TLUE ? Tidbinbilla Lunar Ultra-high energy neutrino Experiment

Physics

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Solar System, Parkes

Scientific paper

Use of radio telescopes for astro-particle physics is a growing new tool toward the forthcoming SKA era. In this project we will use both 70m and 34m antennas at Tidinbilla tracking station (CDSCC) to search for lunar Cherenkov emission generated by ultra-high-energy cosmic rays and neutrinos (Askaryan effect). The Tidbinbilla radio telescopes will provide sensitivity better than any of previous trials using ground based radio telescopes. By covering uniform area along the Moon orbit in the sky, we will have sensitivity better than any past experiments to directions of know ultra-high-energy cosmic ray sources such as Centaurus-A.

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