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THE BAKER-CAMPBELL-HAUSDORFF FORMULA
If
is a bounded linear operator on a Banach
space X, the operator eA can be defined by the usual power
series. If also
, and B commutes with A,
it is easy to see from the power series that eA eB = eA+B.
The BCH formula tells how to compute eA eB in general. We begin
the proof with a simple lemma on differential equations.
Lemma 1 Let Y be a Banach space,
and suppose
,
is a continuous function, and
. Then the initial-value problem

for a function
has a unique solution, given by

In particular, if w is constant,
u(t) = etAu0 + f(t,A) w,
where

The proof is identical to that of the special case
; note however that f(t,z) is an entire function (for every t),
so that f(t,A) is defined.
We now take
. Each
defines a linear operator
by the
formula
![\begin{displaymath}
\mbox{ad$\,A$} (B) = [A,B] := AB - BA \qquad \mbox{for all $B \in {\cal L(X)}$}.\end{displaymath}](img14.gif)
(It is easy to see that
is bounded; in fact
.) The next lemma suggests that
might be a natural object to study.
Lemma 2 Let
; then

Proof For
, define
by

Then
![\begin{displaymath}
\frac{d}{dt} (\rho_t(B))
= [ A, \rho_t(B) ]
= \mbox{ad$\,A$} (\rho_t(B) .
\end{displaymath}](img23.gif)
Noting that
, we see from Lemma 1 that

putting t = 1 gives the result.
Lemma 3 Let
be continuously differentiable. Then

where g(z) = f(1,z).
Proof For
,
, define

Then
while B(0,t) = I. Applying Lemma 1, we find

putting s = 1 gives the result.
Theorem 1 (Baker-Campbell-Hausdorff)
Let A and B
belong to
, with
,
sufficiently
small. Then the operater
is
uniquely defined, and

where, for
,

Proof
The series for h shows that the integral is defined provided
, for all
. Now, for
define

(The standard power series for ez and
show that
C(t) is well-defined on [0,1] if
and
are sufficiently small.) Then

and we deduce from Lemma 3 that
|  |
(1) |
Lemma 2 implies that
, so that

Now
if
, so

and (1) gives

the BCH formula follows by integration.
The integrand in the BCH formula can be expanded as a power
series in
and
applied to A, and integrated
term-by-term. (There are fewer terms than one might expect at
first, because
.) Applying the exponential
function to both sides of the formula, the result can be written
![\begin{displaymath}
e^A e^B = \exp ( A + B + {1\over 2}[A,B] +
\frac{1}{12}([A,[A,B]] - [B,[A,B]]) + \cdots ) .\end{displaymath}](img57.gif)
When A and B commute, we recover the result that
eA eB = eA+B. A less trivial case, which is at least of
some formal relevance to quantum mechanics, is when the commutator
[A,B] commutes with both A and B; in that case
we find
. (In quantum mechanics, we
are interested in operators such that [A,B] is a multiple of the
identity. Unfortunately, it can be easily shown that such a pair of
operators cannot both be bounded, so the proof of BCH breaks down.)
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Kevin B Mcleod
3/12/1999