waves in plasma very short course
DESCRIPTION
Outline Introduction – some definitions Self-consistency, linear theory Transverse waves in unmagnetized plasma Longitudinal waves, Landau damping Waves in magnetized plasma Beam-plasma instabilities, plasma masersTRANSCRIPT
Waves in Plasma
Very short course
Outline
• Introduction – some definitions
• Self-consistency, linear theory
• Transverse waves in unmagnetized plasma
• Longitudinal waves, Landau damping
• Waves in magnetized plasma
• Beam-plasma instabilities, plasma masers
• Introduction – some definitions• Self-consistency, linear theory
• Transverse waves in unmagnetized plasma
• Longitudinal waves, Landau damping
• Waves in magnetized plasma
• Beam-plasma instabilities, plasma masers
What is a wave?A wave is a perturbation propagating in space
Gerald B. Whitham, ``Linear and Nonlinear Waves''
a lot of physical phenomena
Shock wave
Solitary wave
Solitary wave in a lab
Nonlinear waves
Out of scope of the course
We restrict ourselves by considering only linear waves
Linear waves
Mathematically, a process described by linear equations
Wave equation 012
2
2
tc
Partial solution in Cartesian coordinates – monochromatic plain wave
222)( , zyxtrki kkkcckAe
Particularly, Maxwell equations in vacuum are linear equations and can be reduced to the wave equation
What about plasma?
is a linear equation
Plasma is a ``fourth state of a matter'‘ as defined by Russian physicist Frank-Kamenetsky)
Temperature
Solid state Liquid Gas Plasma
Most general definition: plasma is an ensemble of charged particles
(less general one includes the condition of quasi-neutrality)
In the ensemble of charged particles, the long-range forces appear.
The motion of each charged particle is determined by electric and magnetic fields, which, in their turn, are created by a large number of other charged particles, i.e., depend on their velocities and locations.
The motion of ions and electrons occurs in self-consistent fields.
The self-consistent long-range e/m fields allow passing information about particles motion from one region to another without collisions. This is the main difference between plasma waves and, for instance, sound waves and waves at a water surface.
to be described by Maxwell equations
• Introduction – some definitions
• Self-consistency, linear theory• Transverse waves in unmagnetized plasma
• Longitudinal waves, Landau damping
• Waves in magnetized plasma
• Beam-plasma instabilities, plasma masers
Maxwell equations in vacuum
external current and charge densities do not depend on fields
In plasma, assuming 0 ,0 extextj
Only currents and charges remain that depend on fields
40
1
41
E
Ht
Hc
E
jct
Ec
H
),(4
0
1
),(41
trE
Ht
Hc
E
trjct
Ec
H
ext
ext
How to find this dependence?
Vnejne
,
0
1
Vnt
n
VHVc
Eme
dtVd
means a sort of particles
Equation of motion
Continuity equation
Simplest model for the self-consistent set of equations
Kinetic equation in the self-consistent fields
),,( trVf
Distribution function
Number density VdtrVftrn 3),,(),(
;),,( ;),,( 33 VdtrVfVejVdtrVfe
thermal motion is accounted
natural normalizing
Liuville equation: 0
dtVd
Vf
dtrd
rf
tf
dtdf
No particles are born
No particles are died
No collisions (free motion in e/m fields)01
fHVc
EmefV
tf
V
Vlasov equation:
Vlasov + Maxwell = Vlasov-Maxwell set of equations
One more example is the magnetohydrodynamic model
0
0
1
1
D
BtB
cE
tD
cH
Maxwell equations in medium
Plasma as a medium
40
1
41
E
Ht
Hc
E
jct
Ec
H
jtE
tD
HB
4
ED
Dielectric permittivity
For linear waves, only linear terms should be kept for j
and
Accordingly, the permittivity tensor does not depend on fields
Permittivity tensor contains all information about linear properties of a medium and depends on parameters of the medium steady-state: density, temperature, external fields, etc.
Linear theory
tH
cE
tE
cH
1
)ˆ(1 )(0
)(0 , trkitrki eHHeEE
HkiHEkiE
,
EkcH
Ec
Ekkc
ˆ E
ckkEEkk
ˆ)()( 2
2
0ˆ)( 2
22 E
cEkkEk
it
02
22
jjij
jjjii E
cEkkEk 02
22
jjijjiij E
ckkk
0det 2
22 ijjiij c
kkk Dispersion relation
),( kijij
Transverse waves and longitudinal waves
0ˆ)( 2
22 E
cEkkEk
k
E
kE
0Ek
EkEkk
2)(
0det 2
22 ijij c
k
ijij k ),(
0det ijED
For isotropic medium
0),( k0),(2
22 k
ck
Dispersion relation
Dispersion relation
In vacuumno way!ck