Skew-Hamiltonian matrix

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In linear algebra, skew-Hamiltonian matrices are special matrices which correspond to skew-symmetric bilinear forms on a symplectic vector space.

Let V be a vector space, equipped with a symplectic form \Omega . Such a space must be even-dimensional. A linear map A:\;V\mapsto V is called a skew-Hamiltonian operator with respect to \Omega if the form x,y\mapsto \Omega (A(x),y) is skew-symmetric.

Choose a basis e_{1},...e_{{2n}} in V, such that \Omega is written as \sum _{i}e_{i}\wedge e_{{n+i}}. Then a linear operator is skew-Hamiltonian with respect to \Omega if and only if its matrix A satisfies A^{T}J=JA, where J is the skew-symmetric matrix

J={\begin{bmatrix}0&I_{n}\\-I_{n}&0\\\end{bmatrix}}

and In is the n\times n identity matrix.[1] Such matrices are called skew-Hamiltonian.

The square of a Hamiltonian matrix is skew-Hamiltonian. The converse is also true: every skew-Hamiltonian matrix can be obtained as the square of a Hamiltonian matrix.[1][2]

Notes

  1. 1.0 1.1 William C. Waterhouse, The structure of alternating-Hamiltonian matrices, Linear Algebra and its Applications, Volume 396, 1 February 2005, Pages 385-390
  2. Heike Faßbender, D. Steven Mackey, Niloufer Mackey and Hongguo Xu Hamiltonian Square Roots of Skew-Hamiltonian Matrices, Linear Algebra and its Applications 287, pp. 125 - 159, 1999


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