
Gauss's divergence theorem relates the flux of a vector field through a closed surface to the divergence of the field within the volume it encloses.In mathematics, this is the divergence theorem, independently formulated by Carl Friedrich Gauss (for gravity), Mikhail Ostrogradsky (in a more general form), and George Green. In physics, it became the basis of Gauss's law for electricity (one of Maxwell's equations) and for gravity. The idea: the total 'outflow' of a field inside a volume equals the flux through its boundary. For electricity: ∮ E·dA = Q/ε₀ — a charge creates a field, and its flux through any closed surface enclosing the charge is the same.
Carl Friedrich Gauss used this result in 1813 in the theory of magnetic potentials, and in 1828 Mikhail Ostrogradsky gave the first general proof. George Green also derived related theorems. Gauss introduced the theorem into physics, formulating the law for electric fields in 1835. Later, James Clerk Maxwell included Gauss's law in his system of equations, and in the 20th century, the theorem found application in relativity and quantum field theory.
Gauss's theorem allows calculating fields of high symmetry (spheres, cylinders, planes) without complex integration. It is used in engineering calculations of electrostatic shields, gravitational lenses, and in fluid dynamics. Limitation: requires differentiability of the field and smoothness of the surface; for regions with discontinuities (e.g., on charged plates), boundary conditions are used.
Calculation of electric and gravitational fields, design of electrostatic shields and lightning rods.
The theorem works even in the curved space-time of general relativity, where it enters Einstein's equations for gravity.
| \Phi | variable | flux (power per unit area) — irradiance watt per square metre |
| d | variable | distance from source — distance metre |
| M | variable | Total mass of the system — mass kilogram |
| R | variable | Characteristic radius of the system — radius metre |
| v | variable | Velocity dispersion (typical random velocity) — velocity dispersion metre per second |
| G | constant | Constant of universal gravitation — gravitational constant = 6.67430e-11 cubic metre per kilogram per second squared |
| i | variable | index for K-theory group (0 or 1) — index |
| j | variable | homology degree index — index |
| \bigoplus | operator | combines multiple abelian groups into one — direct sum |
| J | variable | Diffusive flux (amount per unit area per unit time) — diffusive flux mole per square metre per second |
| c | variable | Concentration of the diffusing species — concentration mole per cubic metre |
| x | variable | Spatial coordinate along the diffusion direction — position metre |
| D | constant | Material-specific proportionality constant relating flux to concentration gradient — diffusion coefficient = varies square metre per second |
| ∂/∂x | operator | Partial derivative with respect to position — partial derivative |







