Equations of Motion
Consider a dynamical system consisting of particles. Let particle have mass ,
displacement , and velocity
. Suppose that particle is subject to a force
exerted by particle .
Suppose, in addition, that particle is subject to an external force (i.e., a force that originates outside the dynamical
system) . Applying Newton's second law of motion to the particle [see Equation (1.19)], we obtain
|
(1.63) |
assuming that all of the forces acting on particle are superposable. (This is reasonable because
gravitational and electromagnetic forces are superposable.)
Newton's third law of motion, (1.21), can
be generalized to give
|
(1.64) |
for all and . Note, in particular, that
. In other words, particle cannot
exert a force on itself. This accounts for the exclusion of particle
in the sum on the right-hand side of Equation (1.63).
There are equations of motion of analogous form to
Equation (1.63); one for each particle that makes up the system. We can sum all of
these equations to give
|
(1.65) |
Now, every term,
, appearing in the double sum on the right-hand side of the previous
equation, can be paired with another term—
, in this case—that is equal and opposite
according to Newton's third law of motion, (1.64). In other words, the terms in the sum all
cancel out in pairs. It follows that the previous equation reduces to
|
(1.66) |
where
|
(1.67) |
is the net external force acting on the system.