TheoremComplete

Noether's Theorem

Theorem7.1Noether's Theorem (Lagrangian Mechanics)

Let L(q,qΛ™,t)L(q,\dot{q},t) be a Lagrangian for a system with nn degrees of freedom, and suppose the action S=∫t1t2L dtS = \int_{t_1}^{t_2}L\,dt is invariant under the infinitesimal transformation qi↦qi+Ρξi(q,t)q_i \mapsto q_i + \varepsilon\xi_i(q,t), t↦t+Ρ΢(q,t)t \mapsto t + \varepsilon\zeta(q,t). Then the quantity I=βˆ‘i=1nβˆ‚Lβˆ‚qΛ™iΞΎiβˆ’HΞΆI = \sum_{i=1}^n \frac{\partial L}{\partial\dot{q}_i}\xi_i - H\zeta where H=βˆ‘ipiqΛ™iβˆ’LH = \sum_i p_i\dot{q}_i - L is the Hamiltonian, is a first integral of the motion: dI/dt=0dI/dt = 0 along any solution of the Euler-Lagrange equations.


Proof

Proof

Step 1: Invariance condition. The action invariance S[Q,Ο„]=S[q,t]S[Q,\tau] = S[q,t] to first order in Ξ΅\varepsilon reads: ∫t1t2[βˆ‚Lβˆ‚qiΞΎi+βˆ‚Lβˆ‚qΛ™i(ΞΎΛ™iβˆ’qΛ™iΞΆΛ™)+LΞΆΛ™+βˆ‚Lβˆ‚tΞΆ]dt=0\int_{t_1}^{t_2}\left[\frac{\partial L}{\partial q_i}\xi_i + \frac{\partial L}{\partial\dot{q}_i}\left(\dot{\xi}_i - \dot{q}_i\dot{\zeta}\right) + L\dot{\zeta} + \frac{\partial L}{\partial t}\zeta\right]dt = 0

Here we used Ξ΄qΛ™i=ΞΎΛ™iβˆ’qΛ™iΞΆΛ™\delta\dot{q}_i = \dot{\xi}_i - \dot{q}_i\dot{\zeta} (the variation of velocity under simultaneous coordinate and time reparametrization) and dΟ„=(1+Ρ΢˙) dtd\tau = (1+\varepsilon\dot{\zeta})\,dt.

Step 2: Rewrite using total derivatives. Observe that: ddt[βˆ‚Lβˆ‚qΛ™iΞΎi]=ddtβˆ‚Lβˆ‚qΛ™iβ‹…ΞΎi+βˆ‚Lβˆ‚qΛ™iΞΎΛ™i\frac{d}{dt}\left[\frac{\partial L}{\partial\dot{q}_i}\xi_i\right] = \frac{d}{dt}\frac{\partial L}{\partial\dot{q}_i}\cdot\xi_i + \frac{\partial L}{\partial\dot{q}_i}\dot{\xi}_i and ddt[LΞΆ]=LΛ™ΞΆ+LΞΆΛ™=[βˆ‚Lβˆ‚qiqΛ™i+βˆ‚Lβˆ‚qΛ™iqΒ¨i+βˆ‚Lβˆ‚t]ΞΆ+LΞΆΛ™\frac{d}{dt}[L\zeta] = \dot{L}\zeta + L\dot{\zeta} = \left[\frac{\partial L}{\partial q_i}\dot{q}_i + \frac{\partial L}{\partial\dot{q}_i}\ddot{q}_i + \frac{\partial L}{\partial t}\right]\zeta + L\dot{\zeta}

Step 3: Apply Euler-Lagrange. On solutions, βˆ‚Lβˆ‚qi=ddtβˆ‚Lβˆ‚qΛ™i\frac{\partial L}{\partial q_i} = \frac{d}{dt}\frac{\partial L}{\partial\dot{q}_i}. Using this, collect terms: βˆ‚Lβˆ‚qiΞΎi+βˆ‚Lβˆ‚qΛ™iΞΎΛ™i=ddt[βˆ‚Lβˆ‚qΛ™iΞΎi]\frac{\partial L}{\partial q_i}\xi_i + \frac{\partial L}{\partial\dot{q}_i}\dot{\xi}_i = \frac{d}{dt}\left[\frac{\partial L}{\partial\dot{q}_i}\xi_i\right]

The remaining terms combine as: βˆ’βˆ‚Lβˆ‚qΛ™iqΛ™iΞΆΛ™+LΞΆΛ™+βˆ‚Lβˆ‚tΞΆ=βˆ’(HΞΆΛ™)+βˆ‚Lβˆ‚tΞΆ-\frac{\partial L}{\partial\dot{q}_i}\dot{q}_i\dot{\zeta} + L\dot{\zeta} + \frac{\partial L}{\partial t}\zeta = -(H\dot{\zeta}) + \frac{\partial L}{\partial t}\zeta

where H=piqΛ™iβˆ’LH = p_i\dot{q}_i - L. Adding back LΛ™ΞΆβˆ’LΛ™ΞΆ=0\dot{L}\zeta - \dot{L}\zeta = 0: =βˆ’ddt[HΞΆ]+HΛ™ΞΆ+βˆ‚Lβˆ‚tΞΆ= -\frac{d}{dt}[H\zeta] + \dot{H}\zeta + \frac{\partial L}{\partial t}\zeta

Step 4: Conclude. On solutions, HΛ™=βˆ’βˆ‚L/βˆ‚t\dot{H} = -\partial L/\partial t (standard result from Hamiltonian mechanics). Therefore: ddt[βˆ‘iβˆ‚Lβˆ‚qΛ™iΞΎiβˆ’HΞΆ]=0\frac{d}{dt}\left[\sum_i\frac{\partial L}{\partial\dot{q}_i}\xi_i - H\zeta\right] = 0

This establishes dI/dt=0dI/dt = 0. β–‘\square

β– 

ExampleNoether's Theorem for Electromagnetic Fields

The electromagnetic Lagrangian density L=βˆ’14FΞΌΞ½FΞΌΞ½βˆ’AΞΌJΞΌ\mathcal{L} = -\frac{1}{4}F_{\mu\nu}F^{\mu\nu} - A_\mu J^\mu is invariant under spacetime translations xΞΌβ†’xΞΌ+aΞΌx^\mu \to x^\mu + a^\mu. The field-theoretic Noether current gives βˆ‚ΞΌTΞΌΞ½=0\partial_\mu T^{\mu\nu} = 0 with T00=12(E2+B2)T^{00} = \frac{1}{2}(\mathbf{E}^2 + \mathbf{B}^2) (energy density) and T0i=(EΓ—B)iT^{0i} = (\mathbf{E}\times\mathbf{B})^i (Poynting vector), recovering the conservation of electromagnetic energy and momentum.

RemarkConverse of Noether's Theorem

The converse is also true (under mild regularity conditions): every conserved quantity arises from a variational symmetry. More precisely, if I(q,qΛ™,t)I(q,\dot{q},t) is a first integral, then the flow generated by II via the Poisson bracket ΞΎi={qi,I}\xi_i = \{q_i,I\} is a symmetry of the Lagrangian. This establishes a complete bijection between symmetries and conservation laws in Hamiltonian mechanics.