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Electromagnetism

Electrostatics in Vacuum

Physics II 290 words Free to read

Two Statements That Fix the Field

Electrostatics rests on two field equations. Gauss's law says the flux of E\mathbf{E} through any closed surface counts the charge inside it:

EdA=Qencε0\oint \mathbf{E} \cdot d\mathbf{A} = \frac{Q_{enc}}{\varepsilon_0}

with ε0=8.854×1012\varepsilon_0 = 8.854 \times 10^{-12} F/m. Its local form follows from the divergence theorem:

E=ρε0\nabla \cdot \mathbf{E} = \frac{\rho}{\varepsilon_0}

The second statement is that the electrostatic field has no circulation: Edl=0\oint \mathbf{E} \cdot d\mathbf{l} = 0, or locally ×E=0\nabla \times \mathbf{E} = \mathbf{0}. A curl-free field is a gradient, which is exactly what licenses a scalar potential:

E=V\mathbf{E} = -\nabla V

Combining the two gives Poisson's equation 2V=ρ/ε0\nabla^2 V = -\rho/\varepsilon_0, which reduces to Laplace's equation 2V=0\nabla^2 V = 0 wherever the charge density vanishes.

Gauss's law is always true but only useful when symmetry lets you pull EE out of the integral. Three cases carry most of the work:

SymmetryField outsideFalls as
Point / sphereQ/4πε0r2Q/4\pi\varepsilon_0 r^21/r21/r^2
Infinite lineλ/2πε0r\lambda/2\pi\varepsilon_0 r1/r1/r
Infinite planeσ/2ε0\sigma/2\varepsilon_0constant

At a boundary the field obeys continuity conditions: the tangential component of E\mathbf{E} is always continuous, while the normal component jumps by σ/ε0\sigma/\varepsilon_0.

Far from a neutral but polarised object, the leading term is the dipole: p=qd\mathbf{p} = q\mathbf{d}, with a potential falling as 1/r21/r^2 and a field as 1/r31/r^3, faster than a point charge, because the two charges nearly cancel.

Common pitfall: reading a Gaussian surface with zero net flux as a region with no field. Flux counts only the enclosed charge. A surface drawn around a dipole encloses zero net charge and has zero total flux, while the field on it is large everywhere.
Four symmetries, one growing distance: how fast each field falls

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Electromagnetism