Linear dynamical system

Linear dynamical system

In a linear dynamical system, the variation of a state vector (an N-dimensional vector denoted mathbf{x}) equals a constant matrix(denoted mathbf{A}) multiplied by mathbf{x}. This variation can take two forms: either as a flow, in which mathbf{x} varies continuously with time

:frac{d}{dt} mathbf{x}(t) = mathbf{A} cdot mathbf{x}(t)

or (less commonly) as a mapping, in which mathbf{x} varies in discrete steps

:mathbf{x}_{m+1} = mathbf{A} cdot mathbf{x}_{m}

These equations are linear in the following sense: if mathbf{x}(t) and mathbf{y}(t) are two valid solutions, then so is any linear combination of the two solutions, e.g., mathbf{z}(t) stackrel{mathrm{def{=} alpha mathbf{x}(t) + eta mathbf{y}(t) where alpha and etaare any two scalars. It is important to note that the matrix mathbf{A} need not be symmetric.

Linear dynamical systems can be solved exactly, in contrast to most nonlinear ones. Occasionally, a nonlinear system can be solved exactly by a change of variables to a linear system. Moreover, the solutions of (almost) any nonlinear system can be well-approximated by an equivalent linear system near its fixed points. Hence, understanding linear systems and their solutions is a crucial first step to understanding the more complex nonlinear systems.

olution of linear dynamical systems

If the initial vector mathbf{x}_{0} stackrel{mathrm{def{=} mathbf{x}(t=0)is aligned with a right eigenvector mathbf{r}_{k} of the matrix mathbf{A}, the dynamics are simple

:frac{d}{dt} mathbf{x}(t) = mathbf{A} cdot mathbf{r}_{k} = lambda_{k} mathbf{r}_{k}

where lambda_{k} is the corresponding eigenvalue;the solution of this equation is :mathbf{x}(t) = mathbf{r}_{k} e^{lambda_{k} t}as may be confirmed by substitution.

If mathbf{A} is diagonalizable, then any vector in an N-dimensional space can be represented by a linear combination of the right and left eigenvectors (denoted mathbf{l}_{k}) of the matrix mathbf{A}.

:mathbf{x}_{0} = sum_{k=1}^{N} left( mathbf{l}_{k} cdot mathbf{x}_{0} ight)mathbf{r}_{k}

Therefore, the general solution for mathbf{x}(t) is a linear combination of the individual solutions for the righteigenvectors:mathbf{x}(t) = sum_{k=1}^{n} left( mathbf{l}_{k} cdot mathbf{x}_{0} ight)mathbf{r}_{k} e^{lambda_{k} t}

Similar considerations apply to the discrete mappings.

Classification in two dimensions

The roots of the characteristic polynomial det(A - &lambda;I) are the eigenvalues of A. The sign and relation of these roots, lambda_n, to each other may be used to determine the stability of the dynamical system :frac{d}{dt} mathbf{x}(t) = mathbf{A} mathbf{x}(t).For a 2-dimensional system, the characteristic polynomial is of the form lambda^2- aulambda+Delta=0 where au is the trace and Delta is the determinant of A. Thus the two roots are in the form::lambda_1=frac{ au+sqrt{ au^2-4Delta{2}:lambda_2=frac{ au-sqrt{ au^2-4Delta{2}Note also that Delta=lambda_1lambda_2 and au=lambda_1+lambda_2. Thus if Delta<0 then the eigenvalues are of opposite sign, and the fixed point is a saddle. If Delta>0 then the eigenvalues are of the same sign. Therefore if au>0 both are positive and the point is unstable, and if au<0 then both are negative and the point is stable. The discriminant will tell you if the point is nodal or spiral (i.e. if the eigenvalues are real or complex).

ee also

* Linear system
* Dynamic systems
* List of dynamical system topics


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