corner
corner

Phys. Rev. A 70, 042902 (2004) [7 pages]

Contribution of close collisions to the Barkas effect: The classical picture

Download: PDF (84 kB) Buy this article Export: BibTeX or EndNote (RIS)

N. R. Arista1, P. L. Grande2, and A. F. Lifschitz3
1División Colisiones Atómicas, Centro Atómico Bariloche and Instituto Balseiro, Comisión Nacional de Energía Atómica, 8400 S. C. de Bariloche, Argentina
2Instituto de Física da Universidade Federal do Rio Grande do Sul, Avenida Bento Goncalves 9500, 91501-970, Porto Alegre, RS, Brazil
3Laboratoire de Physique des Gaz et des Plasmas, Université Paris Sud, F-91405 Orsay Cedex, France

Received 17 May 2004; published 22 October 2004

According to a previous estimation made by Lindhard [ Nucl. Instrum. Method Phys. Res. 132 1 (1976)] on the basis of qualitative arguments and dimensional analysis, the contribution of close collisions to the Barkas effect in the energy loss of swift ions in solids yields a significant fraction of the total effect, being almost equal to the contribution coming from distant collisions. Here the classical estimation by Lindhard is reconsidered and subjected to a tight numerical test. We analyze in quantitative terms the classical description of the Barkas effect following the line of arguments proposed by Lindhard. We consider a swift ion of charge Z1 interacting with the electrons via a screened potential assuming spherical and nonspherical screening models. We calculate by numerical integration the differential and total transport cross sections and find an important asymmetry of both with respect to the sign of Z1, as well as a departure from the Z12 behavior. These effects are particularly important for impact parameters in the range of the classical collision radius (rcl=Z1e2mv2). This approach clearly shows the contribution of close collisions to the Barkas effect. We analyze the behavior of the Barkas asymmetry with respect to ion charge and velocity, obtaining a good quantitative agreement with Lindhard’s prediction. However, an additional term predicted for nonspherical potentials cannot be reproduced.

© 2004 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevA.70.042902
DOI:
10.1103/PhysRevA.70.042902
PACS:
34.50.Bw, 34.50.Fa