Bevan, S. and Danaher, S. and Perkin, J. and Ralph, S. and Rhodes, C. and Thompson, L. J. and Sloan, T. and Waters, D. and The ACoRNE Collaboration, et al. (2007) Simulation of ultra high energy neutrino induced showers in ice and water. Astroparticle Physics, 28 (3). pp. 366-379. ISSN 0927-6505Full text not available from this repository.
The CORSIKA program, usually used to simulate extensive cosmic ray air showers, has been adapted to work in a water or ice medium. The adapted CORSIKA code was used to simulate hadronic showers produced by neutrino interactions. The simulated showers have been used to study the spatial distribution of the deposited energy in the showers. This allows a more precise determination of the acoustic signals produced by ultra high energy neutrinos than has been possible previously. Some properties of the acoustic signals generated by such showers are described.
|Journal or Publication Title:||Astroparticle Physics|
|Uncontrolled Keywords:||Neutrino ; Showers ; Water ; CORSIKA ; Acoustic|
|Subjects:||Q Science > QC Physics|
|Departments:||Faculty of Science and Technology > Physics|
|Deposited On:||29 Oct 2008 13:38|
|Last Modified:||25 Mar 2017 01:15|
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