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  • Funded Activity

    Discovery Projects - Grant ID: DP0879737

    Funder
    Australian Research Council
    Funding Amount
    $330,000.00
    Summary
    CP Symmetry Violation in Strange B Meson decays at the Belle Experiment. This research exploits very recent development in high energy physics to formulate new tests on the limits of our understanding of matter-antimatter symmetry violation in our universe. The researchers have internationally recognised expertise in distributed Grid computing, which has been pioneered by the high energy physics community, and is now finding wide deployment in other scientific fields. Deployment of a Belle Data .... CP Symmetry Violation in Strange B Meson decays at the Belle Experiment. This research exploits very recent development in high energy physics to formulate new tests on the limits of our understanding of matter-antimatter symmetry violation in our universe. The researchers have internationally recognised expertise in distributed Grid computing, which has been pioneered by the high energy physics community, and is now finding wide deployment in other scientific fields. Deployment of a Belle Data Grid will provide true international interoperability with national Grid infrastructure, and substantial opportunity for expanded international collaboration on eresearch infrastructure. High Energy Physics also provides post-graduate students with the best possible exposure to leading international researchers.
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    Funded Activity

    Federation Fellowships - Grant ID: FF0348478

    Funder
    Australian Research Council
    Funding Amount
    $1,450,370.00
    Summary
    Precision Pulsar Timing and its Applications. The rapidly rotating pulsars known as millisecond pulsars have period stabilities which rival that of the best terrestrial clocks. Observations of many millisecond pulsars spread across the sky should allow detection of the gravitational-wave background - likely to be the first direct detection of gravity waves. It will also enable establishment of a long-term time standard which is independent of and probably superior to that derived from terrestria .... Precision Pulsar Timing and its Applications. The rapidly rotating pulsars known as millisecond pulsars have period stabilities which rival that of the best terrestrial clocks. Observations of many millisecond pulsars spread across the sky should allow detection of the gravitational-wave background - likely to be the first direct detection of gravity waves. It will also enable establishment of a long-term time standard which is independent of and probably superior to that derived from terrestrial clocks. New analysis techniques and establishment of an international observing network will be required. Investigation and application of techniques for overcoming radio interference will be an important part of the project.
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    Funded Activity

    Discovery Projects - Grant ID: DP0666822

    Funder
    Australian Research Council
    Funding Amount
    $120,000.00
    Summary
    Defeating Radio Frequency Interference. The radio spectrum is a valuable resource. Development of techniques which minimize the impact of various users on one another, allowing this resource to be shared, will benefit the entire community. For astronomy in particular, shared use is essential because of the very wide bandwidths needed to obtain sufficient sensitivity. Usage of the radio spectrum is increasing rapidly and radio telescopes are becoming more and more sensitive, compounding the probl .... Defeating Radio Frequency Interference. The radio spectrum is a valuable resource. Development of techniques which minimize the impact of various users on one another, allowing this resource to be shared, will benefit the entire community. For astronomy in particular, shared use is essential because of the very wide bandwidths needed to obtain sufficient sensitivity. Usage of the radio spectrum is increasing rapidly and radio telescopes are becoming more and more sensitive, compounding the problems. The digital signal processing techniques developed under this project will be widely applicable, not only to future radio astronomy facilities such as the Square Kilometer Array, but also to the communications industry generally.
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