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Hamiltonian Mechanics

4.1 Generalised Momentum

The generalised momentum conjugate to qjq_j is

pj=Lq˙jp_j = \frac{\partial L}{\partial \dot{q}_j}

4.2 The Hamiltonian

The Hamiltonian is defined by the Legendre transform:

H(q1,,qn,p1,,pn,t)=j=1npjq˙jLH(q_1, \ldots, q_n, p_1, \ldots, p_n, t) = \sum_{j=1}^n p_j \dot{q}_j - L

When the transformation is regular (i.e., the Hessian 2L/q˙jq˙k\partial^2 L / \partial \dot{q}_j \partial \dot{q}_k Is non-singular), this is well-defined.

If LL does not depend explicitly on time and VV is velocity-independent, then H=T+VH = T + V (total Energy).

4.3 Worked Example: Legendre Transform for the Harmonic Oscillator

Problem. A one-dimensional harmonic oscillator has L=12mx˙212kx2L = \frac{1}{2}m\dot{x}^2 - \frac{1}{2}kx^2. Find the Hamiltonian.

Solution

The conjugate momentum:

p=Lx˙=mx˙    x˙=pmp = \frac{\partial L}{\partial \dot{x}} = m\dot{x} \implies \dot{x} = \frac{p}{m}

The Hamiltonian:

H=px˙L=ppm12mp2m2+12kx2=p22m+12kx2H = p\dot{x} - L = p\frac{p}{m} - \frac{1}{2}m\frac{p^2}{m^2} + \frac{1}{2}kx^2 = \frac{p^2}{2m} + \frac{1}{2}kx^2

This is T+VT + V as expected for a natural system. Hamilton”s equations give:

x˙=Hp=pm,p˙=Hx=kx\dot{x} = \frac{\partial H}{\partial p} = \frac{p}{m}, \quad \dot{p} = -\frac{\partial H}{\partial x} = -kx

Combining: x¨=p˙/m=kx/m\ddot{x} = \dot{p}/m = -kx/mI.e., x¨+(k/m)x=0\ddot{x} + (k/m)x = 0. \blacksquare

4.4 Worked Example: Legendre Transform for the Simple Pendulum

Problem. Find the Hamiltonian for a simple pendulum of mass mm and length ll.

Solution

From Section 3.4, L=12ml2θ˙2+mglcosθL = \frac{1}{2}ml^2\dot{\theta}^2 + mgl\cos\theta.

Conjugate momentum:

pθ=Lθ˙=ml2θ˙    θ˙=pθml2p_\theta = \frac{\partial L}{\partial \dot{\theta}} = ml^2\dot{\theta} \implies \dot{\theta} = \frac{p_\theta}{ml^2}

Hamiltonian:

H=pθθ˙L=pθ2ml2pθ22ml2mglcosθ=pθ22ml2mglcosθH = p_\theta\dot{\theta} - L = \frac{p_\theta^2}{ml^2} - \frac{p_\theta^2}{2ml^2} - mgl\cos\theta = \frac{p_\theta^2}{2ml^2} - mgl\cos\theta

Hamilton’s equations:

θ˙=Hpθ=pθml2,p˙θ=Hθ=mglsinθ\dot{\theta} = \frac{\partial H}{\partial p_\theta} = \frac{p_\theta}{ml^2}, \quad \dot{p}_\theta = -\frac{\partial H}{\partial \theta} = -mgl\sin\theta

\blacksquare

4.5 Hamilton’s Equations

Theorem 4.1 (Hamilton’s Equations). The equations of motion in Hamiltonian form are

q˙j=Hpj,p˙j=Hqj\dot{q}_j = \frac{\partial H}{\partial p_j}, \quad \dot{p}_j = -\frac{\partial H}{\partial q_j}

These are 2n2n first-order ODEs (compared to nn second-order ODEs in the Lagrangian formulation).

Proof. From H=pjq˙jLH = \sum p_j \dot{q}_j - L:

dH=q˙jdpj+pjdq˙jLqjdqjLq˙jdq˙jLtdtdH = \sum \dot{q}_j\, dp_j + \sum p_j\, d\dot{q}_j - \sum \frac{\partial L}{\partial q_j}\, dq_j - \sum \frac{\partial L}{\partial \dot{q}_j}\, d\dot{q}_j - \frac{\partial L}{\partial t}\, dt

Since pj=L/q˙jp_j = \partial L / \partial \dot{q}_jThe dq˙jd\dot{q}_j terms cancel:

dH=q˙jdpjp˙jdqjLtdtdH = \sum \dot{q}_j\, dp_j - \sum \dot{p}_j\, dq_j - \frac{\partial L}{\partial t}\, dt

Comparing with dH=Hpjdpj+Hqjdqj+HtdtdH = \sum \frac{\partial H}{\partial p_j} dp_j + \sum \frac{\partial H}{\partial q_j} dq_j + \frac{\partial H}{\partial t} dt:

q˙j=Hpj,p˙j=Hqj,Ht=Lt\dot{q}_j = \frac{\partial H}{\partial p_j}, \quad \dot{p}_j = -\frac{\partial H}{\partial q_j}, \quad \frac{\partial H}{\partial t} = -\frac{\partial L}{\partial t}

\blacksquare

4.6 Phase Space

Hamiltonian mechanics lives in phase space: the 2n2n-dimensional space with coordinates (q1,,qn,p1,,pn)(q_1, \ldots, q_n, p_1, \ldots, p_n). Each point in phase space represents a complete state of the System (positions and momenta).

A phase portrait is the collection of trajectories in phase space. For a 1D harmonic oscillator, the trajectories are ellipses in the (x,p)(x, p) plane.

4.7 Liouville’s Theorem

Theorem 4.2 (Liouville’s Theorem). The flow in phase space is incompressible: the phase space volume is conserved along trajectories. Equivalently, the phase space density ρ(q,p,t)\rho(q, p, t) satisfies:

dρdt=ρt+j(ρqjq˙j+ρpjp˙j)=0\frac{d\rho}{dt} = \frac{\partial \rho}{\partial t} + \sum_j \left(\frac{\partial \rho}{\partial q_j}\dot{q}_j + \frac{\partial \rho}{\partial p_j}\dot{p}_j\right) = 0

Proof. Consider a volume Ω\Omega in phase space. The rate of change of the volume is:

ddtΩρdqdp=Ωρtdqdp\frac{d}{dt}\int_\Omega \rho\, dq\, dp = \int_\Omega \frac{\partial \rho}{\partial t}\, dq\, dp

By the continuity equation in 2n2n dimensions:

ρt+(ρv)=0\frac{\partial \rho}{\partial t} + \nabla \cdot (\rho \mathbf{v}) = 0

Where v=(q˙1,,q˙n,p˙1,,p˙n)\mathbf{v} = (\dot{q}_1, \ldots, \dot{q}_n, \dot{p}_1, \ldots, \dot{p}_n) is the phase space velocity. Using Hamilton’s equations:

v=jq˙jqj+jp˙jpj=j2Hqjpjj2Hpjqj=0\nabla \cdot \mathbf{v} = \sum_j \frac{\partial \dot{q}_j}{\partial q_j} + \sum_j \frac{\partial \dot{p}_j}{\partial p_j} = \sum_j \frac{\partial^2 H}{\partial q_j \partial p_j} - \sum_j \frac{\partial^2 H}{\partial p_j \partial q_j} = 0

By equality of mixed partial derivatives. Therefore:

ρt+ρ(v)+vρ=ρt+vρ=dρdt=0\frac{\partial \rho}{\partial t} + \rho\,(\nabla \cdot \mathbf{v}) + \mathbf{v} \cdot \nabla\rho = \frac{\partial \rho}{\partial t} + \mathbf{v} \cdot \nabla\rho = \frac{d\rho}{dt} = 0

\blacksquare

Intuition. Liouville’s theorem is the classical analogue of unitarity in quantum mechanics. It tells us that phase space volume is conserved --- like an incompressible fluid flowing through phase space. This underlies the ergodic hypothesis of statistical mechanics.

4.8 Poisson Brackets

Definition. The Poisson bracket of two functions f(q,p,t)f(q, p, t) and g(q,p,t)g(q, p, t) is:

{f,g}=j=1n(fqjgpjfpjgqj)\{f, g\} = \sum_{j=1}^n \left(\frac{\partial f}{\partial q_j}\frac{\partial g}{\partial p_j} - \frac{\partial f}{\partial p_j}\frac{\partial g}{\partial q_j}\right)

Theorem 4.3 (Equations of Motion via Poisson Brackets). For any function f(q,p,t)f(q, p, t):

dfdt=ft+{f,H}\frac{df}{dt} = \frac{\partial f}{\partial t} + \{f, H\}

In particular, Hamilton’s equations become:

q˙j={qj,H},p˙j={pj,H}\dot{q}_j = \{q_j, H\}, \quad \dot{p}_j = \{p_j, H\}

Proof. Using the chain rule:

dfdt=ft+j(fqjq˙j+fpjp˙j)\frac{df}{dt} = \frac{\partial f}{\partial t} + \sum_j \left(\frac{\partial f}{\partial q_j}\dot{q}_j + \frac{\partial f}{\partial p_j}\dot{p}_j\right)

Substituting Hamilton’s equations:

dfdt=ft+j(fqjHpjfpjHqj)=ft+{f,H}\frac{df}{dt} = \frac{\partial f}{\partial t} + \sum_j \left(\frac{\partial f}{\partial q_j}\frac{\partial H}{\partial p_j} - \frac{\partial f}{\partial p_j}\frac{\partial H}{\partial q_j}\right) = \frac{\partial f}{\partial t} + \{f, H\}

\blacksquare

Properties of Poisson Brackets.

Theorem 4.4. The Poisson bracket satisfies:

  1. Antisymmetry: {f,g}={g,f}\{f, g\} = -\{g, f\}
  2. Linearity: {af+bg,h}=a{f,h}+b{g,h}\{af + bg, h\} = a\{f, h\} + b\{g, h\} for constants a,ba, b
  3. Leibniz rule: {fg,h}=f{g,h}+{f,h}g\{fg, h\} = f\{g, h\} + \{f, h\}g
  4. Jacobi identity: {f,{g,h}}+{g,{h,f}}+{h,{f,g}}=0\{f, \{g, h\}\} + \{g, \{h, f\}\} + \{h, \{f, g\}\} = 0

Proof. Properties (1)—(3) follow directly from the definition. For the Jacobi identity, write out the terms explicitly:

{f,{g,h}}=jfqjpjk(gqkhpkgpkhqk)jfpjqjk(gqkhpkgpkhqk)\{f, \{g, h\}\} = \sum_j \frac{\partial f}{\partial q_j}\frac{\partial}{\partial p_j}\sum_k \left(\frac{\partial g}{\partial q_k}\frac{\partial h}{\partial p_k} - \frac{\partial g}{\partial p_k}\frac{\partial h}{\partial q_k}\right) - \sum_j \frac{\partial f}{\partial p_j}\frac{\partial}{\partial q_j}\sum_k \left(\frac{\partial g}{\partial q_k}\frac{\partial h}{\partial p_k} - \frac{\partial g}{\partial p_k}\frac{\partial h}{\partial q_k}\right)

Expanding and collecting terms, the second-order mixed partial derivatives cancel in groups of three (by equality of mixed partials), yielding the Jacobi identity. \blacksquare

Theorem 4.5. A quantity ff is a constant of motion if and only if f/t+{f,H}=0\partial f/\partial t + \{f, H\} = 0. If ff does not depend explicitly on time, ff is conserved if and only if {f,H}=0\{f, H\} = 0.

Proof. Immediate from Theorem 4.3 with df/dt=0df/dt = 0. \blacksquare

Fundamental Poisson Brackets:

{qj,qk}=0,{pj,pk}=0,{qj,pk}=δjk\{q_j, q_k\} = 0, \quad \{p_j, p_k\} = 0, \quad \{q_j, p_k\} = \delta_{jk}

4.9 The Hamilton-Jacobi Equation

Definition. Hamilton’s principal function S(q,t)S(q, t) is the action evaluated along the classical path from (q0,t0)(q_0, t_0) to (q,t)(q, t).

Theorem 4.6 (Hamilton-Jacobi Equation). The function SS satisfies:

H(q1,,qn,Sq1,,Sqn,t)+St=0H\left(q_1, \ldots, q_n, \frac{\partial S}{\partial q_1}, \ldots, \frac{\partial S}{\partial q_n}, t\right) + \frac{\partial S}{\partial t} = 0

This is a first-order nonlinear PDE in n+1n + 1 variables.

Proof. The action from t0t_0 to tt is S=t0tLdtS = \int_{t_0}^{t} L\, dt'. The total time derivative is:

dSdt=L\frac{dS}{dt} = L

But S=S(q1(t),,qn(t),t)S = S(q_1(t), \ldots, q_n(t), t)So by the chain rule:

dSdt=jSqjq˙j+St=L\frac{dS}{dt} = \sum_j \frac{\partial S}{\partial q_j}\dot{q}_j + \frac{\partial S}{\partial t} = L

From the definition of the conjugate momentum, pj=L/q˙j=S/qjp_j = \partial L/\partial \dot{q}_j = \partial S/\partial q_j (this can be shown rigorously by varying the endpoint). Therefore:

L=jpjq˙j+St=H+StL = \sum_j p_j \dot{q}_j + \frac{\partial S}{\partial t} = H + \frac{\partial S}{\partial t}

Since dS/dt=LdS/dt = L:

H+St=L=jpjq˙j+StH + \frac{\partial S}{\partial t} = L = \sum_j p_j\dot{q}_j + \frac{\partial S}{\partial t}

Which gives H+S/t=0H + \partial S/\partial t = 0. \blacksquare

Intuition. The Hamilton-Jacobi equation is the bridge between classical and quantum mechanics. Schrodinger’s equation can be obtained from it via the substitution S=ilnψS = -i\hbar \ln\psi (up to constants), making SS the classical limit of the quantum phase.

Separation of Variables. If HH does not depend explicitly on ttWrite S(q,t)=W(q)EtS(q, t) = W(q) - Et. Then the time-independent Hamilton-Jacobi equation is:

H(q1,,qn,Wq1,,Wqn)=EH\left(q_1, \ldots, q_n, \frac{\partial W}{\partial q_1}, \ldots, \frac{\partial W}{\partial q_n}\right) = E

Where WW is Hamilton’s characteristic function and EE is the constant energy.

4.10 Worked Example: Hamilton-Jacobi for the Harmonic Oscillator

Problem. Solve the Hamilton-Jacobi equation for a 1D harmonic oscillator with H=p2/(2m)+kx2/2H = p^2/(2m) + kx^2/2.

Solution

Since HH is time-independent, write S(x,t)=W(x)EtS(x, t) = W(x) - Et. The HJ equation becomes:

12m(dWdx)2+12kx2=E\frac{1}{2m}\left(\frac{dW}{dx}\right)^2 + \frac{1}{2}kx^2 = E

dWdx=2mEmkx2\frac{dW}{dx} = \sqrt{2mE - mkx^2}

Integrating:

W(x)=2mEmkx2dxW(x) = \int \sqrt{2mE - mkx^2}\, dx

Let x=2E/ksinαx = \sqrt{2E/k}\sin\alphaThen dx=2E/kcosαdαdx = \sqrt{2E/k}\cos\alpha\, d\alpha:

W=2Eω0αcos2αdα=Eω(α+12sin2α)W = \frac{2E}{\omega}\int_0^\alpha \cos^2\alpha'\, d\alpha' = \frac{E}{\omega}\left(\alpha + \frac{1}{2}\sin 2\alpha\right)

Where ω=k/m\omega = \sqrt{k/m}. The solution gives x(t)=2E/ksin(ωt+δ)x(t) = \sqrt{2E/k}\sin(\omega t + \delta) as expected.

\blacksquare

:::caution Common Pitfall The Lagrangian and Hamiltonian formulations are equivalent only when the Legendre transform from LL To HH is regular. If det(2L/q˙iq˙j)=0\det(\partial^2 L / \partial \dot{q}_i \partial \dot{q}_j) = 0The system Has constraints and the Hamiltonian formulation requires special treatment (Dirac brackets or Constraint analysis).

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