Coherent Cherenkov radio emission from EeV showers in dense media through thinned simulations

被引：0
|
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, Dept Fis Particulas, Santiago 15782, Spain
[2] Univ Santiago de Compostela, IGFAE, Santiago 15782, Spain
[3] Univ Adelaide, Sch Chem & Phys, Dept Phys, Adelaide, SA 5005, Australia
来源：
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 2009年 / 604卷 / 1-2期
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; PAIR PRODUCTION; BREMSSTRAHLUNG; PULSES;
D O I：
10.1016/j.nima.2009.03.025
中图分类号：
TH7 [仪器、仪表];
学科分类号：
0804 ; 080401 ; 081102 ;
摘要：
We explore the feasibility of applying "thinning techniques" to the simulation of EeV electromagnetic showers in ice, salt, and the regolith of the Moon. By comparing the results of thinned showers to full simulations, we show that thinning techniques keep a good level of accuracy in the relevant shower and radio observables, and allow a considerable reduction in computing time. We apply thinning techniques to the simulation of EeV electromagnetic showers including the Landau-Pomeranchuk-Migdal effect. Our study is of the utmost importance for the determination of the sensitivity to extremely energetic neutrinos of experiments looking for radiopulses in dense media. (C) 2009 Elsevier B.V. All rights reserved.
引用
收藏
页码：S27 / S29
页数：3
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