Mathematics · Book 4 · Bachelor Year 2

University Mathematics — Year 2

University Mathematics — Year 2 · Bachelor Year 2

16Differential Equations

Year 1 solved the linear equations that admit formulas. This chapter supplies what formulas cannot: the Cauchy–Lipschitz theorem — existence and uniqueness for y=f(t,y)y' = f(t, y) — proved with the Banach fixed point theorem, exactly as promised in Chapter 4; then the complete theory of linear systems X=A(t)X+B(t)X' = A(t)X + B(t), with the matrix exponential and the wronskian as computational engines.

16.1 The Cauchy–Lipschitz theorem

Theorem 16.1 (Cauchy–Lipschitz, global Lipschitz version)

Let II be a segment, f ⁣:I×RnRnf \colon I \times \R^n \to \R^n continuous and Lipschitz in the second variable, uniformly in the first: f(t,y)f(t,z)kyz\norm{f(t, y) - f(t, z)} \leq k\,\norm{y - z} for all tIt \in I. Then for every (t0,y0)I×Rn(t_0, y_0) \in I \times \R^n, the Cauchy problem

y=f(t,y),y(t0)=y0y' = f(t, y), \qquad y(t_0) = y_0

has exactly one solution y ⁣:IRny \colon I \to \R^n of class C1C^1.

Proof. Reformulation. A continuous yy solves the problem iff it satisfies the integral equation

y(t)=y0+t0tf(s,y(s)) ⁣ds=:T(y)(t)y(t) = y_0 + \int_{t_0}^{t} f\bigl(s, y(s)\bigr)\,\dd s =: T(y)(t)

(fundamental theorem of calculus both ways; a continuous solution of the integral equation is automatically C1C^1).

A contraction, after re-norming. On the Banach space E=C(I,Rn)E = C(I, \R^n) with the weighted norm

N(y)=suptI  e2ktt0y(t),N(y) = \sup_{t \in I}\; \eu^{-2k\abs{t - t_0}}\,\norm{y(t)} ,

(equivalent to the sup norm: the weight is bounded above and below on the segment II, so EE stays complete), estimate for y,zEy, z \in E and, say, tt0t \geq t_0:

T(y)(t)T(z)(t)t0tky(s)z(s) ⁣dskN(yz)t0te2k(st0) ⁣dsN(yz)2e2k(tt0).\norm{T(y)(t) - T(z)(t)} \leq \int_{t_0}^{t} k\,\norm{y(s) - z(s)}\,\dd s \leq k\,N(y - z)\int_{t_0}^{t} \eu^{2k(s - t_0)}\dd s \leq \frac{N(y-z)}{2}\,\eu^{2k(t - t_0)} .

Multiplying by e2k(tt0)\eu^{-2k(t - t_0)} and taking the sup (the case t<t0t < t_0 is symmetric): N(T(y)T(z))12N(yz)N\bigl(T(y) - T(z)\bigr) \leq \frac12 N(y - z): TT is a 12\frac12-contraction of the complete (E,N)(E, N). The Banach fixed point theorem (Theorem 4.12) yields a unique fixed point: the unique solution.

Remark 16.2

For ff merely C1C^1 (locally Lipschitz), the theorem holds locally, with a maximal solution on a maximal open interval; solutions can explode in finite time (y=y2y' = y^2, y(0)=1y(0) = 1: y(t)=11ty(t) = \frac{1}{1-t}, gone at t=1t = 1). The global Lipschitz hypothesis is what buys the whole segment. Two consequences worth engraving: solution curves of an ODE with Lipschitz field never cross; and the zero function is the only solution vanishing anywhere of a linear homogeneous equation.

Example 16.3 (Uniqueness is a theorem: a field that leaks)

Consider y=2yy' = 2\sqrt{\abs y} with y(0)=0y(0) = 0. The zero function solves it; so does

y(t)={0t0,t2t0,y(t) = \begin{cases} 0 & t \leq 0,\\ t^2 & t \geq 0, \end{cases}

which is C1C^1 (both pieces have derivative 00 at the glue point) and satisfies y(t)=2t=2t2y'(t) = 2t = 2\sqrt{t^2} for t>0t > 0 — indeed, delaying the take-off gives a solution for every release time c0c \geq 0: infinitely many solutions through the same initial data. No contradiction with Theorem 16.1: near y=0y = 0,

2y2zyz=2y+z+,\frac{\abs{2\sqrt y - 2\sqrt z}}{\abs{y - z}} = \frac{2}{\sqrt y + \sqrt z} \longrightarrow +\infty ,

the field is not Lipschitz in yy, and the theorem is silent. Closing insight: the physical reading is a bucket draining under gravity run backwards — from the empty state, one cannot tell when it started filling; determinism of ODEs is exactly the Lipschitz condition, not a law of nature.

16.2 Linear systems

Theorem 16.4 (Structure of linear systems)

Let A ⁣:IMn(R)A \colon I \to \mathcal{M}_n(\R) and B ⁣:IRnB \colon I \to \R^n be continuous on an interval II. For every (t0,X0)(t_0, X_0) the problem

X=A(t)X+B(t),X(t0)=X0X' = A(t)X + B(t), \qquad X(t_0) = X_0

has exactly one solution on all of II. The solutions of the homogeneous system (B=0B = 0) form a vector space SH\mathcal{S}_H of dimension exactly nn, and evaluation XX(t0)X \mapsto X(t_0) is an isomorphism SHRn\mathcal{S}_H \to \R^n; general solution == particular ++ homogeneous.

Proof. On every segment JIJ \subseteq I containing t0t_0: f(t,X)=A(t)X+B(t)f(t, X) = A(t)X + B(t) is continuous, and Lipschitz in XX with constant k=supJA(t)k = \sup_J \vertiii{A(t)} (finite: continuous on a segment): Theorem 16.1 applies on JJ; letting JJ exhaust II, uniqueness glues the solutions into one on II. Linearity of the solution set and of the evaluation map are clear; evaluation is bijective by existence (surjective) and uniqueness (injective): dimSH=n\dim \mathcal{S}_H = n. The affine structure is Year 1’s argument verbatim.

Example 16.5 (The evaluation isomorphism, concretely)

For y+y=0y'' + y = 0, viewed as the system X=(0110)XX' = \begin{pmatrix} 0 & 1\\ -1 & 0\end{pmatrix}X with X=(y,y)X = (y, y'): the theorem says the solution space is a plane, and that XX(0)=(y(0),y(0))X \mapsto X(0) = (y(0), y'(0)) is an isomorphism onto R2\R^2. The solutions cos\cos and sin\sin evaluate to (1,0)(1, 0) and (0,1)(0, 1) — the canonical basis of R2\R^2 — so they form a basis of the solution space, and every solution is

y(t)=y(0)cost+y(0)sint,y(t) = y(0)\cos t + y'(0)\sin t ,

with the coefficients read directly off the initial data, no linear system to solve. Closing insight: choosing the fundamental system whose initial values are the canonical basis (here cos,sin\cos, \sin) is exactly choosing the columns of etA\eu^{tA}; the evaluation isomorphism is why initial conditions parametrize trajectories — the geometric content of “deterministic dynamics” for linear equations.

Definition 16.6 (Wronskian)

For solutions X1,,XnX_1, \dots, X_n of the homogeneous system, the wronskian is W(t)=det(X1(t),,Xn(t))W(t) = \det\bigl(X_1(t), \dots, X_n(t)\bigr). By the isomorphism above, either WW vanishes identically (the family is linked) or never (a fundamental system); quantitatively, W=tr(A(t))WW' = \operatorname{tr}\bigl(A(t)\bigr) W, so

W(t)=W(t0)exp(t0ttrA(s) ⁣ds)(Liouville’s formula).W(t) = W(t_0)\,\exp\Bigl(\int_{t_0}^{t} \operatorname{tr} A(s)\,\dd s\Bigr) \quad \text{(Liouville's formula)}.

Example 16.7 (Liouville checked on an Euler equation)

On (0,)\intoo{0}{\infty}, the equation t2y+tyy=0t^2y'' + ty' - y = 0 has the solutions y1(t)=ty_1(t) = t and y2(t)=1ty_2(t) = \frac1t (substitute). Their wronskian:

W(t)=det(t1t11t2)=1t1t=2t,W(t) = \det\begin{pmatrix} t & \tfrac1t\\[2pt] 1 & -\tfrac{1}{t^2}\end{pmatrix} = -\frac1t - \frac1t = -\frac2t ,

never zero: a fundamental system. Now check Liouville: in normalized form y+1ty1t2y=0y'' + \frac1t\,y' - \frac{1}{t^2}\,y = 0, the companion matrix A(t)=(011t21t)A(t) = \begin{pmatrix} 0 & 1\\ \frac{1}{t^2} & -\frac1t\end{pmatrix} has trace 1t-\frac1t, so

W(t)=W(1)exp(1t ⁣dss)=2elnt=2t.W(t) = W(1)\exp\Bigl(-\int_1^t\frac{\dd s}{s}\Bigr) = -2\,\eu^{-\ln t} = -\frac2t . \checkmark

Closing insight: Liouville predicts the shape of the wronskian before any solution is known — here, that WW must be ct\frac{c}{t}; this is what powers the reduction-of-order method (Proposition 16.15), where knowing y1y_1 and the wronskian’s form determines y2y_2 by one quadrature.

Proof of Liouville’s formula. W(t)=detM(t)W(t) = \det M(t) with M=AMM' = AM. Differentiating the determinant as a multilinear function of the columns,

W(t)=jdet(X1,,Xj,,Xn)=jdet(X1,,AXj,,Xn).W'(t) = \sum_j \det(X_1, \dots, X_j', \dots, X_n) = \sum_j \det(X_1, \dots, AX_j, \dots, X_n) .

Now the map (C1,,Cn)jdet(C1,,ACj,,Cn)(C_1, \dots, C_n) \mapsto \sum_j \det(C_1, \dots, AC_j, \dots, C_n) is nn-linear and alternating (with two equal columns Ci=CkC_i = C_k, the terms j{i,k}j \notin \{i, k\} vanish outright, and the terms j=ij = i and j=kj = k cancel in pairs after one column swap): by the uniqueness theorem (Theorem 2.14) it is cdetc \cdot \det, with cc read on the canonical columns: c=jdet(e1,,Aej,,en)=jajj=trAc = \sum_j \det(e_1, \dots, Ae_j, \dots, e_n) = \sum_j a_{jj} = \operatorname{tr} A. Hence W=tr(A(t))WW' = \operatorname{tr}\bigl(A(t)\bigr)W: a scalar linear ODE, solved by the Year 1 formula.

16.3 Constant coefficients: the matrix exponential

Theorem 16.8

For AMn(R)A \in \mathcal{M}_n(\R) (or C\C), the exponential etA=k(tA)kk!\eu^{tA} = \sum_k \frac{(tA)^k}{k!} (Example 5.22) satisfies: tetAt \mapsto \eu^{tA} is C1C^1 (indeed CC^\infty) with

 ⁣d ⁣dtetA=AetA=etAA,e(s+t)A=esAetA,(eA)1=eA;\frac{\dd}{\dd t}\,\eu^{tA} = A\,\eu^{tA} = \eu^{tA}A , \qquad \eu^{(s+t)A} = \eu^{sA}\,\eu^{tA}, \qquad (\eu^{A})^{-1} = \eu^{-A} ;

and eA+B=eAeB\eu^{A + B} = \eu^A\eu^B when AB=BAAB = BA. The Cauchy problem X=AXX' = AX, X(0)=X0X(0) = X_0 has the unique solution X(t)=etAX0X(t) = \eu^{tA}X_0; with a source, the variation of constants formula holds:

X(t)=e(tt0)AX0+t0te(ts)AB(s) ⁣ds.X(t) = \eu^{(t - t_0)A}X_0 + \int_{t_0}^{t} \eu^{(t-s)A}B(s)\,\dd s .

Proof. Differentiability: the series tkAkk!\sum \frac{t^kA^k}{k!} and its term-derived series tk1Ak(k1)!=A(tA)k1(k1)!\sum \frac{t^{k-1}A^k}{(k-1)!} = A\sum \frac{(tA)^{k-1}}{(k-1)!} converge normally on every segment (norms (tA)kk!\leq \frac{(\abs t\,\vertiii A)^k}{k!}): differentiate term by term (Theorem 10.11, vector-valued). The two orderings AetAA\eu^{tA} and etAA\eu^{tA}A agree since every partial sum commutes with AA.

Group law: for commuting A,BA, B, the Cauchy product of the two exponential series reorganizes by the binomial theorem exactly as in Example 7.15 (absolute convergence in the Banach algebra justifies it): eA+B=eAeB\eu^{A+B} = \eu^A\eu^B; with B=sAB = sA this gives the one-parameter group law, and B=AB = -A the inverse.

Cauchy problem: X(t)=etAX0X(t) = \eu^{tA}X_0 solves it (differentiate); uniqueness by Theorem 16.4. Variation of constants: set Y(t)=etAX(t)Y(t) = \eu^{-tA}X(t); differentiating, Y=etA(XAX)=etAB(t)Y' = \eu^{-tA}(X' - AX) = \eu^{-tA}B(t); integrate from t0t_0 to tt and multiply back by etA\eu^{tA}.

Method 16.9 (Computing etA\eu^{tA})

Reduce AA (Chapter 3): if A=PDP1A = PDP^{-1} diagonal, etA=PetDP1\eu^{tA} = P\,\eu^{tD}P^{-1} with etD\eu^{tD} diagonal of etλi\eu^{t\lambda_i}; in general use Dunford A=D+NA = D + N (commuting): etA=etDetN\eu^{tA} = \eu^{tD}\,\eu^{tN} with etN\eu^{tN} a polynomial in tt (nilpotence truncates the series). Complex eigenvalues pair into rotation-times-exponential blocks (Exercise 16.5).

Remark 16.10 (Common pitfalls)

(i) eA+BeAeB\eu^{A+B} \neq \eu^A\eu^B without commutation: take A=(0100)A = \begin{pmatrix} 0 & 1\\ 0 & 0\end{pmatrix}, B=(0010)B = \begin{pmatrix} 0 & 0\\ 1 & 0\end{pmatrix}. Then eA=I+A\eu^A = I + A, eB=I+B\eu^B = I + B (nilpotence), so

eAeB=(2111),whileeA+B=cosh(1)I+sinh(1)(A+B)=(cosh1sinh1sinh1cosh1),\eu^A\eu^B = \begin{pmatrix} 2 & 1\\ 1 & 1\end{pmatrix}, \qquad\text{while}\qquad \eu^{A+B} = \cosh(1)\,I + \sinh(1)\,(A + B) = \begin{pmatrix} \cosh 1 & \sinh 1\\ \sinh 1 & \cosh 1 \end{pmatrix},

using (A+B)2=I(A+B)^2 = I; and cosh11.542\cosh 1 \approx 1.54 \neq 2. The group law of Theorem 16.8 carries a genuine hypothesis. (ii) Nonlinear intuition on linear turf: solutions of a linear system with continuous coefficients live on the whole interval (Theorem 16.4) — if a candidate solution explodes inside II, the equation was not linear or the computation is wrong; conversely, for nonlinear equations never promise globality without an argument (y=y2y' = y^2). (iii) Dividing by the unknown: separating variables in y=y(1y)y' = y(1-y) silently discards the constant solutions 00 and 11 — exactly the ones that organize the phase line (Exercise 16.3); list constant solutions first. (iv) Initial data fix vectors, not scalars: an nn-th order scalar equation needs nn conditions (y,y,y, y', \dots at t0t_0); matching only y(t0)y(t_0) leaves an (n1)(n-1)-parameter family, a classic source of “lost” constants.

Example 16.11 (A 3×33\times3 exponential by Dunford)

Solve X=AXX' = AX for A=(210020003)A = \begin{pmatrix} 2 & 1 & 0\\ 0 & 2 & 0\\ 0 & 0 & 3\end{pmatrix}. Dunford by blocks: A=D+NA = D + N with D=diag(2,2,3)D = \operatorname{diag}(2, 2, 3) and N=E12N = E_{12}, which commute (NN lives inside the eigenvalue-22 block), and N2=0N^2 = 0:

etA=etDetN=(e2tte2t00e2t000e3t).\eu^{tA} = \eu^{tD}\,\eu^{tN} = \begin{pmatrix} \eu^{2t} & t\,\eu^{2t} & 0\\ 0 & \eu^{2t} & 0\\ 0 & 0 & \eu^{3t} \end{pmatrix} .

The general solution reads off column by column: X(t)=(e2t(x0+ty0), e2ty0, e3tz0)X(t) = \bigl(\eu^{2t}(x_0 + ty_0),\ \eu^{2t}y_0,\ \eu^{3t}z_0\bigr). Sanity checks: at t=0t = 0 the matrix is II; its determinant is e7t=ettrA\eu^{7t} = \eu^{t\operatorname{tr}A}, as Liouville demands; and the factor tt appears exactly where the eigenvalue 22 is defective. Closing insight: polynomials times exponentials are not a guess to be memorized — they are the truncated series etN\eu^{tN}, and their degree is bounded by the nilpotency index, never more.

Method 16.12 (Solving X=AX+B(t)X' = AX + B(t), start to finish)

  1. Spectrum of AA; then etA\eu^{tA} by Method 16.9 (diagonalize; or Dunford as in Example 16.11; or a polynomial trick like A2=IA^2 = -I).
  2. A particular solution: variation of constants t0te(ts)AB(s) ⁣ds\int_{t_0}^t\eu^{(t-s)A}B(s)\dd s always works; for exponential-polynomial BB, an ansatz of the same shape (degree raised on resonance, Exercise 16.10) is faster.
  3. General solution =e(tt0)AX0+= \eu^{(t-t_0)A}X_0 + particular; fit the initial data last, on the complete formula.
  4. Sanity checks: X(t0)X(t_0) correct; the homogeneous part’s growth matches the eigenvalue real parts (Exercise 16.8); and det\det of a fundamental matrix obeys Liouville.

Example 16.13 (A phase portrait)

X=AXX' = AX with A=(0110)A = \begin{pmatrix} 0 & 1\\ -1 & 0\end{pmatrix}: A2=IA^2 = -I, so the series splits into

etA=(cost)I+(sint)A=(costsintsintcost):\eu^{tA} = (\cos t)\,I + (\sin t)\,A = \begin{pmatrix} \cos t & \sin t\\ -\sin t & \cos t \end{pmatrix} :

trajectories are circles run clockwise — the harmonic oscillator x+x=0x'' + x = 0 in first-order clothes. Eigenvalues ±i\pm\iu on the imaginary axis: a center. More generally the real parts of the eigenvalues of AA decide growth or decay of X(t)\norm{X(t)} (Exercise 16.8).

Two linear phase portraits. Left: a center (eigenvalues ±) — closed circular orbits of the harmonic oscillator. Right: a stable node (eigenvalues -1, -2) — all trajectories fall into the origin tangentially to the slow eigendirection. Two linear phase portraits. Left: a center (eigenvalues ±) — closed circular orbits of the harmonic oscillator. Right: a stable node (eigenvalues -1, -2) — all trajectories fall into the origin tangentially to the slow eigendirection.
Two linear phase portraits. Left: a center (eigenvalues ±i\pm\iu) — closed circular orbits of the harmonic oscillator. Right: a stable node (eigenvalues 1,2-1, -2) — all trajectories fall into the origin tangentially to the slow eigendirection.
The trace–determinant plane for X' = AX in dimension 2: below the horizontal axis, saddles; between the axis and the parabola = 2/4, nodes; inside the parabola, spirals; on the positive -axis, centers. The weekend problem proves this classification and follows one vertical line of it — the damped oscillator — into resonance.
The trace–determinant plane for X=AXX' = AX in dimension 22: below the horizontal axis, saddles; between the axis and the parabola δ=τ2/4\delta = \tau^2/4, nodes; inside the parabola, spirals; on the positive δ\delta-axis, centers. The weekend problem proves this classification and follows one vertical line of it — the damped oscillator — into resonance.

Remark 16.14 (Where this is used)

Linear systems are the local model for everything nonlinear: near an equilibrium, a smooth vector field behaves (in the hyperbolic cases) like its linearization, whose portrait the trace–determinant plane classifies. The weekend problem works out the oscillator story in full — damping, forcing, resonance, and Sturm’s comparison theorems for variable coefficients — the mathematics behind shock absorbers, AC circuits, and spectral gaps alike. The Year 3 volume returns with the qualitative theory (flows, stability, first integrals) on manifolds.

16.4 Second order with variable coefficients

Proposition 16.15

The equation y+a(t)y+b(t)y=c(t)y'' + a(t)y' + b(t)y = c(t) (a,b,ca, b, c continuous on II) is the system X=A(t)X+B(t)X' = A(t)X + B(t) for X=(y,y)X = (y, y'): solutions exist and are unique on all of II for any initial data (y(t0),y(t0))(y(t_0), y'(t_0)); homogeneous solutions form a plane. If one nonvanishing homogeneous solution y1y_1 is known, a second independent one is found by lowering the order: setting y=y1zy = y_1 z turns the homogeneous equation into a first-order equation for zz', solved by quadratures.

Proof. The system form and Theorem 16.4 give everything structural. Lowering: substituting y=y1zy = y_1z,

y1z+(2y1+ay1)z+(y1+ay1+by1)=0z=0:y_1 z'' + (2y_1' + a y_1)z' + \underbrace{(y_1'' + ay_1' + by_1)}_{=\,0}\,z = 0 :

a first-order linear equation in u=zu = z', solvable by the Year 1 formula; integrating uu gives zz, hence y2=y1zy_2 = y_1 z, independent of y1y_1 whenever zz is nonconstant.

Example 16.16

t2y2y=0t^2y'' - 2y = 0 on (0,)\intoo{0}{\infty}: y1=t2y_1 = t^2 is a solution. Substitute y=t2zy = t^2z: from y=t2z+2tzy' = t^2z' + 2tz and y=t2z+4tz+2zy'' = t^2z'' + 4tz' + 2z,

t2y2y=t4z+4t3z=0,i.e.zz=4t:t^2y'' - 2y = t^4 z'' + 4t^3z' = 0, \qquad\text{i.e.}\qquad \frac{z''}{z'} = -\frac4t :

z=t4z' = t^{-4} (up to a constant), z=13t3z = -\frac{1}{3t^3}, and y2=t2z=13ty_2 = t^2z = -\frac{1}{3t}. General solution: y=αt2+βty = \alpha t^2 + \frac{\beta}{t}.

16.5 Exercises

Exercise 16.1

Solve X=AXX' = AX, X(0)=(1,0)TX(0) = (1, 0)^{\mathsf T}, for A=(1102)A = \begin{pmatrix} 1 & 1\\ 0 & 2\end{pmatrix} (diagonalize) and A=(2102)A = \begin{pmatrix} 2 & 1\\ 0 & 2 \end{pmatrix} (Dunford).

Solution

Solution of Exercise 16.1.

First matrix: eigenvalues 1,21, 2, eigenvectors (1,0)(1,0) and (1,1)(1,1). Decompose X0=(1,0)=1(1,0)+0(1,1)X_0 = (1,0) = 1\cdot(1,0) + 0\cdot(1,1): the solution is

X(t)=et(10).X(t) = \eu^{t}\begin{pmatrix}1\\ 0\end{pmatrix} .

(The initial vector is itself an eigenvector.)

Second: A=2I+NA = 2I + N, N=E12N = E_{12}, N2=0N^2 = 0: etA=e2t(I+tN)\eu^{tA} = \eu^{2t}(I + tN), so

X(t)=e2t(1t01)(10)=e2t(10).X(t) = \eu^{2t}\begin{pmatrix} 1 & t\\ 0 & 1\end{pmatrix} \begin{pmatrix}1\\ 0\end{pmatrix} = \eu^{2t}\begin{pmatrix}1\\ 0\end{pmatrix}.

Exercise 16.2

Which Cauchy problems have unique global solutions on R\R by Theorem 16.1? y=sin(ty)y' = \sin(ty);   y=y2\;y' = y^2;   y=y\;y' = \abs y. For the last, solve explicitly with y(0)=0y(0) = 0 and y(0)=1y(0) = 1.

Solution

Solution of Exercise 16.2.

y=sin(ty)y' = \sin(ty): sin(ty)sin(tz)tyz\abs{\sin(ty) - \sin(tz)} \leq \abs t\,\abs{y - z}Lipschitz in yy uniformly on every segment of times: unique global solutions on R\R (apply the theorem on every segment).

y=y2y' = y^2: locally Lipschitz only; no global theorem, and indeed y(0)=1y(0) = 1 explodes at t=1t = 1.

y=yy' = \abs y: \abs\cdot is 11-Lipschitz: global existence and uniqueness. With y(0)=0y(0) = 0: y0y \equiv 0 (uniqueness!). With y(0)=1y(0) = 1: yy stays positive (cannot cross the zero solution), so y=yy' = y: y=ety = \eu^t.

Exercise 16.3

Prove that two distinct maximal solutions of y=f(t,y)y' = f(t,y) (ff Lipschitz in yy) never take the same value at the same time, and deduce that solutions of y=y(1y)y' = y(1 - y) starting in (0,1)\intoo{0}{1} remain in (0,1)\intoo{0}{1} forever.

Solution

Solution of Exercise 16.3.

If y(t1)=z(t1)y(t_1) = z(t_1) at some time, then yy and zz solve the same Cauchy problem at t1t_1: uniqueness forces y=zy = z on their common interval — distinct solutions never meet.

For y=y(1y)y' = y(1-y): the constants 00 and 11 are solutions. A solution starting in (0,1)\intoo{0}{1} can never reach 00 or 11 (it would collide with a constant solution): it stays in (0,1)\intoo{0}{1}, hence is global (bounded: no explosion — e.g. by Exercise 16.9’s criterion, or because the vector field is bounded on the trapped strip).

Exercise 16.4 ★★

Compute etA\eu^{tA} for A=(3111)A = \begin{pmatrix} 3 & 1\\ -1 & 1\end{pmatrix} (Dunford: (A2I)2=0(A - 2I)^2 = 0), and solve X=AX+(e2t0)X' = AX + \begin{pmatrix} \eu^{2t}\\ 0\end{pmatrix}, X(0)=0X(0) = 0, by variation of constants.

Solution

Solution of Exercise 16.4.

(A2I)2=(1111)2=0(A - 2I)^2 = \begin{pmatrix}1 & 1\\ -1 & -1\end{pmatrix}^2 = 0: Dunford with D=2ID = 2I, N=A2IN = A - 2I:

etA=e2t(I+tN)=e2t(1+ttt1t).\eu^{tA} = \eu^{2t}\,(I + tN) = \eu^{2t}\begin{pmatrix} 1 + t & t\\ -t & 1 - t\end{pmatrix}.

Variation of constants with B(s)=(e2s,0)TB(s) = (\eu^{2s}, 0)^{\mathsf T}:

X(t)=0te(ts)AB(s) ⁣ds=e2t0t(1+(ts)(ts)) ⁣ds=e2t(t+t22t22),X(t) = \int_0^t \eu^{(t-s)A}B(s)\,\dd s = \eu^{2t}\int_0^t \begin{pmatrix} 1 + (t-s)\\ -(t-s) \end{pmatrix}\dd s = \eu^{2t}\begin{pmatrix} t + \frac{t^2}{2}\\[2pt] -\frac{t^2}{2} \end{pmatrix},

using e(ts)AB(s)=e2(ts)(I+(ts)N)(e2s,0)T=e2t(1+(ts),(ts))T\eu^{(t-s)A}B(s) = \eu^{2(t-s)}(I + (t-s)N)\,(\eu^{2s}, 0)^{\mathsf T} = \eu^{2t}\bigl(1 + (t-s),\, -(t-s)\bigr)^{\mathsf T}. (Check: X(0)=0X(0) = 0; XAX=(e2t,0)TX' - AX = (\eu^{2t}, 0)^{\mathsf T} by differentiation.)

Exercise 16.5 ★★

For A=(αββα)A = \begin{pmatrix} \alpha & -\beta\\ \beta & \alpha\end{pmatrix}, prove etA=eαt(cosβtsinβtsinβtcosβt)\eu^{tA} = \eu^{\alpha t}\begin{pmatrix} \cos\beta t & -\sin\beta t\\ \sin\beta t & \cos\beta t\end{pmatrix} — spiral trajectories — two ways: via the series (write A=αI+βJA = \alpha I + \beta J, J2=IJ^2 = -I), and via the complex identification z=(α+iβ)zz' = (\alpha + \iu\beta)z.

Solution

Solution of Exercise 16.5.

Series: A=αI+βJA = \alpha I + \beta J with J=(0110)J = \begin{pmatrix}0 & -1\\ 1 & 0\end{pmatrix}, J2=IJ^2 = -I; the two summands commute, so etA=eαteβtJ\eu^{tA} = \eu^{\alpha t}\,\eu^{\beta tJ}, and the series of eβtJ\eu^{\beta t J} splits along even/odd powers into cos(βt)I+sin(βt)J\cos(\beta t)I + \sin(\beta t)J: the stated rotation-scaling matrix.

Complex: identify (x,y)R2(x, y) \in \R^2 with z=x+iyz = x + \iu y; the system X=AXX' = AX reads z=(α+iβ)zz' = (\alpha + \iu\beta)z, whose solution z(t)=eαteiβtz0z(t) = \eu^{\alpha t}\eu^{\iu\beta t}z_0 is exactly the spiral: modulus eαt\eu^{\alpha t}, argument advancing at speed β\beta.

Exercise 16.6 ★★

(Gronwall’s lemma) Let uu be continuous nonnegative with u(t)C+kt0tu(s) ⁣dsu(t) \leq C + k\int_{t_0}^{t} u(s)\,\dd s on [t0,T)\intco{t_0}{T}. Prove u(t)Cek(tt0)u(t) \leq C\,\eu^{k(t - t_0)} (differentiate v(t)=ektt0tuv(t) = \eu^{-kt}\int_{t_0}^t u). Deduce again the uniqueness in Cauchy–Lipschitz and the continuous dependence y(t)z(t)y0z0ektt0\norm{y(t) - z(t)} \leq \norm{y_0 - z_0}\,\eu^{k\abs{t - t_0}} for two solutions with different initial data.

Solution

Solution of Exercise 16.6.

Let v(t)=ek(tt0)t0tuv(t) = \eu^{-k(t - t_0)}\int_{t_0}^t u. Then

v(t)=ek(tt0)(u(t)kt0tu)Cek(tt0),v'(t) = \eu^{-k(t-t_0)}\Bigl(u(t) - k\int_{t_0}^t u\Bigr) \leq C\,\eu^{-k(t-t_0)},

by the hypothesis. Integrating from t0t_0 to tt (v(t0)=0v(t_0) = 0): v(t)Ck(1ek(tt0))v(t) \leq \frac{C}{k}\bigl(1 - \eu^{-k(t - t_0)}\bigr), i.e. kt0tuC(ek(tt0)1)k\int_{t_0}^t u \leq C\bigl(\eu^{k(t-t_0)} - 1\bigr); feeding this back into the hypothesis: u(t)Cek(tt0)u(t) \leq C\eu^{k(t-t_0)}.

Uniqueness/dependence: two solutions y,zy, z of the integral equation satisfy

y(t)z(t)y0z0+kt0tyz,\norm{y(t) - z(t)} \leq \norm{y_0 - z_0} + k\int_{t_0}^{t}\norm{y - z},

and Gronwall with C=y0z0C = \norm{y_0 - z_0} gives the exponential bound; C=0C = 0 gives uniqueness.

Exercise 16.7 ★★

Knowing that y1(t)=sintty_1(t) = \frac{\sin t}{t} solves ty+2y+ty=0ty'' + 2y' + ty = 0 on (0,π)\intoo{0}{\pi}, find a second independent solution by lowering the order, and give the general solution.

Solution

Solution of Exercise 16.7.

Substitute y=y1zy = y_1 z with y1=sintty_1 = \frac{\sin t}{t}: the general lowering formula (Proposition 16.15) gives, for u=zu = z',

y1u+(2y1+2ty1)u=0y_1 u' + \Bigl(2y_1' + \frac{2}{t}\,y_1\Bigr)u = 0

(the equation normalized as y+2ty+y=0y'' + \frac2t y' + y = 0). Compute 2y1+2ty1=2tcostsintt2+2sintt2=2costt2y_1' + \frac2t y_1 = 2\,\frac{t\cos t - \sin t}{t^2} + \frac{2\sin t}{t^2} = \frac{2\cos t}{t}: so

uu=2costttsint=2cottu=1sin2t(up to a constant),\frac{u'}{u} = -\frac{2\cos t}{t}\cdot\frac{t}{\sin t} = -2\cot t \quad\Longrightarrow\quad u = \frac{1}{\sin^2 t} \quad (\text{up to a constant}),

and z=cottz = -\cot t, giving y2=y1z=costty_2 = y_1 z = -\frac{\cos t}{t}. General solution on (0,π)\intoo{0}{\pi}:

y(t)=αsintt+βcostt.y(t) = \alpha\,\frac{\sin t}{t} + \beta\,\frac{\cos t}{t} .

(These are the spherical Bessel functions of order zero.)

Exercise 16.8 ★★★

Let AMn(C)A \in \mathcal{M}_n(\C) with all eigenvalues of (strictly) negative real part. Prove that every solution of X=AXX' = AX tends to 00 as t+t \to +\infty, with an exponential rate: X(t)Ceαt\norm{X(t)} \leq C\,\eu^{-\alpha t} for some α>0\alpha > 0. (Trigonalize; treat the triangular system from the last row up, or use Dunford: etA=etDetN\eu^{tA} = \eu^{tD}\eu^{tN} with etDeαt\norm{\eu^{tD}} \leq \eu^{-\alpha' t} and etN\eu^{tN} polynomial in tt.)

Solution

Solution of Exercise 16.8.

Dunford: A=D+NA = D + N commuting, DD diagonalizable with the same eigenvalues, NN nilpotent, so

etA=etDetN,etN=k<ntkNkk! (a matrix polynomial in t).\eu^{tA} = \eu^{tD}\,\eu^{tN}, \qquad \eu^{tN} = \sum_{k < n} \frac{t^kN^k}{k!} \ \text{(a matrix polynomial in } t).

Let 2α=maxiλi<0-2\alpha = \max_i \Re\lambda_i < 0. In a basis diagonalizing DD, etDe2αt\vertiii{\eu^{tD}} \leq \eu^{-2\alpha t} (entries etλi\eu^{t\lambda_i} of modulus etλi\eu^{t\Re\lambda_i}); norms in different bases differ by constants. Hence

X(t)etAX0Ce2αt(1+t)n1X0CeαtX0,\norm{X(t)} \leq \vertiii{\eu^{tA}}\,\norm{X_0} \leq C'\,\eu^{-2\alpha t}\,(1 + t)^{n-1}\,\norm{X_0} \leq C\,\eu^{-\alpha t}\norm{X_0} ,

absorbing the polynomial into one exponential factor (eαt(1+t)n10\eu^{-\alpha t}(1+t)^{n-1} \to 0, hence bounded).

Exercise 16.9 ★★★

(No escape in finite time for linear growth) Suppose ff is continuous with f(t,y)ay+b\norm{f(t, y)} \leq a\norm y + b on [0,)×Rn\intco{0}{\infty} \times \R^n, locally Lipschitz in yy. Using Gronwall (Exercise 16.6) on the integral form, prove that maximal solutions are global (defined on all of [0,)\intco{0}{\infty}).

Solution

Solution of Exercise 16.9.

Let yy be a maximal solution on [0,T)\intco{0}{T}, TT \leq \infty, and suppose T<T < \infty. The integral form gives, for t<Tt < T,

y(t)y0+0t(ay(s)+b) ⁣ds(y0+bT)+a0ty(s) ⁣ds,\norm{y(t)} \leq \norm{y_0} + \int_0^t \bigl(a\norm{y(s)} + b\bigr)\dd s \leq \bigl(\norm{y_0} + bT\bigr) + a\int_0^t\norm{y(s)}\,\dd s ,

and Gronwall bounds y(t)(y0+bT)eaT=:M\norm{y(t)} \leq (\norm{y_0} + bT)\,\eu^{aT} =: M on [0,T)\intco{0}{T}: the solution stays in a compact ball. Then y=f(t,y)y' = f(t, y) is bounded near TT, so yy is Lipschitz near TT and extends continuously to TT (Cauchy criterion); solving the Cauchy problem at (T,y(T))(T, y(T)) prolongs yy beyond TT, contradicting maximality. Hence T=T = \infty: no finite-time escape under linear growth.

Exercise 16.10

Solve y3y+2y=ety'' - 3y' + 2y = \eu^{t}: homogeneous solutions, then a particular solution of the form αtet\alpha t\,\eu^{t} (why does the naive guess αet\alpha\eu^t fail?); general solution and the solution with y(0)=y(0)=0y(0) = y'(0) = 0.

Solution

Solution of Exercise 16.10.

Characteristic roots of r23r+2r^2 - 3r + 2: 11 and 22, so the homogeneous solutions are aet+be2ta\eu^t + b\eu^{2t}. The guess αet\alpha\eu^t fails because et\eu^t already solves the homogeneous equation (the root r=1r = 1 “resonates” with the right-hand side). With y=αtety = \alpha t\,\eu^t: y=α(1+t)ety' = \alpha(1 + t)\eu^t, y=α(2+t)ety'' = \alpha(2 + t)\eu^t, and

y3y+2y=αet(2+t33t+2t)=αet:y'' - 3y' + 2y = \alpha\eu^t\bigl(2 + t - 3 - 3t + 2t\bigr) = -\alpha\,\eu^t :

α=1\alpha = -1, yp=tety_p = -t\,\eu^t. General solution: y=aet+be2ttety = a\eu^t + b\eu^{2t} - t\eu^t. Initial data y(0)=y(0)=0y(0) = y'(0) = 0: a+b=0a + b = 0 and a+2b1=0a + 2b - 1 = 0: b=1b = 1, a=1a = -1:

y(t)=e2t(1+t)et.y(t) = \eu^{2t} - (1 + t)\,\eu^{t} .

Exercise 16.11 ★★

Compute etA\eu^{tA} for the Jordan block

A=(λ100λ100λ),A = \begin{pmatrix} \lambda & 1 & 0\\ 0 & \lambda & 1\\ 0 & 0 & \lambda\end{pmatrix},

and describe all solutions of X=AXX' = AX: exponentials times polynomial vectors, with degrees up to 22. Where does the polynomial degree come from?

Solution

Solution of Exercise 16.11.

A=λI+NA = \lambda I + N with N=E12+E23N = E_{12} + E_{23}: N2=E13N^2 = E_{13}, N3=0N^3 = 0, and λI\lambda I commutes with NN:

etA=eλt(I+tN+t22N2)=eλt(1tt2201t001).\eu^{tA} = \eu^{\lambda t}\Bigl(I + tN + \frac{t^2}{2}N^2\Bigr) = \eu^{\lambda t}\begin{pmatrix} 1 & t & \frac{t^2}{2}\\ 0 & 1 & t\\ 0 & 0 & 1 \end{pmatrix}.

Solutions: X(t)=eλt(X0+tNX0+t22N2X0)X(t) = \eu^{\lambda t}\bigl(X_0 + tNX_0 + \frac{t^2}2N^2X_0\bigr) — each component is eλt\eu^{\lambda t} times a polynomial of degree 2\leq 2. The degree bound is the nilpotency index minus one: the series of etN\eu^{tN} truncates at N2N^2.

Exercise 16.12 ★★★

(Periodic forcing, periodic response) Let AMn(R)A \in \mathcal{M}_n(\R) and B ⁣:RRnB \colon \R \to \R^n continuous and TT-periodic.

  1. Show that a solution of X=AX+B(t)X' = AX + B(t) is TT-periodic if and only if X(T)=X(0)X(T) = X(0) (compare X(+T)X(\cdot + T) and XX).
  2. Show that eigenvalues of eTA\eu^{TA} are the eTλ\eu^{T\lambda}, λSpA\lambda \in \operatorname{Sp}A (trigonalize over C\C). Deduce: if no eigenvalue of AA lies in 2iπTZ\frac{2\iu\pi}{T}\Z, then IeTAI - \eu^{TA} is invertible.
  3. Under that hypothesis, prove that the system has exactly one TT-periodic solution, with

    X(0)=(IeTA)10Te(Ts)AB(s) ⁣ds.X(0) = \bigl(I - \eu^{TA}\bigr)^{-1} \int_0^{T}\eu^{(T-s)A}B(s)\,\dd s .

    What does the excluded case correspond to, for the harmonic oscillator? (The weekend problem answers: resonance.)

Solution

Solution of Exercise 16.12.

  1. If X(T)=X(0)X(T) = X(0), then Y(t)=X(t+T)Y(t) = X(t + T) solves Y=AY+B(t+T)=AY+B(t)Y' = AY + B(t + T) = AY + B(t) with Y(0)=X(0)Y(0) = X(0): uniqueness (Theorem 16.4) gives Y=XY = X, i.e. XX is TT-periodic. The converse is trivial.
  2. Trigonalize over C\C: A=PTP1A = PT'P^{-1} with TT' upper triangular, diagonal (λi)(\lambda_i). Every power of a triangular matrix is triangular with diagonal (λik)(\lambda_i^k), so eTA=PeTTP1\eu^{TA} = P\eu^{TT'}P^{-1} is triangular in the same basis with diagonal (eTλi)(\eu^{T\lambda_i}): those are the eigenvalues. Then IeTAI - \eu^{TA} is invertible iff eTλ1\eu^{T\lambda} \neq 1 for every eigenvalue, i.e. iff Tλ2iπZT\lambda \notin 2\iu\pi\Z, which is the stated hypothesis.
  3. Variation of constants: X(T)=eTAX(0)+0Te(Ts)AB(s) ⁣dsX(T) = \eu^{TA}X(0) + \int_0^T\eu^{(T-s)A}B(s)\dd s, so X(T)=X(0)X(T) = X(0) reads

    (IeTA)X(0)=0Te(Ts)AB(s) ⁣ds,\bigl(I - \eu^{TA}\bigr)X(0) = \int_0^{T}\eu^{(T-s)A}B(s)\,\dd s ,

    which has a unique solution X(0)X(0) under the invertibility hypothesis: exactly one TT-periodic solution. For the harmonic oscillator (λ=±iω\lambda = \pm\iu\omega), the excluded case is ωT2πZ\omega T \in 2\pi\Z: forcing whose period is a multiple of the natural period — resonance, as the weekend problem quantifies.

16.6 Problem: Oscillations, resonance, and Sturm’s comparison theorems

Problem 16.1

One equation rules the mechanical and electrical world:

x+2ζωx+ω2x=F(t),ω>0, ζ0.x'' + 2\zeta\omega\,x' + \omega^2 x = F(t), \qquad \omega > 0,\ \zeta \geq 0 .

This problem studies it completely — via the trace–determinant classification of planar linear systems, the three damping regimes, the steady-state response to periodic forcing with its resonance peak and the resonance catastrophe — then leaves constant coefficients for Sturm’s separation and comparison theorems, which control the zeros of solutions of y+q(t)y=0y'' + q(t)y = 0 with no formula at all.

Part I — The trace–determinant plane. Let AM2(R)A \in \mathcal M_2(\R), τ=trA\tau = \operatorname{tr}A, δ=detA\delta = \det A, Δ=τ24δ\Delta = \tau^2 - 4\delta.

  1. Show that the eigenvalues of AA are τ±Δ2\frac{\tau\pm\sqrt\Delta}{2} and classify: two real eigenvalues of opposite signs iff δ<0\delta < 0; real eigenvalues of the same sign iff δ>0\delta > 0, Δ0\Delta \geq 0 (sign of τ\tau); nonreal conjugate pair iff Δ<0\Delta < 0 (real part τ2\frac\tau2).
  2. (Saddle, δ<0\delta < 0) With eigenvalues μ<0<λ\mu < 0 < \lambda and eigenvectors v±v_\pm, write the general solution and describe the trajectories: two stable and two unstable rays, all other orbits asymptotic to both. Why can no solution but 00 stay bounded on all of R\R?
  3. (Nodes, δ>0\delta > 0, Δ>0\Delta > 0) For μ<λ<0\mu < \lambda < 0: show every nonzero solution tends to 00 and that all orbits except those on the fast axis arrive tangent to the slow eigendirection (compare eμt\eu^{\mu t} and eλt\eu^{\lambda t}).
  4. (Spirals and centers, Δ<0\Delta < 0) Writing the eigenvalues α±iβ\alpha \pm \iu\beta, use Exercise 16.5 (after a real change of basis, admitted in that generality or proved for the systems of Part II, which are the ones used below) to describe the orbits: spirals converging for α=τ2<0\alpha = \frac\tau2 < 0, diverging for τ>0\tau > 0, closed curves (center) for τ=0\tau = 0.
  5. (Boundary cases) For a double eigenvalue (Δ=0\Delta = 0): show etA=eλt(I+tN)\eu^{tA} = \eu^{\lambda t}(I + tN) with N=AλIN = A - \lambda I nilpotent, and distinguish the star (N=0N = 0) from the improper node (N0N \neq 0). Summarize Part I in the trace–determinant picture of this chapter’s figure.

Part II — The damped oscillator. Now F=0F = 0: x+2ζωx+ω2x=0x'' + 2\zeta\omega x' + \omega^2x = 0, i.e. X=AXX' = AX with A=(01ω22ζω)A = \begin{pmatrix} 0 & 1\\ -\omega^2 & -2\zeta\omega\end{pmatrix}.

  1. Compute τ,δ,Δ\tau, \delta, \Delta and place the three regimes in the trace–determinant plane: underdamped 0<ζ<10 < \zeta < 1 (stable spiral), critically damped ζ=1\zeta = 1 (double eigenvalue), overdamped ζ>1\zeta > 1 (stable node); ζ=0\zeta = 0 is the center.
  2. Solve the three regimes explicitly:

    ζ<1: eζωt(acosωdt+bsinωdt), ωd=ω1ζ2;ζ=1: (a+bt)eωt;\zeta < 1:\ \eu^{-\zeta\omega t}\bigl(a\cos\omega_d t + b\sin\omega_dt\bigr),\ \omega_d = \omega\sqrt{1-\zeta^2}; \qquad \zeta = 1:\ (a + bt)\,\eu^{-\omega t};

    ζ>1\zeta > 1: two real exponentials. Define the pseudo-period 2πωd\frac{2\pi}{\omega_d} and show that the ratio of successive maxima of x\abs x is the constant e2πζ/1ζ2\eu^{-2\pi\zeta/\sqrt{1-\zeta^2}} (the logarithmic decrement).

  3. (The door-closer principle) For ζ1\zeta \geq 1 the decay rate is governed by the slowest eigenvalue λslow=ω(ζζ21)\lambda_{\mathrm{slow}} = -\omega\bigl(\zeta - \sqrt{\zeta^2-1}\bigr). Show that λslow=ωζ+ζ21\abs{\lambda_{\mathrm{slow}}} = \frac{\omega}{\zeta + \sqrt{\zeta^2 - 1}} is a decreasing function of ζ1\zeta \geq 1: critical damping ζ=1\zeta = 1 gives the fastest non-oscillating return to rest.
  4. (Energy) Let E(t)=12x2+12ω2x2E(t) = \frac12x'^2 + \frac12\omega^2x^2. Prove E=2ζωx20E' = -2\zeta\omega\,x'^2 \leq 0, and deduce that for ζ>0\zeta > 0 the equation has no nonzero periodic solution (a period would force EE constant, hence x0x' \equiv 0).
  5. Explain in two sentences why the center ζ=0\zeta = 0 is structurally fragile: any ζ>0\zeta > 0, however small, destroys periodicity — and where that shows in the trace–determinant plane (the center line has empty interior).

Part III — Forced oscillations and resonance. Now F(t)=Fcos(γt)F(t) = F\cos(\gamma t) with F,γ>0F, \gamma > 0.

  1. (ζ>0\zeta > 0: the steady state) Seek xp=(zeiγt)x_p = \Re\bigl(z\,\eu^{\iu\gamma t}\bigr): show

    z=Fω2γ2+2iζωγ,A(γ):=z=F(ω2γ2)2+4ζ2ω2γ2,z = \frac{F}{\omega^2 - \gamma^2 + 2\iu\zeta\omega\gamma}, \qquad A(\gamma) := \abs z = \frac{F}{\sqrt{(\omega^2 - \gamma^2)^2 + 4\zeta^2\omega^2\gamma^2}} ,

    and write xp=A(γ)cos(γtφ)x_p = A(\gamma)\cos(\gamma t - \varphi) with tanφ=2ζωγω2γ2\tan\varphi = \frac{2\zeta\omega\gamma}{\omega^2-\gamma^2}.

  2. Show that every solution is xpx_p plus a transient from Part II, which tends to 00: whatever the initial data, the system locks onto the steady state — amplitude A(γ)A(\gamma), phase lag φ\varphi.
  3. (The resonance curve) Maximize AA: show that A(γ)A(\gamma) has an interior maximum iff ζ<12\zeta < \frac{1}{\sqrt2}, at

    γ=ω12ζ2,A(γ)=F2ζω21ζ2,\gamma_* = \omega\sqrt{1 - 2\zeta^2}, \qquad A(\gamma_*) = \frac{F}{2\zeta\omega^2\sqrt{1-\zeta^2}} ,

    and that for small ζ\zeta the peak amplifies the static response A(0)=Fω2A(0) = \frac F{\omega^2} by the factor 12ζ\approx \frac{1}{2\zeta}.

  4. (ζ=0\zeta = 0, off resonance) For γω\gamma \neq \omega, show that the solution with x(0)=x(0)=0x(0) = x'(0) = 0 is

    x(t)=Fω2γ2(cosγtcosωt)=2Fω2γ2sin(ωγ)t2sin(ω+γ)t2:x(t) = \frac{F}{\omega^2 - \gamma^2}\bigl(\cos\gamma t - \cos\omega t\bigr) = \frac{2F}{\omega^2-\gamma^2} \sin\frac{(\omega-\gamma)t}{2} \sin\frac{(\omega+\gamma)t}{2} :

    bounded, with beats — a fast oscillation under a slow envelope — when γ\gamma is close to ω\omega.

  5. (ζ=0\zeta = 0, resonance) For γ=ω\gamma = \omega, show that xp(t)=F2ωtsin(ωt)x_p(t) = \frac{F}{2\omega}\,t\sin(\omega t) is a solution, and recover it as the limit of question 14 as γω\gamma \to \omega: the amplitude grows linearly forever — the resonance catastrophe.
  6. (Fourier link) A general periodic forcing decomposes into harmonics (the Fourier chapter); by linearity the steady state is the sum of the harmonic responses. For an undamped oscillator of frequency ω=3\omega = 3 forced by the square wave of Exercise 14.1-type (harmonics at all odd integers), which harmonic resonates? One sentence on why engineers fear square waves.

Part IV — Sturm’s theorems. Consider y+q(t)y=0y'' + q(t)\,y = 0 on an interval II, qq continuous. (Any equation y+ay+by=0y'' + ay' + by = 0 reduces to this normal form by the substitution y=uexp(12a)y = u\exp\bigl(-\frac12\int a\bigr); question 21 shows a variant of the trick in action.)

  1. For two solutions y1,y2y_1, y_2, show that the wronskian W=y1y2y1y2W = y_1y_2' - y_1'y_2 is constant, zero iff the solutions are proportional; and that a nonzero solution has only simple, isolated zeros.
  2. (Sturm separation) Let y1,y2y_1, y_2 be independent solutions and a<ba < b two consecutive zeros of y1y_1. Prove that y2y_2 vanishes exactly once in (a,b)\intoo{a}{b} (evaluate the constant WW at aa and bb: W=y1y2W = y_1'y_2 there, and y1(a)y_1'(a), y1(b)y_1'(b) have opposite signs): zeros of independent solutions interlace.
  3. (Sturm comparison) Let q1q2q_1 \leq q_2 on II, y0y \neq 0 with y+q1y=0y'' + q_1y = 0, z0z \neq 0 with z+q2z=0z'' + q_2z = 0, and a<ba < b consecutive zeros of yy. Show that zz vanishes in [a,b]\intcc{a}{b} — strictly inside if q1<q2q_1 < q_2 somewhere on (a,b)\intoo ab (if z0z \neq 0 on (a,b)\intoo ab, study (yzyz)=(q1q2)yz(yz' - y'z)' = (q_1 - q_2)yz with fixed signs for y,zy, z and compare the boundary values).
  4. Deduce the spacing bounds: if 0<m2q(t)M20 < m^2 \leq q(t) \leq M^2 on II, then any two consecutive zeros a<ba < b of a nonzero solution of y+qy=0y'' + qy = 0 satisfy

    πM    ba    πm\frac{\pi}{M} \;\leq\; b - a \;\leq\; \frac{\pi}{m}

    (compare with u+M2u=0u'' + M^2u = 0 and u+m2u=0u'' + m^2u = 0, whose zeros are spaced πM\frac\pi M and πm\frac\pi m). Check on the harmonic oscillator.

  5. Transform ty+2y+ty=0ty'' + 2y' + ty = 0 (Exercise 16.7) by u=tyu = ty into u+u=0u'' + u = 0, recover its solutions sintt\frac{\sin t}t, costt\frac{\cos t}{t} instantly, and conclude that the zeros of every nonzero solution are spaced exactly π\pi: Sturm’s world view — zeros are controlled by the coefficient qq, formulas or not.

Part V — Duhamel and the boundedness frontier.

  1. (Duhamel for the oscillator) Show that for continuous FF, the solution of x+ω2x=F(t)x'' + \omega^2x = F(t) with x(0)=x(0)=0x(0) = x'(0) = 0 is

    x(t)=1ω0tsin(ω(ts))F(s) ⁣ds,x(t) = \frac1\omega\int_0^t\sin\bigl(\omega(t - s)\bigr)F(s)\,\dd s ,

    and re-derive the resonant solution of question 15 from it with F(s)=Fcos(ωs)F(s) = F\cos(\omega s) (product-to-sum).

  2. (ζ>0\zeta > 0: bounded input, bounded output) Show that for ζ>0\zeta > 0 and any bounded continuous FF, every solution of the damped equation is bounded on [0,)\intco{0}{\infty} (variation of constants plus the exponential decay etACeαt\vertiii{\eu^{tA}} \leq C\eu^{-\alpha t} of Exercise 16.8).
  3. (ζ=0\zeta = 0) Show that with no damping, bounded periodic forcing keeps all solutions bounded except exactly at resonance (γ=ω\gamma = \omega, question 15 versus question 14): damping is what turns the boundedness frontier into uniform stability.
  4. Synthesis. In one sentence each: (i) how the trace–determinant plane organizes Parts I–II and where forcing (Part III) leaves it; (ii) the physical meaning of γ\gamma_*, A(γ)A(\gamma_*) and the factor 12ζ\frac1{2\zeta}; (iii) what Sturm’s theorems say that explicit formulas cannot; (iv) which two results of this problem the rest of the book will quietly reuse (Liouville-constant wronskians; bounded-input stability).
Solution

Solution of Problem 16.1.

1. The characteristic polynomial is λ2τλ+δ\lambda^2 - \tau\lambda + \delta, with roots τ±Δ2\frac{\tau\pm\sqrt\Delta}{2}. If δ<0\delta < 0 then Δ=τ24δ>0\Delta = \tau^2 - 4\delta > 0 and the two real roots have product δ<0\delta < 0: opposite signs. If δ>0\delta > 0 and Δ0\Delta \geq 0: real roots of product >0> 0 and sum τ\tau: both of the sign of τ\tau. If Δ<0\Delta < 0: conjugate pair α±iβ\alpha \pm \iu\beta with α=τ2\alpha = \frac\tau2, β=Δ2\beta = \frac{\sqrt{-\Delta}}2.

2. X(t)=aeμtv+beλtv+X(t) = a\,\eu^{\mu t}v_- + b\,\eu^{\lambda t}v_+. Orbits with a=0a = 0 (resp. b=0b = 0) run along the unstable (resp. stable) eigenline; all others have X\norm X \to \infty in both time directions, asymptotic to Rv+\R v_+ as t+t \to +\infty and to Rv\R v_- as tt \to -\infty: the saddle picture. Boundedness on all of R\R forces b=0b = 0 (else explosion at ++\infty) and a=0a = 0 (at -\infty): only the origin.

3. With μ<λ<0\mu < \lambda < 0, both exponentials decay: X(t)0X(t) \to 0. If b0b \neq 0, factor eλt\eu^{\lambda t}:

X(t)=eλt(bvλ+ae(μλ)tvμ),e(μλ)t0:X(t) = \eu^{\lambda t}\bigl(b\,v_\lambda + a\,\eu^{(\mu - \lambda)t}v_\mu\bigr), \qquad \eu^{(\mu-\lambda)t} \to 0 :

the direction of X(t)X(t) tends to Rvλ\R v_\lambda, the slow eigendirection — all orbits but the fast axis arrive tangent to it (the right panel of the chapter’s phase portraits).

4. In the basis where A=(αββα)A = \begin{pmatrix} \alpha & -\beta\\ \beta & \alpha\end{pmatrix} (Exercise 16.5; for the oscillator systems of Part II this form is reached by an explicit real change of basis), the solution is eαt\eu^{\alpha t} times a rotation of angle βt\beta t: logarithmic spirals, contracting when α=τ2<0\alpha = \frac\tau2 < 0, expanding when τ>0\tau > 0, and closed curves (ellipses in the original coordinates) when τ=0\tau = 0: the center.

5. Δ=0\Delta = 0 gives the double eigenvalue λ=τ2\lambda = \frac\tau2; by Cayley–Hamilton (Theorem 3.21), (AλI)2=0(A - \lambda I)^2 = 0, so N=AλIN = A - \lambda I is nilpotent, commutes with λI\lambda I, and etA=eλt(I+tN)\eu^{tA} = \eu^{\lambda t}(I + tN). If N=0N = 0: A=λIA = \lambda I, all rays are orbits (star node). If N0N \neq 0: X(t)=eλt(X0+tNX0)X(t) = \eu^{\lambda t}(X_0 + tNX_0), and for NX00NX_0 \neq 0 the direction converges to the single eigendirection imN\operatorname{im}N: improper node. This completes the trace–determinant picture.

6. τ=2ζω\tau = -2\zeta\omega, δ=ω2>0\delta = \omega^2 > 0, Δ=4ω2(ζ21)\Delta = 4\omega^2(\zeta^2 - 1). So: 0<ζ<10 < \zeta < 1 gives Δ<0\Delta < 0, τ<0\tau < 0: stable spiral; ζ=1\zeta = 1: Δ=0\Delta = 0: degenerate stable node; ζ>1\zeta > 1: Δ>0\Delta > 0, τ<0\tau < 0, δ>0\delta > 0: stable node; ζ=0\zeta = 0: τ=0\tau = 0, δ>0\delta > 0: center. A vertical journey in the plane at δ=ω2\delta = \omega^2.

7. Roots r=ζω±ωζ21r = -\zeta\omega \pm \omega\sqrt{\zeta^2-1}. For ζ<1\zeta < 1: r=ζω±iωdr = -\zeta\omega \pm \iu\omega_d, ωd=ω1ζ2\omega_d = \omega\sqrt{1-\zeta^2}:

x(t)=eζωt(acosωdt+bsinωdt)=Reζωtcos(ωdtφ).x(t) = \eu^{-\zeta\omega t}\bigl(a\cos\omega_dt + b\sin\omega_dt\bigr) = R\,\eu^{-\zeta\omega t}\cos(\omega_dt - \varphi) .

For ζ=1\zeta = 1: x=(a+bt)eωtx = (a + bt)\eu^{-\omega t}. For ζ>1\zeta > 1: x=aert+ber+tx = a\eu^{r_-t} + b\eu^{r_+t}, both rates negative. Successive maxima of x\abs x in the underdamped case occur at times separated by the pseudo-period 2πωd\frac{2\pi}{\omega_d} (same phase of the cosine), and their ratio is eζω2π/ωd=e2πζ/1ζ2\eu^{-\zeta\omega\cdot2\pi/\omega_d} = \eu^{-2\pi\zeta/\sqrt{1-\zeta^2}}: the logarithmic decrement, a damping meter readable on an oscilloscope.

8. Rationalizing,

λslow=ω(ζζ21)=ωζ+ζ21,\abs{\lambda_{\mathrm{slow}}} = \omega\bigl(\zeta - \sqrt{\zeta^2-1}\bigr) = \frac{\omega}{\zeta + \sqrt{\zeta^2 - 1}} ,

whose denominator increases with ζ1\zeta \geq 1: the decay rate is largest at ζ=1\zeta = 1, where it equals ω\omega. An overdamped door closes without slamming but slowly; critical damping is the engineer’s optimum.

9. E=xx+ω2xx=x(2ζωxω2x)+ω2xx=2ζωx20E' = x'x'' + \omega^2xx' = x'\bigl(-2\zeta\omega x' - \omega^2x\bigr) + \omega^2xx' = -2\zeta\omega\,x'^2 \leq 0. If xx were periodic and nonconstant, EE would be periodic and nonincreasing, hence constant, forcing x0x' \equiv 0: xx constant, and then ω2x=0\omega^2x = 0: x0x \equiv 0. So for ζ>0\zeta > 0 the only periodic solution is rest: damping kills every cycle.

10. The center ζ=0\zeta = 0 lives on the line τ=0\tau = 0 of the trace–determinant plane — a set with empty interior: an arbitrarily small perturbation of the matrix (any physical damping) moves τ\tau off zero and turns the closed orbits into spirals. Periodicity of the undamped oscillator is thus a razor’s-edge phenomenon, not a robust one.

11. Substituting xp=(zeiγt)x_p = \Re(z\eu^{\iu\gamma t}) into the equation:

(γ2+2iζωγ+ω2)z=Fz=Fω2γ2+2iζωγ,\bigl(-\gamma^2 + 2\iu\zeta\omega\gamma + \omega^2\bigr)z = F \quad\Longrightarrow\quad z = \frac{F}{\omega^2 - \gamma^2 + 2\iu\zeta\omega\gamma},

so xp=zcos(γtφ)x_p = \abs z\cos(\gamma t - \varphi) with φ=arg(ω2γ2+2iζωγ)\varphi = \arg(\omega^2 - \gamma^2 + 2\iu\zeta\omega\gamma), i.e. tanφ=2ζωγω2γ2\tan\varphi = \frac{2\zeta\omega\gamma}{\omega^2 - \gamma^2}, and the stated A(γ)=zA(\gamma) = \abs z.

12. The difference of two solutions solves the homogeneous equation, which for ζ>0\zeta > 0 decays to 00 (question 7): every solution equals xpx_p plus a transient vanishing at infinity. The steady state is a global attractor: initial conditions are forgotten, only A(γ)A(\gamma) and the phase lag φ\varphi remain.

13. Minimize g(u)=(ω2u)2+4ζ2ω2ug(u) = (\omega^2 - u)^2 + 4\zeta^2\omega^2u over u=γ20u = \gamma^2 \geq 0: g(u)=2(ω2u)+4ζ2ω2=0g'(u) = -2(\omega^2 - u) + 4\zeta^2\omega^2 = 0 at u=ω2(12ζ2)u = \omega^2(1 - 2\zeta^2), interior iff ζ<12\zeta < \frac{1}{\sqrt2}. There

g(u)=4ζ4ω4+4ζ2ω4(12ζ2)=4ζ2ω4(1ζ2),A(γ)=F2ζω21ζ2.g(u_*) = 4\zeta^4\omega^4 + 4\zeta^2\omega^4(1 - 2\zeta^2) = 4\zeta^2\omega^4(1 - \zeta^2), \qquad A(\gamma_*) = \frac{F}{2\zeta\omega^2\sqrt{1 - \zeta^2}} .

Against the static response A(0)=Fω2A(0) = \frac{F}{\omega^2}: amplification 12ζ1ζ212ζ\frac{1}{2\zeta\sqrt{1-\zeta^2}} \approx \frac{1}{2\zeta} for small ζ\zeta — a lightly damped system near γω\gamma_* \approx \omega multiplies the input a hundredfold when ζ=0.005\zeta = 0.005.

14. The stated xx satisfies x(0)=x(0)=0x(0) = x'(0) = 0 and

x+ω2x=F(ω2γ2)cosγtω2γ2=Fcosγtx'' + \omega^2 x = \frac{F(\omega^2 - \gamma^2)\cos\gamma t}{\omega^2 - \gamma^2} = F\cos\gamma t

(the cosωt\cos\omega t parts cancel). The product form follows from cospcosq=2sinq+p2sinqp2\cos p - \cos q = 2\sin\frac{q+p}{2}\sin\frac{q-p}2 with p=γtp = \gamma t, q=ωtq = \omega t. For γ\gamma close to ω\omega, the factor sin(ωγ)t2\sin\frac{(\omega-\gamma)t}2 is a slow envelope modulating the fast oscillation sin(ω+γ)t2\sin\frac{(\omega+\gamma)t}2: beats, with amplitude 2Fω2γ2\frac{2F}{\abs{\omega^2-\gamma^2}} — large, but bounded.

15. For xp=F2ωtsinωtx_p = \frac{F}{2\omega}t\sin\omega t:

xp=F2ω(2ωcosωtω2tsinωt)=Fcosωtω2xp:x_p'' = \frac{F}{2\omega}\bigl(2\omega\cos\omega t - \omega^2t\sin\omega t\bigr) = F\cos\omega t - \omega^2x_p :

a solution. And at fixed tt, letting γω\gamma \to \omega in question 14:

2Fsin(ωγ)t2sin(ω+γ)t2(ωγ)(ω+γ)2F(ωγ)t2/(ωγ)sinωt2ω=Ftsinωt2ω.\frac{2F\sin\frac{(\omega-\gamma)t}2 \sin\frac{(\omega+\gamma)t}{2}} {(\omega-\gamma)(\omega+\gamma)} \longrightarrow \frac{2F\cdot\frac{(\omega-\gamma)t}2\big/(\omega-\gamma) \cdot\sin\omega t}{2\omega} = \frac{F\,t\sin\omega t}{2\omega} .

The amplitude grows linearly without bound: the resonance catastrophe — the reason soldiers break step on bridges.

16. The square wave carries harmonics at every odd frequency n=1,3,5,n = 1, 3, 5, \dots; by linearity, each harmonic nn is amplified by the oscillator’s response at γ=n\gamma = n. For ω=3\omega = 3 the third harmonic hits resonance exactly. Engineers fear square (and sawtooth) inputs because they excite all odd harmonics at once: whatever the natural frequency of the structure, some harmonic is waiting for it.

17. W=y1y2y1y2=qy1y2+qy1y2=0W' = y_1y_2'' - y_1''y_2 = -qy_1y_2 + qy_1y_2 = 0: WW is constant (Liouville with a trace-zero companion matrix). W=0W = 0 at one point makes the initial data of y2y_2 proportional to those of y1y_1, hence y2y_2 proportional to y1y_1 (uniqueness); W0W \neq 0 iff independent. If y(t0)=y(t0)=0y(t_0) = y'(t_0) = 0 then y0y \equiv 0 (uniqueness): a nonzero solution has simple zeros, and a simple zero is isolated (yy' of fixed sign nearby).

18. Between consecutive zeros a<ba < b, y1y_1 keeps one sign, say y1>0y_1 > 0 on (a,b)\intoo ab: then y1(a)>0y_1'(a) > 0 and y1(b)<0y_1'(b) < 0 (simple zeros). Evaluating the constant W=y1y2y1y2W = y_1y_2' - y_1'y_2 at aa and bb:

W=y1(a)y2(a)=y1(b)y2(b),W = -y_1'(a)\,y_2(a) = -y_1'(b)\,y_2(b) ,

so y2(a)y_2(a) and y2(b)y_2(b) have opposite signs (W0W \neq 0 forbids either to vanish): y2y_2 vanishes in (a,b)\intoo ab (intermediate values). It cannot vanish twice there: two zeros of y2y_2 would flank a zero of y1y_1 by the same argument with the roles exchanged, contradicting consecutiveness: exactly one zero — interlacing.

19. Suppose zz has no zero in (a,b)\intoo ab; replacing y,zy, z by their negatives, assume y>0y > 0 and z>0z > 0 on (a,b)\intoo ab. Set φ=yzyz\varphi = yz' - y'z: φ=yzyz=(q1q2)yz0\varphi' = yz'' - y''z = (q_1 - q_2)\,yz \leq 0 on (a,b)\intoo ab: φ\varphi is nonincreasing. But φ(a)=y(a)z(a)0\varphi(a) = -y'(a)z(a) \leq 0 (as y(a)>0y'(a) > 0, z(a)0z(a) \geq 0) and φ(b)=y(b)z(b)0\varphi(b) = -y'(b)z(b) \geq 0 (as y(b)<0y'(b) < 0, z(b)0z(b) \geq 0): a nonincreasing function running from 0\leq 0 to 0\geq 0 vanishes identically, so (q1q2)yz0(q_1 - q_2)yz \equiv 0 on (a,b)\intoo ab. If q1<q2q_1 < q_2 somewhere in (a,b)\intoo ab, this is absurd (y,z>0y, z > 0 there): zz must vanish strictly inside. In general (q1q2q_1 \leq q_2), either zz vanishes in (a,b)\intoo ab, or φ0\varphi \equiv 0 forces zz proportional to yy, which vanishes at aa and bb: in all cases zz has a zero in [a,b]\intcc ab.

20. Upper bound: compare yy (coefficient qm2q \geq m^2) with u(t)=sin(m(ta))u(t) = \sin(m(t - a)) (coefficient m2qm^2 \leq q, so yy plays the role of zz in question 19): if yy had no zero in (a,a+π/m]\intoc{a}{a + \pi/m}, the zeros aa and a+πma + \frac\pi m of uu would be consecutive with y0y \neq 0 between them, contradicting question 19: consecutive zeros of yy are at distance πm\leq \frac\pi m. Lower bound: if two consecutive zeros a<ba < b of yy had ba<πMb - a < \frac\pi M, then z(t)=sin(M(ta))z(t) = \sin(M(t-a)) (coefficient M2qM^2 \geq q) would have to vanish in [a,b](a,a+π/M){a}\intcc ab \subset \intoo{a}{a + \pi/M} \cup\{a\}, where its only zero is aa itself — but question 19 applied on (a,b)\intoo{a}{b} with strictness at the endpoints gives a zero in [a,b]\intcc ab, and z>0z > 0 on (a,b]\intoc ab: contradiction. Hence πMbaπm\frac\pi M \leq b - a \leq \frac\pi m; for qω2q \equiv \omega^2 both bounds collapse to the exact spacing πω\frac\pi\omega of the harmonic oscillator.

21. With u=tyu = ty: u=ty+2yu'' = ty'' + 2y', so ty+2y+ty=u+u=0ty'' + 2y' + ty = u'' + u = 0: u=Asint+Bcost=Rsin(t+φ)u = A\sin t + B\cos t = R\sin(t + \varphi), and y=uty = \frac{u}{t} recovers sintt\frac{\sin t}t and costt\frac{\cos t}t (Exercise 16.7) with no lowering of order. The zeros of any nonzero solution are those of Rsin(t+φ)R\sin(t + \varphi): spaced exactly π\pi — Sturm’s philosophy in action: the coefficient q1q \equiv 1 dictates the zeros, formula or no formula.

22. Set x(t)=1ω0tsin(ω(ts))F(s) ⁣dsx(t) = \frac1\omega\int_0^t\sin(\omega(t-s))F(s)\dd s. Then x(0)=0x(0) = 0;

x(t)=1ωsin(0)F(t)+0tcos(ω(ts))F(s) ⁣ds=0tcos(ω(ts))F(s) ⁣ds,x'(t) = \frac1\omega\sin(0)F(t) + \int_0^t\cos(\omega(t-s))F(s)\dd s = \int_0^t\cos(\omega(t-s))F(s)\dd s ,

so x(0)=0x'(0) = 0; and x(t)=F(t)ω0tsin(ω(ts))F(s) ⁣ds=F(t)ω2x(t)x''(t) = F(t) - \omega\int_0^t\sin(\omega(t-s))F(s)\dd s = F(t) - \omega^2x(t) (differentiation of a parameter integral with variable limit, as in the integration chapter). With F(s)=FcosωsF(s) = F\cos\omega s, product-to-sum gives

0tsin(ω(ts))cos(ωs) ⁣ds=120t(sinωt+sin(ωt2ωs)) ⁣ds=t2sinωt,\int_0^t\sin(\omega(t-s))\cos(\omega s)\dd s = \frac12\int_0^t\bigl(\sin\omega t + \sin(\omega t - 2\omega s)\bigr)\dd s = \frac{t}{2}\sin\omega t ,

(the second piece integrates to zero), so x=F2ωtsinωtx = \frac{F}{2\omega}t\sin\omega t: question 15 again, from Duhamel.

23. In system form X=AX+(0,F(t))TX' = AX + (0, F(t))^{\mathsf T} with SpA\operatorname{Sp}A of negative real parts (ζ>0\zeta > 0): variation of constants and Exercise 16.8 (etACeαt\vertiii{\eu^{tA}} \leq C\eu^{-\alpha t}) give

X(t)CeαtX0+0tCeα(ts)F ⁣dsCX0+CFα:\norm{X(t)} \leq C\eu^{-\alpha t}\norm{X_0} + \int_0^t C\eu^{-\alpha(t-s)}\norm{F}_\infty\dd s \leq C\norm{X_0} + \frac{C\norm F_\infty}{\alpha} :

bounded input, bounded output — uniformly in the initial data after the transient.

24. For ζ=0\zeta = 0 and γω\gamma \neq \omega, question 14’s solution is bounded, and adding any homogeneous solution (bounded: the center’s orbits are circles) keeps it bounded; at γ=ω\gamma = \omega, question 15 grows linearly. So for the undamped oscillator, boundedness under periodic forcing fails at exactly one frequency — resonance — while question 23 shows any positive damping restores boundedness for all bounded inputs.

25. (i) The trace–determinant plane classifies all autonomous planar linear dynamics, and Part II’s oscillator walks a vertical line of it; forcing leaves the plane (non-autonomous), and Duhamel takes over. (ii) γ\gamma_* is the frequency the system prefers, A(γ)A(\gamma_*) the price of exciting it, and 12ζ\frac{1}{2\zeta} the amplification factor — the resonance sharpness engineers call the quality factor. (iii) Sturm’s theorems read oscillation off the sign and size of qq alone: they govern equations (Bessel, Schrödinger) whose solutions have no elementary formulas. (iv) Constant wronskians (question 17, via Liouville) and bounded-input stability (question 23) are reused silently whenever the book meets variable-coefficient equations or perturbed systems.