|
While numerical approximations of
are not unitary, the evolution
(2.1) is conjugated to a unitary evolution.
Other discrete unitary time evolutions have been considered in [4].
The problem to preserve unitarity is similar to
numerical integration problems for ODE's, where for example symplecticity
should be preserved during the discretisation of a Hamiltonian system.
If
has compact support, then
has this property too.
This leads to a finite propagation speed as in a relativistic set-up.
This fact has computational advantages. For example, we know exactly,
after which time, boundary effects begin to influence the value of a wave at
some point.
The discrete evolution preserves the (not necessarily closed)
algebraic field in which L is defined.
For example, if L is an operator defined over the rationals
and if the coordinates of
are rational, then
is rational and
can be determined exactly.
The evolution (2.1) can be defined on all bounded sequences
and not
only on
. For example, the evolution leaves almost periodic
configurations invariant, elements
, for which
the closure of all translated sequences
is compact in the uniform topology
).
This is useful, because solutions of (2.1) define generalized
eigenfunctions
of an operator K defined on space-time.
The unitary operator V=- i U solves
which is a discretisation of the
Schrödinger equation
. Since
, the evolutions U and V are essentially the same.
The discrete evolution
is a second order approximation
to
in the sense that
and
agree up to second order. This second order approximation is
more efficient than the second order but computationally more expensive
Cayley method