## Classical Electrodynamics |

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Page

The general formulas developed in this section, especially (14.65) and (14.67),

will be applied in this chapter and subsequent ones to various problems

involving the

applied ...

The general formulas developed in this section, especially (14.65) and (14.67),

will be applied in this chapter and subsequent ones to various problems

involving the

**emission**of radiation. The magnetic-moment formula (14.74) will beapplied ...

Page

In radiation problems, such as the

decay, the wave nature of the charged ... are relatively hard to include (see

Chapter 17), but also because of the discrete quantum nature of the photons

In radiation problems, such as the

**emission**of bremsstrahlung or radiative betadecay, the wave nature of the charged ... are relatively hard to include (see

Chapter 17), but also because of the discrete quantum nature of the photons

**emitted**.Page

Actually, modifications arise because a neutrino is always

capture process. The probability of

depend on the square of its energy E. When no photon is

has ...

Actually, modifications arise because a neutrino is always

**emitted**in the electron-capture process. The probability of

**emission**of the neutrino can be shown todepend on the square of its energy E. When no photon is

**emitted**, the neutrinohas ...

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### Contents

Introduction to Electrostatics | 1 |

Nš 3 | 3 |

Greens theorem | 14 |

Copyright | |

30 other sections not shown

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