Harvey Gould, and
The classical-physics model of helium is a simple example of a three body problem and is similar to gravitational problem of a heavy sun and two light planets. It consists of two electrons moving in a 2/r potential well and interacting through a 1/r potential. Initial conditions can be set to show phenomena such as autoionization or braided orbits. These conditions are stored in an xml document.
Please note that this resource requires
at least version 1.5 of
Christian, W., Gould, H., & Tobochnik, J. (2008). Classical Helium Program [Computer software]. Retrieved September 3, 2014, from http://www.compadre.org/Repository/document/ServeFile.cfm?ID=7209&DocID=375
%0 Computer Program %A Christian, Wolfgang %A Gould, Harvey %A Tobochnik, Jan %D August 8, 2008 %T Classical Helium Program %8 August 8, 2008 %U http://www.compadre.org/Repository/document/ServeFile.cfm?ID=7209&DocID=375
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