Thermo-acoustic sound generation in the interaction of pulsed proton and laser beams with a water target
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, se...
Saved in:
| Main Authors: | , , , , , , , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
2015
|
| In: |
Astroparticle physics
Year: 2014, Volume: 65, Pages: 69-79 |
| ISSN: | 0927-6505 |
| DOI: | 10.1016/j.astropartphys.2014.12.003 |
| Online Access: | Resolving-System, lizenzpflichtig, Volltext: https://doi.org/10.1016/j.astropartphys.2014.12.003 Verlag, lizenzpflichtig, Volltext: http://www.sciencedirect.com/science/article/pii/S0927650514001893 
|
| Author Notes: | R. Lahmann, G. Anton, K. Graf, J. Hößl, A. Kappes, U. Katz, K. Mecke, S. Schwemmer |
| Summary: | 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. |
|---|---|
| Item Description: | Available online 17 December 2014 Gesehen am 05.06.2020 |
| Physical Description: | Online Resource |
| ISSN: | 0927-6505 |
| DOI: | 10.1016/j.astropartphys.2014.12.003 |