|COOKIES: By using this website you agree that we can place Google Analytics Cookies on your device for performance monitoring.|
The use of the Moon as a Particle Detector
If you have a question about this talk, please contact David Titterington.
The ultra-high-energy end of the spectrum of cosmic rays is critical for understanding the nature and origin of these particles. However, the low flux of cosmic rays at these energies necessitates the use of extremely large detectors. The largest potential aperture is offered by the use of the moon as the detector, with ground-based radio telescopes used to detect the nanosecond-scale pulse produced when an ultra-high-energy particle interacts in the lunar regolith. I will review the motivation and history of these experiments, covering the specialised techniques required to detect pulses on such short timescales and the evaluation of the resulting limits on the fluxes of ultra-high-energy cosmic rays and neutrinos.
This talk is part of the Cavendish Astrophysics Seminars series.
This talk is included in these lists:
Note that ex-directory lists are not shown.
Other listsCRASSH events Populations in Statistical genetics Cambridge University Medical Humanities Society
Other talksEvery Body Matters: Using Action Research to Work Towards Injury Prevention and Health Promotion in Elite Young Instrumental Musicians at a Specialist Music School No general structure Myth, Misogyny, and Magic: Mansplaining Medea in the Middle Ages TBC Production Processes Group Seminar - 'Manufacturing at twice the speed: limits to DoD inkjet printing' Recent progress at Quantum Computing and Devices Laboratories