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Simulation of ultra high energy neutrino induced showers in ice and water.

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Simulation of ultra high energy neutrino induced showers in ice and water. / Bevan, S.; Danaher, S.; Perkin, J. et al.
In: Astroparticle Physics, Vol. 28, No. 3, 11.2007, p. 366-379.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Bevan, S, Danaher, S, Perkin, J, Ralph, S, Rhodes, C, Thompson, LJ, Sloan, T, Waters, D & The ACoRNE Collaboration, EA 2007, 'Simulation of ultra high energy neutrino induced showers in ice and water.', Astroparticle Physics, vol. 28, no. 3, pp. 366-379. https://doi.org/10.1016/j.astropartphys.2007.08.001

APA

Bevan, S., Danaher, S., Perkin, J., Ralph, S., Rhodes, C., Thompson, L. J., Sloan, T., Waters, D., & The ACoRNE Collaboration, E. A. (2007). Simulation of ultra high energy neutrino induced showers in ice and water. Astroparticle Physics, 28(3), 366-379. https://doi.org/10.1016/j.astropartphys.2007.08.001

Vancouver

Bevan S, Danaher S, Perkin J, Ralph S, Rhodes C, Thompson LJ et al. Simulation of ultra high energy neutrino induced showers in ice and water. Astroparticle Physics. 2007 Nov;28(3):366-379. doi: 10.1016/j.astropartphys.2007.08.001

Author

Bevan, S. ; Danaher, S. ; Perkin, J. et al. / Simulation of ultra high energy neutrino induced showers in ice and water. In: Astroparticle Physics. 2007 ; Vol. 28, No. 3. pp. 366-379.

Bibtex

@article{f13f5a373e3b4cbb9ec822d21341d84d,
title = "Simulation of ultra high energy neutrino induced showers in ice and water.",
abstract = "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.",
keywords = "Neutrino, Showers, Water, CORSIKA, Acoustic",
author = "S. Bevan and S. Danaher and J. Perkin and S. Ralph and C. Rhodes and Thompson, {L. J.} and T. Sloan and D. Waters and {The ACoRNE Collaboration}, {et al.}",
year = "2007",
month = nov,
doi = "10.1016/j.astropartphys.2007.08.001",
language = "English",
volume = "28",
pages = "366--379",
journal = "Astroparticle Physics",
issn = "0927-6505",
publisher = "Elsevier",
number = "3",

}

RIS

TY - JOUR

T1 - Simulation of ultra high energy neutrino induced showers in ice and water.

AU - Bevan, S.

AU - Danaher, S.

AU - Perkin, J.

AU - Ralph, S.

AU - Rhodes, C.

AU - Thompson, L. J.

AU - Sloan, T.

AU - Waters, D.

AU - The ACoRNE Collaboration, et al.

PY - 2007/11

Y1 - 2007/11

N2 - 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.

AB - 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.

KW - Neutrino

KW - Showers

KW - Water

KW - CORSIKA

KW - Acoustic

U2 - 10.1016/j.astropartphys.2007.08.001

DO - 10.1016/j.astropartphys.2007.08.001

M3 - Journal article

VL - 28

SP - 366

EP - 379

JO - Astroparticle Physics

JF - Astroparticle Physics

SN - 0927-6505

IS - 3

ER -