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Dr Bruce Dawson
Reader/Associate Professor
Research Interests:
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Ultra-high energy cosmic rays. These are the most energetic particles
known in Nature, and we are part of two large international collaborations
formed to determine the origin of these particles. The cosmic rays
of interest are incredibly energetic (in excess of 10^19 electron-volts)
but they are also incredibly rare (less than 1 particle per square
kilometre per year), so detectors must be large. The High resolution
Fly's Eye is a detector with a collecting area of 3000 square kilometres
during clear, moonless nights. The Pierre Auger Observatory will cover
a similar area 24 hours per day. We are experts on the fluorescence
detection technique, pioneered in Utah in the late 1970's. We are
also interested in interpreting the cosmic ray data, to determine
particle energies and mass, and their arrival directions.
Selected Publications:
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P. Sokolsky, P. Sommers and B.R. Dawson (1992)
Extremely High Energy Cosmic Rays
Physics Reports 217, 225-227
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D.J. Bird et al (1993)
Evidence for Correlated Changes in the Spectrum and Composition of
Cosmic Rays at Extremely High Energies
Physical Review Letters 71, 3401
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B.R. Dawson, H.Y. Dai, P. Sommers and S. Yoshida (1996)
Simulations of a Giant Hybrid Air Shower Detector
Astroparticle Physics 5, 239-247
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Roger Clay and Bruce Dawson Cosmic Bullets - High Energy Particles
in Astrophysics (Book)
(Allen and Unwin, Sydney, 1997; Addison-Wesley, Reading, Mass. 1998;
also published in Chinese and Spanish language versions)
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B.R. Dawson, R. Meyhandan and K.M. Simpson (1998)
A Comparison of Cosmic Ray Composition Measurements at the Highest
Energies
Astroparticle Physics 9 331-338
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T. Abu-Zayyad et al (2000)
Evidence for Changing Cosmic Ray Composition between 10^17eV and 10^18eV
from Multi-Component Measurements
Physical Review Letters 84, 4276-4279
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J.A. Bellido, R.W. Clay, B.R. Dawson and M. Johnston-Hollitt (2001)
Southern Hemisphere Observations of a 10^18eV Cosmic Ray Source Near
the Direction of the Galactic Centre
Astroparticle Physics 15, 167-175
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Physics
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Assoc. Prof Bruce Dawson
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