(a) L = T - U = ½m(x·12 + x·12) - ½kx²
(b) x1 = X + ½x + ½l x2 = X - ½x - ½l
Differentiate, substitute into L: L = mX·2 + ¼mx·2 - ½kx²
Hence: X equation: 2mX¨ = 0
x equation: ½mx¨ = - kx
(c) X(t) = X0 + V0t -- uniform motion (of Center of Mass)
x(t) = A cos (2k/m)½(t-t0) -- simple harmonic motion relative to each other
2. (Problem 7.16)
Since ω = v/R the K.E is T = ½mv² + ½Iω² = ½(m + I/R²)x·2, and the PE is U = -mgx sinα. From L = T - U we then get (m+I/R²)x¨ = mg sinα , or x¨ = (mg sinα)/(m+I/R²).
3. (Problem 7.18)
We'll consider the case when the "pendulum part" of the cylinder hangs down from a fixed point (ring). Let x be the length of that part, and θ its angle from the vertical. The angular velocity of the cylinder is ω = x·/R, and the square of the mass is the usual polar coordinate expression (from 1.44). The PE depends only on the height of m, U = -mgx cosθ. Therefore
|
|
|
4. (Problem 7.21)
See back of book for L. EOM works out to be r¨ – ω² r = 0. The given initial conditions imply A = B = r0/2. so for large r, r ® ½r0 ewt.
The conserved quantity (Hamiltonian) is ½mr·2 - ½mω²r²
5. (Problem 7.38)
(a) In spherical polar coordinates, the angle q is fixed at q = a, so the KE is just T = 1/2m(r·2 +r2 sin2 a f·2). Since the PE is U = mgz = mgrcosa,
|
| (1) |
|