Sylvester's formula
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In matrix theory, Sylvester's formula, named after James Joseph Sylvester, expresses matrix functions in terms of the eigenvalues and eigenvectors of a matrix. It is only valid for diagonalizable matrices; an extension due to Buchheim covers the general case.
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[edit] Statement
Let A be a diagonalizable matrix with k distinct eigenvalues, λ1, …, λk. The Frobenius covariants Ai are defined by
The Frobenius covariants Ai are projections on the eigenspace associated with λi. They can be found by diagonalizing the matrix A. using the eigendecomposition A = SDS−1. First, suppose that A has no multiple eigenvalues. Let A = SDS−1 be the eigendecomposition of A where the diagonal matrix D has the eigenvalues λ1, …, λk (in that order) on the diagonal. Denote the ith column of S by ci and the ith row of S−1 by ri; ci and ri are left and right eigenvectors of A). Then Ai = ciri. If A has multiple eigenvalues then Ai = Σj cjrj, where the sum is over all rows and columns associated with the eigenvalue λi.[2]
Now, let f: D → C with D ⊂ C be a function for which f(A) is well defined; this means that every eigenvalue λi is in the domain D and that every λi with multiplicity mi is in the interior of the domain with f (mi − 1) times differentiable at λi.[3] Then, Sylvester's formula states that
[edit] Example
Consider the two-by-two matrix:
This matrix has two eigenvalues, 5 and −2. Its eigendecomposition is
Hence the Frobenius covariants are
Sylvester's formula states that
For instance, if f is defined by f(x) = x−1, then Sylvester's formula computes the matrix inverse f(A) = A−1 as
[edit] Notes
- ^ Horn & Johnson, equation (6.1.36)
- ^ Horn & Johnson, page 521
- ^ Horn & Johnson, Definition 6.4
- ^ Horn & Johnson, equation (6.2.39)
[edit] References
- Horn, Roger A. & Johnson, Charles R. (1991), Topics in Matrix Analysis, Cambridge University Press, ISBN 9780521467131.
[edit] External links
- Jon F. Claerbout, Sylvester's matrix theorem, a section of Fundamentals of Geophysical Data Processing, published in 1976.







