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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 be calculated to be 2 ...
(14.46) 3 co It is instructive to compare the power radiated for acceleration
parallel to the velocity (14.43) or (14.27) with the power radiated for acceleration
perpendicular to the velocity (14.46) for the same magnitude of applied force.
The sudden creation of a fast electron in nuclear beta decay, for example, can be
viewed for our purposes as the violent acceleration of a charged particle initially
at rest to some final velocity in a very short time interval, or, alternatively, as the ...
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Introduction to Electrostatics
BoundaryValue Problems in Electrostatics I
BoundaryValue Problems in Electrostatics II
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