Thermo-acoustic Sound Generation in the Interaction of Pulsed Proton and Laser Beams with a Water Target
arXiv:1501.01494 · doi:10.1016/j.astropartphys.2014.12.003
Abstract
The generation of hydrodynamic radiation in interactions of pulsed proton and laser beams with matter is explored. The beams were directed into a water target and the resulting acoustic signals were recorded with pressure sensitive sensors. Measurements were performed with varying pulse energies, sensor positions, beam diameters and temperatures. The obtained data are matched by simulation results based on the thermo-acoustic model with uncertainties at a level of 10%. The results imply that the primary mechanism for sound generation by the energy deposition of particles propagating in water is the local heating of the medium. The heating results in a fast expansion or contraction and a pressure pulse of bipolar shape is emitted into the surrounding medium. An interesting, widely discussed application of this effect could be the detection of ultra-high energetic cosmic neutrinos in future large-scale acoustic neutrino detectors. For this application a validation of the sound generation mechanism to high accuracy, as achieved with the experiments discussed in this article, is of high importance.
arXiv comment12 pages, 15 figures
References in corpus (8)
- ANTARES: the first undersea neutrino telescope
- First Year Performance of The IceCube Neutrino Telescope
- Neutrinos from propagation of ultra-high energy protons
- AMADEUS - The Acoustic Neutrino Detection Test System of the ANTARES Deep-Sea Neutrino Telescope
- Experimental Study of Acoustic Ultra-High-Energy Neutrino Detection
- Simulation of Ultra High Energy Neutrino Interactions in Ice and Water
- Underwater Acoustic Detection of Ultra High Energy Neutrinos
- Study of the acoustic signature of UHE neutrino interactions in water and ice
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