Thinned simulations of extremely energetic showers in dense media for radio applications

被引:25
作者
Alvarez-Muniz, J. [1 ,2 ]
James, C. W. [3 ]
Protheroe, R. J. [3 ]
Zas, E. [1 ,2 ]
机构
[1] Univ Santiago de Compostela, Depto Fis Particulas, Santiago De Compostela 15782, Spain
[2] Univ Santiago de Compostela, Inst Galego Fis Altas Enerxias, Santiago De Compostela 15782, Spain
[3] Univ Adelaide, Dept Phys, Sch Chem & Phys, Adelaide, SA 5005, Australia
基金
澳大利亚研究理事会;
关键词
High-energy cosmic rays and neutrinos; High-energy showers; Cherenkov radio emission; HIGH-ENERGIES; NEUTRINO DETECTION; CONDENSED MEDIA; PAIR PRODUCTION; COSMIC-RAYS; EMISSION; BREMSSTRAHLUNG; CASCADES; PULSES; CHARGE;
D O I
10.1016/j.astropartphys.2009.06.005
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This paper presents our results for full 3-D simulations of very-high to ultra-high energy electromagnetic cascades - and the associated coherent Cherenkov radiation - as might be produced by high-energy neutrino interactions in dense media. Using "thinning" techniques, we develop an algorithm based on the existing "ZHS" code, and demonstrate that the new "ZHS-thinned" code can produce fast and accurate results for showers up to 10(20) eV. Using ZHS-thinned, we develop new parameterisations for the radiation from showers in ice, salt, and the lunar regolith, with a separate treatment of the megaregolith (deep regolith). Our parameterisations include for the first time a method to simulate fluctuations in shower length induced by the LPM effect. Our results, which avoid the pit-falls of scaling Simulations from lower energies, allow improved Calculations of the detection probability for experiments searching for high-energy neutrinos using the radio technique. (C) 2009 Elsevier B.V. All rights reserved.
引用
收藏
页码:100 / 111
页数:12
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