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The first part of this volume is a survey of the current state of
the theory of linear integral equations. Material from abstract
operator theory is presented first, before moving on to a detailed
discussion of Fredholm operators and estimates for the eigenvalues
and singular numbers of integral operators. Other sections of this
part are devoted to the theories of one-, and higher-dimensional
singular operators. The second part of the volume concentrates on
theoretical aspects of the boundary integral equation method, with
particular emphasis on the results for equations on non-smooth
surfaces obtained during the last few years. A survey of the
classical theory of harmonic potentials and the boundary integral
equations on smooth surfaces generated by such potentials is given
and the theory is then extended to elastic and hydrodynamic
potentials and to other problems of mathematical physics, including
the oblique derivative problem, the biharmonic equation, the heat
and wave equations and viscoelasticity.
A linear integral equation is an equation of the form XEX. (1)
2a(x)cp(x) - Ix k(x, y)cp(y)dv(y) = f(x), Here (X, v) is a measure
space with a-finite measure v, 2 is a complex parameter, and a, k,
f are given (complex-valued) functions, which are referred to as
the coefficient, the kernel, and the free term (or the right-hand
side) of equation (1), respectively. The problem consists in
determining the parameter 2 and the unknown function cp such that
equation (1) is satisfied for almost all x E X (or even for all x E
X if, for instance, the integral is understood in the sense of
Riemann). In the case f = 0, the equation (1) is called
homogeneous, otherwise it is called inhomogeneous. If a and k are
matrix functions and, accordingly, cp and f are vector-valued
functions, then (1) is referred to as a system of integral
equations. Integral equations of the form (1) arise in connection
with many boundary value and eigenvalue problems of mathematical
physics. Three types of linear integral equations are
distinguished: If 2 = 0, then (1) is called an equation of the
first kind; if 2a(x) i= 0 for all x E X, then (1) is termed an
equation of the second kind; and finally, if a vanishes on some
subset of X but 2 i= 0, then (1) is said to be of the third kind.
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