Classical ElectrodynamicsProblems after each chapter |
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Page 161
The nonlinear relation ( 5.87 ) and the phenomenon of hysteresis allow the creation of permanent magnets . We can solve equations ( 5.112 ) for one relation between Hin and Bin by eliminating M : Bin + 2Hin = = 3B .
The nonlinear relation ( 5.87 ) and the phenomenon of hysteresis allow the creation of permanent magnets . We can solve equations ( 5.112 ) for one relation between Hin and Bin by eliminating M : Bin + 2Hin = = 3B .
Page 346
( c ) What is the meaning of the singularity in the dispersion relation when k · v = w ? V 10.7 Consider the problem of waves in an electronic plasma when an external magnetic field B , is present . Use the fluid model , neglecting the ...
( c ) What is the meaning of the singularity in the dispersion relation when k · v = w ? V 10.7 Consider the problem of waves in an electronic plasma when an external magnetic field B , is present . Use the fluid model , neglecting the ...
Page 627
... for bremsstrahl . ung , 512 Classical electron radius , 490 , 589 Clausius - Mossotti relation , 119 Closure , see Completeness relation Collisions , between charged particles as energy - loss mechanism , 430 relativistic kinematics ...
... for bremsstrahl . ung , 512 Classical electron radius , 490 , 589 Clausius - Mossotti relation , 119 Closure , see Completeness relation Collisions , between charged particles as energy - loss mechanism , 430 relativistic kinematics ...
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Contents
Introduction to Electrostatics | 1 |
References and suggested reading | 23 |
Multipoles Electrostatics of Macroscopic Media | 98 |
Copyright | |
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