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 ?
		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?
		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
		With vectors we get
		y(r, t)  =  A · sin  · æ è r · k  –   w · t ö ø
		This defines k and by definition k is a vector in real space, pointing in the direction of wave propagation.
		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.
		Everything contained in this "basic" module. Everything contained in this module describing the relation of spin and magnetic moment. 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 ?
		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 ?
		"Number" of solution or state. Wave length l = 2l /|k| Momentum p = k Total energy E via dispersion relation (for free electron gas E µ k2 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.
		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
		Do it! Check the link for details to the Boltzmann distribution.

		How does on always derive the density of states D (E) ?
		Volume of "onion skin" in phase space.

		Compare the free electron model with and withour diffraction.
		Free elektron gas Free elektron gas with diffraction Potential V(x,y,z) V = const = 0 Vx = V0 · cos (2p x/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)  =   (2 me)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 Ei – EF kT ö ø + 1 f(E, T)   =  1 exp æ è Ei – EF kT ö ø + 1 the Fermi distributoin always obtains!

With frame

Exercise 2.1-1: Quick Questions to: 2.1 Basic Band Theory

© H. Föll (Semiconductors - Script)