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This book is devoted to mean-square and weak approximations of
solutions of stochastic differential equations (SDE). These
approximations represent two fundamental aspects in the
contemporary theory of SDE. Firstly, the construction of numerical
methods for such systems is important as the solutions provided
serve as characteristics for a number of mathematical physics
problems. Secondly, the employment of probability representations
together with a Monte Carlo method allows us to reduce the solution
of complex multidimensional problems of mathematical physics to the
integration of stochastic equations. Along with a general theory of
numerical integrations of such systems, both in the mean-square and
the weak sense, a number of concrete and sufficiently constructive
numerical schemes are considered. Various applications and
particularly the approximate calculation of Wiener integrals are
also dealt with. This book is of interest to graduate students in
the mathematical, physical and engineering sciences, and to
specialists whose work involves differential equations,
mathematical physics, numerical mathematics, the theory of random
processes, estimation and control theory.
U sing stochastic differential equations we can successfully model
systems that func- tion in the presence of random perturbations.
Such systems are among the basic objects of modern control theory.
However, the very importance acquired by stochas- tic differential
equations lies, to a large extent, in the strong connections they
have with the equations of mathematical physics. It is well known
that problems in math- ematical physics involve 'damned
dimensions', of ten leading to severe difficulties in solving
boundary value problems. A way out is provided by stochastic
equations, the solutions of which of ten come about as
characteristics. In its simplest form, the method of
characteristics is as follows. Consider a system of n ordinary
differential equations dX = a(X) dt. (O.l ) Let Xx(t) be the
solution of this system satisfying the initial condition Xx(O) = x.
For an arbitrary continuously differentiable function u(x) we then
have: (0.2) u(Xx(t)) - u(x) = j (a(Xx(t)), ~~ (Xx(t))) dt.
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