## Classical Electrodynamics |

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Page 295

For ka > 1 , the second form in (9.109) can be used to obtain an asymptotic

oscillations explicitly. These approximate

give the ...

For ka > 1 , the second form in (9.109) can be used to obtain an asymptotic

**expression**, T~ 1 - 2ka sin (ika - -} \ 4/ + (9.110) which exhibits the smalloscillations explicitly. These approximate

**expressions**(9.109) and (9.110) for 7"give the ...

Page 446

The Fermi

energy loss, such as (13.35). But under conditions where polarization effects are

unimportant it yields the same results as before. For example, for nonrelativistic ...

The Fermi

**expression**(13.70) bears little resemblance to our previous results forenergy loss, such as (13.35). But under conditions where polarization effects are

unimportant it yields the same results as before. For example, for nonrelativistic ...

Page 447

where we have used the dipole moment

second term is small, the imaginary part of l/e(w) can be readily calculated and

substituted into (13.70). Then the integral over dw can be performed in the same

...

where we have used the dipole moment

**expression**(13.19). Assuming that thesecond term is small, the imaginary part of l/e(w) can be readily calculated and

substituted into (13.70). Then the integral over dw can be performed in the same

...

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### Contents

Introduction to Electrostatics | 1 |

Scalar potential | 7 |

Greens theorem | 14 |

Copyright | |

19 other sections not shown

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### Common terms and phrases

acceleration angle angular applied approximation assumed atomic average axis becomes boundary conditions calculate called Chapter charge charged particle classical collisions compared component conducting Consequently consider constant coordinates cross section cylinder defined density dependence derivative determine dielectric dimensions dipole direction discussed distance distribution effects electric field electromagnetic electron electrostatic energy equal equation example expansion expression factor force frame frequency function given gives incident inside integral involved light limit Lorentz loss magnetic magnetic field magnetic induction magnitude mass means modes momentum motion moving multipole normal observation obtain origin parallel particle physical plane plasma polarization position potential problem properties radiation radius region relation relative relativistic result satisfy scalar scattering shown in Fig shows side solution space sphere spherical surface transformation unit vanishes vector velocity volume wave written