Acoustic And Radio EEV Neurtrino Detection Activities by Rolf Nahnhauer, Sebastian Boser

By Rolf Nahnhauer, Sebastian Boser

The sector Workshop in Zeuthen was once the 1st to mix widely the fields of acoustic and radio detection suggestions for high-energetic particle cascades from cosmic neutrino interactions. The articles during this quantity include the most recent study paintings which was once provided through over 50 audio system from 10 international locations. The broad assurance contains: theoretical predictions on fluxes and the prospects of recent ideas, theoretical and experimental effects heading in the right direction fabric homes, the basics of interactions and cascade simulation, and present experimental effects and the newest neutrino flux limits. The e-book additionally considers destiny plans and experiments for either radio and acoustic tools with the purpose of giving the reader an updated review of this swiftly constructing box.

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Teor. Fiz. 41, 616 (1961) [Sov. Phys. A. Askar'yan, Sov. Phys. JETP 48, 988 (1965) [21, 658 (1965)]. 4. D. Saltzberg, P. Gorham, D. , Phys. Rev. Lett. 86, 2802 (2001). 5. M. Fujii and J. Nishimura, Proc. 11th Int. Conf. 709 (1969); H. , Nature 435, 313 (2005). 6. J. L. Stanley, "Handbook of World Salt Resources", Plenum Press, New York (1969); T. H. Michel, "Salt Domes", Gulf Publishing Company, Houston (1979). 7. M. Chiba, T. Kamijo, M. Kawaki, H. Athar, M. Inuzuka, M. Ikeda, O. Yasuda, Proc.

3>v{E„,e)dEl/. (1) This probability is the product of the Earth shadow factor Pghadow t n a t c o n ~ siders neutrino absorption of the Earth and of the probability dPVl^x/dr that the neutrino induces a cascade at a certain detection range. The shadow factor depends on the absorption length of the neutrinos in the Earth and in the atmosphere. At energies above the EeV range, the Earth filters most of the neutrino signal and thus, the rates will be calculated assuming a 2 IT detection field above the horizon.

Lett. 49 (1982) 234. 51. B. Eberle et al, Phys. Rev. D 70 (2004) 023007. INVESTIGATION OF E V E N T RATES FOR D I F F E R E N T D E T E C T O R A R R A Y S A N D VARIOUS EXTREMELY HIGH E N E R G Y MODELS J. K. B E C K E R A N D W . de New detection methods for extremely high energy (EHE) neutrinos are being discussed. In this paper, the comparison of different detection methods at energies E > 10 7 ' 5 GeV are examined, using various neutrino flux predictions. Arrays for acoustic and radio signals from neutrino induced electromagnetic cascades as well as the IceCube array with additional strings ("IceCube Plus") are investigated with effective volumes as given in 5 , e .

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