Divergence Theorem Calculator

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Fill in the field components and bounds.

Understanding Gauss's Divergence Theorem

The divergence theorem, also known as Gauss’s theorem, forms one of the three cornerstone identities of vector calculus alongside Stokes’ and Green’s theorems. It links the behavior of a vector field F inside a region to the flux of that field through the region’s boundary. For a solid volume V with a sufficiently smooth boundary surface S oriented outward, the theorem states

SFndS=VFdV.

The left-hand side is a surface integral of the field’s normal component, often interpreted as the net flow or flux leaving the volume. The right-hand side is a triple integral over the volume of the field’s divergence, which measures the instantaneous rate of “outflow” per unit volume. When the divergence is positive at a point, the field behaves like a source, spreading outward; when negative, it resembles a sink, drawing vectors inward. The theorem asserts that accumulating these local source strengths over the entire volume equals the total flux across the boundary. In physical contexts ranging from electromagnetism to fluid dynamics, this result provides a profound conservation principle, guaranteeing that the quantity represented by the field is neither created nor destroyed within the region except by explicit sources or sinks.

Our calculator specializes in verifying the divergence theorem for rectangular boxes. By restricting attention to axis-aligned boxes, we avoid complications of curved surfaces and can perform all integrations numerically using straightforward grid approximations. Users specify the components of F as expressions in x, y, and z. The tool then evaluates both sides of the theorem: a surface flux computed by summing contributions from the six faces of the box, and a volume integral computed by approximating the divergence throughout the interior. When both calculations agree within numerical error, we gain confidence in the theorem and intuition about how divergence quantifies local expansion.

Numerical Strategy

The algorithm uses simple midpoint Riemann sums. Suppose the box spans [x0,x1] in the x-direction, and similarly for y and z. We partition each interval into ten equal segments of width Δx, Δy, and Δz. For the volume integral, the divergence F is estimated at the center of each subcube using finite differences:

FFxx+ε,y,z-Fxx-ε,y,z2ε+Fyx,y+ε,z-Fyx,y-ε,z2ε+Fzx,y,z+ε-Fzx,y,z-ε2ε,

where ε is a tiny fraction of the grid spacing. Multiplying the estimated divergence by the subcube volume Δx Δy Δz and summing over all subcubes yields the approximate volume integral.

For the surface flux, each face is treated as a rectangular region subdivided into a grid. Consider the face at x = x1. Its outward normal is (1,0,0), so the contribution to the flux is y_0y_1z_0z_1Fxx1,y,zdydz. Our algorithm evaluates Fx at the center of each subrectangle and sums FxΔy Δz. The opposite face at x = x0 uses the normal (-1,0,0), so we subtract Fx on that side. Repeating this process for the y- and z-oriented faces accumulates the total flux.

Worked Example

With the default settings, the field is F = (x, y, z) over the unit cube. This field represents uniform expansion from the origin. The divergence is constant: F=3. Integrating over the unit volume gives a theoretical value of 3. For the surface flux, each face contributes either 1 or -1 depending on orientation, and summing the six contributions also yields 3. When you press the calculate button, the numerical estimates displayed should be close to these values, demonstrating the theorem in action.

Algorithm Summary

StepComputation
1Parse the field component expressions and numerical bounds.
2Partition the box into a uniform grid for interior and surface calculations.
3Approximate partial derivatives with finite differences to estimate divergence at subcube centers.
4Sum the divergence over the volume to obtain the right-hand side integral.
5Evaluate field components on each face, multiply by the outward normal, and accumulate the flux across all six faces.
6Report the volume integral, surface flux, and their difference.

Interpreting the Results

When the divergence theorem holds, the two computed values should match closely. Any difference stems from numerical error due to finite grid resolution and finite difference approximations. Doubling the number of grid subdivisions typically halves this error, reflecting the first-order accuracy of midpoint sums. Extremely nonlinear fields or highly skewed boxes may require more subdivisions for convergence. Because all computations occur entirely within your browser using plain JavaScript, you can experiment freely without sending data elsewhere.

The theorem’s significance goes beyond pure mathematics. In fluid mechanics, it translates conservation of mass into the condition that the divergence of velocity equals the local source density. In electromagnetism, Gauss’s law states that the flux of the electric field through a closed surface equals the enclosed charge divided by the permittivity of free space. Computational physicists routinely apply the divergence theorem to convert volumetric integrals into surface terms or vice versa, depending on which is easier to evaluate. By providing a concrete numerical demonstration, this calculator helps build intuition for such applications.

Another subtlety arises when the vector field is not defined everywhere in the volume or is discontinuous. The divergence theorem requires sufficient smoothness to exchange differentiation and integration. If singularities lie inside the region, such as a point charge generating an inverse-square field, the theorem still applies in a distributional sense, but naive numeric approximations may fail. Exploring these edge cases emphasizes the importance of understanding the assumptions behind the theorem.

Historically, Carl Friedrich Gauss developed the divergence theorem in the early nineteenth century while investigating gravitational potentials. His work built on earlier insights from Joseph-Louis Lagrange and Pierre-Simon Laplace about potentials and fluxes. Over time the theorem evolved into a fundamental identity of vector calculus, encapsulating how local divergence translates into global flow. The intuitive idea that “what flows out must come from somewhere” is thus formalized in a precise mathematical statement.

Because the divergence theorem generalizes to higher dimensions and more complex manifolds, mastering the three-dimensional box case lays the groundwork for deeper exploration. Advanced topics include applying the theorem in curvilinear coordinates, proving uniqueness of solutions to partial differential equations, and extending the concept to differential forms in exterior calculus. The simple box example computed here already hints at these broader connections by illustrating how geometry, analysis, and physical interpretation intertwine.

Finally, try experimenting with fields that exhibit sources and sinks, such as F= (x^2, y^2, z^2) or swirling flows like F=(−y, x, 0). Observe how the divergence integral responds: the swirling field has zero divergence everywhere, and correspondingly the flux through any closed surface vanishes, capturing the notion of a solenoidal or incompressible field. Such experiments deepen understanding of vector calculus and demonstrate the power of Gauss’s insight that the behavior of a field within a region is written on its boundary.

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