ConceptComplete

Noether's Theorem and Conservation Laws

Noether's theorem establishes a profound correspondence between continuous symmetries of the action and conserved quantities in physics. It explains why energy, momentum, and angular momentum are conserved, and provides a systematic method for discovering conservation laws in any variational theory.


Symmetries of the Action

Definition7.7Continuous Symmetry of a Lagrangian

A one-parameter family of transformations qiQi(q,q˙,t;ε)q_i \mapsto Q_i(q,\dot{q},t;\varepsilon), tτ(q,q˙,t;ε)t \mapsto \tau(q,\dot{q},t;\varepsilon) (with ε=0\varepsilon = 0 being the identity) is a symmetry of the Lagrangian system if the action S=LdtS = \int L\,dt is invariant: t1t2L(q,q˙,t)dt=τ1τ2L(Q,Q˙,τ)dτ\int_{t_1}^{t_2}L(q,\dot{q},t)\,dt = \int_{\tau_1}^{\tau_2}L(Q,\dot{Q},\tau)\,d\tau for all paths and time intervals. Infinitesimally, write Qi=qi+εξi(q,t)+O(ε2)Q_i = q_i + \varepsilon\xi_i(q,t) + O(\varepsilon^2) and τ=t+εζ(q,t)+O(ε2)\tau = t + \varepsilon\zeta(q,t) + O(\varepsilon^2) where ξi\xi_i and ζ\zeta are the generators of the symmetry.

ExampleFundamental Symmetries

Time translation: tt+εt \mapsto t + \varepsilon, qiqiq_i \mapsto q_i (i.e., ζ=1\zeta = 1, ξi=0\xi_i = 0). The action is invariant when L/t=0\partial L/\partial t = 0. Spatial translation: qiqi+εδijq_i \mapsto q_i + \varepsilon\delta_{ij} for a specific jj (ζ=0\zeta = 0, ξi=δij\xi_i = \delta_{ij}). Invariance requires L/qj=0\partial L/\partial q_j = 0. Rotation: for r=(x,y,z)\mathbf{r} = (x,y,z), rotation about zz gives ξx=y\xi_x = -y, ξy=x\xi_y = x, ξz=0\xi_z = 0. Invariance holds for rotationally symmetric potentials.


Noether's Theorem

Definition7.8Noether's Conserved Current

Noether's theorem (1918): If the action is invariant under a continuous one-parameter symmetry with generators (ξi,ζ)(\xi_i,\zeta), then the quantity I=iLq˙iξi+(LiLq˙iq˙i)ζI = \sum_i \frac{\partial L}{\partial\dot{q}_i}\xi_i + \left(L - \sum_i\frac{\partial L}{\partial\dot{q}_i}\dot{q}_i\right)\zeta is conserved along solutions of the Euler-Lagrange equations: dI/dt=0dI/dt = 0. The term in parentheses is H-H (the negative Hamiltonian). Each independent symmetry yields an independent conserved quantity.

ExampleConservation Laws from Noether's Theorem

Time translation (ξi=0\xi_i = 0, ζ=1\zeta = 1): I=HI = -H, so dH/dt=0dH/dt = 0 (energy conservation). Spatial translation (ξi=δij\xi_i = \delta_{ij}, ζ=0\zeta = 0): I=pj=L/q˙jI = p_j = \partial L/\partial\dot{q}_j (linear momentum conservation). Rotation about zz (ξx=y\xi_x = -y, ξy=x\xi_y = x): I=ypx+xpy=LzI = -yp_x + xp_y = L_z (angular momentum conservation). Galilean boost (ξi=tδij\xi_i = t\delta_{ij}): I=tpjmqjI = tp_j - mq_j (center of mass moves uniformly). Each conservation law corresponds to a geometric symmetry of spacetime.


Field Theory Generalization

Definition7.9Noether's Theorem for Fields

For a field theory with action S[ϕ]=L(ϕ,μϕ,xμ)d4xS[\phi] = \int\mathcal{L}(\phi,\partial_\mu\phi,x^\mu)\,d^4x, a symmetry ϕϕ+εδϕ\phi \mapsto \phi + \varepsilon\delta\phi, xμxμ+εδxμx^\mu \mapsto x^\mu + \varepsilon\delta x^\mu yields the Noether current: jμ=L(μϕ)δϕ+[LδνμL(μϕ)νϕ]δxνj^\mu = \frac{\partial\mathcal{L}}{\partial(\partial_\mu\phi)}\delta\phi + \left[\mathcal{L}\delta^\mu_\nu - \frac{\partial\mathcal{L}}{\partial(\partial_\mu\phi)}\partial_\nu\phi\right]\delta x^\nu. The conservation law is μjμ=0\partial_\mu j^\mu = 0, and the conserved charge is Q=j0d3xQ = \int j^0\,d^3x with dQ/dt=0dQ/dt = 0.

RemarkThe Energy-Momentum Tensor

Spacetime translation invariance δxμ=εμ\delta x^\mu = \varepsilon^\mu of the field Lagrangian yields four conserved currents assembled into the canonical energy-momentum tensor: Tμν=L(μϕ)νϕημνLT^{\mu\nu} = \frac{\partial\mathcal{L}}{\partial(\partial_\mu\phi)}\partial^\nu\phi - \eta^{\mu\nu}\mathcal{L}. The conserved charges are the total energy E=T00d3xE = \int T^{00}\,d^3x and momentum Pi=T0id3xP^i = \int T^{0i}\,d^3x. For the electromagnetic field L=14FμνFμν\mathcal{L} = -\frac{1}{4}F_{\mu\nu}F^{\mu\nu}, symmetrization yields the familiar Maxwell stress-energy tensor Tμν=FμαFνα+14ημνFαβFαβT^{\mu\nu} = F^{\mu\alpha}F^\nu{}_\alpha + \frac{1}{4}\eta^{\mu\nu}F_{\alpha\beta}F^{\alpha\beta}.

RemarkNoether's Second Theorem and Gauge Symmetries

Noether's second theorem addresses infinite-dimensional symmetry groups (gauge symmetries): if the action is invariant under transformations depending on arbitrary functions (not just parameters), the resulting identities are not conservation laws but rather constraints among the equations of motion (generalized Bianchi identities). In electrodynamics, gauge invariance AμAμ+μΛA_\mu \to A_\mu + \partial_\mu\Lambda yields μFμν=Jν\partial_\mu F^{\mu\nu} = J^\nu with the constraint νJν=0\partial_\nu J^\nu = 0 (charge conservation as a consequence of gauge symmetry). In general relativity, diffeomorphism invariance yields the contracted Bianchi identity μGμν=0\nabla_\mu G^{\mu\nu} = 0.