E Classical Mechanics 1273
Taking the time derivatives of Eqs. (E-28) and (E-29), we can write the Lagran-
gian as
L
1
2
m 1
(
.
xc−
m 2
.
x
M
) 2
+
1
2
m 2
(
.
xc+
m 1
.
x
M
) 2
−V(x)
1
2
m 1
⎡
⎣
.
xc
2
− 2 m 2
.
xc
.
x
M
+
(
m 2
.
x
M
) 2 ⎤
⎦+^1
2
m 2
⎡
⎣
.
x
2
c+^2 m^1
.
xc
.
x
M
+
(
m 1
.
x
M
) 2 ⎤
⎦−V(x)
(E-30)
The terms containing
.
xc
.
xcancel, so that
L
1
2
(m 1 +m 2 )
.
x
2
c+
1
2
m 1 m 2 (m 1 +m 2 )
M^2
.
x
2
−V(x)
1
2
M
.
x^2 c+
1
2
μ
.
x^2 −V(x) (E-31)
Thereduced massof the pair of particles is denoted byμand is defined by
μ
m 1 m 2
m 1 +m 2
m 1 m 2
M
(E-32)
The kinetic energy is
K
1
2
M
.
x
2
c+
1
2
μ
.
x
2
(E-33)
Since the variables are separated in the Lagrangian, we obtain separate equations of
motion forxcandx:
M
d
.
xc
dt
∂L
∂xc
0 (E-34)
μ
d
.
x
dt
∂L
∂x
−
dV
dx
(E-35)
If there are no external forces, the center of mass of the two particles moves like a
particle of massMthat has no forces acting on it, while the relative coordinate changes
like the motion of a particle of massμmoving at a distancexfrom a fixed origin
and subject to the potential energyV(x). The motion of two particles moving in the
xdirection has been separated into two one-body problems. The motion in theyand
zdirections is completely analogous, so that in three dimensions we can assert:The
fictitious particle of massμmoves around the origin of its coordinate in the same way
that particle 1 moves relative to particle 2, while the center of mass moves like a free
particle of massM.
The separation is the same in Hamiltonian mechanics. In three dimensions, the
kinetic energy is
K
1
2
M(
.
x
2
c+
.
y
2
c+
.
z
2
c)+
1
2
μ(
.
x
2
+
.
y
2
+
.
z
2
) (E-36)