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Spectral Theory in Hilbert Space

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92 13. FIRST ORDER SYSTEMS<br />

S<strong>in</strong>ce W is assumed locally <strong>in</strong>tegrable it is clear that constant n ×<br />

1 matrices are locally <strong>in</strong> L2 W so (each components of) W u is locally<br />

<strong>in</strong>tegrable if u ∈ L2 W . It is also clear that u and ũ are two different<br />

representatives of the same equivalence class <strong>in</strong> L2 W precisely if W u =<br />

W ũ almost everywhere (Exercise 13.1).<br />

Example 13.3. Any standard scalar differential equation may be<br />

written on the form (13.1) with a constant, skew-Hermitian J. If it<br />

is possible to do this so that Q and W are Hermitian, the differential<br />

equation is called formally symmetric. We have already seen this <strong>in</strong><br />

the case of the Sturm-Liouville equation (10.1), which will be formally<br />

symmetric if p, q and w are real-valued. The first order scalar equation<br />

iu ′ + qu = wv is already of the proper form and formally symmetric if<br />

q and w are real-valued. The fourth order equation (p2u ′′ ) ′′ − (p1u ′ ) ′ +<br />

qu = wv may be written on the form (13.1) by sett<strong>in</strong>g<br />

<br />

<br />

U =<br />

, J =<br />

and Q =<br />

u<br />

hu ′<br />

(p2u ′′ ) ′ −p1u ′<br />

−p2u ′′<br />

0 0 1 0<br />

0 0 0 1<br />

−1 0 0 0<br />

0 −1 0 0<br />

p0 0 0 0<br />

0 p1 1 0<br />

0 1 0 0<br />

0 0 0 −1/p2<br />

as is readily seen, and it will be formally symmetric if the coefficients<br />

w, p0, p1 and p2 are real-valued.<br />

In order to get a spectral theory for (13.1) it is convenient to use<br />

the theory of symmetric relations, s<strong>in</strong>ce it is sometimes not possible<br />

to f<strong>in</strong>d a densely def<strong>in</strong>ed symmetric operator realiz<strong>in</strong>g the equation.<br />

Consequently, we must beg<strong>in</strong> by def<strong>in</strong><strong>in</strong>g a m<strong>in</strong>imal relation, show that<br />

it is symmetric, calculate its adjo<strong>in</strong>t and f<strong>in</strong>d the selfadjo<strong>in</strong>t restrictions<br />

of the adjo<strong>in</strong>t. We def<strong>in</strong>e the m<strong>in</strong>imal relation T0 to be the closure <strong>in</strong><br />

L 2 W ⊕ L2 W of the set of pairs (u, v) of elements <strong>in</strong> L2 W<br />

<br />

,<br />

with compact<br />

support <strong>in</strong> the <strong>in</strong>terior of I (i.e., which are 0 outside some compact<br />

sub<strong>in</strong>terval of the <strong>in</strong>terior of I which may be different for different pairs<br />

(u, v)) and such that u is locally absolutely cont<strong>in</strong>uous and satisfies the<br />

equation Ju ′ + Qu = W v. This relation between u and v may or may<br />

not be an operator (Exercise 13.2).<br />

The next step is to calculate the adjo<strong>in</strong>t of T0. In order to do this,<br />

we shall aga<strong>in</strong> use the classical variation of constants formula, now <strong>in</strong><br />

a more general form than <strong>in</strong> Lemma 10.4. Below we always assume<br />

that c is a fixed (but arbitrary) po<strong>in</strong>t <strong>in</strong> I. Let F (x, λ) be a n × n<br />

matrix-valued solution of JF ′ + QF = λW F with F (c, λ) <strong>in</strong>vertible.<br />

This means precisely that the columns of F are a basis for the solutions<br />

of (13.1) for v = λu. Such a solution is called a fundamental matrix for<br />

this equation. We will always <strong>in</strong> addition suppose that S = F (c, λ) is<br />

<strong>in</strong>dependent of λ and symplectic, i.e., S ∗ JS = J. We may for example<br />

take S equal to the n × n unit matrix or, if J is unitary, S = J.<br />

Lemma 13.4. We have F ∗ (x, λ)JF (x, λ) = J for any complex λ<br />

and x ∈ I. The solution u of Ju ′ + Qu = λW u + W v with <strong>in</strong>itial data

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