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Theory Normal Mode Decomposition
Given a molecule with
$\vec{X}^T = (x_1,x_2,z_1 ... x_N,y_N,z_N)$ $\vec{R}^T = (r_1,r_2 ... r_S)$
Using the Wilson B-Matrix, the coordinate systems can be transformed into each other.
The potential energy of a given molecule can be approximated by the quadratic force constants, which are second derivatives of the energy E with respect to Cartesian or internal coordinates:
$f_{ij} = \frac{\partial^2 E}{\partial x_i \partial x_k}$ $F_{ij} = \frac{\partial^2 E}{\partial r_i \partial r_j}$
Now using the Wilson B-Matrix we defined bevore the matrices can be transformed into each other (Matrix-Transformation
$F = (\tilde{B}^{-1})^T f \tilde{B}^{-1}$ $f = \tilde{B}^T F \tilde{B}$
Here
The mass-weighted Cartesian force constant matrix
$f' = (M^{-1/2})^T f M^{-1/2}$
can be diagonalized (Matrix-Diagonalization)
$\Lambda = L^T f' L$
where the matrix
Now the diagonalization can be rewritten using the (not mass-weighted) Cartesian force constant matrix
$\Lambda = l^T f l$
where one defined
$\Lambda = l^T f l = l^T(B^T F B) l$
now if we define the
$\Lambda = D^T F D$