Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
6933534 | Journal of Computational Physics | 2013 | 36 Pages |
Abstract
A newly developed code, implemented as a part of the MBN Explorer package (Solovʼyov et al., 2012; http://www.mbnexplorer.com/, 2012) [1], [2] to simulate trajectories of an ultra-relativistic projectile in a crystalline medium, is presented. The motion of a projectile is treated classically by integrating the relativistic equations of motion with account for the interaction between the projectile and crystal atoms. The probabilistic element is introduced by a random choice of transverse coordinates and velocities of the projectile at the crystal entrance as well as by accounting for the random positions of the atoms due to thermal vibrations. The simulated trajectories are used for numerical analysis of the emitted radiation. Initial approbation and verification of the code have been carried out by simulating the trajectories and calculating the radiation emitted by ε=6.7 GeV and ε=855 MeV electrons and positrons in oriented Si(110) crystal and in amorphous silicon.The calculated spectra are compared with the experimental data and with predictions of the Bethe-Heitler theory for the amorphous environment.
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Physical Sciences and Engineering
Computer Science
Computer Science Applications
Authors
Gennady B. Sushko, Victor G. Bezchastnov, Ilia A. Solovʼyov, Andrei V. Korol, Walter Greiner, Andrey V. Solovʼyov,