Theoretical Physics II – Exam Essentials

Inclined Plane (Lagrange 1st Kind) - Constraint (plane moves right with s(t)=12at2s(t)=\tfrac{1}{2}at^2):

ϕ(x,y,t)=ytanα[xs(t)]=0\phi(x,y,t)=y-\tan\alpha\,[x-s(t)]=0

  • Cartesian Lagrangian with multiplier λ\lambda:

    L=12m(x˙2+y˙2)mgy+λϕL=\tfrac{1}{2}m(\dot x^2+\dot y^2)-mg y+\lambda\,\phi

    → Equations

    mx¨=λtanα,my¨=mg+λm\ddot x = -\lambda\tan\alpha,\quad m\ddot y = -mg+\lambda

    ϕ=0\phi=0 - Eliminate λ\lambda → single equation along the slope (coordinate qq):

    q¨=sinαgacosα\ddot q = -\sin\alpha\,g- a\cos\alpha

    (down-slope positive). - Solution (with constants fixed by initial data):

    q(t)=q<em>0+q˙</em>0t12(gsinα+acosα)t2q(t)=q<em>0+\dot q</em>0 t-\tfrac{1}{2}(g\sin\alpha + a\cos\alpha)t^2

  • Constraint force magnitude:

    Fc=λ=m(gcosαasinα)\Vert\mathbf F_c\Vert=\Vert\lambda\Vert=m\,(g\cos\alpha-a\sin\alpha)

Atwood Machine (Lagrange 2nd Kind) - Masses m<em>1,m</em>2m<em>1,m</em>2; massless pulley, rope length L=l+πRL=l+\pi R.

  • One degree of freedom: choose downward displacement of m<em>1m<em>1q=l</em>1q=l</em>1 (then l2=LπRql_2=L-\pi R-q).

  • Kinetic & potential

    T=12(m<em>1+m</em>2)q˙2,V=m<em>1gqm</em>2g(LπRq)T=\tfrac{1}{2}(m<em>1+m</em>2)\dot q^2 ,\qquad V = m<em>1 g q - m</em>2 g (L-\pi R-q)

    L=TVL=T-V

  • Lagrange eq.:

    ddt[(m<em>1+m</em>2)q˙]=(m<em>1m</em>2)g\frac{d}{dt}\big[(m<em>1+m</em>2)\dot q\big]=-(m<em>1-m</em>2)g

    q¨=m<em>2m</em>1m<em>1+m</em>2g\ddot q=\frac{m<em>2-m</em>1}{m<em>1+m</em>2}g

  • General solution:

    q(t)=q<em>0+q˙</em>0t+12q¨t2q(t)=q<em>0+\dot q</em>0 t+\tfrac{1}{2}\ddot q\,t^2

Free Fall & Action Integral - Trial paths z<em>1=at,  z</em>2=bt2,  z3=ct3z<em>1=at,\;z</em>2=bt^2,\;z_3=ct^3 with

z(0)=0,  z(T)=g2T2z(0)=0,\;z(T)=-\tfrac{g}{2}T^2 give

  • Action (one-dim.

    L=12mz˙2mgzL=\tfrac{1}{2}m\dot z^2-mg z):

    S<em>1=38mg2T3,    S</em>2=13mg2T3,    S3=516mg2T3S<em>1=\tfrac{3}{8}m g^2 T^3,\;\; S</em>2=\tfrac{1}{3}m g^2 T^3,\;\; S_3=\tfrac{5}{16}m g^2 T^3

  • Minimum action ⇒ parabolic path z<em>2(bt2)z<em>2(bt^2) is physical; z</em>1,z3z</em>1,z_3 ruled out by Hamilton’s principle.

Rotating Water Surface (Variational Method) - Potentials per mass element dmdm (in co-rotating frame):

dU=(12ω2ρ2+gz)dmdU=\big( -\tfrac{1}{2}\omega^2\rho^2 + g z \big) dm

  • Total potential functional (axial symmetry):

    U[f]=<em>02π!dφ</em>0R!dρρ0f(ρ)!dzμ(12ω2ρ2+gz)U[f]=\int<em>0^{2\pi}!d\varphi\int</em>0^R!d\rho\,\rho\int_0^{f(\rho)}!dz\,\mu\Big(-\tfrac{1}{2}\omega^2\rho^2+g z\Big)

  • Volume functional (constraint):

    V[f]=<em>02π!dφ</em>0R!dρρf(ρ)=const=VμV[f]=\int<em>0^{2\pi}!d\varphi\int</em>0^R!d\rho\,\rho\,f(\rho)=\text{const}=\tfrac{V}{\mu}

  • Minimise U[f]+λV[f]U[f]+\lambda V[f] → Euler-Lagrange:

    gf(ρ)ω2ρ+λ=0g f'(\rho)-\omega^2\rho + \lambda =0

    f(ρ)=ω22gρ2+Cf(\rho)=\tfrac{\omega^2}{2g}\rho^2 + C (paraboloid; constant fixed by volume).

Planar Pendulum (Hamilton Formalism)

  • One degree of freedom: angle θ\theta; conjugate momentum p=ml2θ˙p = m l^2 \dot\theta.

  • Hamiltonian:

    H(θ,p)=p22ml2+mgl(1cosθ)H(\theta,p)=\tfrac{p^2}{2 m l^2}+m g l (1-\cos\theta)

  • Hamilton equations:

    θ˙=Hp=pml2,p˙=Hθ=mglsinθ\dot\theta = \frac{\partial H}{\partial p}=\frac{p}{m l^2},\quad \dot p = -\frac{\partial H}{\partial \theta}= -m g l \sin\theta

  • Combine → nonlinear pendulum equation:

    θ¨+glsinθ=0\ddot\theta+\frac{g}{l}\sin\theta=0