C hapter 6: Free Electron Fermi Gas

1. Chapter 6: Free Electron Fermi Gas

2. Free Electron Theory • Conductorsfall into 2 main classes; metals& semiconductors. Here, we focus on metals. • A metalis loosely defined as a solid with valence electrons that are not tightly bound to the atoms but are relatively easily able to move throughthe whole crystal. • The room temperature conductivity of metals is in the range and it increases on the addition of small amounts of impurities. The resistivity normally decreasesmonotonically with decreasing temperature & can be reduced by the addition of small amounts of impurity.

3. Question! Why do mobile(conducting) electrons occur in some solids &not in others? • When the interactions between electrons are • considered,thisbecomes a • Very Difficult Questionto Answer. • D • Some Common Physical Properties of Metals: • Great Physical Strength, High Density, Good • Electrical and Thermal Conductivity, etc. • Here,we outline a surprisingly simple theory • which does a very good job of explaining many of • thesecommon properties ofmetals.

4. “The Free Electron Model” • We begin with the assumptionthat conduction • electrons exist&that they consist of the • valenceelectronsfrom the metal atoms. • Thus, metallicNa,Mg & Al are assumed tohave • 1, 2 & 3mobile electrons per atom, respectively. • This model seems at first as if it is • Way Too Simple! • But, this simple model worksremarkably • wellfor many metals & it will be used to help • to explain many properties ofmetals.

5. According to this Free Electron Model(FEM) the valence electrons are responsible for the conduction of electricity, & for this reason these electrons are called “Conduction Electrons”. • As an example, consider Sodium (Na). • The electron configuration of the Free Na Atomis: 1s2 2s2 2p6 3s1 • The outer electron in the third atomic shell (n = 3, ℓ = 0) is the electron which is responsible for the chemical properties of Na. Valence Electron (loosely bound) Core Electrons

6. When Na atoms are put together to form a Na metal, • Na has a BCC structure & the distance between nearest neighbors is 3.7 A˚ • The radius of the third shell in Na iis1.9 A˚ • In the solid the electron wavefunctions of the Na atoms overlap slightly. From this observation it follows that a valence electron is no longer attached to a particular ion, but belongs to both neighboring ions at the same time. Na metal

7. V -L/2 L/2 0 • Therefore, these conduction electrons can be considered as moving independentlyin a square well of finite depth& the edges of the well correspond to the edges of the sample. • Consider a metal with a cubic shape with edge length L: Ψ and E can be found by solving the Schrödinger equation: Since Use periodic boundary conditions & get the Ψ’s as travelling plane waves.

8. The solutions to the Schrödinger equation are plane waves, where V is the volume of the cube, V=L3 So the wave vector must satisfy where p, q, r taking any integer values; +ve, -ve or zero. Normalization constant

9. The wave function Ψ(x,y,z) corresponds to an energy The corresponding momentum is: The energy is completely kinetic:

10. We know that the number of allowed k values inside a spherical shell of k-space of radiusk is: • Here g(k) is the density of states per unit magnitude of k.

11. Number of Allowed States per Unit Energy Range? Each k state represents two possible electron states, one for spin up, the other is spin down.

12. Ground State of the Free Electron Gas Electrons are Fermions (s = ± ½)and obey the Pauli exclusion principle; each state can accommodate only one electron. The lowest-energy state of N free electrons is therefore obtained by filling the N states of lowest energy.

13. Thus all states are filled up to an energy EF,known as The Fermi energy,obtained by integrating the density of states between 0 and EF, The result should equal N.Remember that Solving for EF(Fermi energy);

14. The occupied states are inside the Fermi sphere in k-space as shown below; the radius is Fermi wave number kF. kz Fermi Surface E=EF kF ky kx From these two equations,kFcan be found as, The surface of the Fermi sphere represents the boundary between occupied & unoccupied k states at absolute zero for the free electron gas.

15. Typical values may be obtained by using monovalent potassium metal (K) as an example; for potassium the atomic density and hence the valence electron density N/V is 1.402x1028 m-3 so that The Fermi (degeneracy) Temperature TF is given by

16. It is only at a temperature of this order that the particles in a classical gas can attain(gain) kinetic energies as high asEF . Only at temperatures above TF will the free electron gas behave like a classical gas. Fermi momentum These are the momentum & velocity values of the electrons at the states on the Fermi surface of the Fermi sphere. So, the Fermi Sphere plays an important role in the behavior of metals.

17. Typical values for monovalent potassium metal;

19. Free Electron Gas at Finite Temperature At a temperature T the probability of occupation of an electron state of energy E is given by the Fermi distribution function The Fermi distribution function determines the probability of finding an electron at energyE.

20. Fermi-Dirac Distribution& The Fermi-LevelMain Application: Electrons in a Conductor • The Density of States g(E)specifies • how many states exist at a given energyE. • The Fermi Function f(E)specifies how many of the • existing states at energyEwill be filledwith electrons. • I • The Fermi Function f(E)specifies, under • equilibrium conditions, theprobabilitythat an • available state at an energy E will be occupied by an • electron. It is a probability distribution function. EF = Fermi Energy or Fermi Level k = Boltzmann Constant T = Absolute Temperature in K 20

21. Fermi-Dirac Statistics β  (1/kT) The Fermi EnergyEF is essentially the same as the Chemical Potentialμ. EFis called The Fermi Energy. Note the following: • When E = EF, the exponential term = 1 and FFD = (½). • In the limit as T → 0: L L • At T = 0, Fermions occupy the lowest energy levels. • Near T = 0, there is little chance that thermal agitation will kick a Fermionto an energy greater than EF.

22. Fermi-Dirac Distribution Consider T 0 K For E > EF : For E < EF : E EF A step function! 0 1 f(E)

23. Fermi Function at T=0 & at a Finite Temperature fFD=? At 0°K a. E < EF b. E > EF fFD(E,T) 0.5 E E<EF EF E>EF

24. Fermi-Dirac Distribution Temperature Dependence

25. Fermi-Dirac Distribution:Consider T> 0 K If E = EFthen f(EF) = ½ . If then So, the following approximation is valid: That is, most states at energies 3kT above EFare empty. If then l So, the following approximation is valid: So, 1 f(E) = probability that a state is empty, decays to zero. So, most states will be filled. kT (at 300 K) = 0.025eV, Eg(Si) = 1.1eV, so 3kT is very small in comparison to other energies relelevant to the electrons. 25

26. Fermi-Dirac Distribution Temperature Dependence T = 0 T > 0

27. The Fermi “Temperature” is defined as TF≡ (EF)/(kB). T > 0 As the temperature increases from T = 0, The Fermi-Dirac Distribution “smears out”. T = 0

28. T = TF T >> TF • As the temperature increases from T = 0, • The Fermi-Dirac Distribution“smears out”. • When T >> TF, FFDapproaches a decaying exponential.

29. At T = 0 the Fermi EnergyEFis the energy • of the highest occupied energy level. • If there are a total of N electrons, then is easy to • show that EFhas the form:

30. Fermi-Dirac Distribution Function

31. T-Dependence of the Chemical Potential Classical

32. n(E,T)number of free electrons per unit energy range is just the area under n(E,T) graph. n(E,T) g(E) T=0 T>0 E EF • Number of electrons per unit energy range according to the free electron model? • The shaded area shows the change in distribution between absolute zero and a finite temperature.

33. n(E,T) g(E) T=0 T>0 E EF • The Fermi-Dirac distribution function is a symmetric function; at finite temperatures, the same number of levels below EF are emptied and same number of levels above EFare filled by electrons.

34. Fermi Surface kz ky kx

35. Fermi-Dirac Distribution Function

36. Examples of Fermi Systems Electrons in metals (dense system)

37. Heat Capacity of the Free Electron Gas From the diagram of n(E,T) the change in the distribution of electrons can be resembled into triangles of height (½)g(EF) and a base of 2kBT so (½)g(EF)kBT electrons increased their energy by kBT. n(E,T) g(E) T=0 T>0 E EF • The difference in thermal energy from the value at T=0°K

38. Differentiating with respect to T gives the heat capacity at constant volume, Heat Capacity of Free Flectron Gas

39. Low-Temperature Heat Capacity Copper

40. Total metallic heat capacity at low temperatures where γ & βare constants found plotting Cv/T as a function of T2 Lattice Heat Capacity Electronic Heat capacity

41. Fermi-Dirac distribution function describes the behaviour of electrons only at equilibrium. If there is an applied field (E or B) or a temperature gradient the transport coefficient of thermal and electrical conductivities must be considered. Transport Properties of Conduction Electrons