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System of ODEs Solver

Solve systems of ordinary differential equations x' = Ax symbolically and numerically. Auto-classifies the equilibrium (saddle, node, spiral, center), derives eigenvalues and eigenvectors step by step, writes the closed-form general and particular solution, and draws an interactive phase portrait with animated trajectory — for 2×2, 3×3 linear and nonlinear 2D systems.

System of ODEs Solver
Solve \(\dfrac{d}{dt}\!\begin{pmatrix}x\\y\end{pmatrix} = A \begin{pmatrix}x\\y\end{pmatrix}\) where \(A\) is a 2×2 matrix with real entries.
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Accepts decimals (e.g. 2.5), negatives (-1), and simple fractions (3/4).
Solve \(\dfrac{d}{dt}\!\begin{pmatrix}x_1\\x_2\\x_3\end{pmatrix} = A \begin{pmatrix}x_1\\x_2\\x_3\end{pmatrix}\) — get eigenvalues, eigenvectors, and the closed-form general solution.
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The default is the companion matrix of \( s^3 + 6s^2 + 11s + 6 \), giving eigenvalues \(-1, -2, -3\).
Solve a general 2D nonlinear system numerically: \(x' = f(x, y)\), \(y' = g(x, y)\). Use functions like sin, cos, exp, sqrt, and constants pi, e.
No closed-form solution is computed; instead a high-accuracy RK4 integration produces the trajectory and phase portrait.
x(0)
y(0)
time span T

Embed System of ODEs Solver Widget

About System of ODEs Solver

The System of ODEs Solver is an all-in-one differential-equations toolbox for coupled linear and nonlinear systems. Paste a 2×2 or 3×3 coefficient matrix and the tool performs the full eigenvalue / eigenvector analysis, writes the closed-form general and particular solution in LaTeX, classifies the equilibrium at the origin as a saddle, node, spiral, or center, and draws an interactive phase portrait with an animated trajectory. For nonlinear planar systems you can type arbitrary right-hand sides \(f(x,y)\) and \(g(x,y)\) and the tool produces a high-accuracy RK4 phase portrait.

What Is a System of ODEs?

A system of ordinary differential equations couples several unknown functions of a single variable — usually time \(t\) — through their derivatives. In the most compact form,

\[ \mathbf{x}'(t) = \mathbf{F}(t, \mathbf{x}(t)) , \qquad \mathbf{x} \in \mathbb{R}^n \]

When \(\mathbf{F}(t, \mathbf{x}) = A\mathbf{x}\) for a constant matrix \(A\), the system is linear and autonomous — and this is where the theory is at its most beautiful: the entire long-term behavior is determined by the eigenvalues of \(A\).

The Eigenvalue Recipe for Linear Systems

For \(\mathbf{x}' = A\mathbf{x}\) the standard method is:

  1. Compute the characteristic polynomial \(\det(\lambda I - A) = 0\).
  2. Solve for the eigenvalues \(\lambda_1, \lambda_2, \dots\).
  3. For each eigenvalue, find an eigenvector \(v\) by solving \((A - \lambda I) v = 0\).
  4. Assemble the general solution as a linear combination: \(\mathbf{x}(t) = c_1 v_1 e^{\lambda_1 t} + c_2 v_2 e^{\lambda_2 t} + \cdots\).
  5. Fix the constants \(c_i\) by plugging the initial condition \(\mathbf{x}(0)\) into the general solution.

Three Cases for 2×2 Systems

Eigenvalues General Solution Portrait
Real distinct \(\lambda_1 \ne \lambda_2\) \(c_1 v_1 e^{\lambda_1 t} + c_2 v_2 e^{\lambda_2 t}\) Saddle if signs differ; node otherwise
Complex conjugate \(\alpha \pm i\beta\) \(e^{\alpha t}[c_1(p\cos\beta t - q\sin\beta t) + c_2(p\sin\beta t + q\cos\beta t)]\) Spiral (\(\alpha \ne 0\)) or center (\(\alpha = 0\))
Repeated \(\lambda_1 = \lambda_2 = \lambda\) \(c_1 v e^{\lambda t} + c_2 (tv + w) e^{\lambda t}\) Degenerate node

The Trace-Determinant Plane

For a 2×2 matrix with trace \(T = a_{11} + a_{22}\) and determinant \(D = a_{11} a_{22} - a_{12} a_{21}\), the whole classification fits in a single diagram:

\[ \begin{array}{l} D < 0 \Rightarrow \text{saddle} \\ D > 0, \; T^2 - 4D > 0 \Rightarrow \text{node (stable if } T < 0\text{)} \\ D > 0, \; T^2 - 4D < 0 \Rightarrow \text{spiral (stable if } T < 0\text{), center if } T = 0 \\ T^2 - 4D = 0 \Rightarrow \text{degenerate node (repeated eigenvalue)} \end{array} \]

This is why the results panel prominently shows \(T\), \(D\), and \(\Delta = T^2 - 4D\) — three numbers are enough to name the equilibrium.

Nonlinear Systems and the Phase Portrait

Most real-world ODEs are nonlinear and have no closed-form solution. The tool handles them by integrating the equations numerically with a 4th-order Runge–Kutta (RK4) method, which has local truncation error \(O(h^5)\) and is the default workhorse for smooth vector fields.

\[ \begin{aligned} k_1 &= f(t_n, y_n) \\ k_2 &= f(t_n + h/2, y_n + h k_1 / 2) \\ k_3 &= f(t_n + h/2, y_n + h k_2 / 2) \\ k_4 &= f(t_n + h, y_n + h k_3) \\ y_{n+1} &= y_n + \tfrac{h}{6}(k_1 + 2k_2 + 2k_3 + k_4) \end{aligned} \]

The phase portrait overlays:

How to Use This Solver

  1. Pick a mode — 2×2 Linear, 3×3 Linear, or Nonlinear 2D — via the tabs at the top of the form.
  2. Fill in coefficients or equations. Click any Quick Example to pre-fill a canonical system (stable node, center, saddle, pendulum, Van der Pol, etc.).
  3. Enter an initial condition \((x_0, y_0)\) and a time span \(T\). Typical \(T\) values are 6–20 for oscillators and 3–6 for fast-decaying stable systems.
  4. Click Solve. The full results page appears with the classification, eigenvalues, eigenvectors, closed-form solution (linear modes), animated phase portrait, and time-series plot.
  5. Replay the trajectory using the button under the phase portrait if you'd like to watch the runner traverse the IC curve again.

Worked Example — Damped Harmonic Oscillator

The damped oscillator \(\ddot{x} + 2\zeta \omega \dot{x} + \omega^2 x = 0\) can be rewritten as a 2D system by letting \(y = \dot{x}\):

\[ \begin{pmatrix} \dot{x} \\ \dot{y} \end{pmatrix} = \begin{pmatrix} 0 & 1 \\ -\omega^2 & -2\zeta\omega \end{pmatrix} \begin{pmatrix} x \\ y \end{pmatrix} \]

For \(\omega = 1\) and \(\zeta = 0.2\) (underdamped), the matrix is \(A = \begin{pmatrix} 0 & 1 \\ -1 & -0.4 \end{pmatrix}\). Trace \(T = -0.4\), determinant \(D = 1\), discriminant \(\Delta = 0.16 - 4 = -3.84 < 0\), so we get a stable spiral with eigenvalues \(-0.2 \pm 0.9798\,i\). The trajectory spirals into the origin, and the time series shows exponentially-decaying sinusoids.

Applications

Tips & Gotchas

Frequently Asked Questions

What is a system of ordinary differential equations?

A system of ordinary differential equations (ODEs) is a set of coupled equations that relate the derivatives of several unknown functions of a single independent variable, typically time. The classic form is \( \mathbf{x}'(t) = F(t, \mathbf{x}(t)) \), where \( \mathbf{x} \) is a vector of states and \(F\) is the vector field. Linear systems can be written compactly as \( \mathbf{x}' = A\mathbf{x} + \mathbf{b} \), and their behavior is determined almost entirely by the eigenvalues of the coefficient matrix \(A\).

How do eigenvalues classify the equilibrium of a 2×2 linear system?

For a 2×2 system \( \mathbf{x}' = A\mathbf{x} \) the origin is classified by the trace \(T\) and determinant \(D\) of \(A\): \(D < 0\) gives a saddle point (unstable); \(D > 0\) with \(T^2 > 4D\) gives a node (stable if \(T < 0\), unstable if \(T > 0\)); \(D > 0\) with \(T^2 < 4D\) gives a spiral (stable if \(T < 0\), unstable if \(T > 0\), a pure center if \(T = 0\)). The borderline \(T^2 = 4D\) produces a degenerate node.

What does the closed-form solution look like when the eigenvalues are complex?

If \(A\) has complex-conjugate eigenvalues \( \alpha \pm i\beta \) with complex eigenvector \( v = p + iq \), the real general solution is \( \mathbf{x}(t) = e^{\alpha t} \left[ c_1 (p \cos\beta t - q \sin\beta t) + c_2 (p \sin\beta t + q \cos\beta t) \right] \). The exponential \(e^{\alpha t}\) controls the amplitude (growing, decaying, or constant), while the sine and cosine handle the rotation.

What happens when the matrix has a repeated eigenvalue?

If the matrix has a repeated eigenvalue \(\lambda\) but only one linearly independent eigenvector \(v\), you also need a generalized eigenvector \(w\) solving \( (A - \lambda I) w = v \). The general solution then takes the form \( \mathbf{x}(t) = c_1 v e^{\lambda t} + c_2 (tv + w) e^{\lambda t} \). If the eigenspace happens to be two-dimensional, the matrix is a scalar multiple of the identity on that invariant subspace and the solution reduces to \( \mathbf{x}(t) = (c_1 v_1 + c_2 v_2) e^{\lambda t} \).

Can this tool solve nonlinear systems symbolically?

The nonlinear mode solves the system numerically using a fourth-order Runge–Kutta (RK4) integrator and plots the phase portrait. Most nonlinear systems have no closed-form solution, so this is the standard approach. You can still read off local behavior near equilibria by linearizing, which the 2×2 linear mode handles — compute the Jacobian at the fixed point and feed it in as \(A\).

What is a phase portrait?

A phase portrait is a geometric picture of the solutions of a 2D system in the \(x\)–\(y\) plane. Each solution traces out a curve called a trajectory, and the collection of trajectories together with the vector field arrows reveals the qualitative behavior: whether solutions spiral in, saddle apart, oscillate, or settle onto equilibria. Phase portraits make the global structure of a system visible at a glance.

Further Reading

Reference this content, page, or tool as:

"System of ODEs Solver" at https://MiniWebtool.com// from MiniWebtool, https://MiniWebtool.com/

by miniwebtool team. Updated: Apr 23, 2026

You can also try our AI Math Solver GPT to solve your math problems through natural language question and answer.

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