
Uncorrected Proof
BookID 160928 ChapID 14 Proof# 1 - 29/07/09
14.7 Cyclotron Waves 435
1. Landau Damping and Doppler Shifted Cyclotron Resonance 222
Suppose an electromagnetic wave of frequency ω and wave number q prop- 223
agates inside a metal. To absorb energy from the electromagnetic wave, 224
the component of the velocity of an electron along the applied dc mag- 225
netic field must satisfy nω
c
+ q
z
v
z
= ω for some integral values of n. 226
When nω
c
− q
z
v
F
<ω<nω
c
+ q
z
v
F
, there are electrons capable of direct 227
absorption of energy from the electromagnetic field and we have cyclotron 228
damping even in the absence of collisions. However, if this condition is 229
not satisfied, then, for example, when | ω − ω
c
|>q
z
v
F
, there does not 230
exist any electron with v
z
=(ω
c
− ω)/q
z
, which would resonantly absorb 231
energy from the wave. For n = 0, this effect is usually known as Landau 232
damping. Then, we have −q
z
v
F
<ω<q
z
v
F
or −v
F
<v
phase
<v
F
.It 233
corresponds to having a phase velocity v
phase
parallel to B
0
equal to the 234
velocity of some electrons in the solid, i.e., −v
F
<v
z
<v
F
. These electrons 235
will ride the wave and thus absorb power from it resulting in collision- 236
less damping of the wave. For n = 0, the effect is usually called Doppler 237
shifted cyclotron resonance, because the effective frequency seen by the 238
moving electron is ω
eff
= ω −q
z
v
z
and it is equal to n times the cyclotron 239
resonance frequency ω
c
. 240
2. Bernstein Modes or Cyclotron Modes 241
These are the modes of vibration inanelectronplasma,whichoccur242
only when σ has a q-dependence. They are important in plasma physics, 243
where they are known as Bernstein modes. In solid-state physics, they are 244
known as nonlocal waves or cyclotron waves. These modes start out at 245
ω = nω
c
for q = 0. They propagate perpendicular to the dc magnetic field, 246
and depend for their existence (even at very long wavelengths) on the q 247
dependence of σ. 248
3. Quantum Waves 249
These are waves which arise from the gigantic quantum oscillations in σ. 250
These quantum effects depend, of course, on the q dependence of σ. 251
14.7 Cyclotron Waves 252
We will give only one example of the new kind of wave that can occur when 253
the q dependence of σ is taken into account. We consider the magnetic field in 254
the z-direction and the wave vector q in the y-direction. The secular equation 255
for wave propagation is the familiar 256
ε
xx
− ξ
2
ε
xy
0
−ε
xy
ε
yy
0
00ε
zz
− ξ
2
=0. (14.68)