# Two-Body Coulomb Collisions

Consider a two-body Coulomb collision between a species- particle, with mass and charge , and a species- particle, with mass and charge . The equations of motion of the two particles take the form

 (3.38) (3.39)

where

 (3.40)

and denotes a time derivative. Here, and are the respective position vectors, and is the relative position vector. It is easily demonstrated that

 (3.41) (3.42)

where

 (3.43)

is the vector position of the center of mass (which does not accelerate). Equations (3.38) and (3.39) can be combined to give a single equation of relative motion,

 (3.44)

Two relations that immediately follow from the previous equation are

 (3.45) (3.46)

where

 (3.47)

is the conserved angular momentum per unit mass, and

 (3.48)

the conserved energy.

Equation (3.47) implies that . This is the equation of a plane that passes through the origin, and whose normal is parallel to the constant vector . We, therefore, conclude that the relative position vector is constrained to lie in this plane, which implies that the trajectories of both colliding particles are coplanar. Let the plane coincide with the - plane, so that we can write . It is convenient to define the standard plane polar coordinates and . When expressed in terms of these coordinates, the conserved angular momentum per unit mass becomes

 (3.49)

where

 (3.50)

Furthermore, the conserved energy takes the form

 (3.51)

Suppose that , where and . It follows that

 (3.52)

Hence, Equation (3.51) transforms to give

 (3.53)

It is convenient to define the relative velocity at large distances,

 (3.54)

as well as the impact parameter,

 (3.55)

The latter parameter is simply the distance of closest approach of the two particles in the situation in which there is no Coulomb force acting between them, and they, consequently, move in straight-lines. (See Figure 3.1.) The previous three equations can be combined to give

 (3.56)

Figure 3.1 shows the collision in a frame of reference in which the species- particle remains stationary at the origin, , whereas the species- particle traces out the path . Point corresponds to the closest approach of the two particles. It follows, by symmetry (because Coulomb collisions are reversible), that the angles and shown in the figure are equal to one another. Hence, we deduce that

 (3.57)

Here, is the angle through which the path of the species- (or the species- particle) is deviated as a consequence of the collision, whereas is the angle through which the relative position vector, , rotates as the species- particle moves from point (which is assumed to be infinity far from point ) to point . Suppose that point corresponds to . It follows that

 (3.58)

Here, , where is the distance of closest approach. Now, by symmetry, , so Equation (3.56) implies that

 (3.59)

Combining Equations (3.56) and (3.58), we obtain

 (3.60)

where , and

 (3.61)

Integration (Speigel, Liu, and Lipschutz 1999) yields

 (3.62)

Hence, from Equation (3.57), we get

 (3.63)

which can be rearranged to give

 (3.64)

Note that the analysis in this section tacitly assumes that Coulomb collisions are not significantly modified by any magnetic field that might pervade the plasma. This assumption is justified provided that the particle gyroradii are all much larger than the Debye length.