Part C · the analytic toolkit · spine
A linear system that cannot answer before it is asked has a frequency response with no poles in one half of the complex plane — and that one fact ties refraction to absorption, turns unit 06's step function into a theorem, and evaluates integrals nothing else can.
needs 06~3½ h slides + 7 h problemsproblems: ./mr problems 20
20 · overview
Unit 06 found the response of the galvanometer to a drive at one frequency, $\chi(\omega)$, and to one kick, $G(t)$. This unit proves they are one object seen twice — and inverts $\chi$ by closing a contour: up for $t < 0$, where there are no poles, so $G$ vanishes; down for $t > 0$, collecting two residues.
Inversion, Plancherel, convolution, uncertainty.
$\delta$ defined; $LG = \delta$ proved.
Cauchy–Riemann, Goursat, Cauchy, Liouville.
Laurent, residues, Jordan, cuts, Rouché.
Poles, Kramers–Kronig, glass, Bromwich.
Watson, Laplace, stationary phase, saddles, packets.
A dotted underline is a glossary term — click it, or press G. A solid underline like the Green's function is the running example: hover it. N shows the notes, where the long proofs are.
section 1
A drive that is not periodic is still a superposition of frequencies — continuously many of them.
20 · transform
$f:\mathbb R\to\mathbb C$ is absolutely integrable if $\int_{-\infty}^\infty|f(t)|\,\mathrm dt < \infty$ (an improper Riemann integral). For such $f$:
It converges absolutely, since $|e^{i\omega t}| = 1$, and $|\hat f(\omega)| \le \int|f|$.
$\hat f$ is continuous and $\hat f(\omega)\to0$ as $|\omega|\to\infty$.
Shift, modulation and scaling, each one substitution: $f(t-a)\mapsto e^{i\omega a}\hat f$, $\ e^{-i\nu t}f\mapsto\hat f(\omega-\nu)$, $\ f(t/a)\mapsto |a|\hat f(a\omega)$.
Unit 06 drove with $e^{i\omega t}$ and got $\chi_{06} = 1/(\omega_0^2 - \omega^2 + i\gamma\omega)$. From here on a single frequency is $e^{-i\omega t}$ — the convention of every later unit and of the physics literature — and
$$\chi(\omega) = \frac{1}{\omega_0^2 - \omega^2 - i\gamma\omega} = \chi_{06}(-\omega).$$For real $\omega$ that is the complex conjugate: same modulus, lag $\varphi$ now read as $\arg\chi$. The poles move to the lower half-plane.
Why a transform at all: the galvanometer's response to $e^{-i\omega t}$ is $\chi(\omega)e^{-i\omega t}$. If a drive is a superposition of such exponentials, linearity gives the response as the same superposition, each term multiplied by $\chi$. The transform finds the weights.
20 · transform
If $f$ is $C^1$ and $f, f'$ are absolutely integrable, then $\widehat{f'}(\omega) = -i\omega\hat f(\omega)$. If $f$ and $tf$ are absolutely integrable, then $\hat f$ is $C^1$ and $\widehat{tf} = -i\,\hat f\,{}'$.
Proof of the first. Integrate by parts on $[-T, T]$: $\int f'e^{i\omega t} = [fe^{i\omega t}]_{-T}^{T} - i\omega\int fe^{i\omega t}$, and $f(\pm T)\to0$ because $f$ has limits at $\pm\infty$ ($f'$ integrable) which must be $0$ ($f$ integrable). $\square$
Apply it to the galvanometer, $\ddot x + \gamma\dot x + \omega_0^2x = f$:
$$(\omega_0^2 - \omega^2 - i\gamma\omega)\,\hat x = \hat f,\quad\text{so}\quad\hat x = \chi\,\hat f .$$A differential equation has become division. Dimensions: $[\chi] = \mathrm T^2$, $[\hat f] = [x]\mathrm T^{-2}\cdot\mathrm T$, so $[\hat x] = [x]\mathrm T$ ✓.
$f(t) = e^{-t^2/2}$. It satisfies $f' = -tf$. Transform both sides with the dictionary:
$$-i\omega\hat f = i\hat f\,{}',\quad\text{so}\quad\hat f\,{}' = -\omega\hat f .$$Separable (unit 00), unique through its initial value (unit 01), and $\hat f(0) = \int e^{-t^2/2}\mathrm dt = \sqrt{2\pi}$ (notes):
$$\hat f(\omega) = \sqrt{2\pi}\,e^{-\omega^2/2}.$$A Gaussian is its own transform, up to $\sqrt{2\pi}$. By scaling, $e^{-t^2/2\sigma^2}\mapsto\sigma\sqrt{2\pi}\,e^{-\sigma^2\omega^2/2}$: width $\sigma$ in time, $1/\sigma$ in frequency.
Check: $\sigma\to\infty$, a constant signal, piles the spectrum up at $\omega = 0$; both sides carry $\mathrm T$ ✓.
20 · transform
If $f$ is continuous and both $f$ and $\hat f$ are absolutely integrable, then for every $t$
$$f(t) = \frac{1}{2\pi}\int_{-\infty}^{\infty}\hat f(\omega)\,e^{-i\omega t}\,\mathrm d\omega .$$The kernels $K_\varepsilon$ of the proof: every one has area $1$, and as $\varepsilon\to0$ the area piles up at $u = 0$. Averaging $f$ against a kernel this narrow returns $f(t)$.
The idea of the proof. Insert a Gaussian $e^{-\varepsilon\omega^2/2}$ to make the double integral absolutely convergent, swap the order, and recognise the result:
$$\frac1{2\pi}\!\int\!\hat f e^{-i\omega t}e^{-\varepsilon\omega^2/2}\mathrm d\omega = \!\int\! f(s)K_\varepsilon(t - s)\mathrm ds,$$where $K_\varepsilon(u) = e^{-u^2/2\varepsilon}/\sqrt{2\pi\varepsilon}$ is worked example 1 read backwards: positive, total integral $1$, concentrating at $u = 0$ as $\varepsilon\to0$. So the right side tends to $f(t)$, and the left side to the inversion integral.
On the running example: $G$ is continuous and integrable and $|\chi|\le C/(1+\omega^2)$ is integrable, so $G$ is recovered from $\chi$ by this formula. Section 5 evaluates it.
In particular $\hat f = 0$ forces $f = 0$: the transform is injective, so an identity between transforms is an identity between functions.
20 · transform
The box $f = \mathbf 1_{[-1,1]}$ has $\hat f(\omega) = 2\sin\omega/\omega$, which is not absolutely integrable — because $f$ jumps. At the jump the symmetric limit $\lim_{W\to\infty}\frac1{2\pi}\int_{-W}^{W}$ still converges, to the midpoint $\frac12$ (notes).
The truncated inversion $f_W(t) = \frac1{2\pi}\int_{-W}^{W}\hat f(\omega)e^{-i\omega t}\,\mathrm d\omega$ can be written down: with $\operatorname{Si}(x) = \int_0^x\frac{\sin u}{u}\,\mathrm du$,
$$f_W(t) = \tfrac1\pi\big[\operatorname{Si}\big(W(1+t)\big) + \operatorname{Si}\big(W(1-t)\big)\big].$$At $t = 1$ it is $\operatorname{Si}(2W)/\pi$, which tends to $\frac12$ because $\int_0^\infty\frac{\sin u}{u}\mathrm du = \frac\pi2$ (worked example 2, section 4). A slowly decaying transform is the signature of a jump.
Top: $\hat f$ falls off only like $1/\omega$. Bottom: the truncated inversions for $W = 6$ and $W = 30$. Away from the jumps they close in on the box; at $t = \pm1$ they pass near the midpoint. Both overshoot by about $9\%$ beside each jump — the larger $W$ narrower, not lower.
20 · transform
For $f, g$ as in the inversion theorem,
$$\int f\,\bar g\,\mathrm dt = \frac1{2\pi}\int\hat f\,\bar{\hat g}\,\mathrm d\omega,$$and in particular $\int|f|^2\mathrm dt = \frac1{2\pi}\int|\hat f|^2\mathrm d\omega$.
Proof, one line. Write $\bar g$ by inversion, swap (Fubini): $\int f(t)\frac{1}{2\pi}\int\bar{\hat g}(\omega)e^{i\omega t}\mathrm d\omega\,\mathrm dt = \frac{1}{2\pi}\int\bar{\hat g}\hat f\,\mathrm d\omega$. $\square$
Energy in time equals energy in frequency: the transform is, up to $\sqrt{2\pi}$, an isometry. It extends to all square-integrable functions (cited: Stein–Shakarchi, Real Analysis, ch. 5 §1).
If $f, g$ are absolutely integrable and bounded, $(f*g)(t) = \int f(s)g(t-s)\,\mathrm ds$ satisfies
$$\widehat{f*g} = \hat f\,\hat g .$$Proof: swap the two integrals and substitute $u = t - s$, which splits $e^{i\omega t} = e^{i\omega s}e^{i\omega u}$. $\square$ So unit 06's $x = G*f$ becomes $\hat x = \hat G\hat f$ — and comparing with the dictionary slide,
$$\hat G(\omega) = \chi(\omega).$$$\int_0^\infty G^2\,\mathrm dt = \dfrac{1}{2\gamma\omega_0^2} = 0.01953125\ \mathrm{s^3}$, and $\dfrac1{2\pi}\displaystyle\int|\chi|^2\mathrm d\omega = \dfrac{0.1227185}{2\pi} = 0.01953125$ ✓.
20 · transform
For $f$ with $\int|f|^2 = 1$ define the spreads about the means $\bar t$, $\bar\omega$:
$$\begin{aligned}\Delta t^2 &= \textstyle\int(t-\bar t)^2|f|^2\,\mathrm dt,\\ \Delta\omega^2 &= \textstyle\frac1{2\pi}\int(\omega - \bar\omega)^2|\hat f|^2\,\mathrm d\omega .\end{aligned}$$If $f$ is $C^1$ with $f, tf, f'$ square-integrable and $\sqrt{|t|}f\to0$ at $\pm\infty$,
$$\Delta t\,\Delta\omega \ge \tfrac12,$$with equality exactly for Gaussians $f = Ce^{-a(t - \bar t)^2 - i\bar\omega t}$, $a > 0$.
Physics: a short pulse cannot be monochromatic. A 10 fs laser pulse carries a spread of frequencies of order $10^{14}\ \mathrm{s^{-1}}$, whatever the laser.
Translate and modulate so $\bar t = \bar\omega = 0$ (neither changes $\Delta t$, $\Delta\omega$). Integrate by parts:
$$1 = -\!\int t\,(|f|^2)'\,\mathrm dt = -2\operatorname{Re}\!\int t\bar ff'\,\mathrm dt .$$Cauchy–Schwarz: $1\le2\,\|tf\|\,\|f'\|$. By the dictionary and Plancherel, $\|f'\|^2 = \frac1{2\pi}\int\omega^2|\hat f|^2 = \Delta\omega^2$, and $\|tf\|^2 = \Delta t^2$. So $1\le 2\Delta t\,\Delta\omega$. $\square$
Equality: $e^{-t^2/2}/\pi^{1/4}$ has $\Delta t^2 = \Delta\omega^2 = \frac12$ ✓. Dimensions: $\mathrm T\cdot\mathrm T^{-1}$ ✓. The running example: $G$ gives $\Delta t\,\Delta\omega = \sqrt{Q^2 - \frac12 + \frac1{4Q^2}} = 19.9875$ — far from minimal, and P2 says why.
section 2
A kick too short to resolve is not a function of time. It is a rule for what happens to every smooth test of it.
20 · distributions
$\mathcal D = C_c^\infty(\mathbb R)$: smooth functions vanishing outside a bounded set. $\varphi_n\to\varphi$ in $\mathcal D$ means: all supports in one bounded set, and $\varphi_n^{(k)}\to\varphi^{(k)}$ uniformly for every $k$.
They exist: $\psi(t) = e^{-1/(1-t^2)}$ for $|t|<1$, $0$ otherwise, is $C^\infty$.
A linear map $T:\mathcal D\to\mathbb C$, written $\varphi\mapsto\langle T,\varphi\rangle$, that is continuous: $\varphi_n\to\varphi$ implies $\langle T,\varphi_n\rangle\to\langle T,\varphi\rangle$.
Physics first, here too: a ballistic galvanometer reads $\int i\,\mathrm dt$ and nothing else about the pulse (unit 06). An idealised kick is exactly that: defined by what it does to smooth responses, not by its values.
Three examples.
The next slide draws the delta as a limit of pulses, and shows it is not a function.
20 · distributions
A sequence $T_n\to T$ in distributions if $\langle T_n,\varphi\rangle\to\langle T,\varphi\rangle$ for each $\varphi$. Unit 06's square pulses of unit area, $p_\varepsilon = \varepsilon^{-1}\mathbf 1_{[0,\varepsilon]}$, have
$$\langle p_\varepsilon,\varphi\rangle = \frac1\varepsilon\int_0^\varepsilon\varphi\,\mathrm dt\ \to\ \varphi(0) = \langle\delta,\varphi\rangle,$$so $p_\varepsilon\to\delta$ — whatever the pulse shape, provided its area is $1$.
If $\int f\varphi = \varphi(0)$ for all $\varphi$, then $\int f\varphi = 0$ for every $\varphi$ vanishing near $0$, so $f = 0$ away from $0$, so $\int f\varphi = 0$ always — contradicting $\varphi(0)\ne0$.
The pulses converge; their pointwise limit (infinite at $0$, zero elsewhere) is no function at all. The limit lives only in what it does to $\varphi$.
Three pulses of area $1$, $\varepsilon = 1, \frac12, \frac14$, against a test function $\varphi$ (a stretched copy of the bump $\psi$). Pairing a pulse with $\varphi$ averages $\varphi$ over $[0,\varepsilon]$, and those averages close in on $\varphi(0)$.
20 · distributions
For $C^1$ functions this is integration by parts, so nothing old changes. Every distribution now has derivatives of all orders.
The step: $H = \mathbf 1_{t>0}$ has $\langle H',\varphi\rangle = -\int_0^\infty\varphi' = \varphi(0)$, so $H' = \delta$.
If $f$ is $C^1$ on $t<0$ and on $t>0$ with one-sided limits, jump $[f] = f(0^+) - f(0^-)$, then
$$f' = \{f'\} + [f]\,\delta,$$$\{f'\}$ being the classical derivative off $0$. Proof: split $-\int f\varphi'$ at $0$ and integrate each half by parts. $\square$
Let $L = \frac{\mathrm d^2}{\mathrm dt^2} + \gamma\frac{\mathrm d}{\mathrm dt} + \omega_0^2$ and $G$ vanish for $t < 0$, $C^2$ on $t > 0$ with one-sided limits. Then $LG = \delta$ in distributions iff
$LG = 0$ on $t>0$, $\ G(0^+) = 0$, $\ \dot G(0^+) = 1$.
The galvanometer's $G$ was built in unit 06 to meet exactly these three conditions. So $LG = \delta$ — the defining property, now a statement about a well-defined object. The proof, and a picture of the three conditions, are on the next slide.
20 · distributions
Proof. The jump formula once gives $\dot G = \{\dot G\} + [G]\,\delta$. Differentiate that, using the jump formula again on $\{\dot G\}$:
$$\ddot G = \{\ddot G\} + [\dot G]\,\delta + [G]\,\delta' .$$Add $\gamma\dot G + \omega_0^2G$ ($G$ itself is a function, so $\omega_0^2G$ brings no delta):
$$LG = \{LG\} + \big([\dot G] + \gamma[G]\big)\delta + [G]\,\delta' .$$$\delta$ and $\delta'$ are independent (test with $\varphi$ having $\varphi(0) = 0\ne\varphi'(0)$, and conversely), so $LG = \delta$ iff $\{LG\} = 0$, $[G] = 0$ and $[\dot G] = 1$. $\square$
The galvanometer's $G$ and $\dot G$ across the kick. $G$ is continuous with a corner, so $[G] = 0$ and no $\delta'$ appears; $\dot G$ jumps by exactly $1$, which is the single $\delta$ in $LG$.
20 · distributions
$\mathcal S$: smooth $\varphi$ with $t^m\varphi^{(k)}$ bounded for all $m, k$ (the Schwartz class). The dictionary maps $\mathcal S$ to itself. A tempered distribution is a continuous linear map on $\mathcal S$; since $\int\hat f\varphi = \int f\hat\varphi$ (swap the integrals), define
| $T$ | $\hat T$ | why |
|---|---|---|
| $\delta$ | $1$ | $\hat\varphi(0) = \int\varphi$ |
| $1$ | $2\pi\delta$ | inversion at $t = 0$ |
| $e^{-i\nu t}$ | $2\pi\delta(\omega - \nu)$ | modulation |
| $\operatorname{sgn}t$ | $2i\,\mathrm{PV}\frac1\omega$ | limit of $e^{-\varepsilon|t|}\operatorname{sgn}t$ |
As distributions, $\displaystyle\lim_{\varepsilon\to0^+}\frac{1}{x \mp i\varepsilon} = \mathrm{PV}\frac1x \pm i\pi\,\delta$.
Proof. $\dfrac{1}{x - i\varepsilon} = \dfrac{x}{x^2 + \varepsilon^2} + \dfrac{i\varepsilon}{x^2 + \varepsilon^2}$. The second is $i\pi$ times a positive kernel of total mass $1$ concentrating at $0$, so tends to $i\pi\delta$; the first tends to $\mathrm{PV}\frac1x$ (notes). $\square$
As $\gamma\to0$, $\chi$ $\to\dfrac{1}{\omega_0^2 - (\omega + i0)^2}$ — shorthand for $\omega + i\varepsilon$ with the limit $\varepsilon\to0^+$ taken last, as in Sokhotski (here $\varepsilon = \gamma/2$; section 5 names it the $i0$ prescription) — and
$$\operatorname{Im}\chi\to\frac{\pi}{2\omega_0}\big[\delta(\omega - \omega_0) - \delta(\omega + \omega_0)\big].$$A lossless oscillator absorbs only at resonance — as a spike. Weight check: $\int_0^\infty\omega\operatorname{Im}\chi\,\mathrm d\omega = \frac\pi2$ for every $\gamma$ (section 5), and the spike gives $\omega_0\cdot\frac{\pi}{2\omega_0}$ ✓.
section 3
Ask for a derivative in the complex sense and get, for free, infinitely many derivatives, a convergent power series, and Cauchy's theorem.
20 · holomorphy
$f$ on an open $U\subseteq\mathbb C$ is complex-differentiable at $z$ if $\displaystyle f'(z) = \lim_{h\to0,\ h\in\mathbb C}\frac{f(z+h) - f(z)}{h}$ exists; holomorphic on $U$ if at every point. Entire: holomorphic on $\mathbb C$.
Sums, products, quotients and compositions obey the real rules, with the real proofs. So polynomials and rational functions are holomorphic off the zeros of their denominators — $\chi$ on $\mathbb C\setminus\{\omega_+,\omega_-\}$.
Physics: $\chi$ at complex $\omega = \omega_r + i\omega_i$ is the response to $e^{-i\omega t} = e^{\omega_it}e^{-i\omega_rt}$ — a drive growing in time when $\omega_i > 0$, switched on from nothing at $t = -\infty$.
Partial derivatives, all this unit needs of them: for $u(x, y)$, $u_x$ is the derivative of $x\mapsto u(x,y)$ with $y$ held fixed, and $u_y$ likewise.
If $f = u + iv$ is complex-differentiable at $z = x + iy$, then
$$u_x = v_y,\qquad u_y = -v_x,\qquad f' = u_x + iv_x .$$Proof. Let $h\to0$ along the reals: $f' = u_x + iv_x$. Along $h = ik$: $f' = \frac1i(u_y + iv_y) = v_y - iu_y$. Equate. $\square$
$\bar z = x - iy$: $u_x = 1\ne-1 = v_y$ everywhere. $|z|^2$ is differentiable at $0$ only. Holomorphy is a strong condition, and everything in this section is its price.
20 · holomorphy
For a piecewise $C^1$ curve $\gamma:[a,b]\to U$ and continuous $f$,
$$\int_\gamma f(z)\,\mathrm dz := \int_a^b f(\gamma(s))\,\gamma'(s)\,\mathrm ds,$$an ordinary integral of a complex-valued function of one real variable. Reparametrising does not change it (substitution); reversing the direction flips its sign.
with $L(\gamma) = \int_a^b|\gamma'(s)|\,\mathrm ds$ the length.
Every arc estimate in this unit is this inequality, used carefully.
If $F' = f$ on $U$ then $\int_\gamma f\,\mathrm dz = F(\gamma(b)) - F(\gamma(a))$, and $\oint_\gamma f\,\mathrm dz = 0$ round every closed curve.
Proof: $\frac{\mathrm d}{\mathrm ds}F(\gamma(s)) = F'(\gamma(s))\gamma'(s)$, from the definition of $F'$; then the fundamental theorem of calculus. $\square$
Round $\gamma(s) = re^{is}$, $0\le s\le2\pi$, the integrand is $ir^{n+1}e^{i(n+1)s}$, so
$$\oint z^n\,\mathrm dz = \begin{cases}2\pi i, & n = -1,\\ 0, & n\ne-1.\end{cases}$$So $1/z$ has no primitive on $\mathbb C\setminus\{0\}$. Residue theory is this computation, organised.
20 · holomorphy
If $f$ is holomorphic on $U$ and $T\subset U$ is a closed solid triangle, then $\displaystyle\oint_{\partial T}f\,\mathrm dz = 0$.
Join the midpoints of the sides: four triangles, whose boundary integrals sum to $\oint_{\partial T}$ (inner edges cancel). One, $T_1$, has $|\oint_{\partial T_1}|\ge\frac14|\oint_{\partial T}|$. Repeat: nested $T_n$ of diameter $2^{-n}d$, perimeter $2^{-n}p$, and $|\oint_{\partial T_n}f|\ge4^{-n}|\oint_{\partial T}f|$.
Compactness: $\bigcap T_n = \{z_0\}$, and $f(z) = f(z_0) + f'(z_0)(z - z_0) + \epsilon(z)(z - z_0)$ with $\epsilon\to0$. The linear part has a primitive; ML on the rest:
$4^{-n}|\oint_{\partial T}f|\le\sup_{T_n}|\epsilon|\cdot2^{-n}d\cdot2^{-n}p$. Multiply by $4^n$; let $n\to\infty$. $\square$
One subdivision. The four boundaries, each run anticlockwise, add up to $\partial T$: every inner edge is run once each way and cancels. The shaded $T_1$ keeps at least a quarter of the integral; its own subdivisions (darker) close down on $z_0$. Schematic.
20 · holomorphy
Only the existence of $f'$ at each point: not its continuity, not Green's theorem, not a double integral. Cauchy (1825) assumed $f'$ continuous; Goursat showed it superfluous — as it must be, for $f'$ to come out smooth on the next slides.
The conclusion still holds if $f$ is continuous on $U$ and holomorphic on $U\setminus\{p\}$. This is what the integral formula will need.
Proof. If $p$ is a vertex, cut off a tiny triangle $T_\eta$ there, of perimeter $\le\eta$; the rest splits into triangles without $p$, whose integrals vanish, so $|\oint_{\partial T}f|\le\eta\max_T|f|\to0$. Otherwise split $T$ into triangles having $p$ as a vertex. $\square$
The two cases. Only the tiny shaded triangle can carry an integral, and its perimeter goes to zero while $f$ stays bounded.
For $\chi$: any triangle avoiding $\omega_\pm$ has $\oint\chi = 0$. A triangle enclosing $\omega_+$ need not — the next section computes what it gives.
20 · holomorphy
If $f$ is holomorphic on a convex open set $U$, then $F(z) = \int_{[c,z]}f$ (straight segment from a fixed $c$) is a primitive of $f$, and so $\oint_\gamma f\,\mathrm dz = 0$ for every closed curve $\gamma$ in $U$.
Proof. Goursat on the triangle $c, z, z+h$: $F(z+h) - F(z) = \int_{[z,z+h]}f = hf(z) + \int_{[z,z+h]}(f - f(z))$, and the last term is at most $|h|\max_{[z,z+h]}|f - f(z)| = o(|h|)$. So $F' = f$; then the primitive rule. $\square$
Semicircles, rectangles and sectors are convex. For keyholes and indented lines the theorem holds too: cut the region into convex pieces (notes). The general form — $\oint_\gamma f = 0$ when $\gamma$ winds zero times round every point outside $U$ — is cited: Ahlfors, Complex Analysis, ch. 4 §4.
If $f$ is holomorphic on an open set containing the closed disc $|\zeta - z_0|\le r$, then for $|z - z_0| < r$
$$f(z) = \frac{1}{2\pi i}\oint_{|\zeta - z_0| = r}\frac{f(\zeta)}{\zeta - z}\,\mathrm d\zeta .$$Proof. $g(\zeta) = \frac{f(\zeta) - f(z)}{\zeta - z}$, with $g(z) = f'(z)$, is continuous, and holomorphic except at $z$; so $\oint g = 0$ (exceptional-point Goursat, convex version, on a slightly larger disc). Hence $\oint\frac{f(\zeta)}{\zeta - z} = f(z)\oint\frac{\mathrm d\zeta}{\zeta - z} = 2\pi i\,f(z)$ (notes). $\square$
The values of a holomorphic function inside a circle are determined by its values on the circle. Nothing like this is true of real $C^\infty$ functions — the bump function of section 2 is zero on a whole interval and not zero.
20 · holomorphy
A holomorphic $f$ is infinitely differentiable, with
$$f^{(n)}(z) = \frac{n!}{2\pi i}\oint\frac{f(\zeta)}{(\zeta - z)^{n+1}}\,\mathrm d\zeta,$$and it is analytic: its Taylor series at $z_0$ converges to $f$ on the largest open disc about $z_0$ inside $U$.
Cauchy estimates: if $|f|\le M$ on the circle of radius $r$, then $|f^{(n)}(z_0)|\le n!M/r^n$ — ML on the formula.
A bounded entire function is constant. Proof: $|f'(z_0)|\le M/r$ for every $r$. $\square$
A nonconstant polynomial $p$ has a complex root. Proof: otherwise $1/p$ is entire, and $\to0$ as $|z|\to\infty$, so bounded, so constant. $\square$ Unit 06's debt, paid.
Maximum modulus: if $|f|$ has a local maximum in a connected $U$, $f$ is constant. Morera: a continuous $f$ with $\oint_{\partial T}f = 0$ for every triangle is holomorphic.
20 · holomorphy
$\chi$ is holomorphic on $|\omega| < |\omega_\pm| = \sqrt{\omega_\mathrm d^2 + \gamma^2/4} = \omega_0 = 8$, so its low-frequency series $\chi = \omega_0^{-2}\big(1 + i\gamma\omega/\omega_0^2 + \dots\big)$ converges exactly for $|\omega| < \omega_0$: the stiffness-dominated description fails at resonance, and the poles say so.
Read the plot: below $\omega_0$ the polynomials hug $\chi$, more closely the higher the degree; past $\omega_0$ they run away, and raising the degree only makes them run faster. On the real axis $\chi$ is smooth at $8$, merely large; the series fails there because of two poles $0.2$ below the axis.
$|\chi(\omega)|$ on the real axis (log scale) against its Taylor polynomials about $0$ of degree $10$ and $40$. Both follow $\chi$ inside the disc $|\omega| < 8$ and diverge outside it: the radius is the distance to the poles.
20 · holomorphy
If $f, g$ are holomorphic on a connected open $U$ and agree on a set with a limit point in $U$ — a segment of the real axis, say — then $f = g$ on all of $U$.
Proof, in outline. Let $h = f - g$. The set of points where every derivative of $h$ vanishes is closed, and open (the Taylor series there is $0$ on a disc), and nonempty (at the limit point, the first nonzero Taylor coefficient would make the zeros isolated). Connectedness. $\square$
A holomorphic $F$ on $U\supset V$ extending $f$ on $V$. By the identity theorem it is unique — so a formula valid on part of a domain is valid wherever both sides make sense.
For $a > 0$, $\int e^{-at^2/2}\mathrm dt = \sqrt{2\pi/a}$ (scaling). Both sides are holomorphic in $a$ on $\operatorname{Re}a > 0$ (left: Morera; right: the principal square root). They agree on the positive reals, so
$$\int_{-\infty}^\infty e^{-at^2/2}\,\mathrm dt = \sqrt{\frac{2\pi}{a}},\qquad\operatorname{Re}a > 0 .$$Section 6 uses this with $a = \sigma_0^2 + i\beta t$: a spreading wave packet.
The running example. The integral $\int_0^\infty G(t)e^{i\omega t}\mathrm dt$ converges only for $\operatorname{Im}\omega > -\gamma/2$. The rational formula for $\chi$ is its continuation to $\mathbb C\setminus\{\omega_\pm\}$: the integral fails below the line through the poles; the function does not.
section 4
Round a closed contour, only the singularities inside speak — and each says one number.
20 · residues
If $f$ is holomorphic on the annulus $r < |z - z_0| < R$, then on it
$$f(z) = \sum_{n\in\mathbb Z}a_n(z - z_0)^n,$$$a_n = \frac{1}{2\pi i}\oint f(\zeta)(\zeta - z_0)^{-n-1}\mathrm d\zeta$ round any circle in the annulus. The negative powers are the principal part.
An isolated singularity: $f$ holomorphic on $0 < |z - z_0| < R$. Three kinds:
It is the one Laurent coefficient that survives integration: every other power has a primitive on the punctured disc.
$\chi$ $= \dfrac{-1}{(\omega - \omega_+)(\omega - \omega_-)}$ has simple poles at $\omega_\pm = \pm\omega_\mathrm d - i\gamma/2$ and is holomorphic everywhere else, including at $\infty$ in the sense that $\chi(1/w)$ has a removable singularity at $w = 0$.
Physics: a pole is a free mode — its real part the ringing frequency $7.9975\ \mathrm{s^{-1}}$, its imaginary part the decay rate $0.2\ \mathrm{s^{-1}}$. Its residue will be that mode's amplitude in $G$.
20 · residues
Let $\gamma$ be a circle, or a contour of the kinds on the Cauchy slide, traversed anticlockwise, and $f$ holomorphic on an open set containing $\gamma$ and its inside, except at finitely many points $z_1,\dots,z_k$ inside. Then
$$\oint_\gamma f\,\mathrm dz = 2\pi i\sum_{j=1}^k\operatorname*{Res}_{z_j}f .$$Proof. Let $P_j$ be the principal part at $z_j$; it converges on $\mathbb C\setminus\{z_j\}$. Then $f - \sum P_j$ has only removable singularities, so its integral is $0$ by Cauchy. And $\oint P_j = 2\pi i\,a^{(j)}_{-1}$, term by term, by the circle computation. $\square$
Simple pole, $f = g/h$ with $h(z_0) = 0\ne h'(z_0)$, $g$ holomorphic: $\operatorname{Res}f = g(z_0)/h'(z_0)$.
Pole of order $m$: $\operatorname{Res}f = \dfrac{1}{(m-1)!}\lim\limits_{z\to z_0}\dfrac{\mathrm d^{m-1}}{\mathrm dz^{m-1}}\big[(z - z_0)^mf(z)\big]$.
$h(\omega) = \omega_0^2 - \omega^2 - i\gamma\omega$ has $h'(\omega) = -2\omega - i\gamma$, so $h'(\omega_\pm) = \mp2\omega_\mathrm d$ and
$$\operatorname*{Res}_{\omega_\pm}\chi(\omega)e^{-i\omega t} = \mp\frac{e^{-i\omega_\pm t}}{2\omega_\mathrm d} .$$Dimensions: $\mathrm T^{-1}\cdot\mathrm T^{2}$ per pole = $\mathrm T$ — a residue of $\chi$ carries $[\chi][\omega]$ ✓.
20 · residues
Let $C_R$ be the upper semicircle $z = Re^{i\theta}$, $0\le\theta\le\pi$, and $M_R = \max_{C_R}|g|\to0$ as $R\to\infty$. Then for every $a > 0$
$$\Big|\int_{C_R}g(z)e^{iaz}\,\mathrm dz\Big|\le\frac{\pi M_R}{a}\to0 .$$$|e^{iaz}| = e^{-aR\sin\theta}$ on $C_R$, so the integral is at most $M_RR\int_0^\pi e^{-aR\sin\theta}\mathrm d\theta = 2M_RR\int_0^{\pi/2}e^{-aR\sin\theta}\mathrm d\theta$. Concavity gives Jordan's inequality $\sin\theta\ge2\theta/\pi$ on $[0,\pi/2]$, so this is at most $2M_RR\int_0^\infty e^{-2aR\theta/\pi}\mathrm d\theta = \pi M_R/a$. $\square$
ML gives $\pi RM_R$: useless when $g\sim1/R$ — $\sin x/x$, Kramers–Kronig, any transform of a function with a jump. The exponential's decay over most of the arc is what saves you.
$|e^{-i\omega t}| = e^{t\operatorname{Im}\omega}$: it decays in the upper half-plane when $t < 0$, in the lower when $t > 0$.
For $e^{-i\omega t}$ the lemma applies with $a = -t$ above (if $t < 0$) or, reflected, with $a = t$ below (if $t > 0$). The sign of $t$ chooses the half-plane. For $\chi$, $M_R\sim1/R^2$.
20 · residues · example
Step 1 — the function. Not $\sin z/z$: $\sin z$ grows like $e^{|\operatorname{Im}z|}$ in both half-planes. Take $f(z) = e^{iz}/z$: imaginary part $\sin x/x$ on the axis, decaying upwards.
Step 2 — the contour. $[-R,-\varepsilon]$, the small upper semicircle $c_\varepsilon$ clockwise round the pole at $0$, $[\varepsilon,R]$, the big semicircle $C_R$. Nothing inside, so the total is $0$.
Step 2's contour. The pole at $0$ is stepped round from above, so nothing is inside; schematic.
Step 3 — the straight parts. Pair $x$ with $-x$: $\int_{\varepsilon<|x|<R}\frac{e^{ix}}{x}\mathrm dx = \int_\varepsilon^R\frac{e^{ix} - e^{-ix}}{x}\mathrm dx = 2i\int_\varepsilon^R\frac{\sin x}{x}\mathrm dx$.
Step 4 — the big arc. Jordan with $g = 1/z$, $M_R = 1/R$, $a = 1$: at most $\pi/R\to0$.
Step 5 — the small arc. $e^{iz}/z = 1/z + h(z)$, $h$ bounded near $0$. $\int_{c_\varepsilon}\mathrm dz/z = \int_\pi^0i\,\mathrm d\theta = -\pi i$, and $|\int_{c_\varepsilon}h|\le\pi\varepsilon\max|h|\to0$.
Step 6 — assemble. $2i\int_0^\infty\frac{\sin x}{x}\mathrm dx - \pi i = 0$, so
$$\int_0^\infty\frac{\sin x}{x}\,\mathrm dx = \frac\pi2 = 1.5708 .$$Checks. $\int_0^\infty\frac{\sin ax}{x}\mathrm dx = \frac\pi2\operatorname{sgn}a$, independent of $|a|$, as $u = ax$ demands; with $x$ a time, a pure number ✓.
20 · residues
If $f$ has a simple pole at $x_0$ and $c_\varepsilon$ is an anticlockwise arc of angle $\alpha$ of $|z - x_0| = \varepsilon$, then $\int_{c_\varepsilon}f\to i\alpha\operatorname*{Res}_{x_0}f$. A half-circle gives half a residue.
Proof. $f = \frac{c}{z - x_0} + h$ with $h$ bounded near $x_0$; on the arc $\int\frac{c\,\mathrm dz}{z - x_0} = ic\alpha$ exactly, and $|\int h|\le\alpha\varepsilon\max|h|\to0$. $\square$
Step 3 read differently: $\mathrm{PV}\!\int_{-\infty}^{\infty}\frac{e^{ix}}{x}\mathrm dx = i\pi$. A pole on the contour contributes $\pm i\pi\operatorname{Res}$, the sign set by which way you step round it — Sokhotski–Plemelj, seen from the complex plane.
Two ways round the pole of $e^{iz}/z$. Above, the arc is clockwise ($-\pi i$) and nothing is enclosed; below, it is anticlockwise ($+\pi i$) and the residue $1$ is enclosed. Both give $2i\int_0^\infty\frac{\sin x}{x}\mathrm dx = \pi i$.
20 · residues
$\oint\mathrm dz/z = 2\pi i$ means no continuous logarithm exists on $\mathbb C\setminus\{0\}$: each turn round $0$ adds $2\pi i$. Remove a ray and one does:
On $\mathbb C\setminus(-\infty,0]$, the principal logarithm $\operatorname{Log}z = \ln|z| + i\operatorname{Arg}z$, $\operatorname{Arg}\in(-\pi,\pi)$, is holomorphic with derivative $1/z$. Then $z^a := e^{a\log z}$ for any $a\in\mathbb C$.
$0$ is a branch point: continuing $z^a$ once round it multiplies it by $e^{2\pi ia}$. The cut is a choice; the branch point is not.
Choose the cut and the branch before writing an integral, and state the value of $\arg z$ on each edge of the cut.
The keyhole: cut along $[0,\infty)$, $\arg\in(0,2\pi)$. The two edges of the cut are the same points with different values of $z^a$.
What it buys. For $\int_0^\infty x^{a-1}R(x)\,\mathrm dx$ the two edges give $(1 - e^{2\pi ia})\int_0^\infty$; the circles vanish; the residue theorem finishes. P8: $\displaystyle\int_0^\infty\frac{x^{a-1}}{1 + x}\mathrm dx = \frac{\pi}{\sin\pi a}$ for $0 < a < 1$.
20 · residues
If $f$ is holomorphic inside and on a circle (or toy contour) $\gamma$ except for poles, with no zeros or poles on $\gamma$, then
$$\frac{1}{2\pi i}\oint_\gamma\frac{f'(z)}{f(z)}\,\mathrm dz = Z - P,$$zeros minus poles inside, with multiplicity: the number of times $f(\gamma)$ winds round $0$.
Proof. Near a zero of order $m$, $f = (z - z_0)^mk$ with $k(z_0)\ne0$, so $f'/f = \frac{m}{z - z_0} + \frac{k'}{k}$: residue $m$. At a pole of order $m$, residue $-m$. Residue theorem. $\square$
If $f, g$ are holomorphic inside and on $\gamma$ and $|g| < |f|$ on $\gamma$, then $f$ and $f + g$ have the same number of zeros inside $\gamma$.
Proof. For $s\in[0,1]$, $|f + sg|\ge|f| - |g| > 0$ on $\gamma$. So $N(s) = \frac1{2\pi i}\oint\frac{(f + sg)'}{f + sg}$ is defined, continuous in $s$, and an integer: constant. $N(0) = N(1)$. $\square$
20 · residues
On $|z| = 2$: $|3z + 1|\le7 < 32 = |z^5|$, so all five roots have $|z| < 2$. On $|z| = 1$: $|z^5 + 1|\le2 < 3 = |3z|$, so exactly one has $|z| < 1$. (Computed: $-0.33199$, and four of modulus $1.2629$ and $1.3743$ ✓.)
P10 uses Rouché to show Kepler's equation has exactly one root in a disc for every $|e| < 0.6627$ — and that is the Laplace limit.
Why it works: on a circle where one term dominates, $f$ cannot reach $0$, and its image winds round $0$ as often as the dominant term's does — $z^5$ five times on $|z| = 2$, $3z$ once on $|z| = 1$.
Left: the five roots, computed, with $|z| = 1$ and $|z| = 2$. Right: the image of $|z| = 1$ under $f(z) = z^5 + 3z + 1$. It never reaches $0$ and goes round it once — one zero inside, by the argument principle. (The image of $|z| = 2$, too large to draw here, goes round five times.)
section 5
A system that cannot respond before it is driven has a frequency response holomorphic in the upper half-plane — and conversely.
20 · causality · example
Step 0 — what is to be computed. By inversion, $G(t) = \dfrac1{2\pi}\displaystyle\int_{-\infty}^\infty\frac{e^{-i\omega t}\,\mathrm d\omega}{\omega_0^2 - \omega^2 - i\gamma\omega}$, the limit of $\int_{-R}^R$.
Step 1 — the poles. $\omega^2 + i\gamma\omega - \omega_0^2 = 0$ gives $\omega_\pm = \pm\omega_\mathrm d - i\gamma/2 = \pm7.9975 - 0.2\,i$. Both below the real axis.
Step 2 — the arcs. On $|\omega| = R$: $|\omega_0^2 - \omega^2 - i\gamma\omega|\ge R^2 - \gamma R - \omega_0^2$, so $|\chi|\le2/R^2$ once $R\ge12$; and $|e^{-i\omega t}| = e^{t\operatorname{Im}\omega}\le1$ on whichever semicircle has $t\operatorname{Im}\omega\le0$. ML: arc $\le\pi R\cdot2/R^2\to0$.
Step 3 — $t < 0$: close upwards. On the upper arc $t\operatorname{Im}\omega\le0$ ✓. Inside the half-disc there is no pole, so by Cauchy $\int_{-R}^R + \int_{\text{arc}} = 0$ for every $R$; the arc $\to0$. Therefore
$$G(t) = 0\quad\text{for } t < 0 \quad\text{— exactly.}$$The two closures, poles drawn deeper than their true $0.2$ below the axis. Which one is allowed is decided by the sign of $t$ alone.
20 · causality · example
Step 4 — $t > 0$: close downwards, clockwise, enclosing both poles:
$$\int_{-R}^R + \int_{\text{arc}} = \frac{-2\pi i}{2\omega_\mathrm d}\big(e^{-i\omega_-t} - e^{-i\omega_+t}\big),$$the residues from the residue slide. With $e^{-i\omega_\pm t} = e^{-\gamma t/2}e^{\mp i\omega_\mathrm dt}$ the bracket is $2i\,e^{-\gamma t/2}\sin\omega_\mathrm dt$. Let $R\to\infty$, divide by $2\pi$, and $(-i)(2i)/2\omega_\mathrm d = 1/\omega_\mathrm d$:
$$G(t) = e^{-\gamma t/2}\,\frac{\sin\omega_\mathrm dt}{\omega_\mathrm d} .$$Step 5 — $t = 0$. No exponential; both closures are legitimate by ML, and the upper one gives $G(0) = 0$: continuous, as unit 06 required.
The result, plotted: exactly $0$ before the kick (Step 3), then a ring at $\omega_\mathrm d = 7.9975\ \mathrm{s^{-1}}$ inside the envelope $\pm e^{-\gamma t/2}/\omega_\mathrm d$ (dashed).
Checks. Unit 06's $G$, to the letter ✓. $[G] = \mathrm T$ ✓. $\gamma\to0$: $\sin(\omega_0t)/\omega_0$, the undamped kick ✓. Number: first maximum near $t = \pi/2\omega_\mathrm d = 0.1964$ s, $G = 0.1202$ s.
20 · causality
The example used two facts only: $\chi\to0$ at infinity, and no poles in the upper half-plane. Any response with those two properties vanishes for $t < 0$, by Step 3 verbatim. And for $t > 0$
$$G(t) = -i\sum_{\text{poles } \omega_k}\operatorname*{Res}_{\omega_k}\chi(\omega)e^{-i\omega t},$$a sum of damped modes, one per pole — when there are finitely many poles and $\chi$ decays.
With no damping, $\chi = 1/(\omega_0^2 - \omega^2)$ has poles on the axis and the inversion integral is undefined. Causality decides: replace $\omega$ by $\omega + i0$ — poles pushed below, contour passing above — and
$$G_\mathrm{ret}(t) = H(t)\,\frac{\sin\omega_0t}{\omega_0} .$$In the damped case no choice is left: $\gamma > 0$ has already moved the poles down by $\gamma/2$, and the real-axis integral is the retarded one. Dissipation and causality point the same way.
Forward: unit 24 inverts the wave operator's $1/(\omega^2/c^2 - k^2)$ with exactly this prescription, and it is how light is emitted after, not before, the charge moves.
20 · causality
Pass below both poles and closing upwards for $t < 0$ collects them: $G_\mathrm{adv}(t) = -H(-t)\sin(\omega_0t)/\omega_0$, which also satisfies $LG = \delta$ (its $\dot G$ jumps from $-1$ to $0$). Principal values at both poles give $\frac12(G_\mathrm{ret} + G_\mathrm{adv})$. The equation admits all of them; the choice of half-plane is the physics.
The difference $G_\mathrm{ret} - G_\mathrm{adv} = \sin(\omega_0t)/\omega_0$ for all $t$: a free oscillation, which $L$ annihilates. Any two solutions of $LG = \delta$ differ by one, and the contour picks which.
Undamped poles at $\pm\omega_0$ on the axis, with $\omega_0 = 8$. Passing above them (poles pushed below, $\omega + i0$) gives the retarded $G$, silent before the kick. Passing below gives the advanced one, which rings before the kick and stops dead at it.
20 · causality
Let $G$ be continuous except possibly at $0$, with $G$, $tG$ and $\chi = \hat G$ absolutely integrable. The following are equivalent:
(a) causality: $G(t) = 0$ for all $t < 0$;
(b) analyticity: $\chi$ extends continuously to $\operatorname{Im}\omega\ge0$, holomorphic on $\operatorname{Im}\omega > 0$, with $\max_{|\omega| = R,\,\operatorname{Im}\omega\ge0}|\chi|\to0$;
(c) dispersion: for every real $\omega$,
$$\chi(\omega) = \frac{1}{i\pi}\,\mathrm{PV}\!\!\int_{-\infty}^{\infty}\frac{\chi(\omega')}{\omega' - \omega}\,\mathrm d\omega' .$$The sharp form, for square-integrable $\chi$, is Titchmarsh's theorem (cited: Titchmarsh, Introduction to the Theory of Fourier Integrals, 1937, Thm 95).
$\chi(\omega) = \int_0^\infty G(t)e^{i\omega t}\mathrm dt$ and $|e^{i\omega t}| = e^{-t\operatorname{Im}\omega}\le1$ for $t\ge0$: absolutely convergent on the closed upper half-plane, continuous there, holomorphic inside (Morera). Decay: for $G$ the indicator of $[a,b]\subset[0,\infty)$, $|\chi|\le2/|\omega|$; approximate by steps. $\square$
For $t < 0$ close upwards: no singularity inside, and Jordan's lemma with $a = -t > 0$ kills the arc. So $\int_{-R}^R\chi e^{-i\omega t}\mathrm d\omega = -\int_\text{arc}\to0$, and by inversion $G(t) = 0$. $\square$
(a) ⇔ (c) is the next slide. On the running example: $G$, $tG$, $\chi$ are integrable; (a) is unit 06's construction, (b) the position of two poles, and (c) is checked with numbers two slides on.
20 · causality
1. Causality says $G(t) = \operatorname{sgn}(t)\,G(t)$ for $t\ne0$. Transforms are injective, so (a) $\iff\chi = \widehat{\operatorname{sgn}\cdot G}$.
2. The transform of a product is $\frac1{2\pi}$ times the convolution of the transforms (the convolution theorem run backwards, notes), and $\widehat{\operatorname{sgn}} = 2i\,\mathrm{PV}\frac1\omega$:
$$\widehat{\operatorname{sgn}\cdot G}(\omega) = \frac{i}{\pi}\,\mathrm{PV}\!\!\int\frac{\chi(\omega')}{\omega - \omega'}\,\mathrm d\omega' .$$3. That is the right side of (c). $\square$
Real and imaginary parts, $\chi = \chi' + i\chi''$:
$$\chi'(\omega) = \frac1\pi\mathrm{PV}\!\!\int\frac{\chi''(\omega')\,\mathrm d\omega'}{\omega' - \omega},$$ $$\chi''(\omega) = -\frac1\pi\mathrm{PV}\!\!\int\frac{\chi'(\omega')\,\mathrm d\omega'}{\omega' - \omega}.$$A real $G$ gives $\chi(-\omega) = \overline{\chi(\omega)}$: $\chi'$ even, $\chi''$ odd. Folding the integrals onto $\omega' > 0$:
$$\chi'(\omega) = \frac2\pi\,\mathrm{PV}\!\!\int_0^\infty\frac{\omega'\chi''(\omega')}{\omega'^2 - \omega^2}\,\mathrm d\omega',$$ $$\chi''(\omega) = -\frac{2\omega}{\pi}\,\mathrm{PV}\!\!\int_0^\infty\frac{\chi'(\omega')}{\omega'^2 - \omega^2}\,\mathrm d\omega' .$$Read it: the in-phase (reactive, dispersive) response at one frequency is an integral of the out-of-phase (absorptive) response at all frequencies. Neither can be designed without the other.
Dimensions: $[\chi''][\omega]/[\omega] = [\chi]$ ✓. Limit: $\chi''\equiv0$ forces $\chi'\equiv0$ — the glass slide.
20 · causality · example
Step 1 — the two parts. With $D(\omega) = (\omega_0^2 - \omega^2)^2 + \gamma^2\omega^2$,
$$\chi' = \frac{\omega_0^2 - \omega^2}{D},\qquad \chi'' = \frac{\gamma\omega}{D} .$$$\chi''>0$ for $\omega>0$: the oscillator absorbs.
Step 2 — at $\omega = 0$, exactly. The first relation gives
$$\chi'(0) = \frac2\pi\int_0^\infty\frac{\chi''(\omega')}{\omega'}\mathrm d\omega' = \frac{2\gamma}{\pi}\int_0^\infty\frac{\mathrm d\omega'}{D},$$and P5's integral makes this $\frac{2\gamma}{\pi}\cdot\frac{\pi}{2\gamma\omega_0^2} = \frac1{\omega_0^2}$. That is $\chi(0) = 1/64 = 0.015625\ \mathrm{s^2}$: the static stiffness ✓.
The two parts of $\chi$ on the real axis. $\chi''$ is a narrow absorption peak at $\omega_0$; $\chi'$ swings through zero there. Kramers–Kronig computes either curve from the other; the dots are Step 4's check at $\omega = 7$.
20 · causality · example
Step 3 — at large $\omega$. For $\omega$ beyond the region where $\chi''$ lives, the first relation gives $\chi'(\omega)\approx-\frac{2}{\pi\omega^2}\int_0^\infty\omega'\chi''\,\mathrm d\omega'$. But directly $\chi'\approx-1/\omega^2$ — a free mass. So the sum rule
$$\int_0^\infty\omega\,\chi''(\omega)\,\mathrm d\omega = \frac\pi2$$must hold, whatever $\gamma$ and $\omega_0$. Directly: $\gamma\int_0^\infty\omega^2/D = \gamma\cdot\frac{\pi}{2\gamma} = \frac\pi2$ ✓.
Step 4 — at $\omega = 7\ \mathrm{s^{-1}}$, off every special point: $\chi(7) = 0.0644219 + 0.0120254\,i$. The principal-value integrals, computed numerically, return $0.06442192$ and $0.01202542$ ✓.
Dimensions in Step 3: $[\omega\chi''\,\mathrm d\omega] = \mathrm T^{-1}\mathrm T^2\mathrm T^{-1} = 1$ ✓.
The sum rule, drawn: $\omega\chi''(\omega)$ for the galvanometer's $\gamma = 0.4$ and for $\gamma = 2$ (same $\omega_0$). Damping trades height for width; the area under each curve is $\pi/2$.
20 · causality
Physics, cited: in a dielectric made of bound charges $q$, mass $m$, density $N$, each a copy of the oscillator with its own $\omega_0$, light sees the relative permittivity $\varepsilon(\omega)$ (Jackson, Classical Electrodynamics, §7.5; not derived in this course). Here $n$ is the refractive index — light travels at $c/n$, $c$ its speed in vacuum — and $\varepsilon_0$ the vacuum permittivity, a constant; this $\varepsilon$ is not the small $\varepsilon$ of earlier slides.
$$n(\omega)^2 = \varepsilon(\omega) = 1 + \frac{Nq^2}{\varepsilon_0m}\,\chi(\omega) .$$$\varepsilon - 1$ is a causal response, so Kramers–Kronig applies to it.
Sellmeier is Kramers–Kronig with each absorption line squeezed to a delta function — the undamped limit of the Sokhotski slide.
If $\operatorname{Im}\varepsilon = 0$ at every frequency, then $\operatorname{Re}\varepsilon = 1$ at every frequency. Proof: the first dispersion relation for $\varepsilon - 1$. $\square$ So transparent glass with $n\ne1$ in the visible must absorb somewhere else — and $n(0)^2 - 1 = \frac2\pi\int_0^\infty\frac{\operatorname{Im}\varepsilon}{\omega}\mathrm d\omega > 0$.
Its Sellmeier formula $n^2 = 1 + \sum_{i=1}^3\frac{B_i\lambda^2}{\lambda^2 - C_i}$ is three undamped oscillators, $\frac{B_i\lambda^2}{\lambda^2 - C_i} = \frac{B_i\omega_i^2}{\omega_i^2 - \omega^2}$ with $\omega_i = 2\pi c/\sqrt{C_i}$ ($\lambda = 2\pi c/\omega$ the vacuum wavelength).
The resonances sit at $\sqrt{C_i} = 77.5$ nm, $141.5$ nm (ultraviolet) and $10.18\ \mu$m (infrared) — where glass is opaque.
20 · causality
From the maker's Sellmeier coefficients:
| blue, 486.1 nm | $n = 1.52238$ |
| yellow, 587.6 nm | $n = 1.51680$ |
| red, 656.3 nm | $n = 1.51432$ |
$n_\mathrm{blue} - n_\mathrm{red} = 0.00805$: blue bends more, so a prism fans white light out, blue deflected most.
Why that way round: the visible band lies between the ultraviolet and infrared resonances, on the rising flank of the ultraviolet ones. Below a resonance an oscillator's $\chi'$ is positive and grows as $\omega$ approaches it — the left flank of the galvanometer's curve two slides back — and $n$ grows with it: higher frequency, shorter $\lambda$, larger $n$.
$n(\lambda)$ for BK7 from its Sellmeier formula. Steep towards the ultraviolet resonances, nearly flat through the visible band (shaded), falling again towards the infrared one. The three dots are the table's blue, yellow and red lines.
20 · causality
for $f$ on $[0,\infty)$ with $|f|\le Ce^{\sigma t}$; it converges and is holomorphic on $\operatorname{Re}s > \sigma$. For real $c > \sigma$ — a number here, not the speed of light — it is the Fourier transform of $f(t)e^{-ct}H(t)$ at $\omega$, with $s = c - i\omega$.
For $c > \sigma$, at points where $f$ is continuous and when $F(c - i\omega)$ is integrable in $\omega$,
$$f(t) = \frac{1}{2\pi i}\int_{c - i\infty}^{c + i\infty}F(s)\,e^{st}\,\mathrm ds .$$Proof: Fourier inversion for $f(t)e^{-ct}H(t)$, then $s = c - i\omega$, $\mathrm ds = -i\,\mathrm d\omega$. $\square$
Why bother: it takes growing functions and initial data in its stride, $\mathcal L[\dot f] = sF - f(0)$, so it solves an initial value problem in one pass.
For the oscillator with data $x(0)$, $\dot x(0)$ and drive $u$, applying the rule twice:
$$(s^2 + \gamma s + \omega_0^2)X = U + (s + \gamma)x(0) + \dot x(0).$$The initial conditions arrive as a polynomial on the right, and the transient comes from it.
P9 uses it for the galvanometer's response to a switched-on current: the needle overshoots to $1.9244$ times its final deflection.
20 · causality
$\mathcal L[G](s) = \dfrac{1}{s^2 + \gamma s + \omega_0^2}$, poles $s = -\gamma/2\pm i\omega_\mathrm d$ — in the left half-plane — and $\chi(\omega) = \mathcal L[G](-i\omega)$: the same picture turned a quarter-turn.
The Bromwich line runs to the right of every singularity. For $t > 0$, $e^{st}$ decays to the left: close left, collect the poles. For $t < 0$ close right: nothing there, $f = 0$. Causality, once more.
With $s = -i\omega$ the $s$-plane is the $\omega$-plane rotated: the $\omega$-plane's lower half-plane is the left half here, and the real $\omega$-axis is the imaginary $s$-axis.
The galvanometer in the $s$-plane: poles at $-0.2\pm7.9975i$ (drawn further left than to scale), the Bromwich line to their right, and the closure to the left that collects them for $t > 0$. For $t < 0$, $e^{st}$ decays to the right, where there is nothing.
section 6
When an integral has no closed form, find the one small region that decides it — moving the contour until there is one.
20 · asymptotics
Notation (unit 21 develops it): $f = O(g)$ if $|f|\le C|g|$ eventually; $f\sim g$ if $f/g\to1$; and $f(\lambda)\sim\sum a_n\varphi_n(\lambda)$, an asymptotic expansion, if for every $N$ the error after $N$ terms is $O(\varphi_N)$ — convergent or not.
The Gamma function: $\Gamma(\alpha) = \int_0^\infty t^{\alpha-1}e^{-t}\mathrm dt$ for $\alpha>0$; $\Gamma(n+1) = n!$ by parts, $\Gamma(\frac12) = \sqrt\pi$ by $t = u^2$.
If $|g(t)|\le Ce^{bt}$ and $g(t)\sim\sum_{n\ge0}a_nt^{\alpha_n}$ as $t\to0^+$, with $-1 < \alpha_0 < \alpha_1 < \dots\to\infty$, then as $\lambda\to+\infty$
$$\int_0^\infty g(t)e^{-\lambda t}\,\mathrm dt\sim\sum_{n\ge0}\frac{a_n\,\Gamma(\alpha_n+1)}{\lambda^{\alpha_n+1}} .$$Only $t\lesssim1/\lambda$ matters: expand $g$ there, integrate term by term to $\infty$.
From the ODE, $G$ $= t - \frac\gamma2t^2 + \frac{\gamma^2 - \omega_0^2}{6}t^3 + \dots$ near $0^+$ ($G(0) = 0$, $\dot G = 1$, $\ddot G = -\gamma$). Watson:
$$\mathcal L[G](s)\sim\frac1{s^2} - \frac{\gamma}{s^3} + \frac{\gamma^2 - \omega_0^2}{s^4} .$$Directly, $1/(s^2 + \gamma s + \omega_0^2)$ expands in powers of $1/s$ to the same thing ✓ — and that Laurent series converges for $|s| > \omega_0$, so the expansion holds on the imaginary axis too. With $s = -i\omega$:
$$\chi(\omega) = -\frac{1}{\omega^2} + \frac{i\gamma}{\omega^3} + O(\omega^{-4}) .$$A free mass, $\ddot x = f$, is $-1/\omega^2$: at high frequency every oscillator is pure inertia, and the coefficient is the jump $\dot G(0^+) = 1$ — the sum rule's constant.
20 · asymptotics
Let $h$ be $C^2$ on $[a,b]$ with a unique maximum at an interior $t_0$, $h''(t_0) < 0$, and $g$ continuous with $g(t_0)\ne0$. Then as $\lambda\to\infty$
$$\int_a^bg(t)e^{\lambda h(t)}\,\mathrm dt\sim g(t_0)\,e^{\lambda h(t_0)}\sqrt{\frac{2\pi}{\lambda|h''(t_0)|}} .$$Why. $e^{\lambda h}$ is a spike of height $e^{\lambda h(t_0)}$ and width $\sim(\lambda|h''|)^{-1/2}$; inside the spike $h\approx h(t_0) - \frac12|h''|(t - t_0)^2$ and $g\approx g(t_0)$, and the Gaussian integral does the rest. Everything outside is exponentially smaller. Full proof in the notes.
Dimensions: with $t$ a time, $\lambda h$ dimensionless, $\sqrt{1/\lambda|h''|}$ is a time, and both sides carry $[g]\,\mathrm T$ ✓.
The spike, for $h(u) = \ln u - u$ (the next slide's integrand), scaled to height $1$. As $n$ grows it narrows like $n^{-1/2}$ and becomes the Gaussian that Laplace's method integrates (dashed): only the neighbourhood of the maximum survives.
20 · asymptotics
$n! = \Gamma(n+1) = \int_0^\infty t^ne^{-t}\mathrm dt$. Put $t = nu$:
$$n! = n^{n+1}\int_0^\infty e^{n(\ln u - u)}\,\mathrm du .$$$h(u) = \ln u - u$: maximum at $u = 1$, $h(1) = -1$, $h''(1) = -1$. So
$$n!\sim n^{n+1}e^{-n}\sqrt{\frac{2\pi}{n}} = \sqrt{2\pi n}\,\Big(\frac ne\Big)^n .$$Check at $n = 10$: $3\,598\,695.6$ against $10! = 3\,628\,800$, low by $0.83\%$. The next term multiplies by $1 + \frac1{12n}$ and gives $3\,628\,684.7$, low by $3\times10^{-5}$.
Real integrand, real maximum. Stationary phase and steepest descent are what to do when the exponent is imaginary, or when there is no real maximum at all.
The relative error of Stirling's formula against $n$, computed. The leading form errs by about $1/12n$ (slope $-1$); with the factor $1 + \frac1{12n}$ the error drops to about $1/288n^2$ (slope $-2$). Asymptotic, and good from the start.
20 · asymptotics
Let $g, \psi$ be smooth and real-valued ($\psi$) on $[a,b]$, with $\psi'\ne0$ except at one interior $t_0$, where $\psi''(t_0)\ne0$. Then
$$\begin{aligned}\int_a^bg\,e^{i\lambda\psi}\mathrm dt ={}& g(t_0)\sqrt{\frac{2\pi}{\lambda|\psi''(t_0)|}}\,e^{i\lambda\psi(t_0)\pm i\pi/4}\\ &+ O(1/\lambda),\end{aligned}$$the sign being that of $\psi''(t_0)$.
Where $\psi'\ne0$ the integral is $O(1/\lambda)$, by one integration by parts:
$$\int ge^{i\lambda\psi} = \Big[\frac{ge^{i\lambda\psi}}{i\lambda\psi'}\Big] - \frac{1}{i\lambda}\!\int\!\Big(\frac{g}{\psi'}\Big)'e^{i\lambda\psi}.$$Near $t_0$ the phase stands still, the contributions stop cancelling, and a Fresnel integral — $\int e^{i\lambda u^2/2}\mathrm du = \sqrt{2\pi/\lambda}\,e^{i\pi/4}$, problem P6 — gives the size.
Why the stationary point decides. Top: $\cos(\lambda t^2/2)$ oscillates ever faster away from $t = 0$, slowly in the shaded zone of width $\sim\lambda^{-1/2}$. Bottom: its running integral barely moves outside the zone and climbs to nearly the whole answer, $\sqrt{2\pi/\lambda}\cos\frac\pi4$ (dashed), inside it.
20 · asymptotics
Bessel's integral $J_n(x) = \frac1{2\pi}\int_{-\pi}^{\pi}e^{i(n\theta - x\sin\theta)}\mathrm d\theta$ has phase $-\sin\theta$, stationary at $\theta = \pm\frac\pi2$ with $\psi'' = \pm1$. Two contributions, complex conjugates (P11):
$$J_n(x)\approx\sqrt{\frac{2}{\pi x}}\cos\Big(x - \frac{n\pi}{2} - \frac\pi4\Big).$$$J_0(10) = -0.245936$ against $-0.246761$; $J_0(20) = 0.167025$ against $0.166656$ ✓.
Physics: in a superposition of waves, what survives at large distance or time is the part whose phase is stationary — Kelvin's argument (1887) for the V of a ship's wake, and the wave-packet slide's argument for group velocity.
$J_0$ (solid, computed) against the stationary-phase form (dashed). Useless near $x = 0$, where it diverges; by $x = 5$ the two are hard to tell apart. The dots are the slide's checks at $x = 10$ and $20$.
20 · asymptotics
For $I(\lambda) = \int_Cg(z)e^{\lambda\varphi(z)}\mathrm dz$ with $g, \varphi$ holomorphic, Cauchy lets you move $C$, paying for any arcs by estimates. Where to?
$|e^{\lambda\varphi}| = e^{\lambda\operatorname{Re}\varphi}$ has no local maximum (maximum modulus). The best available is a saddle, $\varphi'(z_0) = 0$. Through it, the curve on which $\operatorname{Im}\varphi = \operatorname{Im}\varphi(z_0)$ is the path of steepest descent: along it there is no oscillation and $\operatorname{Re}\varphi$ falls as fast as possible.
On that path the integral is a Laplace integral, and
$$I(\lambda)\sim g(z_0)\,e^{\lambda\varphi(z_0)}\sqrt{\frac{2\pi}{-\lambda\varphi''(z_0)}},$$the root's branch set by the direction in which the path crosses $z_0$.
Why the level curves of $\operatorname{Im}\varphi$. With $\varphi = u + iv$, Cauchy–Riemann makes the vectors of partials orthogonal: $u_xv_x + u_yv_y = u_xv_x - v_xu_x = 0$. So a level curve of $v$ runs along the direction of fastest change of $u$. Near $z_0$, $\varphi\approx\varphi(z_0) + \frac12\varphi''(z_0)(z - z_0)^2$, and the descent direction $e^{i\theta}$ makes $\varphi''(z_0)e^{2i\theta}$ negative real.
Laplace: real saddle, real path. Stationary phase: saddle on the real axis, path crossing it at $45^\circ$ — the $e^{\pm i\pi/4}$. Genuinely complex saddles: exponentially small answers that real methods see only as "$O(\lambda^{-N})$ for all $N$".
The saddle is two lines. The proof is the arc estimates that justify the move — the checkpoint's second clause.
20 · asymptotics · example
Step 1 — real methods fail. The phase $t^3/3 + t$ has derivative $t^2 + 1 > 0$: no stationary point. Integrating by parts repeatedly shows only $I = O(\lambda^{-N})$ for every $N$.
Step 2 — the saddles. $\varphi(z) = i(z^3/3 + z)$, $\varphi' = i(z^2 + 1) = 0$ at $z = \pm i$, with $\varphi(i) = i(-\frac i3 + i) = -\frac23$ and $\varphi(-i) = +\frac23$. Go up to $z = i$, where the integrand is small.
Step 3 — the arcs. Rectangle $-R, R, R+i, -R+i$; the integrand is entire. On the side $z = \pm R + iy$, $0\le y\le1$:
$$\operatorname{Re}\,\lambda\varphi = \lambda\big(-R^2y + \tfrac{y^3}3 - y\big)\le-\lambda R^2y,$$so each side is at most $\int_0^1e^{-\lambda R^2y}\mathrm dy\le\frac{1}{\lambda R^2}\to0$.
The landscape of $\operatorname{Re}\varphi$, $\varphi = i(z^3/3 + z)$: level curves cross at the saddles $\pm i$. The real-axis contour is moved up through $i$ to $z = s + i$, the short sides vanishing as $R\to\infty$. Above the axis the integrand is small; below, near $-i$, it is huge.
20 · asymptotics · example
Step 4 — on the line through the saddle, $z = s + i$: expanding, $i\big(\frac{(s+i)^3}3 + s + i\big) = -\frac23 - s^2 + \frac{is^3}{3}$. So, exactly,
$$I(\lambda) = e^{-2\lambda/3}\!\int e^{-\lambda s^2}\cos\tfrac{\lambda s^3}3\,\mathrm ds .$$No cancellation left: a Gaussian times a slowly turning phase.
Step 5 — Laplace. $\cos x = 1 - \frac{x^2}2 + O(x^4)$ and $\int s^6e^{-\lambda s^2} = \frac{15}{8}\sqrt\pi\,\lambda^{-7/2}$:
$$I = \sqrt{\frac\pi\lambda}\,e^{-2\lambda/3}\Big(1 - \frac{5}{48\lambda} + O(\lambda^{-2})\Big).$$Check at $\lambda = 5$: quadrature gives $0.0277624$; one term $0.0282775$ ($+1.9\%$); two terms $0.0276884$ ($-0.27\%$) ✓. Limit: exponentially small, consistent with Step 1.
The same integral, before and after the move, at $\lambda = 5$. On the real axis the integrand swings between $\pm1$ for ever and cancels down to $0.0278$. On the line through the saddle it is one positive bump of height $e^{-2\lambda/3} = 0.036$: nothing left to cancel.
20 · asymptotics
A wave in a dispersive medium obeys a dispersion relation $\omega = \omega(k)$, and a packet is a superposition
$$u(x,t) = \frac1{2\pi}\int A(k)\,e^{i(kx - \omega(k)t)}\,\mathrm dk .$$Each component's crests move at the phase velocity $v_\mathrm p = \omega/k$. Where is the packet?
Look along $x = vt$ as $t\to\infty$: the phase is $t\,(kv - \omega(k))$, stationary where $\omega'(k) = v$. So
$$u(vt, t)\approx\frac{A(k_*)\,e^{it(k_*v - \omega(k_*))\mp i\pi/4}}{\sqrt{2\pi t|\omega''(k_*)|}},$$where $\omega'(k_*) = v$.
If $A$ is concentrated near $k_0$, $u$ is small unless $x/t\approx\omega'(k_0)$: the packet moves at $v_\mathrm g = \mathrm d\omega/\mathrm dk$, and decays like $t^{-1/2}$ — it spreads.
In glass $k = n(\omega)\omega/c$, so $1/v_\mathrm g = \mathrm dk/\mathrm d\omega$ gives $v_\mathrm g = c/n_\mathrm g$ with the group index $n_\mathrm g = n - \lambda\frac{\mathrm dn}{\mathrm d\lambda}$. From the Sellmeier formula:
$n = 1.51680$, $v_\mathrm p = 0.65928\,c$;
$n_\mathrm g = 1.54136$, $v_\mathrm g = 0.64878\,c$.
A pulse travels $1.6\%$ slower than its own crests; the crests slide forward through it. Normal dispersion, $\mathrm dn/\mathrm d\lambda < 0$, is what makes $n_\mathrm g > n$.
Checks. No dispersion, $n$ constant: $n_\mathrm g = n$, $v_\mathrm g = v_\mathrm p$ ✓. Dimensions: $\mathrm d\omega/\mathrm dk$ is a speed ✓.
20 · asymptotics
Take a Gaussian packet, $A(k) = e^{-\sigma_0^2(k - k_0)^2/2}$, and expand the dispersion relation to second order: $\omega\approx\omega_0 + v_\mathrm g q + \frac12\beta q^2$, $q = k - k_0$. Then
$$u = \frac{e^{i(k_0x - \omega_0t)}}{2\pi}\int e^{-aq^2/2 + iq(x - v_\mathrm gt)}\,\mathrm dq,$$a Gaussian integral with complex width $a = \sigma_0^2 + i\beta t$, $\operatorname{Re}a > 0$: by analytic continuation it is $\sqrt{2\pi/a}\,e^{-(x - v_\mathrm gt)^2/2a}$. Taking the modulus:
A Gaussian packet at $\beta t/\sigma_0^2 = 0$, $1$, $2.5$, moving at $v_\mathrm g$: thick, $|u|$; thin, $\operatorname{Re}u$. The envelope widens as $\sigma(t)$ and its height falls as $\sigma(t)^{-1/2}$; the carrier is squeezed at one end and stretched at the other — the chirp. Parameters chosen to be visible, not physical.
Checks. $\beta = 0$: no spreading ✓. Late times $\sigma\approx|\beta|t/\sigma_0$: the narrower the packet, the faster it spreads — the uncertainty relation, moving. $[\beta] = \mathrm L^2\mathrm T^{-1}$, so $\beta t/\sigma_0^2$ is a number ✓.
20 · asymptotics
In time rather than space: $k(\omega)\approx k_0 + (\omega - \omega_0)/v_\mathrm g + \frac12k''(\omega - \omega_0)^2$, and the same algebra gives a duration $\tau(z) = \tau_0\sqrt{1 + (k''z/\tau_0^2)^2}$.
BK7 at 800 nm: $k'' = 44.65\ \mathrm{fs^2\,mm^{-1}}$ from the Sellmeier formula. A pulse of intensity full width $10$ fs has $\tau_0 = 6.006$ fs; after $z = 10$ mm, $k''z = 446.5\ \mathrm{fs^2}$ and
$$\tau/\tau_0 = 12.42:\quad10\ \mathrm{fs}\to124\ \mathrm{fs}.$$A centimetre of ordinary glass stretches the pulse twelvefold. Ultrafast optics spends much of its ingenuity undoing exactly this.
The pulse's intensity before and after $1$ cm of BK7, from the formula. Twelve times longer and twelve times lower, the same area: the energy is all still there, spread over $124$ fs. The dashed curve is the output magnified tenfold.
20 · summary
1 $\chi = \hat G$. 2 $LG = \delta$. 3 Two poles on $|\omega| = \omega_0$; the Taylor series dies at resonance. 4 Residues $\mp e^{-i\omega_\pm t}/2\omega_\mathrm d$. 5 Close up: $G = 0$ for $t < 0$; close down: unit 06's $G$; Kramers–Kronig to seven digits. 6 $\chi\sim-1/\omega^2$: inertia, and the sum rule.
| unit | what it takes from here |
|---|---|
| 24 | The wave operator's retarded Green's function in three dimensions, by residues, with the $i0$ prescription made explicit; its two-dimensional cousin, which has a tail. |
| 38 | Gravitational waves, radiated through that same retarded Green's function. |
1. A linear time-invariant system is one function of frequency, and its poles are its free modes.
2. Causality is holomorphy in a half-plane: it decides which way a contour closes, which Green's function is physical, and why dispersion and absorption come together.
3. An integral is decided by its critical points — the maximum, the stationary point, the saddle — once the contour has been moved to where there is no cancellation left.
20 · checkpoint
On paper and without notes, you can:
A Green's function nonzero before the kick; a contour closed where the exponential grows; an arc dropped without a bound; the wrong saddle or a lost $e^{i\pi/4}$; a Laplace limit asserted, not proved.
21 divergent series · 24 Maxwell, where this contour is closed in four dimensions.