Interleaved — Phase 2

Physics interleaved practice

printable — key stays hidden on paper

Instructions. Work each problem independently. The problems deliberately jump between subtopics — before solving, identify which framework applies (Lagrangian, Hamiltonian, Poisson-bracket, rigid-body, etc.). Show all steps. Use gg for gravitational acceleration. Marks in [ ]. Total: 72 marks.


1. [6] A bead of mass mm slides on a rigid wire bent into the shape y=ax2y = ax^2 in a vertical plane. State how many degrees of freedom the system has, classify the constraint (holonomic/non-holonomic, scleronomic/rheonomic), choose a suitable generalized coordinate, and write the kinetic energy TT in that coordinate.

2. [7] For a particle in a central potential V(r)V(r) in a plane, using polar coordinates (r,θ)(r,\theta): (a) Write the Lagrangian. (b) Identify any cyclic coordinate and state the corresponding conserved quantity. (c) Write the generalized momenta prp_r and pθp_\theta.

3. [8] Two equal masses mm are connected by three identical springs (constant kk) in a line between two fixed walls: wall–spring–mm–spring–mm–spring–wall. Find the normal mode frequencies and describe the normal coordinates.

4. [6] A disk of mass MM, radius RR rolls without slipping down an incline of angle α\alpha. Using a Lagrange multiplier for the rolling constraint, find the equation of motion and the constraint (friction) force.

5. [6] Given the Hamiltonian H=p22m+12mω2q2H = \frac{p^2}{2m} + \frac{1}{2}m\omega^2 q^2, write Hamilton's equations and sketch (describe) the phase-space trajectories. What is conserved and what is the shape of the trajectories?

6. [6] Compute the Poisson brackets (a) {q,p}\{q, p\}, (b) {Lx,Ly}\{L_x, L_y\} where Li=ϵijkxjpkL_i = \epsilon_{ijk} x_j p_k, and (c) state the connection between the Poisson bracket and the quantum commutator.

7. [7] A symmetric top (moments I1=I2I3I_1 = I_2 \ne I_3) undergoes torque-free rotation. Starting from Euler's equations, show that ω3\omega_3 is constant and that the transverse angular velocity precesses at a fixed rate. Give that rate.

8. [7] For a Lagrangian LL invariant under time translation, use Noether's theorem (or the total time derivative of LL) to show that the energy function h=iq˙iLq˙iLh = \sum_i \dot q_i \frac{\partial L}{\partial \dot q_i} - L is conserved. State the symmetry ↔ conservation law correspondence.

9. [6] The inertia tensor of a body in some frame is I=(400031013)  (units of MR2).I = \begin{pmatrix} 4 & 0 & 0 \\ 0 & 3 & 1 \\ 0 & 1 & 3 \end{pmatrix} \; (\text{units of } MR^2). Find the principal moments of inertia and the principal axes.

10. [7] Use the Hamilton–Jacobi method for a free particle in one dimension (H=p2/2mH = p^2/2m). Write the H–J equation, separate the time dependence, solve for Hamilton's principal function S(x,t)S(x,t), and recover x(t)x(t).

11. [6] A generating function F1(q,Q)=12mωq2cotQF_1(q,Q) = \tfrac{1}{2}m\omega q^2 \cot Q defines a canonical transformation for the harmonic oscillator. Find pp and PP, and show the new Hamiltonian gives action-angle-like variables.

Answer keyMark scheme & solutions

1. Subtopics 2.1.1, 2.1.2, 2.1.3. Why: cues "wire shape" + "classify constraint" force the constraints/DOF/KE combination.

The bead is confined to the curve y=ax2y=ax^2: this is one equation relating x,yx,y, time-independent → holonomic and scleronomic. In 2D there were 2 coordinates; one constraint leaves 1 DOF. Choose q=xq=x. y=ax2,y˙=2axx˙.y = ax^2,\quad \dot y = 2ax\dot x. T=12m(x˙2+y˙2)=12mx˙2(1+4a2x2).T = \tfrac12 m(\dot x^2 + \dot y^2) = \tfrac12 m\dot x^2\left(1 + 4a^2x^2\right).


2. Subtopics 2.1.4, 2.1.8, 2.1.7. Why: central potential → recognize θ\theta cyclic.

(a) L=12m(r˙2+r2θ˙2)V(r)L = \tfrac12 m(\dot r^2 + r^2\dot\theta^2) - V(r). (b) θ\theta does not appear in LLcyclic. Conserved: pθ=mr2θ˙=p_\theta = mr^2\dot\theta = angular momentum \ell. (c) pr=Lr˙=mr˙p_r = \dfrac{\partial L}{\partial \dot r} = m\dot r, pθ=Lθ˙=mr2θ˙\quad p_\theta = \dfrac{\partial L}{\partial\dot\theta}= mr^2\dot\theta.


3. Subtopic 2.1.20. Why: two coupled masses with symmetric spring chain — classic normal-mode problem.

Displacements x1,x2x_1,x_2. Equations: mx¨1=kx1+k(x2x1)=2kx1+kx2,m\ddot x_1 = -kx_1 + k(x_2-x_1) = -2kx_1 + kx_2, mx¨2=k(x2x1)kx2=kx12kx2.m\ddot x_2 = -k(x_2-x_1) - kx_2 = kx_1 - 2kx_2. Matrix km(2112)\frac{k}{m}\begin{pmatrix}2 & -1\\-1 & 2\end{pmatrix}, eigenvalues ω2=km(21)\omega^2 = \frac{k}{m}(2\mp1).

  • Symmetric mode Q+=x1+x2Q_+ = x_1+x_2: ω1=k/m\omega_1 = \sqrt{k/m} (masses move together).
  • Antisymmetric mode Q=x1x2Q_- = x_1-x_2: ω2=3k/m\omega_2 = \sqrt{3k/m} (masses move oppositely). Normal coordinates Q±=12(x1±x2)Q_\pm = \tfrac{1}{\sqrt2}(x_1\pm x_2) decouple the equations.

4. Subtopic 2.1.10. Why: "find the constraint force" is the trigger for Lagrange multipliers rather than just eliminating the constraint.

Coordinates ss (down-slope distance) and ϕ\phi (rotation), constraint f=sRϕ=0f = s - R\phi = 0. L=12Ms˙2+12Iϕ˙2+MgSsinα,I=12MR2.L = \tfrac12 M\dot s^2 + \tfrac12 I\dot\phi^2 + MgS\sin\alpha,\quad I=\tfrac12 MR^2. E–L with multiplier λ\lambda: Ms¨Mgsinα=λ,Iϕ¨=λR.M\ddot s - Mg\sin\alpha = \lambda,\qquad I\ddot\phi = -\lambda R. Constraint: s¨=Rϕ¨\ddot s = R\ddot\phi. Substitute: Ms¨Mgsinα=λ,12MR2s¨R=λR12Ms¨=λ.M\ddot s - Mg\sin\alpha = \lambda,\quad \tfrac12 MR^2 \frac{\ddot s}{R} = -\lambda R \Rightarrow \tfrac12 M\ddot s = -\lambda. So Ms¨Mgsinα=12Ms¨32Ms¨=MgsinαM\ddot s - Mg\sin\alpha = -\tfrac12 M\ddot s \Rightarrow \tfrac32 M\ddot s = Mg\sin\alpha, s¨=23gsinα,λ=12Ms¨=13Mgsinα.\boxed{\ddot s = \tfrac23 g\sin\alpha},\qquad \lambda = -\tfrac12 M\ddot s = -\tfrac13 Mg\sin\alpha. The friction (constraint) force magnitude is 13Mgsinα\tfrac13 Mg\sin\alpha.


5. Subtopics 2.1.12, 2.1.13. Why: given HH → Hamilton's equations + phase portrait.

q˙=Hp=pm,p˙=Hq=mω2q.\dot q = \frac{\partial H}{\partial p} = \frac{p}{m},\qquad \dot p = -\frac{\partial H}{\partial q} = -m\omega^2 q. H=EH = E is conserved. Trajectories are level sets p22m+12mω2q2=E\frac{p^2}{2m} + \tfrac12 m\omega^2 q^2 = E = ellipses in (q,p)(q,p) space, traversed clockwise. Rescaling p/mp/\sqrt m, qmωq\sqrt m\omega makes them circles.


6. Subtopic 2.1.15. Why: direct PB computation and quantum connection.

(a) {q,p}=qqppqppq=1\{q,p\} = \dfrac{\partial q}{\partial q}\dfrac{\partial p}{\partial p} - \dfrac{\partial q}{\partial p}\dfrac{\partial p}{\partial q} = 1. (b) {Lx,Ly}=Lz\{L_x,L_y\} = L_z (angular-momentum algebra), and cyclically. (c) Correspondence: {A,B}1i[A^,B^]\{A,B\} \longrightarrow \dfrac{1}{i\hbar}[\hat A,\hat B]. Thus {Lx,Ly}=Lz\{L_x,L_y\}=L_z becomes [L^x,L^y]=iL^z[\hat L_x,\hat L_y]=i\hbar\hat L_z.


7. Subtopics 2.1.21, 2.1.23. Why: "torque-free symmetric top, Euler's equations" specifically selects Euler's equations.

Euler's equations, Ni=0N_i=0: I1ω˙1=(I2I3)ω2ω3,    I2ω˙2=(I3I1)ω3ω1,    I3ω˙3=(I1I2)ω1ω2.I_1\dot\omega_1 = (I_2-I_3)\omega_2\omega_3,\;\; I_2\dot\omega_2=(I_3-I_1)\omega_3\omega_1,\;\; I_3\dot\omega_3=(I_1-I_2)\omega_1\omega_2. With I1=I2I_1=I_2: third gives ω˙3=0ω3=\dot\omega_3 = 0 \Rightarrow \omega_3= const. Define Ω=(I3I1)I1ω3\Omega = \dfrac{(I_3-I_1)}{I_1}\omega_3 (constant). First two become ω˙1=Ωω2,ω˙2=+Ωω1.\dot\omega_1 = -\Omega\omega_2,\quad \dot\omega_2 = +\Omega\omega_1. So ω1+iω2=AeiΩt\omega_1+i\omega_2 = A e^{i\Omega t}: the transverse angular velocity precesses at rate Ω=I3I1I1ω3\boxed{\Omega = \frac{I_3-I_1}{I_1}\omega_3} (body-frame precession).


8. Subtopics 2.1.9, 2.1.11. Why: time-translation symmetry → energy conservation (Noether).

dLdt=i(Lqiq˙i+Lq˙iq¨i)+Lt.\frac{dL}{dt} = \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}. Using E–L, Lqi=ddtLq˙i\frac{\partial L}{\partial q_i}=\frac{d}{dt}\frac{\partial L}{\partial\dot q_i}: dLdt=iddt ⁣(q˙iLq˙i)+Lt.\frac{dL}{dt} = \sum_i\frac{d}{dt}\!\left(\dot q_i\frac{\partial L}{\partial\dot q_i}\right)+\frac{\partial L}{\partial t}. Thus ddt(iq˙iLq˙iL)=Lt\frac{d}{dt}\Big(\sum_i \dot q_i\frac{\partial L}{\partial\dot q_i}-L\Big) = -\frac{\partial L}{\partial t}. If LL has no explicit tt (time-translation symmetry), h=q˙ipiLh=\sum\dot q_ip_i-L is conserved — this is the energy. Symmetry (time translation) ↔ energy conservation.


9. Subtopic 2.1.22. Why: given a matrix → diagonalize for principal axes.

The xx-axis is already principal: I=4I=4. Remaining 2×22\times2 block (3113)\begin{pmatrix}3&1\\1&3\end{pmatrix} has eigenvalues 3±1=4,23\pm1 = 4, 2, eigenvectors (0,1,1)/2(0,1,1)/\sqrt2 and (0,1,1)/2(0,1,-1)/\sqrt2. Principal moments: {4,4,2}MR2\{4, 4, 2\}\,MR^2. Principal axes: x^\hat x; (0,1,1)/2(0,1,1)/\sqrt2; (0,1,1)/2(0,1,-1)/\sqrt2.


10. Subtopic 2.1.17. Why: "Hamilton–Jacobi" named explicitly.

H–J equation: St+12m(Sx)2=0.\dfrac{\partial S}{\partial t} + \dfrac{1}{2m}\left(\dfrac{\partial S}{\partial x}\right)^2 = 0. Separate S=W(x)EtS = W(x) - Et: 12m(W)2=EW=2mE=p\frac{1}{2m}(W')^2 = E \Rightarrow W' = \sqrt{2mE}=p, so W=pxW = px. S=pxp22mt.S = px - \frac{p^2}{2m}t. New constant β=Sp=xpmtx=β+pmt\beta = \frac{\partial S}{\partial p} = x - \frac{p}{m}t \Rightarrow x = \beta + \frac{p}{m}t — uniform motion. ✓


11. Subtopics 2.1.16, 2.1.18. Why: given a generating function → canonical transformation, leading to action-angle.

F1(q,Q)=12mωq2cotQF_1(q,Q)=\tfrac12 m\omega q^2\cot Q. p=F1q=mωqcotQ,P=F1Q=mωq22sin2Q.p = \frac{\partial F_1}{\partial q} = m\omega q\cot Q,\qquad P = -\frac{\partial F_1}{\partial Q} = \frac{m\omega q^2}{2\sin^2 Q}. Invert: q=2PmωsinQq = \sqrt{\dfrac{2P}{m\omega}}\sin Q, p=2PmωcosQp=\sqrt{2Pm\omega}\cos Q. Then H=p22m+12mω2q2=ωPH = \frac{p^2}{2m}+\tfrac12 m\omega^2 q^2 = \omega P. Since HH is independent of QQ, QQ is cyclic and P=E/ωP=E/\omega is constant (the action variable); Q˙=ω\dot Q = \omega, $