e in Magnetic - TU Graz
Transcript of e in Magnetic - TU Graz
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Institute of Solid State PhysicsTechnische Universität Graz
Free Electrons in a Magnetic Field
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Charged particle in a magnetic field
F ev B ma
2
zmvevB
R
x
y
kx
ky
2c
Rv RT
zc
eBm
Institute of Solid State PhysicsTechnische Universität Graz
Magnetron
zeB Rvm
solve for velocity
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Why don't metals in a B field radiate?
x
y
kx
ky
zc
eBm
Magnetron
There are no lower lying states to fall into. We need a quantum description.
2 2
2 ( )2
d V x Em dx
Magnetic force depends on the velocity, not on the position.
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Electrons in a magnetic field
Euler Lagrange equations
Lagrangian:
Kittel: Appendix Ghttp://lamp.tu-graz.ac.at/~hadley/ss2/IQHE/cpimf.php
F q E v B
0i i
d L Ldt x x
212 , ,L mv qV r t qv A r t
Lorentz force law
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Lagrangian
,
x xx x
x
x x x x x
x x x x xx y z
dv dAd L d mv qA m qdt v dt dt dt
dv A A A Adx dy dzm qdt dt x dt y dt z t
dv A A A Am q v v vdt x y z t
212 , ,L mv qV r t qv A r t
yx zx y z
AA AL Vq q v v vx x x x x
yx x x xzy z
Adv A A AAVm q q v vdt x t x y x z
0i i
d L Ldt x x
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kinetic momentum field momentum(inductance)
yx x x xzy z
Adv A A AAVm q q v vdt x t x y x z
Lagrangian
212 , ,L mv qV r t qv A r t
and AE V B At
xx x
dvm q E v Bdt
x x xx
Lp mv qAv
1x x xv p qA
m
conjugate variable:
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Hamiltonian
Schrödinger equation
p i
Classical result
212 , ,L mv qV r t qv A r t
H v p L
Legendre transformation
212
H p qA qVm
212
i i qA qVt m
1x x xv p qA
m
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Landau Levels
21 ( ) ( ).2
i qA r E rm
free particles in a magnetic field
ˆ.zA B xy
Landau gauge
V = 0
ˆ ˆ ˆ ˆ.y yx xz zz
dA dAdA dAdA dAB A B xy x y zdy dz dz dx dx dy
ˆ.zB B z
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Landau Levels
21 ( ) ( ).2
i qA r E rm
free particles in a magnetic field
ˆ.zA B xy
Landau gauge
2 2 2 2 21 2 .2 z z
di qB x q B x Em dy
( ).y zik y ik ze e x
The solution has the form
V = 0
2
ˆ ˆz zi qA i qB xy i qB xy
ˆ ˆ ˆ ˆˆz z zd d d di qB xy i x y z qB xy i qB xdx dy dz dy
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Landau Levels
2 2 2 2 21 2 .2 z z
di qB x q B x Em dy
( ).y zik y ik ze e x
The solution has the form
22 2 2 2 2 2 2 2
2
1 2 ( ) ( ).2 z y z y zk k qB k x q B x x E x
m x
Substitute this into the equation
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The equation for (x) is
This is the equation for a harmonic oscillator
22 2 2 2 2 2 2 2
2
1 2 ( ) ( ).2 z y z y zk k qB k x q B x x E x
m x
2 2 222 2 2
2
1 ( ) ( ).2 2
y zz
z
k kq B x x E xm x qB m
2 2
202 ( ) ( ).
2 2K x x x E x
m x
Landau Levels
2
y zk qB x
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This is the equation for a harmonic oscillator
2 22
22 2 202
1 ( ) ( ).2 2
zz
kq B x x x E xm x m
2 2
1, 22z
zk v c
kE vm
zc
qBm
Landau Levels
0y
z
kx
qB
2 2
2 2z
zc
q BKm
qBKm m
2 2
202 ( ) ( ).
2 2K x x x E x
m x
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Charged particle in a magnetic field
x
y
Circular motion is harmonic motion. Harmonic motion is quantized.
2
2 212 2v c x yE v k k
m
2 R v
v labels the Landau level
kx
ky
Bohr - Sommerfeld quantization
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Landau levels
The number of solutions is conserved
kx
ky
B = 0
kx
ky
B 0
22L
In 2-D, the k-volume per k state is:
0( ).yik ye x x 0y
z
kx
qB
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Density of states 2D
12v cE v
The number of states between ring v-1 and ring v is
2 21
22v vk k
L
2 2
122
vc
k vm
2 2 1 11 2 2
2 21c cv v
m mk k v v
2
2cm L
kx
kykv
The number of states between ring v-1 and ring v is
The density of states per spin is2
cm
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Spin
In a magnetic field, there is a shift of the energy of the electrons because of their spin.
Bohr magneton
2cm
2 BgE B B
D(E)
E0
D(E)
E0
2
m
c
2Be
em
1 12 4 2 4
0
( )2
g gcc c
v
mD E E v E v
B = 0 B 0
g-factor 2g 2c BeB Bm
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Energy spectral density 2d
At T = 0
unfilled Landau level
analog to the Planck radiation law
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Fermi energy 2d
Periodic in 1/BWhen there is only one Landau level, the Fermi energy rises linearly with field.
2 2c
FeBEm
Large field limit
( )FE
n D E dE
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Internal energy 2d
At T = 0
2 2c eBu n n
m
Large field limit
( )FE
u ED E dE
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Magnetization 2d
At T = 0
2du em ndB m
Large field limit
de Haas - van Alphen oscillations
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Shubnikov-De Haas oscillations
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Scattering at the Fermi surface
At room temperature, phonon energies are much less than the Fermi energy. The energy of electrons hardly changes as they scatter from phonons. Electrons scatter from a point close to the Fermi surface to another point close to the Fermi surface.
Changing the magnetic field changes the number of states at the Fermi energy.
There are oscillations in the electrical conductivity as a function of magnetic field.