Linkage Infrastructure, Equipment And Facilities - Grant ID: LE160100094
Funder
Australian Research Council
Funding Amount
$150,000.00
Summary
The Mopra Radio Telescope. The Mopra Radio Telescope:
This project aims to use Australia’s Mopra Radio Telescope – the largest millimetre-wave dish in the southern hemisphere – to complete a survey of the distribution of molecular gas across the southern Milky Way. The millimetre-wavelength sky holds the key for understanding molecular clouds in which stars are born, and the Mopra Telescope is the world’s most capable facility for imaging these clouds. The expected outcome is an order of magnit ....The Mopra Radio Telescope. The Mopra Radio Telescope:
This project aims to use Australia’s Mopra Radio Telescope – the largest millimetre-wave dish in the southern hemisphere – to complete a survey of the distribution of molecular gas across the southern Milky Way. The millimetre-wavelength sky holds the key for understanding molecular clouds in which stars are born, and the Mopra Telescope is the world’s most capable facility for imaging these clouds. The expected outcome is an order of magnitude improvement in the clarity of our view of this central component of the Galaxy. The project also aims to enable Mopra to serve as a key element in the Australian Long Baseline Array. The project aims to ensure Australian involvement in three grand design international endeavours.Read moreRead less
Particle astrophysics with the Pierre Auger observatory. Australia's scientific reputation is enhanced through participation in international collaborations that aim to solve long-standing mysteries in science. The Pierre Auger Observatory covers a huge 3000 square km in western Argentina, where we are attempting to solve one of the biggest puzzles in modern astrophysics - the origin of the highest energy cosmic rays, particles 100 million times more energetic than we can produce on Earth. Ade ....Particle astrophysics with the Pierre Auger observatory. Australia's scientific reputation is enhanced through participation in international collaborations that aim to solve long-standing mysteries in science. The Pierre Auger Observatory covers a huge 3000 square km in western Argentina, where we are attempting to solve one of the biggest puzzles in modern astrophysics - the origin of the highest energy cosmic rays, particles 100 million times more energetic than we can produce on Earth. Adelaide scientists were founding members of the Auger project, and now have leading roles within the experiment. This is providing our students with access to world-class facilities and researchers in a field which has moved to the mainstream of astrophysics research.Read moreRead less
Searches for the Origin of Ultra-High Energy Cosmic Rays. The highest energy cosmic rays are the most energetic particles known in the Universe, but we do not know their origin. The ARC-supported Pierre Auger Project is now beginning data acquistion, and will be fully constructed in 2005, with a collecting power 10 times larger than previous experiments. The proposed fellow will collaborate with the Adelaide group in searching for clusters of arrival directions, with an aim of discovering astro ....Searches for the Origin of Ultra-High Energy Cosmic Rays. The highest energy cosmic rays are the most energetic particles known in the Universe, but we do not know their origin. The ARC-supported Pierre Auger Project is now beginning data acquistion, and will be fully constructed in 2005, with a collecting power 10 times larger than previous experiments. The proposed fellow will collaborate with the Adelaide group in searching for clusters of arrival directions, with an aim of discovering astrophysical sources. This project will involve sophisticated event reconstruction and analysis techniques, which take advantage of Auger's unique combination of huge collecting power and good control of systematic uncertainties.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE170100217
Funder
Australian Research Council
Funding Amount
$850,000.00
Summary
Australian Partnership in Advanced LIGO+. This project aims to improve the sensitivity of the Advanced Laser Interferometer Gravitational wave Observatory (aLIGO). aLIGO’s detection of gravitational waves proved general relativity in the strong field limit and the existence of black hole binary systems. The increased sensitivity will enable daily detections and new classes of events, opening the field of gravitational wave astronomy. Since telescopes can detect only 5% of the stuff in the univer ....Australian Partnership in Advanced LIGO+. This project aims to improve the sensitivity of the Advanced Laser Interferometer Gravitational wave Observatory (aLIGO). aLIGO’s detection of gravitational waves proved general relativity in the strong field limit and the existence of black hole binary systems. The increased sensitivity will enable daily detections and new classes of events, opening the field of gravitational wave astronomy. Since telescopes can detect only 5% of the stuff in the universe, this is expected to greatly improve understanding of the universe. This Australian partnership will put its physicists and astronomers at the vanguard of this field and inspire the next generation to study the physical sciences.Read 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
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE130100032
Funder
Australian Research Council
Funding Amount
$990,000.00
Summary
Australian partnership in advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) - continuation. Advanced Laser Interferometer Gravitational-Wave Obervatory (LIGO) will be the first gravitational wave observatory capable of frequent observation of known sources of gravitational waves leading to the birth of gravitational wave astronomy. By playing a key role in this facility, Australia will reap the scientific rewards of being part of the most exciting frontier of physics in the 2 ....Australian partnership in advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) - continuation. Advanced Laser Interferometer Gravitational-Wave Obervatory (LIGO) will be the first gravitational wave observatory capable of frequent observation of known sources of gravitational waves leading to the birth of gravitational wave astronomy. By playing a key role in this facility, Australia will reap the scientific rewards of being part of the most exciting frontier of physics in the 21st century.Read moreRead less
Ultra High Energy Cosmic Ray and Neutrino Astronomy using Radio Telescopes. There will be an increase in Australian visibility in the high energy astrophysics community and stronger links between and within the fields of radio astronomy and high energy astrophysics in Australia, and internationally. This project will enhance Australian participation in the international Square Kilometre Array. By making observations using the Australia Telescope we may discover the first UHE neutrino - this wo ....Ultra High Energy Cosmic Ray and Neutrino Astronomy using Radio Telescopes. There will be an increase in Australian visibility in the high energy astrophysics community and stronger links between and within the fields of radio astronomy and high energy astrophysics in Australia, and internationally. This project will enhance Australian participation in the international Square Kilometre Array. By making observations using the Australia Telescope we may discover the first UHE neutrino - this would have huge impact and prestige for Australia. The technology developed resulting from this project will contribute to Australia's IT base. Read moreRead less
LUNASKA, a theoretical and experimental project for UHE neutrino astrophysics using a giant radio observatory. There will be an increase in Australian visibility in the high energy astrophysics community and stronger links between and within the fields of radio astronomy and high energy astrophysics in Australia, and internationally. This project will enhance Australian participation in the international Square Kilometre Array. By making observations using the Australia Telescope we may discov ....LUNASKA, a theoretical and experimental project for UHE neutrino astrophysics using a giant radio observatory. There will be an increase in Australian visibility in the high energy astrophysics community and stronger links between and within the fields of radio astronomy and high energy astrophysics in Australia, and internationally. This project will enhance Australian participation in the international Square Kilometre Array. By making observations using the Australia Telescope we may discover the first UHE neutrino - this would have huge impact and prestige for Australia. The technology developed resulting from this project will contribute to Australia's IT base. Hosting an international workshop will benefit national prestige and economy. Read moreRead less
Dark gas and the formation of molecular clouds. Using frontline radio telescopes in Australia, Chile and Antarctica the project aims to understand how molecular clouds are formed in space, a part of the life cycle of our galaxy, and the role of hard-to-detect 'dark gas' in this process. Australia's Mopra telescope plays a central role in this international endeavour.
Energetic particle interactions in the universe: consequences for cosmic ray, gamma ray and neutrino astrophysics. The most energetic phenomena in the Universe will be explored with giant cosmic ray, neutrino and gamma ray telescopes. Particles accelerated or produced in astrophysical sources interact in their magnetic, matter and radiation environment, making cosmic rays, gamma rays and neutrinos. Subsequently, interactions in space as they travel to Earth change what we see. With theoretical w ....Energetic particle interactions in the universe: consequences for cosmic ray, gamma ray and neutrino astrophysics. The most energetic phenomena in the Universe will be explored with giant cosmic ray, neutrino and gamma ray telescopes. Particles accelerated or produced in astrophysical sources interact in their magnetic, matter and radiation environment, making cosmic rays, gamma rays and neutrinos. Subsequently, interactions in space as they travel to Earth change what we see. With theoretical work proposed in this project we aim to determine where in the Universe the highest energy cosmic rays originate, and the fundamental processes responsible for them. It will also lead to a greater understanding of how active galaxies and other astrophysical objects function.Read moreRead less