Classical ElectrodynamicsProblems after each chapter |
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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 2213 % 3 all ' u ' 1 + c2 1 + + 1/2 × ( a ' × u ' ) ) x x C2 ...
... 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 2213 % 3 all ' u ' 1 + c2 1 + + 1/2 × ( a ' × u ' ) ) x x C2 ...
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 is a factor of 2 larger than with a parallel acceleration . 14.4 Radiation Emitted by a Charge in Arbitrary , Extreme Relativistic Motion For a charged particle undergoing arbitrary , extreme relativistic motion the ...
... acceleration is a factor of 2 larger than with a parallel acceleration . 14.4 Radiation Emitted by a Charge in Arbitrary , Extreme Relativistic Motion For a charged particle undergoing arbitrary , extreme relativistic motion the ...
Contents
1 | 1 |
BoundaryValue Problems in Electrostatics I | 26 |
Dielectrics | 98 |
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4-vector acceleration Ampère's law angular distribution approximation atomic axis behavior boundary conditions bremsstrahlung calculation Chapter charge q charged particle Cherenkov radiation classical coefficients collisions component conducting conductor consider constant coordinate cross section cylinder d³x dielectric diffraction dipole direction discussed E₁ electric field electromagnetic fields electron electrostatic emitted energy loss energy transfer equation of motion factor force equation frame frequency given Green's function impact parameter incident particle integral Lagrangian limit Lorentz force Lorentz invariant Lorentz transformation m₁ magnetic field magnetic induction magnitude Maxwell's equations meson modes momentum multipole nonrelativistic obtain orbit oscillations P₁ P₂ parallel perpendicular photon plane plasma polarization power radiated problem quantum quantum-mechanical radius region relativistic result scalar scattering screen shown in Fig shows sin² solid angle solution spectrum sphere spherical surface transverse V₁ vanishes vector potential wave number wavelength ΦΩ