Math 642-600 Assignments — Spring 2019
Assignment 1 - Due Wednesday, 1/23/19
- Read section 5.1.
- Do the following problems.
- Problem 2, page 204 (§ 5.1).
- Problem 7, page 204 (§ 5.1).
- Hanging chain problem. A chain having uniform linear
density ρ hangs between the points (0,0) and (1,0). The total mass
m, which is fixed, and the total energy E of the chain are
Assuming that the chain hangs in a shape that minimizes the
energy, find the shape of the hanging chain.
- Consider the functional J(y) =
∫abF(x,y,y′)dx, where y ∈
C1 and y(a)=A, y(b)=B are fixed.
- Let y extremize J, subject to all of the conditions above. Verify
that if η ∈ C1 and η(a)=η(b)=0,
then
Δ J = ∫ab (-g(x) +
Fy′(x,y,y′))η′(x)dx, where g(x) =
∫axFy(u,y,y′)du.
- Use (a) to show that -g+Fy′(x,y,y′)=c, a
constant. From this, it follows that
Fy′(x,y,y′)∈ C1. (Du
Bois-Reymond, 1879. The point is that one need not assume that
y′′ exists.)
- Smoothing spline. Let J[y] =
∫01 (y′(x))2dx. Let the
admissible set for J be all piecewise C1 curves on [0,1]
that satisfy y(k/n) = yk , for k = 0, 1, 2, ..., n, with
the discontinuities in y′ appearing only at the points
xk = k/n. Use
the previous problem to show that the minimizer for J is a linear
spline passing through all of the points {(xk,yk), k = 0,
..., n}. (Hint: y(x) is in C1[xk,
xk+1]).)
Assignment 2 - Due Monday, 2/4/2019.
- Do the following problems.
- Problem 5, page 204 (§ 5.1).
- Problem 9, page 204 (§ 5.1).
- Problem 11, page 204 (§ 5.1).
- Show that the functional $J(y):=\int_0^1( xy^2+y'^2)dx$ is
Fréchet differentiable, if the the $C^1[0,1]$ norm is used.
- The metric of a surface in $\mathbb R^3$ having parametric form
$x=x(u,v),y=y(u,v), z=z(u,v)$ is defined by $ds^2=E(u,v)du^2 +
2F(u,v)dudv +G(u,v)dv^2$. Consider the torus (surface of a
"doughnut") obtained by rotating a circle with center $(R,0,0)$ and
radius $r < R $ about the $z$ axis. Find the metric for it and use
it to obtain the 2nd order differential equations for the geodesics.
- Problem 6, page 205 (§ 5.2).
- Find the Legendre transformation H(p) for F(x) =
xT A x, where x is in
Rn and A is a symmetric, positive definite n×n
matrix.
Assignment 3 - Due Monday, 2/18/2019.
- Do the following problems.
- Problem 7, page 206 (§ 5.2). (See Fig. 5.4, p. 205 for a
diagram.)
- Problem 8, page 206 (§ 5.2). (Note: There is an error in the
expression for L. The (dθ/dt)2
sin2θ) should be replaced by
(dφ/dt)2 sin2θ.)
- For a planet having mass $m$ in orbit around the sun (mass=$M$),
the potential is $V(r)=-mMG/r$, where $G$ is the gravitational
constant. In class, we showed that the Hamiltonian for this system is
$H=\frac{1}{2m} (p_r^2+r^{-2}p_\theta^2) - mMGr^{-1}$, and that $E=H$
and $\ell=p_\theta$ are constants of motion for the system. Inserting
these constants in $H$, we have
$E=\frac{1}{2m}\big(p_r^2+r^{-2}\ell^2\big)-mMGr^{-1}$.
- Show that $p_r = \ell r^{-2} \frac{dr}{d\theta} = - \ell
\frac{d}{d\theta}(r^{-1})$, if we change the independent variable from
$t$ to $\theta$.
- Let $u = r^{-1}- m^2MG\ell^{-2}$. Show that $2m E\ell^{-2} +
m^4M^2G^2\ell^{-4} = \big(\frac{du}{d\theta}\big)^2 + u^2$. To
simplify notation, let $\rho=(m^2MG\ell^{-2})^{-1}$ and
$\gamma=2m\rho^2 E \ell^{-2}$. This puts the equation above in the
form $u=r^{-1} -\rho^{-1}$ and
$\rho^{-2}(1+\gamma)=\big(\frac{du}{d\theta} \big)^2 +
u^2$. (Obviously, $\gamma+1>0$. For the orbit to be closed, one needs
$\gamma <0$. Consequently, $0<\gamma+1<1$.) Solve this differential
equation for $u$ in terms of $\theta$ and obtain $r=r(\theta)$.
- Use your solution to the previous part to establish Kepler's laws
of planetary motion:
- The orbit of a planet is an ellipse, with the sun at one
focus.
- The radius vector from the sun to the planet sweeps out equal
areas in equal times.
- The square of the period of any planet is proportional to the
cube of the semimajor axis of its orbit. The proportionality constant
is the same for all planets.
Assignment 4 - Due Friday, 3/1/2019.
- Do the following problems.
- Problem 1, page 207 (§ 5.4). (Hint: Use Minimax Principle.)
- Use a quadratic polynomial to estimate the lowest eigenvalue for
the Sturm-Liouville problem with Lu = − u′′ =
λu, u(0) = 0, u′(1)+u(1) = 0.
- Problem 6, page 208 (§ 5.4). Take Ω to be a 2D disk
centered at 0 and having radius r = a. How does the lowest
eigenvalue change with a? Explain.
- Consider $f(z)=1/z$, which is analytic, and therefore continuous,
in $\mathbb C \setminus \{0\}$. Show that $f$ has no analytic
anti-derivative in $\mathbb C \setminus \{0\}$. Does this contradict
Morera's Theorem? Explain.
- Show that the coefficients for a Laurent series valid in
a given annulus are unique.
- Find all of the Laurent expansions about $z=0$ for $f(z) =
\frac{1}{(z^2-1)(z+3)}$.
Assignment 5 - Due Wednesday, 3/20/2019.
- Read section 6.5.1, 6.5.2 and 7.1.
- Do the following problems.
- Section 6.4: 3, 7 (assume $a$ and $k$ are positive), 9, 20, 25.
- Let $\xi \in \mathbb R$ and consider the integral
$G(\xi)=\int_{-\infty}^\infty e^{-x^2}e^{i\xi x}dx$. Show that
$G(\xi)= \sqrt{\pi}e^{-\xi^2/4}$, given that $G(0)=\sqrt{\pi}$.
- Show that $\Gamma(z)=\int_0^\infty t^{z-1}e^{-t}dt$ is analytic
for $\text{Re}(z)>0$.
Updated 3/8/2019 (fjn)