Classical ElectrodynamicsProblems after each chapter |
From inside the book
Results 1-3 of 85
Page 169
... magnetic phenomena disappears when we consider time - dependent problems . Time - varying magnetic fields give rise to electric fields and vice - versa . We then must speak of electromagnetic fields , rather than electric or magnetic fields ...
... magnetic phenomena disappears when we consider time - dependent problems . Time - varying magnetic fields give rise to electric fields and vice - versa . We then must speak of electromagnetic fields , rather than electric or magnetic fields ...
Page 189
... electromagnetic fields E and B is qv . E , where v is the velocity of the charge . The magnetic field does no work , since the magnetic force is perpendicular to the velocity . If there exists a continuous distribution of charge and ...
... electromagnetic fields E and B is qv . E , where v is the velocity of the charge . The magnetic field does no work , since the magnetic force is perpendicular to the velocity . If there exists a continuous distribution of charge and ...
Page 380
... Electromagnetic Fields Since the fields E and B are elements of the field - strength tensor F their transformation properties can be found from Fuv = aμ¿avo Fio μες ( 11.113 ) With transformation ( 11.75 ) from a system K to K ' moving ...
... Electromagnetic Fields Since the fields E and B are elements of the field - strength tensor F their transformation properties can be found from Fuv = aμ¿avo Fio μες ( 11.113 ) With transformation ( 11.75 ) from a system K to K ' moving ...
Other editions - View all
Common terms and phrases
4-vector Ampère's law angle angular distribution approximation atomic axis boundary conditions calculate Chapter charge density charge q charged particle coefficients collisions component conductor consider coordinates cross section current density cylinder d³x delta function dielectric constant diffraction dimensions dipole direction discussed E₁ electric field electromagnetic fields electron electrostatic energy loss expansion expression factor frequency given Green's function impact parameter incident particle inside integral inversion Laplace's equation linear Lorentz transformation macroscopic magnetic field magnetic induction magnetic moment magnitude Maxwell's equations meson modes molecules momentum motion multipole nonrelativistic normal obtain oscillations P₁ parallel plasma point charge Poisson's equation polarization problem radiation radius region relativistic result scalar scalar potential scattering shown in Fig shows solution spherical surface surface-charge density theorem transverse unit V₁ vanishes vector potential velocity volume wave equation wave number wavelength written zero ΦΩ