Mathematical Methods Handbook

Sufficient conditions and direct methods

Second variation and the variational treatment of eigenvalue problems.

In this chapter 4

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  1. The second variation
  2. Variational eigenvalue problems and direct methods

The second variation

2

Theorem

The second variation and Legendre's condition

Adapted

At a weak minimum of a functional the second variation is nonnegative in every direction, which forces F_{y'y'} >= 0 at every point of the curve (Legendre's condition); the unit also writes the second variation in the form used for sufficient conditions.

Prerequisites: The Euler-Lagrange equation, Differentiation under the integral sign, Taylor's theorem

DefinitionAdaptedAdapted from Gelfand & Fomin (1963), Ch. 5, §§24–25, pp. 99–101; Evans (2010), §8.1.3, p. 431

Let F(x,y,z)F(x, y, z) be a real function on [a,b]×R×R[a, b] \times \mathbb{R} \times \mathbb{R} with continuous partial derivatives up to order two, and consider

J[y]=∫abF(x,y(x),y′(x)) dxJ[y] = \int_a^b F\bigl(x, y(x), y'(x)\bigr)\, dx

on the admissible curves y∈C1[a,b]y \in C^1[a, b] with y(a)=Ay(a) = A, y(b)=By(b) = B. The variations are the functions in

H={ h∈C1[a,b]:h(a)=h(b)=0 },∥h∥1=max⁡[a,b]∣h∣+max⁡[a,b]∣h′∣.H = \{\, h \in C^1[a, b] : h(a) = h(b) = 0 \,\}, \qquad \|h\|_1 = \max_{[a,b]} |h| + \max_{[a,b]} |h'| .

An admissible yy is a weak minimum of JJ if there is r>0r > 0 with J[y^]≥J[y]J[\hat y] \ge J[y] for every admissible y^\hat y with ∥y^−y∥1<r\|\hat y - y\|_1 < r. "Weak" means that a competitor must be close to yy in both value and slope.

Throughout, Fy′y′F_{y'y'} denotes ∂2F/∂z2\partial^2 F / \partial z^2 evaluated at (x,y(x),y′(x))(x, y(x), y'(x)), and similarly Fyy′F_{yy'} and FyyF_{yy}. The second variation of JJ at yy in the direction h∈Hh \in H is

δ2J[y;h]=d2dε2J[y+εh]∣ε=0=∫ab(Fyy h2+2Fyy′ hh′+Fy′y′ h′2) dx.\delta^2 J[y; h] = \frac{d^2}{d\varepsilon^2} J[y + \varepsilon h] \Big|_{\varepsilon = 0} = \int_a^b \bigl( F_{yy}\, h^2 + 2F_{yy'}\, h h' + F_{y'y'}\, h'^2 \bigr)\, dx .

Convention. Gelfand and Fomin define the second variation as the quadratic part of the increment J[y+h]−J[y]J[y+h] - J[y], which is half of ours, so their coefficients PP and QQ are half of the ones below. Evans uses the second derivative, as we do.

TheoremAdaptedAdapted from Gelfand & Fomin (1963), Ch. 5, §24 Thm 1, p. 99, and §25, formula (10) and Legendre's theorem, pp. 102–103

Let FF have continuous second partial derivatives and let yy be admissible.

  1. (Second-order necessary condition.) If yy is a weak minimum of JJ, then δ2J[y;h]≥0\delta^2 J[y; h] \ge 0 for every h∈Hh \in H.
  2. (Legendre's condition.) If yy is a weak minimum of JJ, then Fy′y′(x,y(x),y′(x))≥0for every x∈[a,b].F_{y'y'}\bigl(x, y(x), y'(x)\bigr) \ge 0 \qquad \text{for every } x \in [a, b]. For a weak maximum the inequality is reversed.
  3. (Integrated form.) If in addition FF has continuous third partial derivatives and y∈C2[a,b]y \in C^2[a, b], then for every h∈Hh \in H δ2J[y;h]=∫ab(P h′2+Q h2) dx,P=Fy′y′,Q=Fyy−ddxFyy′.\delta^2 J[y; h] = \int_a^b \bigl( P\, h'^2 + Q\, h^2 \bigr)\, dx, \qquad P = F_{y'y'}, \quad Q = F_{yy} - \frac{d}{dx} F_{yy'} .
Idea of the proofOriginal

Along the straight line ε↦y+εh\varepsilon \mapsto y + \varepsilon h in function space, JJ becomes an ordinary function of one variable with a minimum at ε=0\varepsilon = 0, so its second derivative there cannot be negative. For Legendre's condition we pick a direction hh concentrated near one point: a bump of height δ\delta and width δ\delta. Its slope stays of size one while the bump itself is of size δ\delta, so the three terms of δ2J\delta^2 J scale like δ\delta, δ2\delta^2 and δ3\delta^3. The h′2h'^2 term wins, and its sign is the sign of Fy′y′F_{y'y'} at that point.

ProofAdaptedAdapted from Evans (2010), §8.1.3, pp. 431–432; Gelfand & Fomin (1963), Ch. 5, §25, Lemma, p. 103

Part 1. Fix h∈Hh \in H, h≠0h \ne 0, and put φ(ε)=J[y+εh]\varphi(\varepsilon) = J[y + \varepsilon h].

  1. φ\varphi is twice continuously differentiable. The integrand F(x,y+εh,y′+εh′)F(x, y + \varepsilon h, y' + \varepsilon h') has first and second ε\varepsilon-derivatives that are continuous in (x,ε)(x, \varepsilon) on [a,b]×[−1,1][a, b] \times [-1, 1], because FF has continuous second derivatives and y,y′,h,h′y, y', h, h' are continuous. So differentiation under the integral sign applies twice, and φ′′(0)\varphi''(0) is the integral displayed in the definition.
  2. φ\varphi has a local minimum at 00. For ∣ε∣<r/∥h∥1|\varepsilon| < r / \|h\|_1 the curve y+εhy + \varepsilon h is admissible (it has the right end values because h(a)=h(b)=0h(a) = h(b) = 0) and lies within rr of yy in the norm ∥⋅∥1\|\cdot\|_1. The weak-minimum hypothesis gives φ(ε)≥φ(0)\varphi(\varepsilon) \ge \varphi(0).
  3. Conclusion. A local minimum forces φ′(0)=0\varphi'(0) = 0. If φ′′(0)\varphi''(0) were negative, then by Taylor's theorem with the Lagrange remainder, φ(ε)=φ(0)+12φ′′(θε) ε2\varphi(\varepsilon) = \varphi(0) + \tfrac12 \varphi''(\theta\varepsilon)\, \varepsilon^2 for some θ∈(0,1)\theta \in (0,1), and continuity of φ′′\varphi'' would make this smaller than φ(0)\varphi(0) for small ε≠0\varepsilon \ne 0. Hence δ2J[y;h]=φ′′(0)≥0\delta^2 J[y; h] = \varphi''(0) \ge 0.

Part 2. Write P=Fy′y′P = F_{y'y'}, R=Fyy′R = F_{yy'} and S=FyyS = F_{yy} along the curve; these are continuous on [a,b][a, b]. Let M=max⁡[a,b](∣R∣+∣S∣)M = \max_{[a,b]} (|R| + |S|). Suppose, for a contradiction, that P(x0)<0P(x_0) < 0 for some x0∈[a,b]x_0 \in [a, b].

  1. A short interval where PP is negative. By continuity of PP there are β>0\beta > 0, an interior point x1∈(a,b)x_1 \in (a, b) and δ0>0\delta_0 > 0 with [x1−δ0,x1+δ0]⊂(a,b)[x_1 - \delta_0, x_1 + \delta_0] \subset (a, b) and P≤−βP \le -\beta on that interval. (If x0x_0 is an endpoint, move slightly inside; PP is still negative there.)
  2. A rescaled bump. Let g(s)=(1−s2)2g(s) = (1 - s^2)^2 for ∣s∣≤1|s| \le 1 and g(s)=0g(s) = 0 otherwise. Then g∈C1(R)g \in C^1(\mathbb{R}), because gg and g′g' both vanish at s=±1s = \pm 1. For 0<δ≤δ00 < \delta \le \delta_0 put hδ(x)=δ g ⁣(x−x1δ),hδ′(x)=g′ ⁣(x−x1δ).h_\delta(x) = \delta\, g\!\left( \frac{x - x_1}{\delta} \right), \qquad h_\delta'(x) = g'\!\left( \frac{x - x_1}{\delta} \right). So hδ∈Hh_\delta \in H, with support in [x1−δ,x1+δ][x_1 - \delta, x_1 + \delta].
  3. Size of the three terms. Substitute x=x1+δsx = x_1 + \delta s, so dx=δ dsdx = \delta\, ds. With G1=∫−11g′(s)2 ds=256105G_1 = \int_{-1}^{1} g'(s)^2\, ds = \tfrac{256}{105} and the constant G2=∫−11(2∣gg′∣+g2) dsG_2 = \int_{-1}^{1} \bigl( 2|g g'| + g^2 \bigr)\, ds, ∫abP hδ′2 dx=δ∫−11P(x1+δs) g′(s)2 ds≤−βG1 δ,\int_a^b P\, h_\delta'^2\, dx = \delta \int_{-1}^{1} P(x_1 + \delta s)\, g'(s)^2\, ds \le -\beta G_1\, \delta , because P≤−βP \le -\beta on the support. Since δ≤1\delta \le 1 may be assumed, δ3≤δ2\delta^3 \le \delta^2 and ∣∫ab(2R hδhδ′+S hδ2) dx∣≤M(2δ2∫∣gg′∣ ds+δ3∫g2 ds)≤MG2 δ2.\left| \int_a^b \bigl( 2R\, h_\delta h_\delta' + S\, h_\delta^2 \bigr)\, dx \right| \le M \bigl( 2\delta^2 \textstyle\int |g g'|\, ds + \delta^3 \int g^2\, ds \bigr) \le M G_2\, \delta^2 .
  4. Contradiction. Adding, δ2J[y;hδ]≤δ (−βG1+MG2 δ)\delta^2 J[y; h_\delta] \le \delta\, (-\beta G_1 + M G_2\, \delta), which is negative once δ<βG1/(MG2)\delta < \beta G_1 / (M G_2) (any δ\delta works if M=0M = 0). This contradicts Part 1. Hence P≥0P \ge 0 on [a,b][a, b]. For a weak maximum, apply this to −J-J, whose minimum it is.

Part 3. If FF has continuous third derivatives and y∈C2y \in C^2, the chain rule makes R(x)=Fyy′(x,y(x),y′(x))R(x) = F_{yy'}(x, y(x), y'(x)) continuously differentiable. Since 2hh′=(h2)′2hh' = (h^2)' and h(a)=h(b)=0h(a) = h(b) = 0, integration by parts gives

∫ab2R hh′ dx=[R h2]ab−∫abR′ h2 dx=−∫abR′ h2 dx.\int_a^b 2R\, h h'\, dx = \bigl[ R\, h^2 \bigr]_a^b - \int_a^b R'\, h^2\, dx = - \int_a^b R'\, h^2\, dx .

Substituting this into δ2J\delta^2 J gives ∫ab(Ph′2+(S−R′)h2) dx\int_a^b \bigl( P h'^2 + (S - R') h^2 \bigr)\, dx, which is the claimed form with Q=S−R′Q = S - R'. □\square

RemarkOriginal

Where the hypotheses are used.

  • Second derivatives of FF continuous: this makes φ\varphi twice differentiable (Part 1, step 1) and PP continuous, so that a negative value at one point persists on an interval (Part 2, step 1). Part 2 never integrates by parts, so it needs no third derivatives; only Part 3 does.
  • Weak minimum: used only in Part 1, step 2, for the small multiples εh\varepsilon h of one fixed direction. The bumps hδh_\delta are not small in ∥⋅∥1\|\cdot\|_1, since their slopes stay of size one, but they are never compared with yy directly; only εhδ\varepsilon h_\delta for small ε\varepsilon is.
  • Fixed endpoints: h(a)=h(b)=0h(a) = h(b) = 0 keeps y+εhy + \varepsilon h admissible and removes the boundary term in Part 3.

Necessary, not sufficient. Even the strict inequality Fy′y′>0F_{y'y'} > 0 does not make an extremal a minimum. Take J[y]=∫02π(y′2−y2) dxJ[y] = \int_0^{2\pi} (y'^2 - y^2)\, dx with y(0)=y(2π)=0y(0) = y(2\pi) = 0. Here Fy′y′=2>0F_{y'y'} = 2 > 0 and y≡0y \equiv 0 is an extremal, yet h=sin⁡(x/2)h = \sin(x/2) gives

δ2J[0;h]=2∫02π(14cos⁡2x2−sin⁡2x2) dx=2(π4−π)=−3π2<0.\delta^2 J[0; h] = 2\int_0^{2\pi} \Bigl( \tfrac14 \cos^2 \tfrac{x}{2} - \sin^2 \tfrac{x}{2} \Bigr)\, dx = 2\Bigl( \frac{\pi}{4} - \pi \Bigr) = -\frac{3\pi}{2} < 0 .

Legendre's condition is a statement about single points, so it cannot detect that the interval is too long. That global information is what Jacobi's condition supplies.

ExampleOriginal

A double-well integrand. Let J[y]=∫01(y′2−1)2 dxJ[y] = \int_0^1 (y'^2 - 1)^2\, dx with y(0)=0y(0) = 0 and y(1)=12y(1) = \tfrac12.

The extremal. F=(z2−1)2F = (z^2 - 1)^2 depends only on the slope, so the Euler–Lagrange equation says Fz(y′)F_z(y') is constant. The straight line y0(x)=x/2y_0(x) = x/2 satisfies it and the boundary conditions, and J[y0]=(14−1)2=916J[y_0] = (\tfrac14 - 1)^2 = \tfrac{9}{16}.

Legendre's test. Fzz=12z2−4F_{zz} = 12 z^2 - 4, which at z=12z = \tfrac12 equals 3−4=−1<03 - 4 = -1 < 0. So y0y_0 is not a weak minimum. (Legendre's condition holds only for slopes with ∣z∣≥1/3|z| \ge 1/\sqrt3.)

A direct check. Take h=sin⁡πx∈Hh = \sin \pi x \in H and put u=επcos⁡πxu = \varepsilon \pi \cos \pi x, so (y0+εh)′=12+u(y_0 + \varepsilon h)' = \tfrac12 + u and the integrand is

(u2+u−34)2=u4+2u3−12u2−32u+916.\bigl( u^2 + u - \tfrac34 \bigr)^2 = u^4 + 2u^3 - \tfrac12 u^2 - \tfrac32 u + \tfrac{9}{16}.

Over [0,1][0, 1] the averages of cos⁡πx\cos \pi x and cos⁡3πx\cos^3 \pi x are 00, that of cos⁡2πx\cos^2 \pi x is 12\tfrac12 and that of cos⁡4πx\cos^4 \pi x is 38\tfrac38. Therefore

J[y0+εh]=916−π24 ε2+3π48 ε4.J[y_0 + \varepsilon h] = \frac{9}{16} - \frac{\pi^2}{4}\, \varepsilon^2 + \frac{3\pi^4}{8}\, \varepsilon^4 .

The second derivative at ε=0\varepsilon = 0 is −π2/2-\pi^2/2, which agrees with the formula ∫01Fy′y′h′2 dx=−π2∫01cos⁡2πx dx=−π2/2\int_0^1 F_{y'y'} h'^2\, dx = -\pi^2 \int_0^1 \cos^2 \pi x\, dx = -\pi^2/2. The perturbed curve beats the line whenever 0<∣ε∣<6/(3π)≈0.25990 < |\varepsilon| < \sqrt6/(3\pi) \approx 0.2599. For instance ε=0.1\varepsilon = 0.1 gives J≈0.5625−0.02467+0.00365=0.54148<0.5625J \approx 0.5625 - 0.02467 + 0.00365 = 0.54148 < 0.5625.

ApplicationOriginal
  • Mechanics. For a Lagrangian L=12mq˙2−V(q)L = \tfrac12 m \dot q^2 - V(q) one has Lq˙q˙=m>0L_{\dot q \dot q} = m > 0. So the action can never have a maximum at a nontrivial motion: Legendre's condition for a maximum fails at every point. A true path is either a minimum or a saddle of the action, and which one it is depends on the length of the time interval (see conjugate points).
  • Materials and phase transitions. Energies like the double well (y′2−1)2(y'^2 - 1)^2 model materials with two preferred strains, as in martensitic transformations. Where the imposed average strain lies in the region in which Legendre's condition fails, the material lowers its energy by forming fine mixtures of the two preferred strains (microstructure) instead of deforming uniformly. In several variables the same test becomes the Legendre–Hadamard (strong ellipticity) condition of elasticity; the scalar case is derived in Evans (Evans (2010), §8.1.3, p. 432).

Theorem · advanced

Conjugate points and Jacobi's condition

Adapted

Along an extremal with F_{y'y'} > 0, the second variation is positive definite exactly when the Jacobi equation has no conjugate point, which gives Jacobi's necessary condition and a set of sufficient conditions for a weak minimum.

Prerequisites: The second variation and Legendre's condition, Sturm-Liouville eigenvalue problems, Dependence on initial data and Gronwall's inequality, Structure of linear equations and the Wronskian, Taylor's theorem, Differentiation under the integral sign

DefinitionAdaptedAdapted from Gelfand & Fomin (1963), Ch. 5, §26, p. 106, and §27, Defs 1–2, p. 112

Let J[y]=∫abF(x,y,y′) dxJ[y] = \int_a^b F(x, y, y')\, dx with y(a)=Ay(a) = A, y(b)=By(b) = B, where FF has continuous third partial derivatives, and let y∈C2[a,b]y \in C^2[a, b] be an extremal. As in the second variation, put

P=Fy′y′,Q=Fyy−ddxFyy′P = F_{y'y'}, \qquad Q = F_{yy} - \frac{d}{dx} F_{yy'}

along yy, so that δ2J[y;h]=I[h]\delta^2 J[y; h] = I[h] for h∈H={h∈C1[a,b]:h(a)=h(b)=0}h \in H = \{ h \in C^1[a,b] : h(a) = h(b) = 0 \}, where

I[h]=∫ab(P h′2+Q h2) dx,I[g,k]=∫ab(P g′k′+Q gk) dx.I[h] = \int_a^b \bigl( P\, h'^2 + Q\, h^2 \bigr)\, dx , \qquad I[g, k] = \int_a^b \bigl( P\, g' k' + Q\, g k \bigr)\, dx .

The same two integrals make sense, and define a symmetric bilinear form I[g,k]I[g, k] with I[h]=I[h,h]I[h] = I[h, h], for all continuous, piecewise C1C^1 functions on [a,b][a, b], since their derivatives are bounded with finitely many jumps. The proof of Part 2 uses II on such functions.

Assume the strengthened Legendre condition P>0P > 0 on [a,b][a, b].

The Jacobi equation of JJ along yy is the Euler–Lagrange equation of II:

−(Pu′)′+Qu=0.-(P u')' + Q u = 0 .

We read it as the first-order linear system u′=v/Pu' = v / P, v′=Quv' = Q u for the pair (u,v)=(u,Pu′)(u, v) = (u, P u'). Its coefficients are continuous because P>0P > 0, so by the theory of linear equations each initial value (u(x0),v(x0))(u(x_0), v(x_0)) has exactly one solution on all of [a,b][a, b], and uu and Pu′P u' are C1C^1. Let uau_a be the solution with ua(a)=0u_a(a) = 0 and ua′(a)=1u_a'(a) = 1.

A point c∈(a,b]c \in (a, b] is conjugate to aa if ua(c)=0u_a(c) = 0. Equivalently, some solution that is not identically zero vanishes at both aa and cc, since every solution vanishing at aa is a multiple of uau_a.

TheoremAdaptedAdapted from Gelfand & Fomin (1963), Ch. 5, §26 Thms 1–3, pp. 106–111, §27 (Jacobi's necessary condition), p. 112, and §28 (Theorem), p. 116

Let P,QP, Q be continuous on [a,b][a, b] with P>0P > 0.

  1. (Strong positivity.) If no point of (a,b](a, b] is conjugate to aa, there is α>0\alpha > 0 with

    I[h]≥α2∫abh′2 dxfor all h∈H.I[h] \ge \alpha^2 \int_a^b h'^2\, dx \qquad \text{for all } h \in H .
  2. (Loss of positivity.) If bb is conjugate to aa, then I[ua]=0I[u_a] = 0 with ua∈Hu_a \in H, ua≠0u_a \ne 0. If some c∈(a,b)c \in (a, b) is conjugate to aa, then I[h]<0I[h] < 0 for some h∈Hh \in H.

    Together, 1 and 2 say: I[h]>0I[h] > 0 for all nonzero h∈Hh \in H if and only if no point of (a,b](a, b] is conjugate to aa.

  3. (Jacobi's necessary condition.) If the extremal yy is a weak minimum of JJ and P>0P > 0 on [a,b][a, b], then no point of the open interval (a,b)(a, b) is conjugate to aa.

  4. (Sufficient conditions for a weak minimum.) If y∈C2[a,b]y \in C^2[a, b] is an extremal, P>0P > 0 on [a,b][a, b] and no point of (a,b](a, b] is conjugate to aa, then yy is a strict weak minimum: there is r>0r > 0 such that J[y+h]>J[y]J[y + h] > J[y] for every nonzero h∈Hh \in H with ∥h∥1<r\|h\|_1 < r.

Idea of the proofOriginal

The sign of II is settled by completing the square, an idea due to Legendre. If the Jacobi equation has a solution uu that stays positive on all of [a,b][a, b], the integrand Ph′2+Qh2P h'^2 + Q h^2 equals P (h′−hu′/u)2P\,(h' - h u'/u)^2 plus an exact derivative, so I≥0I \ge 0, with equality only for h=0h = 0. Such a uu exists precisely when uau_a does not vanish again, which is the no-conjugate-point condition. Conversely, if uau_a returns to zero at an interior point cc, then uau_a cut off at cc gives I=0I = 0 but has a corner at cc. Because of the corner, a small perturbation near cc makes II negative, and rounding off the corner afterwards keeps it negative. For sufficiency, a second variation bounded below by α2∫h′2\alpha^2 \int h'^2 dominates the Taylor remainder of JJ for nearby curves.

Proof(Part 1: strong positivity)AdaptedAdapted from Gelfand & Fomin (1963), Ch. 5, §26 Thm 1 and footnote 9, pp. 106–108, and §28, pp. 116–117
  1. Picone's identity. Let P~\tilde P be continuous and positive, and let uu be a solution of −(P~u′)′+Qu=0-(\tilde P u')' + Q u = 0 (in the system sense) with u>0u > 0 on [a,b][a, b]. For h∈Hh \in H, expanding the derivative and using (P~u′)′=Qu(\tilde P u')' = Q u, (P~u′u h2)′=Qh2+2P~u′hh′u−P~u′2h2u2,soP~h′2+Qh2=P~(h′−u′uh)2+(P~u′u h2)′.\Bigl( \frac{\tilde P u'}{u}\, h^2 \Bigr)' = Q h^2 + \frac{2 \tilde P u' h h'}{u} - \frac{\tilde P u'^2 h^2}{u^2}, \qquad\text{so}\qquad \tilde P h'^2 + Q h^2 = \tilde P \Bigl( h' - \frac{u'}{u} h \Bigr)^2 + \Bigl( \frac{\tilde P u'}{u}\, h^2 \Bigr)' . Integrating over [a,b][a, b], the exact derivative contributes nothing because h(a)=h(b)=0h(a) = h(b) = 0. Hence ∫ab(P~h′2+Qh2) dx=∫abP~ (h′−hu′/u)2 dx≥0\int_a^b (\tilde P h'^2 + Q h^2)\, dx = \int_a^b \tilde P\, (h' - h u'/u)^2\, dx \ge 0.
  2. A positive solution of the Jacobi equation. Assume no point of (a,b](a, b] is conjugate to aa. Then ua>0u_a > 0 on (a,b](a, b]: it is positive just to the right of aa because ua′(a)=1u_a'(a) = 1, and by the intermediate value theorem it cannot become negative without a zero. Let u1u_1 be the solution with u1(a)=1u_1(a) = 1, (Pu1′)(a)=0(P u_1')(a) = 0. By continuity choose η>0\eta > 0 with ua′≥12u_a' \ge \tfrac12 and u1≥12u_1 \ge \tfrac12 on [a,a+η][a, a + \eta]. Put m=min⁡[a+η,b]ua>0m = \min_{[a + \eta, b]} u_a > 0, K=max⁡[a,b]∣u1∣≥1K = \max_{[a,b]} |u_1| \ge 1 and ϵ=m/(2K)\epsilon = m / (2K). Then u=ua+ϵu1u = u_a + \epsilon u_1 is positive on all of [a,b][a, b]: on [a,a+η][a, a + \eta] because ua≥0u_a \ge 0 and ϵu1≥ϵ/2\epsilon u_1 \ge \epsilon/2, and on [a+η,b][a + \eta, b] because u≥m−ϵK=m/2u \ge m - \epsilon K = m/2.
  3. Perturbing PP. For 0≤α2≤12min⁡P0 \le \alpha^2 \le \tfrac12 \min P, let u(α)u^{(\alpha)} be the solution of −((P−α2)w′)′+Qw=0-((P - \alpha^2) w')' + Q w = 0 with the same initial data as uu at aa: w(a)=ϵw(a) = \epsilon, ((P−α2)w′)(a)=P(a)((P - \alpha^2) w')(a) = P(a). In system form the coefficients 1/(P−α2)1/(P - \alpha^2) and QQ depend continuously on (x,α)(x, \alpha). By continuous dependence on parameters, u(α)→u(0)=uu^{(\alpha)} \to u^{(0)} = u uniformly on [a,b][a, b] as α→0\alpha \to 0. Since min⁡u>0\min u > 0, there is α>0\alpha > 0 with u(α)>0u^{(\alpha)} > 0 on [a,b][a, b].
  4. Conclusion. Step 1 with P~=P−α2>0\tilde P = P - \alpha^2 > 0 and the solution u(α)u^{(\alpha)} gives ∫ab((P−α2)h′2+Qh2) dx≥0\int_a^b \bigl( (P - \alpha^2) h'^2 + Q h^2 \bigr)\, dx \ge 0, that is, I[h]≥α2∫abh′2 dxI[h] \ge \alpha^2 \int_a^b h'^2\, dx. □\square
Proof(Part 2: loss of positivity)AdaptedAdapted from do Carmo (2016), §5-9, Lemma 2 and Thm 2, pp. 427–429
  1. The Jacobi solution has zero energy between its zeros. Let c∈(a,b]c \in (a, b] be conjugate to aa. Since Pua′P u_a' is C1C^1, integration by parts on [a,c][a, c] gives ∫ac(Pua′2+Qua2) dx=[Pua′ua]ac+∫acua(−(Pua′)′+Qua) dx=0,\int_a^c \bigl( P u_a'^2 + Q u_a^2 \bigr)\, dx = \bigl[ P u_a' u_a \bigr]_a^c + \int_a^c u_a \bigl( -(P u_a')' + Q u_a \bigr)\, dx = 0 , because ua(a)=ua(c)=0u_a(a) = u_a(c) = 0 and uau_a solves the Jacobi equation. If c=bc = b, then ua∈Hu_a \in H, ua≠0u_a \ne 0 and I[ua]=0I[u_a] = 0.
  2. Cutting off at an interior conjugate point. Now let c∈(a,b)c \in (a, b). Define h^=ua\hat h = u_a on [a,c][a, c] and h^=0\hat h = 0 on [c,b][c, b]. It is continuous and C1C^1 on each piece, and I[h^]=0I[\hat h] = 0 by step 1. Moreover ua′(c)≠0u_a'(c) \ne 0: otherwise (ua,Pua′)(u_a, P u_a') would vanish at cc, and uniqueness for the system would force ua≡0u_a \equiv 0. So h^\hat h has a genuine corner at cc.
  3. Pushing below zero. Take w∈Hw \in H with w(c)=1w(c) = 1, for instance a C1C^1 bump supported in (a,b)(a, b). Integrating by parts on [a,c][a, c] exactly as in step 1, I[h^,w]=∫ac(Pua′w′+Quaw) dx=[Pua′w]ac=P(c) ua′(c)≠0.I[\hat h, w] = \int_a^c \bigl( P u_a' w' + Q u_a w \bigr)\, dx = \bigl[ P u_a' w \bigr]_a^c = P(c)\, u_a'(c) \ne 0 . For real tt, bilinearity gives I[h^−tw]=−2t P(c)ua′(c)+t2I[w]I[\hat h - t w] = -2t\, P(c) u_a'(c) + t^2 I[w]. Choosing tt small, with the sign of P(c)ua′(c)P(c) u_a'(c), makes this negative. The function g=h^−twg = \hat h - t w vanishes at aa and bb and is C1C^1 except at cc.
  4. Rounding the corner (smoothing lemma). Let gg be continuous on [a,b][a, b], C1C^1 on [a,c][a, c] and on [c,b][c, b], with g(a)=g(b)=0g(a) = g(b) = 0, and let G=sup⁡∣g′∣G = \sup |g'|. For small δ>0\delta > 0 let kδ=g′k_\delta = g' outside (c−δ,c+δ)(c - \delta, c + \delta) and let kδk_\delta be linear on that interval, joining g′(c−δ)g'(c - \delta) to g′(c+δ)g'(c + \delta). Then kδk_\delta is continuous, ∣kδ∣≤G|k_\delta| \le G, and kδk_\delta differs from g′g' only on a set of length 2δ2\delta, so ∫ab∣kδ−g′∣ dx≤4Gδ\int_a^b |k_\delta - g'|\, dx \le 4G\delta. Put gδ(x)=∫axkδ dt−x−ab−a∫abkδ dt.g_\delta(x) = \int_a^x k_\delta\, dt - \frac{x - a}{b - a} \int_a^b k_\delta\, dt . Then gδ∈Hg_\delta \in H. Since ∫abg′ dx=g(b)−g(a)=0\int_a^b g'\, dx = g(b) - g(a) = 0, the correction term is at most 4Gδ4G\delta in size, so gδ→gg_\delta \to g uniformly and ∫ab(gδ′−g′)2 dx→0\int_a^b (g_\delta' - g')^2\, dx \to 0 as δ→0\delta \to 0. Because PP and QQ are bounded, the Cauchy–Schwarz inequality applied to I[g]−I[gδ]=I[g−gδ, g+gδ]I[g] - I[g_\delta] = I[g - g_\delta,\, g + g_\delta] shows I[gδ]→I[g]<0I[g_\delta] \to I[g] < 0. So I[gδ]<0I[g_\delta] < 0 for small δ\delta, with gδ∈Hg_\delta \in H. □\square
Proof(Parts 3 and 4: Jacobi's condition and sufficiency)AdaptedAdapted from Gelfand & Fomin (1963), Ch. 5, §27, p. 112, and §28, pp. 116–117

Part 3. If yy is a weak minimum, the second-order necessary condition gives I[h]=δ2J[y;h]≥0I[h] = \delta^2 J[y; h] \ge 0 for every h∈Hh \in H. A point of (a,b)(a, b) conjugate to aa would produce h∈Hh \in H with I[h]<0I[h] < 0 by Part 2. So there is none.

Part 4. Let α\alpha be as in Part 1, and fix a nonzero h∈Hh \in H with ∥h∥1≤ρ≤1\|h\|_1 \le \rho \le 1, where ρ\rho is chosen below. Put φ(t)=J[y+th]\varphi(t) = J[y + t h].

  1. Taylor expansion. As in the second-variation unit, φ\varphi is C2C^2 (we may differentiate under the integral twice), with φ′′(t)\varphi''(t) given by the second-variation integral at the curve y+thy + t h. Taylor's formula with integral remainder gives J[y+h]−J[y]=φ′(0)+∫01(1−t) φ′′(t) dt=12 I[h]+∫01(1−t)(φ′′(t)−φ′′(0)) dt.J[y + h] - J[y] = \varphi'(0) + \int_0^1 (1 - t)\, \varphi''(t)\, dt = \tfrac12\, I[h] + \int_0^1 (1 - t) \bigl( \varphi''(t) - \varphi''(0) \bigr)\, dt . Here φ′(0)=0\varphi'(0) = 0 because yy is an extremal, and φ′′(0)=I[h]\varphi''(0) = I[h].
  2. Controlling the remainder. The second derivatives Fyy,Fyy′,Fy′y′F_{yy}, F_{yy'}, F_{y'y'} are uniformly continuous on the compact set {(x,y(x)+s,y′(x)+σ):x∈[a,b], ∣s∣,∣σ∣≤1}\{ (x, y(x) + s, y'(x) + \sigma) : x \in [a,b],\ |s|, |\sigma| \le 1 \}. Let ω(ρ)\omega(\rho) be the largest change of any of them when ∣s∣,∣σ∣≤ρ|s|, |\sigma| \le \rho; then ω(ρ)→0\omega(\rho) \to 0 as ρ→0\rho \to 0. For t∈[0,1]t \in [0, 1], ∣φ′′(t)−φ′′(0)∣≤ω(ρ)∫ab(h2+2∣hh′∣+h′2) dx≤2ω(ρ)∫ab(h2+h′2) dx|\varphi''(t) - \varphi''(0)| \le \omega(\rho) \int_a^b (h^2 + 2|h h'| + h'^2)\, dx \le 2\omega(\rho) \int_a^b (h^2 + h'^2)\, dx.
  3. A Poincaré inequality. Since h(a)=0h(a) = 0, Cauchy–Schwarz gives h(x)2=(∫axh′)2≤(x−a)∫abh′2h(x)^2 = \bigl( \int_a^x h' \bigr)^2 \le (x - a) \int_a^b h'^2, and integrating, ∫abh2≤12(b−a)2∫abh′2\int_a^b h^2 \le \tfrac12 (b - a)^2 \int_a^b h'^2. With C=1+12(b−a)2C = 1 + \tfrac12 (b - a)^2 and ∫01(1−t) dt=12\int_0^1 (1 - t)\, dt = \tfrac12, steps 1 and 2 and Part 1 give J[y+h]−J[y]≥(α22−C ω(ρ))∫abh′2 dx.J[y + h] - J[y] \ge \Bigl( \frac{\alpha^2}{2} - C\, \omega(\rho) \Bigr) \int_a^b h'^2\, dx .
  4. Conclusion. Choose ρ≤1\rho \le 1 with C ω(ρ)<α2/2C\,\omega(\rho) < \alpha^2/2. A nonzero h∈Hh \in H has ∫h′2>0\int h'^2 > 0 (otherwise hh would be constant, hence 00), so J[y+h]>J[y]J[y + h] > J[y] whenever 0<∥h∥1<ρ0 < \|h\|_1 < \rho. □\square
RemarkOriginal

Where the hypotheses are used.

  • P>0P > 0 on the closed interval. It turns the Jacobi equation into a regular linear system, so that uau_a exists and has isolated zeros with ua′≠0u_a' \ne 0 there (Part 2, step 2). It also makes the square in Picone's identity nonnegative, and it leaves room to subtract α2\alpha^2 (Part 1, step 3). Where PP vanishes the Jacobi equation is singular, and conjugate points need a separate analysis.
  • The endpoint bb. Sufficiency asks that bb itself not be conjugate; necessity only excludes the open interval. The gap is real. For J[y]=∫0π(y′2−y2) dxJ[y] = \int_0^\pi (y'^2 - y^2)\, dx with y(0)=y(π)=0y(0) = y(\pi) = 0, the Jacobi equation is −2u′′−2u=0-2u'' - 2u = 0, so ua=sin⁡xu_a = \sin x and b=πb = \pi is conjugate. Here y≡0y \equiv 0 is a minimum, because J[h]=12I[h]=∫0π(h′2−h2) dx≥0J[h] = \tfrac12 I[h] = \int_0^\pi (h'^2 - h^2)\, dx \ge 0 for h∈Hh \in H. To see this, apply Picone's identity (Part 1, step 1) with P~=1\tilde P = 1 and u=sin⁡xu = \sin x on [ε,π−ε][\varepsilon, \pi - \varepsilon]: the integral there is ∫(h′−hcot⁡x)2 dx≥0\int (h' - h \cot x)^2\, dx \ge 0 plus the boundary values of h2cot⁡xh^2 \cot x, and these tend to 00 as ε→0\varepsilon \to 0 because ∣h(x)∣≤max⁡∣h′∣⋅min⁡(x,π−x)|h(x)| \le \max|h'| \cdot \min(x, \pi - x). (This is the statement that the lowest Dirichlet eigenvalue of −u′′-u'' on [0,π][0, \pi] is 11; see the variational characterization of eigenvalues.) The minimum is not a strict one: J[εsin⁡x]=0=J[0]J[\varepsilon \sin x] = 0 = J[0]. On a longer interval [0,ℓ][0, \ell] with ℓ>π\ell > \pi, the conjugate point π\pi is interior, and indeed J[sin⁡(πx/ℓ)]=ℓ2(π2/ℓ2−1)<0J[\sin(\pi x/\ell)] = \tfrac{\ell}{2}\bigl( \pi^2/\ell^2 - 1 \bigr) < 0.
  • Extremal. Used only to remove φ′(0)\varphi'(0) in Part 4.
  • Weak, not strong. Part 4 compares yy only with curves whose slopes are close to y′y'. A minimum against all curves close in value alone (a strong minimum) needs further conditions, such as Weierstrass's condition, which this unit does not treat.

Conjugate points and neighbouring extremals. Suppose y(x;s)y(x; s) is a smooth family of extremals through the point (a,A)(a, A), with y(x;0)=y(x)y(x; 0) = y(x). Differentiating the Euler–Lagrange equation in ss at s=0s = 0 shows that ∂sy(x;0)\partial_s y(x; 0) solves the Jacobi equation and vanishes at aa. So a conjugate point is where extremals leaving (a,A)(a, A) with slightly different slopes come back, to first order, to meet yy (Gelfand & Fomin (1963), §27, pp. 112–115). A point cc is conjugate to aa exactly when 00 is an eigenvalue of the Sturm–Liouville problem −(Pu′)′+Qu=μu-(P u')' + Q u = \mu u on [a,c][a, c] with u(a)=u(c)=0u(a) = u(c) = 0.

ExampleOriginal

When does a catenary minimize? Take F=y1+y′2F = y\sqrt{1 + y'^2}. Up to a factor 2π2\pi, JJ is then the area of the surface swept out by rotating the curve about the xx-axis (a soap film between two coaxial rings). Consider the arc of y=cosh⁡xy = \cosh x starting at a=−1a = -1.

Extremal. Fy=1+y′2=cosh⁡xF_y = \sqrt{1 + y'^2} = \cosh x and Fy′=yy′/1+y′2=sinh⁡xF_{y'} = y y'/\sqrt{1 + y'^2} = \sinh x, whose derivative is cosh⁡x=Fy\cosh x = F_y. So y=cosh⁡xy = \cosh x satisfies the Euler–Lagrange equation.

Coefficients. Along the curve 1+y′2=cosh⁡2x1 + y'^2 = \cosh^2 x, and

P=y(1+y′2)3/2=1cosh⁡2x>0,Fyy=0,Fyy′=y′1+y′2=tanh⁡x,Q=−1cosh⁡2x.P = \frac{y}{(1 + y'^2)^{3/2}} = \frac{1}{\cosh^2 x} > 0, \qquad F_{yy} = 0, \qquad F_{yy'} = \frac{y'}{\sqrt{1 + y'^2}} = \tanh x, \qquad Q = -\frac{1}{\cosh^2 x}.

So the Jacobi equation is (h′/cosh⁡2x)′+h/cosh⁡2x=0\bigl( h'/\cosh^2 x \bigr)' + h/\cosh^2 x = 0.

Two solutions from two families of catenaries. Translating, cosh⁡(x−d)\cosh(x - d), and rescaling, scosh⁡(x/s)s \cosh(x/s), give families of extremals. Their dd- and ss-derivatives at d=0d = 0, s=1s = 1 suggest h1=sinh⁡xh_1 = \sinh x and h2=cosh⁡x−xsinh⁡xh_2 = \cosh x - x \sinh x. Direct substitution confirms both. For h1h_1: h1′/cosh⁡2x=1/cosh⁡xh_1'/\cosh^2 x = 1/\cosh x, whose derivative −tanh⁡x/cosh⁡x-\tanh x/\cosh x cancels h1/cosh⁡2x=tanh⁡x/cosh⁡xh_1/\cosh^2 x = \tanh x/\cosh x. For h2h_2: h2′=−xcosh⁡xh_2' = -x\cosh x, and (−x/cosh⁡x)′=−1/cosh⁡x+xtanh⁡x/cosh⁡x(-x/\cosh x)' = -1/\cosh x + x \tanh x/\cosh x cancels h2/cosh⁡2x=1/cosh⁡x−xtanh⁡x/cosh⁡xh_2/\cosh^2 x = 1/\cosh x - x\tanh x/\cosh x. Their Wronskian is h1h2′−h1′h2=−cosh⁡2x≠0h_1 h_2' - h_1' h_2 = -\cosh^2 x \ne 0, so they are independent.

The conjugate point. The solution with u(a)=0u(a) = 0, u′(a)=1u'(a) = 1 is

ua(x)=h1(x) h2(a)−h2(x) h1(a)cosh⁡2a,u_a(x) = \frac{h_1(x)\, h_2(a) - h_2(x)\, h_1(a)}{\cosh^2 a},

since the numerator has derivative cosh⁡2a\cosh^2 a at x=ax = a. For a<0a < 0 we have ua(0)=−sinh⁡a/cosh⁡2a>0u_a(0) = -\sinh a/\cosh^2 a > 0. For x≠0x \ne 0, dividing by sinh⁡asinh⁡x\sinh a \sinh x shows that ua(x)=0u_a(x) = 0 exactly when

coth⁡x−x=coth⁡a−a.\coth x - x = \coth a - a .

The function coth⁡t−t\coth t - t has derivative −1/sinh⁡2t−1<0-1/\sinh^2 t - 1 < 0, so it is strictly decreasing on (−∞,0)(-\infty, 0) and on (0,∞)(0, \infty). On (a,0)(a, 0) it stays below its value at aa, so there is no zero there. On (0,∞)(0, \infty) it falls from +∞+\infty to −∞-\infty, so there is exactly one zero. For a=−1a = -1, coth⁡(−1)+1≈−0.313035\coth(-1) + 1 \approx -0.313035, and solving numerically gives the conjugate point c≈1.433605c \approx 1.433605.

Verdict. Write c=1.433605…c = 1.433605\ldots for the conjugate point found above. By Part 4, the arc of cosh⁡x\cosh x over [−1,b][-1, b] is a strict weak minimum of the area when b<cb < c. By Part 3, it is not even a weak minimum when b>cb > c. As a check, the tangent to cosh⁡x\cosh x at tt meets the xx-axis at t−coth⁡tt - \coth t. This is 0.3130350.313035 both for t=−1t = -1 and for t=ct = c, so the tangents at a point and at its conjugate point meet on the axis, a classical property of the catenary.

ApplicationOriginal
  • Least action is only stationary action. For a harmonic oscillator, L=12m(q˙2−ω2q2)L = \tfrac12 m(\dot q^2 - \omega^2 q^2), the Jacobi equation is the equation of motion itself, and ua=sin⁡(ω(t−a))/ωu_a = \sin(\omega(t - a))/\omega. The first conjugate time is half a period, π/ω\pi/\omega. A true motion minimizes the action over a time interval shorter than π/ω\pi/\omega but is a saddle over a longer one.
  • Geodesics. On a sphere the point conjugate to MM along a great circle is the antipode of MM (Gelfand & Fomin (1963), §27, p. 115), so a great-circle arc longer than a half-circle is not even a local minimum of length. In optics and gravitational lensing, conjugate points are the foci and caustics where neighbouring rays cross.
  • Counting instabilities. For an extremal with P>0P > 0, the number of points conjugate to aa in (a,b)(a, b) equals the number of negative eigenvalues of the second variation (Morse index theorem, stated here without proof). Engineers use this to count unstable buckling modes, and physicists to count unstable fluctuation modes about a classical solution.

Variational eigenvalue problems and direct methods

2

Theorem

Variational characterization of eigenvalues

Adapted

The eigenvalues of a regular Sturm-Liouville problem are the successive minima of the Rayleigh quotient, and each one is also a min-max over subspaces, which gives upper bounds and comparison theorems without solving the equation.

Prerequisites: Isoperimetric problems, Sturm-Liouville eigenvalue problems, Eigenfunction expansions

DefinitionAdaptedAdapted from Strauss (2008), §11.1, p. 300, and §11.4, p. 314

Consider the regular Sturm–Liouville problem with Dirichlet conditions

−(pu′)′+qu=λ w uon [a,b],u(a)=u(b)=0,-(p u')' + q u = \lambda\, w\, u \quad \text{on } [a, b], \qquad u(a) = u(b) = 0,

where p∈C1[a,b]p \in C^1[a, b], q,w∈C[a,b]q, w \in C[a, b], and p>0p > 0, w>0w > 0 on [a,b][a, b]. Write (u,v)w=∫abw u v dx(u, v)_w = \int_a^b w\, u\, v\, dx and ∥u∥w2=(u,u)w\|u\|_w^2 = (u, u)_w. By Sturm–Liouville theory and the expansion theorem, the eigenvalues are real and simple and form a sequence λ1<λ2<⋯→∞\lambda_1 < \lambda_2 < \cdots \to \infty. Their eigenfunctions φn\varphi_n can be chosen real, in C2C^2, with (φm,φn)w=δmn(\varphi_m, \varphi_n)_w = \delta_{mn}, and complete: every continuous uu satisfies Parseval's identity ∑n(u,φn)w2=∥u∥w2\sum_n (u, \varphi_n)_w^2 = \|u\|_w^2.

A trial function is a continuous, piecewise C1C^1 function uu on [a,b][a, b] with u(a)=u(b)=0u(a) = u(b) = 0 and u≢0u \not\equiv 0. Let A\mathcal{A} be the set of trial functions together with 00; it is a vector space. The energy and the Rayleigh quotient are

D[u,v]=∫ab(p u′v′+q uv) dx,D[u]=D[u,u],R[u]=D[u]∥u∥w2.D[u, v] = \int_a^b \bigl( p\, u' v' + q\, u v \bigr)\, dx, \qquad D[u] = D[u, u], \qquad \mathcal{R}[u] = \frac{D[u]}{\|u\|_w^2} .
TheoremAdaptedAdapted from Strauss (2008), §11.1 Thms 1–2, pp. 301–303, and §11.2 Thm 1 (minimax principle), pp. 307–308

Under the hypotheses above:

  1. (Ground state.) R[u]≥λ1\mathcal{R}[u] \ge \lambda_1 for every trial function uu, with equality exactly when uu is a multiple of φ1\varphi_1. So λ1=min⁡R\lambda_1 = \min \mathcal{R}.
  2. (Higher eigenvalues.) If uu is a trial function with (u,φk)w=0(u, \varphi_k)_w = 0 for k=1,…,n−1k = 1, \dots, n - 1, then R[u]≥λn\mathcal{R}[u] \ge \lambda_n, with equality exactly when uu is a multiple of φn\varphi_n.
  3. (Courant–Fischer min-max.) For each nn, λn=min⁡V⊂Adim⁡V=n max⁡u∈V∖{0}R[u],\lambda_n = \min_{\substack{V \subset \mathcal{A} \\ \dim V = n}} \ \max_{u \in V \setminus \{0\}} \mathcal{R}[u], and the minimum is attained at V=span⁡{φ1,…,φn}V = \operatorname{span}\{\varphi_1, \dots, \varphi_n\}. Equivalently, λn\lambda_n is the largest value, over all choices of n−1n - 1 continuous functions v1,…,vn−1v_1, \dots, v_{n-1} on [a,b][a, b], of the infimum of R\mathcal{R} over trial functions ww-orthogonal to all vkv_k. The largest value is attained at vk=φkv_k = \varphi_k, where the infimum is a minimum (this form is stated here without proof).
Idea of the proofAdaptedAdapted from Gelfand & Fomin (1963), §41.1, p. 198; Riley, Hobson & Bence (2006), §22.6, pp. 791–792, and §22.7, p. 793

Minimizing the energy D[u]D[u] subject to ∥u∥w2=1\|u\|_w^2 = 1 is an isoperimetric problem. Its Euler–Lagrange equation with multiplier λ\lambda is exactly −(pu′)′+qu=λwu-(p u')' + q u = \lambda w u, and multiplying by uu and integrating shows that the minimum value equals the multiplier. So a minimizer, if one exists, is an eigenfunction, and the minimum is an eigenvalue. To avoid the question of existence, the proof goes the other way. We expand an arbitrary trial function in eigenfunctions, with coefficients cnc_n. Then the energy is at least ∑λncn2\sum \lambda_n c_n^2 while the norm is ∑cn2\sum c_n^2, so the quotient is at least a weighted average of the eigenvalues, and hence at least the smallest one.

ProofAdaptedAdapted from Strauss (2008), §11.3, proof of Thm 2, pp. 311–313, and §11.2, proof of Thm 1, p. 308
  1. Energy against an eigenfunction. For u∈Au \in \mathcal{A} and every nn, D[u,φn]=λn (u,φn)w.D[u, \varphi_n] = \lambda_n\, (u, \varphi_n)_w . Integrate ∫p u′φn′\int p\, u' \varphi_n' by parts on each interval where uu is C1C^1. The interior boundary terms cancel because uu and pφn′p \varphi_n' are continuous, and the end terms vanish because u(a)=u(b)=0u(a) = u(b) = 0. This leaves D[u,φn]=∫abu (−(pφn′)′+qφn) dx=λn∫abw u φn dxD[u, \varphi_n] = \int_a^b u\, \bigl( -(p \varphi_n')' + q \varphi_n \bigr)\, dx = \lambda_n \int_a^b w\, u\, \varphi_n\, dx. In particular D[φm,φn]=λnδmnD[\varphi_m, \varphi_n] = \lambda_n \delta_{mn}.
  2. Making the energy nonnegative. Pick κ≥0\kappa \ge 0 with q+κw≥0q + \kappa w \ge 0 on [a,b][a, b], possible because ww has a positive minimum. Then Dκ[u]=D[u]+κ∥u∥w2=∫(pu′2+(q+κw)u2) dx≥0D_\kappa[u] = D[u] + \kappa \|u\|_w^2 = \int (p u'^2 + (q + \kappa w) u^2)\, dx \ge 0 for all u∈Au \in \mathcal{A}, since p>0p > 0. Step 1 holds for DκD_\kappa with λn+κ\lambda_n + \kappa in place of λn\lambda_n.
  3. The energy dominates partial sums. For a trial function uu let cn=(u,φn)wc_n = (u, \varphi_n)_w and uN=∑n≤Ncnφnu_N = \sum_{n \le N} c_n \varphi_n, which lies in A\mathcal{A}. Expanding by bilinearity and using step 1 with orthonormality, 0≤Dκ[u−uN]=Dκ[u]−2∑n≤Ncn(λn+κ)cn+∑n≤N(λn+κ)cn2=Dκ[u]−∑n≤N(λn+κ) cn2.0 \le D_\kappa[u - u_N] = D_\kappa[u] - 2\sum_{n \le N} c_n (\lambda_n + \kappa) c_n + \sum_{n \le N} (\lambda_n + \kappa) c_n^2 = D_\kappa[u] - \sum_{n \le N} (\lambda_n + \kappa)\, c_n^2 .
  4. Parts 1 and 2. Suppose ck=0c_k = 0 for k<nk < n (no condition when n=1n = 1). Since λk≥λn\lambda_k \ge \lambda_n for k≥nk \ge n, step 3 gives Dκ[u]≥(λn+κ)∑k≤Nck2D_\kappa[u] \ge (\lambda_n + \kappa) \sum_{k \le N} c_k^2. Letting N→∞N \to \infty and using Parseval, Dκ[u]≥(λn+κ)∥u∥w2D_\kappa[u] \ge (\lambda_n + \kappa) \|u\|_w^2, that is, R[u]≥λn\mathcal{R}[u] \ge \lambda_n. The value at φn\varphi_n is D[φn]=λnD[\varphi_n] = \lambda_n by step 1, so the bound is attained.
  5. Equality. If R[u]=λn\mathcal{R}[u] = \lambda_n, then splitting off the gap λn+1−λn>0\lambda_{n+1} - \lambda_n > 0 in step 3 gives (λn+κ)∥u∥w2≥(λn+κ)∑k≤Nck2+(λn+1−λn)∑n<k≤Nck2.(\lambda_n + \kappa)\|u\|_w^2 \ge (\lambda_n + \kappa) \sum_{k \le N} c_k^2 + (\lambda_{n+1} - \lambda_n) \sum_{n < k \le N} c_k^2 . As N→∞N \to \infty the first sum tends to ∥u∥w2\|u\|_w^2, so ck=0c_k = 0 for all k>nk > n. By Parseval ∥u−cnφn∥w2=∑k≠nck2=0\|u - c_n \varphi_n\|_w^2 = \sum_{k \ne n} c_k^2 = 0. Since w>0w > 0 and both functions are continuous, u=cnφnu = c_n \varphi_n. Simplicity of the eigenvalues, which makes the gap positive, is used here.
  6. Part 3, lower bound. Let V⊂AV \subset \mathcal{A} have dimension nn. The n−1n - 1 linear conditions (u,φk)w=0(u, \varphi_k)_w = 0, k<nk < n, on the nn-dimensional space VV have a nonzero solution uu, and Part 2 gives max⁡VR≥R[u]≥λn\max_V \mathcal{R} \ge \mathcal{R}[u] \ge \lambda_n. The maximum exists: since w>0w > 0 and the elements of VV are continuous, ∥⋅∥w\|\cdot\|_w is a norm on VV, and R\mathcal{R} is unchanged by scaling, so it suffices to maximize the continuous function DD on the unit sphere of VV, which is compact because VV is finite-dimensional.
  7. Part 3, attainment. For u=∑k≤ndkφk≠0u = \sum_{k \le n} d_k \varphi_k \ne 0, step 1 gives D[u]=∑k≤nλkdk2D[u] = \sum_{k \le n} \lambda_k d_k^2 and ∥u∥w2=∑k≤ndk2\|u\|_w^2 = \sum_{k \le n} d_k^2. So R[u]≤λn\mathcal{R}[u] \le \lambda_n, with equality at u=φnu = \varphi_n. Hence max⁡VR=λn\max_V \mathcal{R} = \lambda_n for V=span⁡{φ1,…,φn}V = \operatorname{span}\{\varphi_1, \dots, \varphi_n\}. □\square
RemarkOriginal

Where the hypotheses are used.

  • Boundary conditions. They kill the end terms in step 1. If a trial function violates them, the bound fails. For −u′′=λu-u'' = \lambda u on [0,π][0, \pi] with u(0)=u(π)=0u(0) = u(\pi) = 0 we have λ1=1\lambda_1 = 1, but the constant u=1u = 1, which is not a trial function, gives R=0\mathcal{R} = 0.
  • Completeness (Parseval) turns the partial-sum inequality of step 3 into a statement about uu itself (steps 4–5). Without it, a trial function with a component outside the span of the eigenfunctions would escape the argument.
  • p>0p > 0 and w>0w > 0: p>0p > 0 makes DκD_\kappa nonnegative (step 2), and w>0w > 0 makes (⋅,⋅)w(\cdot,\cdot)_w an inner product, so that zero norm forces zero function (step 5). They also underlie the regular Sturm–Liouville theory quoted in the definition.
  • Simplicity of the eigenvalues is used only for the equality cases.

Other boundary conditions. For a Robin condition pu′=σup u' = \sigma u at bb (with σ\sigma a constant), the Rayleigh quotient acquires the boundary term −σu(b)2-\sigma u(b)^2 in DD, and trial functions need not satisfy any condition at bb. For the Neumann condition u′(b)=0u'(b) = 0, trial functions are simply free at bb: the condition is a natural boundary condition, produced by the minimization itself (Strauss (2008), §11.3 Thm 1, p. 310, and §11.4, p. 315).

Comparison. Since every λn\lambda_n is a min-max of R\mathcal{R}, a change that does not lower R[u]\mathcal{R}[u] for any trial function does not lower any eigenvalue. This applies to increasing pp or qq, and to shrinking the interval (a trial function on a subinterval, extended by zero, is a trial function on the larger one). Decreasing ww raises R[u]\mathcal{R}[u] only when D[u]>0D[u] > 0. So it does not lower any eigenvalue when q≥0q \ge 0, because then D[u]≥∫abp u′2 dx>0D[u] \ge \int_a^b p\, u'^2\, dx > 0 for every trial function (u′≢0u' \not\equiv 0, since uu vanishes at aa and is not identically zero). Without q≥0q \ge 0 this fails: −u′′−100u=λwu-u'' - 100 u = \lambda w u on [0,π][0, \pi] with Dirichlet conditions has eigenfunctions sin⁡nx\sin nx, with λ1=−99\lambda_1 = -99 for w=1w = 1 but λ1=−198\lambda_1 = -198 for w=12w = \tfrac12. The min-max gives only non-strict inequalities in all these comparisons.

ExampleOriginal

A string with linearly increasing density. Take −u′′=λ(1+x)u-u'' = \lambda (1 + x) u on [0,1][0, 1] with u(0)=u(1)=0u(0) = u(1) = 0, so p=1p = 1, q=0q = 0 and w=1+xw = 1 + x.

Two-sided bounds from min-max. For every trial function, ∫u2≤∫(1+x)u2≤2∫u2\int u^2 \le \int (1 + x) u^2 \le 2 \int u^2, so

12 R1[u]≤R[u]≤R1[u],\tfrac12\, \mathcal{R}_1[u] \le \mathcal{R}[u] \le \mathcal{R}_1[u],

where R1\mathcal{R}_1 is the quotient for −u′′=λu-u'' = \lambda u, whose eigenvalues are n2π2n^2 \pi^2. Taking the min-max of each side gives

12 n2π2≤λn≤n2π2,so4.935≤λ1≤9.870.\tfrac12\, n^2 \pi^2 \le \lambda_n \le n^2 \pi^2, \qquad \text{so} \qquad 4.935 \le \lambda_1 \le 9.870 .

A sharper upper bound from one trial function. With u=sin⁡πxu = \sin \pi x: ∫01u′2 dx=π2/2\int_0^1 u'^2\, dx = \pi^2/2, and since ∫01xsin⁡2πx dx=14\int_0^1 x \sin^2 \pi x\, dx = \tfrac14, the weighted norm is ∫01(1+x)sin⁡2πx dx=12+14=34\int_0^1 (1 + x) \sin^2 \pi x\, dx = \tfrac12 + \tfrac14 = \tfrac34. Hence

λ1≤R[sin⁡πx]=π2/23/4=2π23≈6.5797.\lambda_1 \le \mathcal{R}[\sin \pi x] = \frac{\pi^2/2}{3/4} = \frac{2\pi^2}{3} \approx 6.5797 .

The exact value is λ1≈6.5484\lambda_1 \approx 6.5484 (found by shooting: integrate from x=0x = 0 with u(0)=0u(0) = 0, u′(0)=1u'(0) = 1 and adjust λ\lambda until u(1)=0u(1) = 0). The bound is 0.5%0.5\% high.

A warning about higher eigenvalues. The same computation with sin⁡2πx\sin 2\pi x gives R=(2π2)/(3/4)=8π2/3≈26.319\mathcal{R} = (2\pi^2)/(3/4) = 8\pi^2/3 \approx 26.319, while λ2≈26.465\lambda_2 \approx 26.465. The quotient is below λ2\lambda_2. There is no contradiction: sin⁡2πx\sin 2\pi x is not ww-orthogonal to φ1\varphi_1, so Part 2 does not apply, and Part 1 only guarantees 26.319≥λ126.319 \ge \lambda_1. Upper bounds for λ2\lambda_2 need a two-dimensional space of trial functions, as in the Rayleigh–Ritz method.

ApplicationOriginal
  • Vibrations. For a string or a membrane the eigenvalues are squared frequencies, ωn2=λn\omega_n^2 = \lambda_n (up to the tension). Part 1 is Rayleigh's principle: the squared fundamental frequency ω12\omega_1^2 is the minimum, over admissible shapes, of the ratio of potential energy to mass-weighted kinetic energy. When q≥0q \ge 0 (for instance a string on an elastic foundation), comparison says that stiffening a structure does not lower any frequency, and adding mass does not raise any.
  • Quantum mechanics. For H=−ℏ22md2dx2+V(x)H = -\frac{\hbar^2}{2m}\frac{d^2}{dx^2} + V(x) in a box, Part 1 states that the ground-state energy is the minimum of (ψ,Hψ)/(ψ,ψ)(\psi, H\psi)/(\psi, \psi). Any normalized guess bounds it from above. Part 3 extends this to excited states without knowledge of the lower eigenfunctions.
  • Heat flow and diffusion. The slowest decay rate of a solution of w ut=(pux)x−quw\, u_t = (p u_x)_x - q u with fixed ends is λ1\lambda_1. Min-max bounds on λ1\lambda_1 therefore bound the time a rod, or a diffusing population, takes to relax.

Method

The Rayleigh-Ritz method

Adapted

Restricting the Rayleigh quotient to the span of N trial functions turns a Sturm-Liouville eigenvalue problem into a small matrix problem K c = Lambda M c whose eigenvalues are guaranteed upper bounds for the first N eigenvalues and decrease to them as the trial space grows.

Prerequisites: Variational characterization of eigenvalues, Generalized eigenproblems and normal modes

DefinitionAdaptedAdapted from Strauss (2008), §11.2, pp. 305–307

Use the setting of the variational characterization: the problem −(pu′)′+qu=λwu-(p u')' + q u = \lambda w u on [a,b][a, b] with u(a)=u(b)=0u(a) = u(b) = 0, the energy D[u,v]=∫ab(pu′v′+quv) dxD[u, v] = \int_a^b (p u' v' + q u v)\, dx, the weighted inner product (u,v)w(u, v)_w, the space A\mathcal{A} of continuous, piecewise C1C^1 functions vanishing at both ends, and eigenvalues λ1<λ2<⋯\lambda_1 < \lambda_2 < \cdots.

Choose NN linearly independent trial functions ψ1,…,ψN∈A\psi_1, \dots, \psi_N \in \mathcal{A} and let VNV_N be their span. The Ritz matrices are the N×NN \times N symmetric matrices

Kij=D[ψi,ψj]=∫ab(p ψi′ψj′+q ψiψj) dx,Mij=(ψi,ψj)w=∫abw ψiψj dx.K_{ij} = D[\psi_i, \psi_j] = \int_a^b \bigl( p\, \psi_i' \psi_j' + q\, \psi_i \psi_j \bigr)\, dx, \qquad M_{ij} = (\psi_i, \psi_j)_w = \int_a^b w\, \psi_i \psi_j\, dx .

MM is the Gram matrix of independent functions in the inner product (⋅,⋅)w(\cdot, \cdot)_w, hence positive definite. For u=∑iciψiu = \sum_i c_i \psi_i,

R[u]=cTKccTMc.\mathcal{R}[u] = \frac{c^{\mathsf T} K c}{c^{\mathsf T} M c} .

The Ritz values Λ1(N)≤⋯≤ΛN(N)\Lambda_1^{(N)} \le \cdots \le \Lambda_N^{(N)} are the roots of det⁡(K−ΛM)=0\det(K - \Lambda M) = 0, that is, the eigenvalues of the pencil Kc=ΛMcK c = \Lambda M c. If c(k)c^{(k)} is an eigenvector for Λk(N)\Lambda_k^{(N)}, then ∑ici(k)ψi\sum_i c^{(k)}_i \psi_i is the kk-th Ritz function.

MethodAdaptedAdapted from Stakgold & Holst (2011), Thm 6.5.3 and Remark 4, pp. 398–400; Gelfand & Fomin (1963), §40.1, Theorem, p. 196
  1. (Upper bounds.) λk≤Λk(N)\lambda_k \le \Lambda_k^{(N)} for k=1,…,Nk = 1, \dots, N. In particular Λ1(N)=min⁡VN∖{0}R\Lambda_1^{(N)} = \min_{V_N \setminus \{0\}} \mathcal{R} is an upper bound for λ1\lambda_1, with equality exactly when φ1∈VN\varphi_1 \in V_N.
  2. (Monotonicity.) If VN⊂VN+1V_N \subset V_{N+1}, then Λk(N+1)≤Λk(N)\Lambda_k^{(N+1)} \le \Lambda_k^{(N)} for k≤Nk \le N.
  3. (Convergence, statement.) Let ψ1,ψ2,…\psi_1, \psi_2, \dots be an infinite sequence in A\mathcal{A} that is complete in energy: for every u∈Au \in \mathcal{A} and every ϵ>0\epsilon > 0 there are NN and g∈VNg \in V_N with ∫ab((u′−g′)2+(u−g)2) dx<ϵ\int_a^b \bigl( (u' - g')^2 + (u - g)^2 \bigr)\, dx < \epsilon. Then Λk(N)↓λk\Lambda_k^{(N)} \downarrow \lambda_k as N→∞N \to \infty, for each fixed kk.
Idea of the proofOriginal

A Ritz value is a min-max of the Rayleigh quotient taken over subspaces of VNV_N only. The true eigenvalue is the same min-max over subspaces of all of A\mathcal{A}. Minimizing over fewer subspaces can only give a larger answer, so every Ritz value lies above the eigenvalue it approximates. Enlarging VNV_N lets the min-max see more subspaces and pushes the Ritz values down. If the trial spaces eventually approximate everything, they approximate the true eigenfunctions, and the Ritz values close in.

ProofAdaptedAdapted from Strauss (2008), §11.2, proof of Thm 1, pp. 307–308; Stakgold & Holst (2011), proof of Thm 6.5.3, p. 399; Gelfand & Fomin (1963), §40.1, proof of the Theorem, p. 196
  1. The pencil. Since KK is symmetric and MM is symmetric positive definite, the generalized eigenvalue problem Kc=ΛMcK c = \Lambda M c has real eigenvalues Λ1(N)≤⋯≤ΛN(N)\Lambda_1^{(N)} \le \dots \le \Lambda_N^{(N)} and eigenvectors e1,…,eNe_1, \dots, e_N with eiTMej=δije_i^{\mathsf T} M e_j = \delta_{ij}.
  2. Part 1. Fix k≤Nk \le N and let WkW_k be the set of functions ∑iciψi\sum_i c_i \psi_i with c∈span⁡{e1,…,ek}c \in \operatorname{span}\{e_1, \dots, e_k\}. Because the ψi\psi_i are independent, WkW_k is a kk-dimensional subspace of A\mathcal{A}. Writing c=∑j≤kdjejc = \sum_{j \le k} d_j e_j gives cTKc=∑j≤kΛj(N)dj2c^{\mathsf T} K c = \sum_{j \le k} \Lambda_j^{(N)} d_j^2 and cTMc=∑j≤kdj2c^{\mathsf T} M c = \sum_{j \le k} d_j^2, so max⁡WkR=Λk(N)\max_{W_k} \mathcal{R} = \Lambda_k^{(N)}. The min-max characterization (Part 3 of the variational-characterization unit) gives λk≤max⁡WkR=Λk(N)\lambda_k \le \max_{W_k} \mathcal{R} = \Lambda_k^{(N)}. For k=1k = 1, the case of equality is the equality case of R≥λ1\mathcal{R} \ge \lambda_1: the minimum over VNV_N equals λ1\lambda_1 exactly when some multiple of φ1\varphi_1 lies in VNV_N.
  3. Part 2. The proof of the min-max formula, repeated word for word for the pencil, shows Λk(N)=min⁡max⁡WR\Lambda_k^{(N)} = \min \max_{W} \mathcal{R} over kk-dimensional subspaces W⊂VNW \subset V_N. Every such WW is also a subspace of VN+1V_{N+1}, so the minimum over subspaces of VN+1V_{N+1} is no larger.
  4. Part 3 for k=1k = 1. By Part 2, Λ1(N)\Lambda_1^{(N)} decreases, and it is bounded below by λ1\lambda_1. Since p,q,wp, q, w are bounded and ∥φ1∥w=1\|\varphi_1\|_w = 1, the numerator and denominator of R\mathcal{R} depend continuously on uu with respect to ∫((u′)2+u2)\int \bigl( (u')^2 + u^2 \bigr), so R\mathcal{R} is continuous at φ1\varphi_1 in that sense. Given ϵ>0\epsilon > 0, completeness in energy gives g∈VNg \in V_N so close to φ1\varphi_1 that R[g]<λ1+ϵ\mathcal{R}[g] < \lambda_1 + \epsilon. Then λ1≤Λ1(N′)≤R[g]<λ1+ϵ\lambda_1 \le \Lambda_1^{(N')} \le \mathcal{R}[g] < \lambda_1 + \epsilon for all N′≥NN' \ge N. The case k≥2k \ge 2 uses the same idea with kk-dimensional subspaces close to span⁡{φ1,…,φk}\operatorname{span}\{\varphi_1, \dots, \varphi_k\}, and we only state it. □\square
MethodAdaptedAdapted from Strauss (2008), §11.2, pp. 305–307; Stakgold & Holst (2011), §6.5, Remark 6, p. 400
  1. Write the problem in Sturm–Liouville form. Identify pp, qq, ww and the boundary conditions, and write down DD and R\mathcal{R}. For Robin or Neumann conditions, use the modified quotient described in the variational-characterization unit.
  2. Choose trial functions. They must satisfy the Dirichlet (essential) conditions; Neumann and Robin conditions are natural and need not be imposed. Use independent functions shaped like the modes you expect. Polynomials times a factor that vanishes at the ends, sines, or piecewise-linear "hat" functions are standard. Prefer nearly orthogonal families: raw monomials make MM badly conditioned when NN is large.
  3. Assemble Kij=D[ψi,ψj]K_{ij} = D[\psi_i, \psi_j] and Mij=(ψi,ψj)wM_{ij} = (\psi_i, \psi_j)_w, exactly or by accurate quadrature.
  4. Solve Kc=ΛMcK c = \Lambda M c, for example with a symmetric generalized eigensolver (scipy.linalg.eigh(K, M)), or by hand from det⁡(K−ΛM)=0\det(K - \Lambda M) = 0 when N≤2N \le 2.
  5. Read off the bounds λk≤Λk(N)\lambda_k \le \Lambda_k^{(N)} and the Ritz functions ∑ici(k)ψi\sum_i c^{(k)}_i \psi_i as approximate eigenfunctions.
  6. Refine. Add trial functions so that the spaces are nested, and watch Λk(N)\Lambda_k^{(N)} decrease. Stop when successive values agree to the accuracy you need. The method gives only upper bounds; a lower bound needs a different argument, such as comparison through the min-max principle.
RemarkAdaptedAdapted from Riley, Hobson & Bence (2006), §22.7, p. 793; Arfken, Weber & Harris (2013), §22.4, p. 1119

Why few trial functions give good eigenvalues. Write a trial function as u=φ1+eu = \varphi_1 + e with (e,φ1)w=0(e, \varphi_1)_w = 0. By step 1 of the variational-characterization proof, D[φ1,e]=λ1(φ1,e)w=0D[\varphi_1, e] = \lambda_1 (\varphi_1, e)_w = 0. Hence D[u]=λ1+D[e]D[u] = \lambda_1 + D[e] and ∥u∥w2=1+∥e∥w2\|u\|_w^2 = 1 + \|e\|_w^2, and exactly

R[u]−λ1=D[e]−λ1∥e∥w21+∥e∥w2.\mathcal{R}[u] - \lambda_1 = \frac{D[e] - \lambda_1 \|e\|_w^2}{1 + \|e\|_w^2} .

The numerator is nonnegative by the variational characterization, since ee is orthogonal to φ1\varphi_1. The error in the eigenvalue is quadratic in the error ee of the eigenfunction. For example, if ∥e∥w=0.1\|e\|_w = 0.1, the eigenvalue error is 0.01 (R[e]−λ1)/1.010.01\,(\mathcal{R}[e] - \lambda_1)/1.01, about one hundredth of the gap between R[e]\mathcal{R}[e] and λ1\lambda_1. The Ritz functions themselves converge more slowly than the Ritz values.

ExampleOriginal

Variable stiffness. Estimate the first two eigenvalues of

−((1+x) u′)′=λuon [0,1],u(0)=u(1)=0,-\bigl( (1 + x)\, u' \bigr)' = \lambda u \quad \text{on } [0, 1], \qquad u(0) = u(1) = 0,

so p=1+xp = 1 + x, q=0q = 0, w=1w = 1. Take ψ1=x(1−x)\psi_1 = x(1 - x) and ψ2=x2(1−x)\psi_2 = x^2(1 - x), which vanish at both ends, so ψ1′=1−2x\psi_1' = 1 - 2x and ψ2′=2x−3x2\psi_2' = 2x - 3x^2.

One trial function. K11=∫01(1+x)(1−2x)2 dx=13+16=12K_{11} = \int_0^1 (1 + x)(1 - 2x)^2\, dx = \tfrac13 + \tfrac16 = \tfrac12 and M11=∫01x2(1−x)2 dx=130M_{11} = \int_0^1 x^2 (1 - x)^2\, dx = \tfrac{1}{30}. So λ1≤Λ1(1)=15\lambda_1 \le \Lambda_1^{(1)} = 15.

Two trial functions. The remaining integrals are polynomial:

K=(1217601760730),M=(1301601601105).K = \begin{pmatrix} \tfrac12 & \tfrac{17}{60} \\[2pt] \tfrac{17}{60} & \tfrac{7}{30} \end{pmatrix}, \qquad M = \begin{pmatrix} \tfrac{1}{30} & \tfrac{1}{60} \\[2pt] \tfrac{1}{60} & \tfrac{1}{105} \end{pmatrix}.

Expanding the determinant,

det⁡(K−ΛM)=Λ225200−13Λ4200+1313600=Λ2−78Λ+91725200,\det(K - \Lambda M) = \frac{\Lambda^2}{25200} - \frac{13\Lambda}{4200} + \frac{131}{3600} = \frac{\Lambda^2 - 78\Lambda + 917}{25200},

so Λ1,2(2)=39∓2151≈14.4236\Lambda^{(2)}_{1,2} = 39 \mp 2\sqrt{151} \approx 14.4236 and 63.576463.5764.

Exact values. With t=1+xt = 1 + x the equation becomes (tut)t+λu=0(t u_t)_t + \lambda u = 0, solved by J0(2λt)J_0(2\sqrt{\lambda t}) and Y0(2λt)Y_0(2\sqrt{\lambda t}). The boundary conditions at t=1t = 1 and t=2t = 2 give the eigenvalue condition

J0(2λ) Y0(22λ)−J0(22λ) Y0(2λ)=0,J_0(2\sqrt{\lambda})\, Y_0(2\sqrt{2\lambda}) - J_0(2\sqrt{2\lambda})\, Y_0(2\sqrt{\lambda}) = 0,

whose first two roots are λ1≈14.33767\lambda_1 \approx 14.33767 and λ2≈57.48028\lambda_2 \approx 57.48028. Adding x3(1−x)x^3(1 - x) and x4(1−x)x^4(1 - x) to the basis, computed the same way, gives the table below.

NN Λ1(N)\Lambda_1^{(N)} Λ2(N)\Lambda_2^{(N)}
1 15 —
2 14.4236 63.5764
3 14.3467 59.7992
4 14.33773 57.7910
exact 14.33767 57.48028

Every entry lies above the exact value and decreases with NN, as Parts 1 and 2 require. The lowest Ritz value is already within 0.6%0.6\% at N=2N = 2, while the second is 10.6%10.6\% high. This is typical: with a fixed basis, the higher Ritz values are less accurate.

ApplicationOriginal
  • Quantum chemistry. Expanding a wavefunction in a finite basis of atomic orbitals and diagonalizing the Hamiltonian matrix is the Rayleigh–Ritz method with MM the overlap matrix. Part 1 guarantees that each computed level lies above the true one (the Hylleraas–Undheim–MacDonald theorem for excited states), so a larger basis can only improve the energies.
  • Structural dynamics and buckling. Engineers estimate natural frequencies and critical buckling loads of beams, plates and frames from a few assumed mode shapes. The guaranteed upper bound on a frequency means the estimate errs on a known side.
  • Finite elements. With piecewise-linear hat functions as trial functions, the Ritz matrices become the sparse stiffness and mass matrices of the finite element method. The upper-bound and convergence statements of this unit then apply to finite-element eigenvalues computed on nested meshes.