HW#1 The first four homework problems may be found in my Lambert oscillator notes.
HW#2 [1] Find an integral invariant under the
rms-arithmetic mean
iteration: an , bn → an+1 = (an2/2+bn2/2)1/2
, bn+1 = an/2+bn/2.
[2] Critique the latest "physicist's proof" of the Riemann
hypothesis, as given here.
HW#3 [1] Compute Lyapunov exponents for the logistic map in
the
special case, xn+1 = 4xn(1-xn).
[2] Find limit cycles and bifurcations, numerically, for the
damped, driven Lambert oscillator.
[3]
Show that upon averaging phase space volume shrinks, <dV/dt> <
0, for any driven oscillator with damping.
[4]
Show the Schwarzian derivative of F is negative for various maps on the
unit interval: F = ρx(1-x); F = 1-μ|x|r; F = a
sin(πx). All parameters here are positive, with r > 1.
Also recall the Schwarzian
derivative is
defined as D[F] = F'''/F' - 3 (F''/F')2/2.
HW#4 [1] For a charged particle in a magnetic dipole field,
consider trajectories which are in the equatorial plane containing the
dipole, with the dipole normal to the plane. Numerically compute
and plot examples of "trapped" and "tightly wound" trajectories, as
sketched in lecture.
[2] Again for equatorial plane trajectories of a charged particle
in a magnetic dipole field, express the azimuthal angle φ(x) in terms
of elliptic integrals, where ρcircle ρ ≡ x, and ρcircle
is the radius of the stable circular orbit. Find at least one
particular case where the elliptic integrals reduce to elementary
functions (logarithms).
[3] For any central force problem, with potential V(r), show that
H = p2/2m + V(r), Lz, and L2 are
in involution (i.e. for
any pair of them, {A,B} = 0). Determine whether these are
functionally independent for the Coulomb potential, V(r) = - α/r, for
constant α.
[4] Read M A Almeida et al 1992 J.
Phys. A: Math. Gen. 25 L227-L230, "On
the nonintegrability of the Stormer problem."
HW#5 [1] As a trivial exercise in Floquet theory, determine
the standard basis functions and the matrix R (as defined in your class
notes) for the simple harmonic oscillator with time-independent frequency ω.
[2]
Read Frenkel and Portugal, J. Phys. A:
Math. Gen. 34 (2001) 3541-3551, "Algebraic methods to compute Mathieu
functions".
[3]
Find a Lagrangian to describe a particle moving on the xy-plane in a
time-dependent but spatial-independent magnetic field perpendicular to
the plane, i.e. B(t) = B(t) ez . Obtain the
equations of motion from this Lagrangian.
[4]
Solve numerically for some solutions of the driven pendulum. Take
the pivot to move with a single frequency, y(t) = A sin(νt) .
Determine some numerical values of A and ν so that stable "inverted"
solutions exist, and plot one of these inverted solutions as a function
of time.
[5]
Read Blackburn, Smith, and Jensen, Am. J. Phys. 60 (1992) 903, "Stability and Hopf
Bifurcations in the Inverted Pendulum".
HW#6 [1] Determine a classical generating function F[φ,θ]
that leaves invariant the "hyperbolic" Mathieu Hamiltonian
H. Show that H[φ] and H[θ] have the same effect when acting
on exp(iF).
[2] Use
the integral equation satisfied by the 2π periodic Mathieu functions to
compute the first few terms in their Fourier series
representations. Also determine the integral equation eigenvalues
to the same order.
[3] Find an on-line version of Theory
and Application of Mathieu Functions by N. W. McLachlan.
[4]
Show the consistency of the canonical transformation generated by
F[φ,θ] = ∫dx κ1
cos(φ(x,t)-θ(x,t)) - κ2 cos(φ(x,t)+θ(x,t)) + φ(x,t)∂xθ(x,t)
requires that both φ and θ obey the same sine-Gordon
equation, the latter equation involving only the product κ1κ2.