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Ion Implantation and Synthesis of Materials - Studium

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3.5 Motion under a Central Force 31coordinate system. Since potential-energy involves only the radial distance, theproblem has spherical symmetry, indicating any rotation about a fixed axis canhave no effect on the solution; i.e., if either particle is located at the origin, theforce on the other is given by a central force, F(r), which only depends on theseparation distance, r.In the problem examined in this section, we will assume that, in the laboratorysystem, one <strong>of</strong> the particles is practically at rest at the origin, O, while the otherone moves with velocity v – a good approximation when the stationary particle ismuch heavier than the moving particle.3.5.1 Energy Conservation in a Central ForceFor conservative central forces <strong>and</strong> a defined interaction potential, V(r), we canwrite a statement for the total mechanical energy for a particle <strong>of</strong> mass M, adistance r away from a central force F asM 2 2E = ⎡ +θ⎤+( ),2 ⎣vrv ⎦ V r(3.20)where v r <strong>and</strong> v θ are the radial <strong>and</strong> transverse velocities, respectively. The first termon the right-h<strong>and</strong> side <strong>of</strong> (3.20) represents the kinetic energy in polar coordinates.In addition to the total energy equation given above, we also have the condition<strong>of</strong> conservation <strong>of</strong> angular momentum,l=Mrvθ(3.21)The quantities E <strong>and</strong> l are the constants <strong>of</strong> motion, while V(r) is the potentialenergyfor a particle <strong>of</strong> mass M in a central field. We rewrite (3.20) in the form2 2Mv= ( ) = r lE E r + + V( r).22 2Mr(3.22)All terms in (3.22) are a function <strong>of</strong> r only. The first term is the kinetic energyfor the radial component; the term l2 /2Mr 2 is referred to as the centrifugal energy;<strong>and</strong> V(r) is the interatomic potential-energy. The centrifugal energy is the portion<strong>of</strong> the kinetic energy term that is due to the particle’s motion transverse to thedirection <strong>of</strong> the radius vector. It is because the centrifugal energy can be describedas a function <strong>of</strong> radial position r alone that we can treat the radial motion <strong>of</strong> aparticle as a one-dimensional problem in r. Equation (3.22) is now simply afunction <strong>of</strong> r only.

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