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State-transition matrix

Tool in control theory

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Record originEnglish Wikipedia
Text licenseCC BY-SA 4.0
Source revisionJul 31, 2026
Entity authorityQ7602993
Source-derived summary

In control theory and dynamical systems theory, the state-transition matrix is a matrix function that describes how the state of a linear system changes over time. Essentially, if the system's state is known at an initial time ⁠

t

0

{\displaystyle t_{0}}

⁠, the state-transition matrix allows for the calculation of the state at any future time ⁠

t

{\displaystyle t}

⁠.

The matrix is used to find the general solution to the homogeneous linear differential equation

x

˙

(

t

)

=

A

(

t

)

x

(

t

)

{\displaystyle {\dot {\mathbf {x} }}(t)=\mathbf {A} (t)\mathbf {x} (t)}

and is also a key component in finding the full solution for the non-homogeneous (input-driven) case.

For linear time-invariant (LTI) systems, where the matrix

A

{\displaystyle \mathbf {A} }

is constant, the state-transition matrix is the matrix exponential ⁠

exp

(

A

(

t

t

0

)

)

{\displaystyle \textstyle \exp {(\mathbf {A} (t-t_{0}))}}

⁠. In the more complex time-variant case, where

A

(

t

)

{\displaystyle \mathbf {A} (t)}

can change over time, there is no simple formula, and the matrix is typically found by calculating the Peano–Baker series.

Linear systems solutions

The state-transition matrix is used to find the solution to a general state-space representation of a linear system in the following form

x

˙

(

t

)

=

A

(

t

)

x

(

t

)

+

B

(

t

)

u

(

t

)

,

x

(

t

0

)

=

x

0

,

{\displaystyle {\dot {\mathbf {x} }}(t)=\mathbf {A} (t)\mathbf {x} (t)+\mathbf {B} (t)\mathbf {u} (t),\;\mathbf {x} (t_{0})=\mathbf {x} _{0},}

where

x

(

t

)

{\displaystyle \mathbf {x} (t)}

are the states of the system;

u

(

t

)

{\displaystyle \mathbf {u} (t)}

is the input signal;

A

(

t

)

{\displaystyle \mathbf {A} (t)}

and

B

(

t

)

{\displaystyle \mathbf {B} (t)}

are matrix functions; and

x

0

{\displaystyle \mathbf {x} _{0}}

is the initial condition at ⁠

t

0

{\displaystyle t_{0}}

⁠. Using the state-transition matrix ⁠

Φ

(

t

,

τ

)

{\displaystyle \mathbf {\Phi } (t,\tau )}

⁠, the solution is given by:

x

(

t

)

=

Φ

(

t

,

t

0

)

x

(

t

0

)

+

t

0

t

Φ

(

t

,

τ

)

B

(

τ

)

u

(

τ

)

d

τ

.

{\displaystyle \mathbf {x} (t)=\mathbf {\Phi } (t,t_{0})\mathbf {x} (t_{0})+\int _{t_{0}}^{t}\mathbf {\Phi } (t,\tau )\mathbf {B} (\tau )\mathbf {u} (\tau )\ d\tau .}

The first term is known as the zero-input response and represents how the system's state would evolve in the absence of any input. The second term is known as the zero-state response and defines how the inputs impact the system.

Peano–Baker series

The most general transition matrix is given by a product integral, referred to as the Peano–Baker series:

Φ

(

t

,

τ

)

=

I

+

τ

t

A

(

σ

1

)

d

σ

1

+

τ

t

A

(

σ

1

)

τ

σ

1

A

(

σ

2

)

d

σ

2

d

σ

1

+

τ

t

A

(

σ

1

)

τ

σ

1

A

(

σ

2

)

τ

σ

2

A

(

σ

3

)

d

σ

3

d

σ

2

d

σ

1

+

,

{\displaystyle {\begin{aligned}\mathbf {\Phi } (t,\tau )=\mathbf {I} &+\int _{\tau }^{t}\mathbf {A} (\sigma _{1})\,d\sigma _{1}\\&+\int _{\tau }^{t}\mathbf {A} (\sigma _{1})\int _{\tau }^{\sigma _{1}}\mathbf {A} (\sigma _{2})\,d\sigma _{2}\,d\sigma _{1}\\&+\int _{\tau }^{t}\mathbf {A} (\sigma _{1})\int _{\tau }^{\sigma _{1}}\mathbf {A} (\sigma _{2})\int _{\tau }^{\sigma _{2}}\mathbf {A} (\sigma _{3})\,d\sigma _{3}\,d\sigma _{2}\,d\sigma _{1}\\&+\cdots ,\end{aligned}}}

where

I

{\displaystyle \mathbf {I} }

is the identity matrix.

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