocal energy release at Alfvenic fronts, 3D reconnection at magnetic nulls, and bulk energization of electrons.
`Coherence? in sources of coherent emission will be quantified and a model for its interpretation for highly intermittent wave growth will be formulated.Read moreRead less
The application of Markov Chain Monte Carlo methods to the search for space-time variations of fundamental constants. This work will establish Australia as the world leader in one of the most vibrant topics in current physics research. The results obtained could reveal extra dimensions in our universe and provide the first experimental evidence for string theories. The proposed research will also fundamental new information about dark matter and dark energy, the two most pressing problems in c ....The application of Markov Chain Monte Carlo methods to the search for space-time variations of fundamental constants. This work will establish Australia as the world leader in one of the most vibrant topics in current physics research. The results obtained could reveal extra dimensions in our universe and provide the first experimental evidence for string theories. The proposed research will also fundamental new information about dark matter and dark energy, the two most pressing problems in cosmology. The solutions of these problems will revolutionise our understanding of the universe. This program involves collaborations with major international institutes and provides a superb training-ground for Australian postgraduate students.Read moreRead less
ARC Complex Open Systems Research Network. Complexity is the common frontier in the physical, biological and social sciences. This Network will link specialists in all three sciences through five generic conceptual and mathematical theme activities. It will promote research into how subsystems self-organise into new emergent structures when assembled into an open, non-equilibrium system. Outcomes will include new technologies and software tools and deeper understanding of fundamental questions i ....ARC Complex Open Systems Research Network. Complexity is the common frontier in the physical, biological and social sciences. This Network will link specialists in all three sciences through five generic conceptual and mathematical theme activities. It will promote research into how subsystems self-organise into new emergent structures when assembled into an open, non-equilibrium system. Outcomes will include new technologies and software tools and deeper understanding of fundamental questions in science. An essential function of the network will be introducing researchers end users to new tools and broadening the horizons of graduate students.Read moreRead less
Fluctuations in the properties of nonequilibrium fluids and the influence of thermostatting mechanisms. The behaviour of nonequilibrium fluids will be studied by combining ideas from liquid state theory, statistical mechanics and dynamical systems theory. This work will result in development and testing of mathematical expressions (Fluctuation Theorems) that are consistent with the Second Law of Thermodynamics, which determines the direction of any change in any macroscopic system, but are also ....Fluctuations in the properties of nonequilibrium fluids and the influence of thermostatting mechanisms. The behaviour of nonequilibrium fluids will be studied by combining ideas from liquid state theory, statistical mechanics and dynamical systems theory. This work will result in development and testing of mathematical expressions (Fluctuation Theorems) that are consistent with the Second Law of Thermodynamics, which determines the direction of any change in any macroscopic system, but are also applicable to microscopic systems. The expressions will determine the probability that finite sized systems will violate the Second Law for small periods of time and will therefore contribute to development of a fundamental understanding of microscopic systems and the development of nanotechnology.
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Fluid properties and chaotic dynamics in equilibrium and nonequilibrium states. Over the last decade a revolution has been taking place in nonequilibrium statistical mechanics [Physics Today, Sept, 2002]. This revolution is characterized by adapting the mathematical theory of chaos to nonequilibrium statistical mechanics. Fundamental new theorems and algorithms for computing transport coefficients have been derived. The CIs have played a key role in this revolution. We seek to broaden these dev ....Fluid properties and chaotic dynamics in equilibrium and nonequilibrium states. Over the last decade a revolution has been taking place in nonequilibrium statistical mechanics [Physics Today, Sept, 2002]. This revolution is characterized by adapting the mathematical theory of chaos to nonequilibrium statistical mechanics. Fundamental new theorems and algorithms for computing transport coefficients have been derived. The CIs have played a key role in this revolution. We seek to broaden these developments by: generalizing a theorem which relates transport coefficients to chaoticity; detailed studies of the influence of thermostatting mechanisms on nonequilibrium chaoticity and fluctuations, and by understanding the range of applicability of a nonequilibrium fluctuation theorem for non-isoenergetic systems.Read moreRead less