Classical Mechanics
11/12/2007
Stanford
class with Leonard Susskind.
Velocity:
Kinetic energy:
Potential energy:
Potential energy is at a minimum when .
The Lagrangian is:
Angular momentum is:
The Euler-Lagrange equations are
is constant, so the equations of motion are
The Hamiltonian is the total energy.
Specifically, for the pendulum,
Substituting
The double pendulum has two “bob’s”, in this case “Bob” and “Herman”.
Kinetic energy of Bob:
Velocity of Herman:
Add the velocity of Herman with respect to Bob to get the velocity of Herman.
Kinetic energy of Herman:
Sum of the kinetic energies of Bob and Herman is:
The sum of the potential energies of Bob and Herman is:
The Lagrangian becomes:
No conserved quantity under the force of gravity.
However, investigate case (no gravity):
Noether symmetry
then
Total angular momentum should be conserved.
Calculate the equation of motion for .
Approximate:
Substitute into the Lagrangian for simple harmonic motion, and drop the constant term.
Use the variable “x”. Consider a spring.
x=0 at equilibrium.
The potential energy is the work done against the spring from equilibrium.
“k” is the spring constant.
The force exerted by the spring is (Hooke’s Law):
The Lagrangian for simple harmonic motion is:
The Euler-Lagrange equations are (F=ma)
Let
then
Substitute:
The Sine is also a solution. In general, the solution to this second order equation is:
A specific solution requires the initial position and velocity.
Another way of putting the solution
where at .
is conserved.
Instead of use . Solve for in terms of .
Hamiltonian mechanics is symmetric between x and p.
is conserved.
Therefore, the shape of the trajectory in phase space is that of an ellipse. is the square of the semi-major and minor axis.
when
What is the period of the orbit? It is the frequency . All the elliptical orbits are repeated with frequency .
Phase space is fundamental. An orbit in phase space is a contour of constant energy. Area in phase space is preserved in time. In quantum mechanics this is “unitarity” or conservation of probability.