Classical MechanicsBSc · Notes

1. What a conserved quantity tells us

An equation of motion predicts acceleration from the present state. A conserved quantity supplies a different kind of information: a combination of positions and velocities keeps the same value along the entire motion. It can reduce the order of a calculation and reveal a symmetry that was hidden in the original force components.

In Cartesian coordinates we already recognize linear momentum and angular momentum. Generalized coordinates place them in one scheme. The momentum belonging to a coordinate is determined by how the Lagrangian depends on that coordinate's velocity.

2. Generalized momentum and cyclic coordinates

Definition. The momentum conjugate to qiq_i is

pi=∂L∂q˙i.\boxed{p_i=\frac{\partial L}{\partial\dot q_i}.}(9.1)

Its dimensions are energy times time divided by the dimensions of qiq_i. For a Cartesian distance, this is linear momentum. For an angle, it is angular momentum. For more general coordinates, pip_i need not equal a particle mass times q˙i\dot q_i.

A coordinate is cyclic, or ignorable, when LL has no explicit dependence on that coordinate: ∂L/∂qi=0\partial L/\partial q_i=0. Its velocity may still occur. Lagrange's equation reads

p˙i=∂L∂qi+Qi.\dot p_i=\frac{\partial L}{\partial q_i}+Q_i.(9.2)

Therefore, for a cyclic coordinate with Qi=0Q_i=0,

p˙i=0,pi=constant.\boxed{\dot p_i=0,\qquad p_i=\text{constant}.}(9.3)

This is the complete proof. Its assumptions are indispensable: cyclicity of LL alone does not imply conservation in a driven or damped system. A cyclic coordinate is not necessarily constant either. A free particle's position changes even while its momentum stays fixed.

3. Translation and rotation

Suppose translating an entire isolated system by the same small distance ϵ\epsilon along xx leaves its Lagrangian unchanged. Then δxa=ϵ\delta x_a=\epsilon, δx˙a=0\delta\dot x_a=0. To first order,

δL=ϵ∑a∂L∂xa=0.\delta L=\epsilon\sum_a\frac{\partial L}{\partial x_a}=0.(9.4)

For unforced Euler–Lagrange motion, ∂L/∂xa=d(∂L/∂x˙a)/dt\partial L/\partial x_a=d(\partial L/\partial\dot x_a)/dt. Thus

ddt∑apax=0.\frac{d}{dt}\sum_a p_{ax}=0.(9.5)

For the ordinary Cartesian kinetic energy and a velocity-independent potential, pax=max˙ap_{ax}=m_a\dot x_a, so the conserved quantity is total linear momentum in the xx direction. Translation symmetry in all three directions gives conservation of the full total momentum vector. Individual particle momenta may still change through internal forces.

For planar rotations about a fixed origin, a small rotation ϵ\epsilon gives δxa=−yaϵ\delta x_a=-y_a\epsilon, δya=xaϵ\delta y_a=x_a\epsilon, and the same relations for velocities. Rotational invariance implies

0=δLϵ=∑a[−ya∂L∂xa+xa∂L∂ya−y˙apax+x˙apay].0=\frac{\delta L}{\epsilon}=\sum_a\left[-y_a\frac{\partial L}{\partial x_a}+x_a\frac{\partial L}{\partial y_a}-\dot y_a p_{ax}+\dot x_a p_{ay}\right].(9.6)

Replace the coordinate derivatives by p˙ax,p˙ay\dot p_{ax},\dot p_{ay}:

0=∑a(−yap˙ax+xap˙ay−y˙apax+x˙apay)=ddt∑a(xapay−yapax).0=\sum_a(-y_a\dot p_{ax}+x_a\dot p_{ay}-\dot y_a p_{ax}+\dot x_a p_{ay}) =\frac{d}{dt}\sum_a(x_ap_{ay}-y_ap_{ax}).(9.7)

The bracket is the zz component of total angular momentum. In a central potential it is usually shorter to choose the polar angle itself as a coordinate: its absence from LL makes the same conservation law immediate. The Cartesian proof shows why that conserved conjugate momentum is angular momentum.

These are specific symmetry proofs. The general Noether theorem extends the idea to much broader transformations; its full machinery is not needed here.

4. Time independence and the energy function

Time is the evolution parameter, not an extra generalized coordinate in these equations. To obtain the relevant conserved quantity, define the Lagrangian energy function

E=∑iq˙ipi−L.\mathcal E=\sum_i\dot q_i p_i-L.(9.8)

Differentiate the product and expand the total derivative of LL:

dEdt=∑i(q¨ipi+q˙ip˙i)−∑i(∂L∂qiq˙i+∂L∂q˙iq¨i)−∂L∂t.\frac{d\mathcal E}{dt}=\sum_i(\ddot q_i p_i+\dot q_i\dot p_i) -\sum_i\left(\frac{\partial L}{\partial q_i}\dot q_i+\frac{\partial L}{\partial\dot q_i}\ddot q_i\right)-\frac{\partial L}{\partial t}.(9.9)

Since pi=∂L/∂q˙ip_i=\partial L/\partial\dot q_i, the acceleration terms cancel in pairs. The remaining terms are

dEdt=∑iq˙i(p˙i−∂L∂qi)−∂L∂t.\frac{d\mathcal E}{dt}=\sum_i\dot q_i\left(\dot p_i-\frac{\partial L}{\partial q_i}\right)-\frac{\partial L}{\partial t}.(9.10)

Use Lagrange's equation to obtain the energy balance:

dEdt=∑iQiq˙i−∂L∂t.\boxed{\frac{d\mathcal E}{dt}=\sum_iQ_i\dot q_i-\frac{\partial L}{\partial t}.}(9.11)

If Qi=0Q_i=0 and ∂L/∂t=0\partial L/\partial t=0, then E\mathcal E is constant. This proof does not assume that E=T+V\mathcal E=T+V. That further identification requires a velocity-independent potential and kinetic energy homogeneous of degree two in generalized velocities, as happens for time-independent coordinate transformations. The next chapter proves that condition carefully.

The partial derivative ∂L/∂t\partial L/\partial t means time dependence with q,q˙q,\dot q held fixed. An autonomous pendulum has ∂L/∂t=0\partial L/\partial t=0 even though L(θ(t),θ˙(t))L(\theta(t),\dot\theta(t)) usually changes during its motion.

5. Applications

Example 1 · Horizontal momentum during a fall

For L=m(x˙2+y˙2)/2−mgyL=m(\dot x^2+\dot y^2)/2-mgy, xx is cyclic and Qx=0Q_x=0. Therefore px=mx˙p_x=m\dot x is conserved. The vertical coordinate is not cyclic: p˙y=∂L/∂y=−mg\dot p_y=\partial L/\partial y=-mg.

The autonomous energy function is E=m(x˙2+y˙2)/2+mgy\mathcal E=m(\dot x^2+\dot y^2)/2+mgy. Its constancy allows loss of height to become kinetic energy. Horizontal translation is a symmetry; vertical translation changes this chosen gravitational potential by a constant, a case where a broader boundary-term symmetry argument is possible. The direct force equation nevertheless shows that vertical momentum is not conserved.

Example 2 · A particle in a radial potential

Choose plane polar coordinates. The energies are T=m(r˙2+r2θ˙2)/2T=m(\dot r^2+r^2\dot\theta^2)/2, V=V(r)V=V(r), and L=T−VL=T-V. Since θ\theta is absent,

pθ=mr2θ˙=ℓ.p_\theta=mr^2\dot\theta=\ell.(9.12)

The constant ℓ\ell is the perpendicular angular momentum. At r=2 mr=2\,\mathrm m, a particle of mass 0.5 kg0.5\,\mathrm{kg} with θ˙=3 s−1\dot\theta=3\,\mathrm{s^{-1}} has ℓ=6 kg m2 s−1\ell=6\,\mathrm{kg\,m^2\,s^{-1}}. At r=3 mr=3\,\mathrm m, the same orbit has θ˙=ℓ/(mr2)=4/3 s−1\dot\theta=\ell/(mr^2)=4/3\,\mathrm{s^{-1}}.

Angular speed decreases as r−2r^{-2}, whereas tangential speed rθ˙r\dot\theta decreases as r−1r^{-1}. Confusing the two produces an incorrect area law.

Example 3 · Internal forces and total momentum

Two particles on a line interact through V=k(x2−x1−a)2/2V=k(x_2-x_1-a)^2/2. Choose center position X=(m1x1+m2x2)/(m1+m2)X=(m_1x_1+m_2x_2)/(m_1+m_2) and separation s=x2−x1s=x_2-x_1. Put M=m1+m2M=m_1+m_2 and μ=m1m2/M\mu=m_1m_2/M. Then

x1=X−m2Ms,x2=X+m1Ms.x_1=X-\frac{m_2}{M}s,\qquad x_2=X+\frac{m_1}{M}s.(9.13)

Expanding the two squared velocities, the cross coefficient is −m1m2/M+m2m1/M=0-m_1m_2/M+m_2m_1/M=0. The kinetic energy becomes T=MX˙2/2+μs˙2/2T=M\dot X^2/2+\mu\dot s^2/2, while V=k(s−a)2/2V=k(s-a)^2/2. Thus LL is independent of XX, and PX=MX˙=m1x˙1+m2x˙2P_X=M\dot X=m_1\dot x_1+m_2\dot x_2 is constant.

The separation equation is μs¨+k(s−a)=0\mu\ddot s+k(s-a)=0. The particles exchange momentum through the spring while their center of mass moves uniformly. This same center/relative decomposition will return in the two-body central-force problem.

Example 4 · A cyclic coordinate with drag

A free particle on a horizontal line has L=mx˙2/2L=m\dot x^2/2. Although xx is cyclic, a drag force Qx=−cx˙Q_x=-c\dot x gives p˙=−cp/m\dot p=-cp/m. Separate variables: dp/p=−(c/m)dtdp/p=-(c/m)dt, so

p(t)=p0e−ct/m,x(t)=x0+p0c(1−e−ct/m).p(t)=p_0e^{-ct/m},\qquad x(t)=x_0+\frac{p_0}{c}(1-e^{-ct/m}).(9.14)

The energy function is p2/(2m)p^2/(2m) and decreases at rate −cx˙2-c\dot x^2. Neither cyclicity nor absence of explicit time in LL overrides the right-hand-side force. As c→0c\to0, expand 1−e−ct/m≃ct/m1-e^{-ct/m}\simeq ct/m to recover x=x0+p0t/mx=x_0+p_0t/m.

6. Conservation arguments in written solutions

A complete cyclic-coordinate argument identifies the missing coordinate, calculates its conjugate momentum, states that the corresponding remaining force vanishes, and then sets its time derivative to zero. For energy, write the energy function before identifying it with mechanical energy. For translation or rotation, identify which transformation leaves the physical system unchanged; a fixed external support or field can remove a symmetry even when the particles' mutual interaction has it.

The useful conclusion is structural: conservation laws follow from the dependence of the equations on position, orientation, and time. They are not separate assumptions to add after solving a problem.

Exercises

Hints and solutions are collected separately.

  1. 9.1 Can a cyclic coordinate change with time?

  2. 9.2 Prove the cyclic-momentum result including its force qualification.

  3. 9.3 Derive the energy balance for E=∑iq˙ipi−L\mathcal E=\sum_i\dot q_ip_i-L.

  4. 9.4 For L=m(x˙2+y˙2)/2−V(y)L=m(\dot x^2+\dot y^2)/2-V(y), identify a conserved momentum.

  5. 9.5 A central orbit changes radius from rr to 2r2r. By what factors do θ˙\dot\theta and tangential speed change?

  6. 9.6 For L=12mx˙2−12k(t)x2L=\tfrac12m\dot x^2-\tfrac12k(t)x^2, find E˙\dot{\mathcal E}.

  7. 9.7 Prove conservation of total xx momentum from simultaneous translation invariance.

  8. 9.8 What angular momentum is conserved for the spherical pendulum?

  9. 9.9 Two particles interacting only through V(x2−x1)V(x_2-x_1) have masses m,2mm,2m and velocities 4v,−v4v,-v. Find their center velocity.

  10. 9.10 Explain why dL/dt=0dL/dt=0 and ∂L/∂t=0\partial L/\partial t=0 are different statements.

  11. 9.11 If a potential is unchanged by rotation about zz, derive the conserved Cartesian quantity.

  12. 9.12 Does conservation of energy imply conservation of every momentum?

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