Chapter 13 - Hamiltonian Mechanics
Section 13.1 - The Basic Variables
Definition. Consider a Laplacian defined as \(\mathcal{L} = \mathcal{L}(q_1, \ldots, q_n, \dot{q}_1, \ldots, \dot{q}_n, t)\). Then, the set of coordinates \(q_1, \ldots, q_n\) are the configuration space while the set of coordinates \(q_1, \ldots, q_n, \dot{q}_1, \ldots, \dot{q}_n\) are known as the state space.
Recall that the generalized momenta \(p_i\) is also defined such that
Definition. The generalized momenta is also called the canonical momentum or the momentum conjugate to \(q_i\).
Definition. The Hamiltonian is defined as
Section 13.2 - Hamilton's Equations for One-Dimensional Systems
We see that for a pendulum, \(\mathcal{L} = \frac{1}{2} m L^2 \dot{\phi}^2 - mgL(1 - \cos \phi)\). For a bead sliding on a frictionless wire of height \(y = f(x)\), we see \(\mathcal{L} = \frac{1}{2}m[1 + f'(x)^2] - mgf(x)\).
Notably, using natural coordinates, \(\mathcal{L} = \frac{1}{2}A(q)\dot{q}^2 - U(q)\). Then, we can define \(\mathcal{H} = p\dot{q} - \mathcal{L}\).
We know that \(p = \frac{\partial \mathcal{L}}{\partial \dot{q}} = A(q)\dot{q}\). Then, \(\mathcal{H} = p\dot{q} - \mathcal{L} = A(q)\dot{q}^2 - \frac{1}{2} A(q) \dot{q}^2 + U(q) = 2T - T + U = T + U\)
Similarly, we can solve for \(\dot{q}\) from the definition of the generalized momentum to see that \(\dot{q} = \frac{q}{A(q)}\).
Deriving Hamilton's Equations is thus simple. We see that \(\frac{\partial \mathcal{H}}{\partial q} = p \frac{\partial \dot{q}}{\partial q} - [\frac{\partial \mathcal{L}}{\partial q} + \frac{\mathcal{L}}{\partial \dot{q}} \frac{\partial \dot{q}}{\partial q}] = p \frac{\partial \dot{q}}{\partial q} - [\frac{\partial \mathcal{L}}{\partial q} + q\frac{\partial \dot{q}}{\partial q}] = -\frac{\partial \mathcal{L}}{\partial q} = -\dot{p}\)
Differentiating instead with respect to \(p\), we see that \(\frac{\partial \mathcal{H}}{\partial p} = [\dot{q} + p \frac{\partial \dot{q}}{\partial p}] - \frac{\partial \mathcal{L}}{\partial \dot{q}} \frac{\partial \dot{q}}{\partial p} = [\dot{q} + p \frac{\partial \dot{q}}{\partial p}] - p \frac{\partial \dot{q}}{\partial p} = \dot{q}\)
Section 13.3 - Hamilton's Equations in Several Dimensions
We know that
Here, the generalized momenta are defined as
This tells us that \(\dot{\mathbf{q}} = \dot{\mathbf{q}}(\mathbf{q}, \mathbf{p}, t)\). Then, we can define the Hamiltonian as
We can differentiate with respect to \(p_i\) to see that
We can differentiate with respect to \(q_i\) to see that
For a system with \(n\) coordinates, this gives us \(2n\) first-order differential equations rather than \(n\) second-order differential equations as seen in the Lagrange equations.
We then can calculate
We can then substitute Hamilton's equations to see that
From section 7.8, we know that if the relation from the generalized coordinates to rectangular coordinates is independent of \(t\) (that is, our generalized coordinates are natural), than \(\mathcal{H} = T + U\).
Section 13.4 - Ignorable Coordinates
Definition. If \(\mathcal{H}\) is independent of a coordinate \(q_i\), it immediately follows that \(\dot{p}_i = 0\) and thus \(p_i\) is a constant. Note that this definition immediately follows from the Lagrangian definition.
Section 13.5 - Lagrange's Equations vs. Hamilton's Equations
Skipped.
Section 13.6 - Phase-Space Orbits
Skipped.
Section 13.7 - Liouville's Theorem
Skipped.