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The Cartesian equations of motion of our system take
the form
 |
(670) |
for
, where
are each equal to the mass of the
first particle,
are each equal to the mass of the
second particle, etc. Furthermore, the kinetic energy of the
system can be written
 |
(671) |
Now, since
, we can write
 |
(672) |
for
.
Hence, it follows that
. According to the
above equation,
 |
(673) |
where we are treating the
and the
as independent
variables.
Multiplying Eq. (673) by
, and then differentiating
with respect to time, we obtain
 |
(674) |
Now,
 |
(675) |
Furthermore,
 |
(676) |
and
where use has been made of Eq. (675). Thus, it follows
from Eqs. (674), (676), and (677) that
 |
(678) |
Let us take the above equation, multiply by
, and then sum over all
.
We obtain
 |
(679) |
where use has been made of Eqs. (670) and (671). Thus, it follows from Eq. (667) that
 |
(680) |
Finally, making use of Eq. (669), we get
 |
(681) |
It is helpful to introduce a function
, called the Lagrangian, which
is defined as the difference between the kinetic and potential energies of the dynamical system under investigation:
 |
(682) |
Since the potential energy
is clearly independent of the
, it follows from Eq. (681) that
 |
(683) |
for
. This equation is known as Lagrange's equation.
According to the above analysis, if we can express the kinetic and
potential energies of our dynamical system solely in terms of our generalized
coordinates and their time derivatives, then we can immediately write
down the equations of motion of the system, expressed in terms
of the generalized coordinates, using Lagrange's equation, (683).
Unfortunately, this scheme only works for conservative systems.
Let us now consider some examples.
Next: Motion in a Central
Up: Lagrangian Dynamics
Previous: Generalized Forces
Contents
Richard Fitzpatrick
2008-01-13