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The use of potential energy functions will usually be restricted to
problems involving a single particle or a single rigid body, because
the conservative force must be a function of the CM position only.
However, one can sometimes rework the model description so that the
mathematics is the same as if the above were true, even though it was
not true in the original model. As a very useful example consider the
dumbbell system of two masses interacting through a central force
F(|R|); R is the vector locating mass 1 from mass 2 and F(|R|) depends
only on its magnitude. This could be the model for a variety of
physical systems, from a hydrogen molecule to a binary star system. We
are interested in the time behavior of the vector R, ie.; the motion of
M1 relative to M2, assuming the dumbbell system is isolated from other
forces.
R2 R1
M2<-----------------------CM----------------------------------------------------->M1
------------------------------------------------------------------------------->
R
The difficulty is that if we define M1 as our system, the force on it
depends not only on its location, but also on the location of M2, which
will not stand still for us. However:
From the definition of the CM, M1*R1 + M2*R2 = 0 (Eq #1)
By construction, R = R1 - R2 = R1*(1 + M1/M2) , after using Eq
#1. (Eq #2)
Since the CM is an inertial origin, M1*R1'' = F(|R|) * R / |R| ; ('' =
2nd time derivative) (Eq#3)
Using Eq#2, m*R'' = F(|R|) * R / |R| , where m = (M1*M2)/(M1+M2), the
"reduced" mass. (Eq #4)
Eq (4) describes the behavior of the vector R, which locates M1 from
(the moving) M2, and says that its behavior is the same as that of a
particle of mass m under the influence of the central force F(|R|) of a
FIXED source. Obviously, the MET can use a potential energy function to
describe the behavior of R in Eq #4.