Classical Electrodynamics |
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Page 388
... acceleration a ' . Find the Lorentz transformation law for accelerations , and show that in the system K the components of acceleration parallel and perpendicular to v are al a 1 + - 22131⁄2 2 c2 ( 1-9 ) 1 + c2 3 a ‚ ' x ( a ' x u ...
... acceleration a ' . Find the Lorentz transformation law for accelerations , and show that in the system K the components of acceleration parallel and perpendicular to v are al a 1 + - 22131⁄2 2 c2 ( 1-9 ) 1 + c2 3 a ‚ ' x ( a ' x u ...
Page 472
... acceleration . For relativistic motion the acceleration fields depend on the velocity as well as the acceleration . Consequently the angular distribution is more complicated . From ( 14.14 ) the radial component of Poynting's vector can ...
... acceleration . For relativistic motion the acceleration fields depend on the velocity as well as the acceleration . Consequently the angular distribution is more complicated . From ( 14.14 ) the radial component of Poynting's vector can ...
Page 475
... acceleration perpendicular to the velocity ( 14.46 ) for the same magnitude of applied force . For circular motion ... acceleration is a factor of y2 larger than with a parallel acceleration . 14.4 Radiation Emitted by a Charge in ...
... acceleration perpendicular to the velocity ( 14.46 ) for the same magnitude of applied force . For circular motion ... acceleration is a factor of y2 larger than with a parallel acceleration . 14.4 Radiation Emitted by a Charge in ...
Common terms and phrases
4-vector acceleration Ampère's law angle angular distribution antenna approximation atomic axis Babinet's principle behavior boundary conditions calculate cavity Chapter charge q charged particle coefficients collisions component conducting conductor constant coordinate cross section cylinder d³x dielectric dielectric constant diffraction dipole direction discussed E₁ electric field electromagnetic fields electron electrostatic energy loss factor force equation frame frequency given Green's function impact parameter incident particle integral Kirchhoff Lagrangian Laplace's equation Lorentz force Lorentz invariant Lorentz transformation m₁ magnetic field magnetic induction magnitude Maxwell's equations meson modes momentum multipole nonrelativistic obtain oscillations P₁ P₂ parallel perpendicular phase velocity plane wave plasma polarization power radiated problem propagation radius region relativistic result scalar scattering screen shown in Fig shows sin² solution sphere spherical surface transverse unit V₁ vanishes vector potential velocity wave guide wave number wavelength ΦΩ