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Comparison with (2.81)–(2.83) shows that form invariance of Faraday’s law under the
                        Lorentz transformation requires




                                      E = E x ,   E = γ(E y − vB z ),  E = γ(E z + vB y ),
                                       x           y                    z
                        and
                                                            v                      v

                                   B = B x ,   B = γ B y +    E z ,    B = γ B z −   E y .



                                     x           y           2          z           2
                                                            c                      c
                        To generalize v to any direction, we simply note that the components of the fields parallel
                        to the velocity direction are identical in the moving and laboratory frames, while the
                        components perpendicular to the velocity direction convert according to a simple cross
                        product rule. After similar analyses with Ampere’s and Gauss’s laws (see Problem 2.2),
                        we find that

                                        E = E   ,   B = B   ,   D = D   ,   H = H   ,




                                                    E = γ(E ⊥ + β × cB ⊥ ),                    (2.87)

                                                     ⊥

                                                   cB = γ(cB ⊥ − β × E ⊥ ),                    (2.88)
                                                     ⊥

                                                   cD = γ(cD ⊥ + β × H ⊥ ),                    (2.89)
                                                     ⊥

                                                    H = γ(H ⊥ − β × cD ⊥ ),                    (2.90)
                                                     ⊥
                        and

                                                      J = γ(J   − ρv),                         (2.91)


                                                      J = J ⊥ ,                                (2.92)
                                                       ⊥

                                                     cρ = γ(cρ − β · J),                       (2.93)
                        where the symbols   and ⊥ designate the components of the field parallel and perpen-
                        dicular to v, respectively.
                          These conversions are self-consistent, and the Lorentz transformation is the transfor-
                                                                                  2
                                                                             2
                        mation under which Maxwell’s equations are covariant. If v   c , then γ ≈ 1 and to
                        first order (2.87)–(2.93) reduce to (2.61)–(2.66). If v/c   1, then the first-order fields
                        reduce to the Galilean fields (2.49)–(2.54).
                          To convert in the opposite direction, we can swap primed and unprimed fields and
                        change the sign on v:


                                                    E ⊥ = γ(E − β × cB ),                      (2.94)
                                                            ⊥         ⊥


                                                   cB ⊥ = γ(cB + β × E ),                      (2.95)
                                                             ⊥        ⊥


                                                   cD ⊥ = γ(cD − β × H ),                      (2.96)
                                                             ⊥        ⊥


                                                    H ⊥ = γ(H + β × cD ),                      (2.97)
                                                             ⊥        ⊥
                        and


                                                      J   = γ(J + ρ v),                        (2.98)


                                                     J ⊥ = J ,                                 (2.99)
                                                           ⊥
                                                      cρ = γ(cρ + β · J ).                    (2.100)


                          The conversion formulas can be written much more succinctly in dyadic notation:
                                                                  ¯

                                                  E = γ ¯α −1  · E + γ β · (cB),              (2.101)
                                                          ¯
                                                 cB =−γ β · E + γ ¯α −1  · (cB),              (2.102)

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