Solutions to

Quick Questions to

2.1 Basic Band Theory

Solutions to quick questions to 2.1.1: Essentials of the Free Electron Gas
What happens, if you do not choose U = U0 = 0 but U = U1 ?
{short description of image} The Energy scale for the total energy E moves up or down by U1 since U1 · y can be added to E · y.
What does the sentence "...a plane wave with amplitude (1/L)3/2 moving in the direction of the wave vector k" mean"? Wave vectors, after all, are defined in reciprocal space with a dimension 1/cm. What, exactly, is their direction in real space?
{short description of image} The velocity vector of a car in real space has the dimension cm/s - the dimension 1/cm for wave vectors thus means nothing. The wave vector comes into being by writing the components of a plane wave as follows
 
y(xi, t)  =  A · sin  · æ
è
2p xi
li
 –   w · t ö
ø
 
{short description of image} With vectors we get
 
y(r, t)  =  A · sin  · æ
è
r · k  –   w · t ö
ø
   
{short description of image} This defines k and by definition k is a vector in real space, pointing in the direction of wave propagation.
{short description of image} The better question is: If we know k in reciprocal space (= Fourier transform of the real space), how can we conclude on the direction in real space? The answer is. Reciprocal lattice vectors with components kh.k.l are perpendicular to the lattice plane in real space with Miller indices (hkl) - the direction in real space is thus given
Recount what you know bout the spin of an electron.
{short description of image}
  1. Everything contained in this "basic" module.
  2. Everything contained in this module describing the relation of spin and magnetic moment.
  3. The catchword "Spintronics" should also come up in this context.
Where does the (1/L)3/2 in the solution come from? What would one expect for a crystal woth the dimension Lx, Ly, Lz?
{short description of image} From the normalizing condition. The factor should change from (1/L)3/2 = (1/L3)1/2 to (1/V3)1/2.
What kind of information is contained in the wave vector k?
  1. "Number" of solution or state.
  2. Wave length l = 2l/|k|
  3. Momentum p = {short description of image}k
  4. Total energy E via dispersion relation (for free electron gas E µ k2
  5. Propagation direction pf plane wave with k
Consider a system with some given energy levels (including possibly energy continua). Distribute a number N of classical particles, of Fermions and of Bosons on these levels. Describe the basic priciples.
{short description of image} Fermions = Fermi-Dirac distribution
Bosons = Bose-Einstein distribution (which we don't know so far)
Classical = Boltzmann distribution and an approximation to the two fundamental ones
{short description of image} Do it! Check the link for details to the Boltzmann distribution.
 
Fermi-Dirac distribution
 
1
f(E, T) =  
  exp æ
è
EEF
kT
ö
ø
 +  1
Bose- Einstein distribution
 
1
f(E, T) 
  exp æ
è
EEF
kT
ö
ø
   1
Boltzmann distribution


f(E, T)   =  exp– æ
è
E
kT
ö
ø


 
How does on always derive the density of states D(E)?
{short description of image} Volume of "onion skin" in phase space.
{short description of image}
     
Compare the free electron model with and withour diffraction.
{short description of image}

Free elektron gas Free elektron gas
with diffraction
Potential
V(x,y,z)
V = const = 0 Vx = V0 · cos (2px/a1)
Vy = V0 · cos (2py/a2)
Vz = V0 · cos (2pz/a3)
V0 ® 0
Wavefunktion
y(x,y,z)
y  =  æ
ç
è
1
L
ö
÷
ø
3/2 · eikr  
y  =   æ
ç
è
1
L
ö
÷
ø
3/2 · eikr  
except for wavevectors kB that are being diffracted.
Wave vectors
k
kx = ± nx · 2p / L
ky = ± ny · 2p / L
kz = ± nz · 2p / L
 
ni = 0, ±1, ±2, ...
kx = ± nx · 2p / L
ky = ± ny · 2p / L
kz = ± nz · 2p / L
 
ni = 0, ±1, ±2, ...
Energy E Total energy = const = Ekin Total energy = const = Ekin
except for wavevectors kB that are being diffracted; then some potential energy comes into play.
Dispersion function
E(k)
E  =   2k2
2m
E  = 2k2
2m

except for wavevectors kB that are being diffracted.
Density of states
D(E)
D(E)  =  (2me)3/2
23p2
E1/2
D(E)  =   (2me)3/2
23p2
E1/2
as a first approximation., Could be rather different, however.
Probability of
state being
occupied

f(E,T)
f(E, T)   =  


1
exp æ
è
EiEF
kT
ö
ø
+ 1
f(E, T)   = 


1
exp æ
è
EiEF
kT
ö
ø
+ 1
the Fermi distributoin always obtains!
     
     

Zum Index Zum Index

gehe zu 2.1.1 Das Bindungspotential

gehe zu 2.1.2 Bindungspotentiale, Federn, und der Elastizitätsmodul

gehe zu 2.1.3 Bindungspotentiale und weitere Eigenschaften

gehe zu 2.1.4 Vom Bindungspotential zum Kristall

gehe zu 2.1.5 Merkpunkte zu Kapitel 2.1

© H. Föll