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Formulas in Electrodynamics Based on course by Yuri Lyubarsky and Edited By Eitan Rothstein Department of Physics, Ben-Gurion University, Beer-Sheva 84105, Israel 1 p·r̂ Electric dipole moment potential Vdip (r) = 4π 2 , with the electric dipole moment p = 0 r 1 1 The electric field of an electric dipole is Edip (r) = 4π 3 [3(p · r̂) · r̂ − p]. 0 r µ0 1 The magnetic field of a magnetic dipole is B (r) = dip 4π r 3 [3(m · r̂) · r̂ − m], R with the magnetic moment: m = 21 r × JdV Boundary conditions: 1 E1⊥ = 2 E2⊥ , k k E1 = E2 , B1⊥ = B2⊥ , R r0 ρ(r0 )d3 r0 = P i qi ri . 1 k 1 k B1 = B . µ1 µ2 2 Poynting vector: S = µ1 E × B. 1 Energy density: u = 2 E 2 + 2µ B2. 1 1 Maxwell stress tensor: Tij = 0 Ei Ej − δij E 2 + Bi Bj − 2 µ0 −1/2 Speed of light: c = (µ) . The electric dipole radiation. The electric field in the wave zone: 1 δij B 2 . 2 µ0 [[p̈ × n] × n]. 4πr µ0 [n × m̈]. The magnetic dipole radiation. The electric field in the wave zone: E = 4πcr Liénard-Wiechert potentials: V (r, t) = 1 qc , 4π0 r̃c − r̃ · v A(r, t) = E= v V (r, t), c2 where r̃ is the vector from the retarded position to the field point r and v is the velocity of the charge at the retarded time. Lorentz transformation: x̄ = γ(x − vt), v t̄ = γ(t − 2 x), c 1 γ = p . 1 − v 2 /c2 Intervals: ds2 = c2 dt2 − dx2 − dy 2 − dz 2 . eB Relativistic cyclotron frequency: ωB = mcγ . The field tensor: 0 −Ex /c −Ey /c −Ez /c ∂Aν ∂Aµ 0 Bz −By E /c Fµν = − = x Ey /c −Bz 0 Bx ∂xµ ∂xν Ez /c By −Bx 0 Transformation of fields: Ēk = Ek , B̄k = Bk , Ē⊥ = γ(E⊥ + v × B⊥ ), 1 B̄⊥ = γ(B⊥ − 2 v × E⊥ ). c Energy momentum four vector: P = mcγ(1, v/c).