Encounters
September 2002
The position and velocity of each nucleus is measured by averaging the positions and velocities of a selected subset of particles. Ideally this subset would contain only those particles most tightly bound to the nucleus, but it's expensive to redefine this subset at each time step. However, there's relatively little diffusion in binding energy, so it's possible to sort the particles in each realization by initial binding energy, and use those particles most tightly bound initially to determine fairly accurate nuclear coordinates.
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Fig. 1 gives an overview of the encounters. All three were launched on the same initial orbit. A pair of point masses started on this orbit would have a single parabolic passage with separation rp = 0.25 at time tp = 40 and then recede to infinity. In practice the first passages of these extended systems are slightly later and somewhat wider than the point-mass trajectory would imply; once they begin to interpenetrate, the acceleration of each nucleus falls below that of a corresponding point mass. There's also some variation among the first passages of these three encounters; for example, the γ1 = 1, γ2 = 2 passage is distinctly closer than the others. This variation is presumably due to fluctuations which transfer momentum within each participant.
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| γ1 = γ2 = 1 | γ1 = 1, γ2 = 2 | γ1 = γ2 = 2 |
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| γ1 = γ2 = 1 | γ1 = 1, γ2 = 2 | γ1 = γ2 = 2 |
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Last modified: September 3, 2002
http://www.ifa.hawaii.edu/~barnes/research/cusp_mergers/encounters.html