Monte Carlo simulations of photohadronic processes in astrophysics

被引:330
|
作者
Mücke, A
Engel, R
Rachen, JP
Protheroe, RJ
Stanev, T
机构
[1] Univ Adelaide, Dept Phys & Math Phys, Adelaide, SA 5005, Australia
[2] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA
[3] Penn State Univ, Dept Astron, University Pk, PA 16802 USA
[4] Univ Utrecht, Sterrekundig Inst, NL-3584 CC Utrecht, Netherlands
基金
美国国家航空航天局; 澳大利亚研究理事会;
关键词
photon-hadron interactions; resonance production; resonance decay; photoproduction cross section; Monte Carlo event generator; multiparticle production;
D O I
10.1016/S0010-4655(99)00446-4
中图分类号
TP39 [计算机的应用];
学科分类号
081203 ; 0835 ;
摘要
A new Monte Carlo program for photohadronic interactions of relativistic nucleons with an ambient photon radiation field is presented. The event generator is designed to fulfill typical astrophysical requirements, but can also be used for radiation and background studies at high energy colliders such as LEP2 and HERA, as well as for simulations of photon induced air showers. We consider the full photopion production cross section from the pion production threshold up to high energies. it includes resonance excitation and decay, direct single pion production and diffractive and non-diffractive multiparticle production. The cross section of each individual process is calculated by fitting experimental data, while the kinematics is determined by the underlying particle production process. We demonstrate that our model is capable of reproducing known accelerator data over a wide energy range. (C) 2000 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:290 / 314
页数:25
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