FYS3410 - Vår 2014 (Kondenserte fasers fysikk) http://www.uio.no/studier/emner/matnat/fys/fys3410/v14/index.html



Similar documents
FYS Vår 2015 (Kondenserte fasers fysikk)

FYS Vår 2015 (Kondenserte fasers fysikk)

FYS Vår 2014 (Kondenserte fasers fysikk)

FYS Vår 2016 (Kondenserte fasers fysikk)

Free Electron Fermi Gas (Kittel Ch. 6)

Energy Transport. Focus on heat transfer. Heat Transfer Mechanisms: Conduction Radiation Convection (mass movement of fluids)

Lecture 3: Optical Properties of Bulk and Nano. 5 nm

Lecture 3: Optical Properties of Bulk and Nano. 5 nm

Solid State Detectors = Semi-Conductor based Detectors

NORGES TEKNISK- NATURVITENSKAPELIGE UNIVERSITET INSTITUTT FOR FYSIKK. Eksamen i Emne TFY4220 Faste Stoffers Fysikk

3. Diodes and Diode Circuits. 3. Diodes and Diode Circuits TLT-8016 Basic Analog Circuits 2005/2006 1

Resistivity. V A = R = L ρ (1)

Name Date Class ELECTRONS IN ATOMS. Standard Curriculum Core content Extension topics

Theoretical calculation of the heat capacity

The quantum mechanics of particles in a periodic potential: Bloch s theorem

Chem 1A Exam 2 Review Problems

KINETIC MOLECULAR THEORY OF MATTER

Kinetic Molecular Theory of Matter

Structure Factors

Solid-State Physics: The Theory of Semiconductors (Ch ) SteveSekula, 30 March 2010 (created 29 March 2010)

CLASSICAL CONCEPT REVIEW 8

The properties of an ideal Fermi gas are strongly determined by the Pauli principle. We shall consider the limit: µ >> k B T βµ >> 1,

Calculating particle properties of a wave

Chapter 5. Second Edition ( 2001 McGraw-Hill) 5.6 Doped GaAs. Solution

Size effects. Lecture 6 OUTLINE

1. Degenerate Pressure

CURRENT ELECTRICITY - I

COURSE: PHYSICS DEGREE: COMPUTER ENGINEERING year: 1st SEMESTER: 1st

3. What would you predict for the intensity and binding energy for the 3p orbital for that of sulfur?

DO PHYSICS ONLINE FROM QUANTA TO QUARKS QUANTUM (WAVE) MECHANICS

Energy band diagrams. Single atom. Crystal. Excited electrons cannot move. Excited electrons can move (free electrons)

Introduction To Materials Science FOR ENGINEERS, Ch. 5. Diffusion. MSE 201 Callister Chapter 5

Semiconductors, diodes, transistors

Study the following diagrams of the States of Matter. Label the names of the Changes of State between the different states.

Crystalline solids. A solid crystal consists of different atoms arranged in a periodic structure.

- thus, the total number of atoms per second that absorb a photon is

Lecture 6 Scanning Tunneling Microscopy (STM) General components of STM; Tunneling current; Feedback system; Tip --- the probe.

Lecture 15 - application of solid state materials solar cells and photovoltaics. Copying Nature... Anoxygenic photosynthesis in purple bacteria

PS-6.2 Explain the factors that determine potential and kinetic energy and the transformation of one to the other.

SEMICONDUCTOR I: Doping, semiconductor statistics (REF: Sze, McKelvey, and Kittel)

Chapter 5: Diffusion. 5.1 Steady-State Diffusion

Fall 2004 Ali Shakouri

Vacuum Evaporation Recap

The rate of change of velocity with respect to time. The average rate of change of distance/displacement with respect to time.

European Benchmark for Physics Bachelor Degree

Types of Epitaxy. Homoepitaxy. Heteroepitaxy

Lecture 2 - Semiconductor Physics (I) September 13, 2005

CONTENTS. Preface Energy bands of a crystal (intuitive approach)

Chapter 2. Atomic Structure and Interatomic Bonding

University of California at Santa Cruz Electrical Engineering Department EE-145L: Properties of Materials Laboratory

FUNDAMENTAL PROPERTIES OF SOLAR CELLS

SUPERCONDUCTIVITY. PH 318- Introduction to superconductors 1

High Open Circuit Voltage of MQW Amorphous Silicon Photovoltaic Structures

Atomic Structure Ron Robertson

2 Absorbing Solar Energy

STUDY MATERIAL FOR CLASS Physics- CURRENT ELECTRICITY. The flow of electric charges in a particular direction constitutes electric current.

Introduction OLEDs OTFTs OPVC Summary. Organic Electronics. Felix Buth. Walter Schottky Institut, TU München. Joint Advanced Student School 2008

Name Class Date. In the space provided, write the letter of the term or phrase that best completes each statement or best answers each question.

PHOTOELECTRIC EFFECT AND DUAL NATURE OF MATTER AND RADIATIONS

DIFFUSION IN SOLIDS. Materials often heat treated to improve properties. Atomic diffusion occurs during heat treatment

Define the notations you are using properly. Present your arguments in details. Good luck!

Chapter 6. Current and Resistance

HEAT UNIT 1.1 KINETIC THEORY OF GASES Introduction Postulates of Kinetic Theory of Gases

Chemistry 13: States of Matter

ELECTRICAL CONDUCTION

10.7 Kinetic Molecular Theory Kinetic Molecular Theory. Kinetic Molecular Theory. Kinetic Molecular Theory. Kinetic Molecular Theory

Lesson 3. Chemical Bonding. Molecular Orbital Theory

(1) The size of a gas particle is negligible as compared to the volume of the container in which the gas is placed.

Modern Construction Materials Prof. Ravindra Gettu Department of Civil Engineering Indian Institute of Technology, Madras

14:635:407:02 Homework III Solutions

13.1 The Nature of Gases. What is Kinetic Theory? Kinetic Theory and a Model for Gases. Chapter 13: States of Matter. Principles of Kinetic Theory

The Physics of Energy sources Renewable sources of energy. Solar Energy

Physics 9e/Cutnell. correlated to the. College Board AP Physics 1 Course Objectives

Chapter 2: Atomic Structure and Chemical Bonding

White Dwarf Properties and the Degenerate Electron Gas

Plate waves in phononic crystals slabs

13- What is the maximum number of electrons that can occupy the subshell 3d? a) 1 b) 3 c) 5 d) 2

A Course Material on. Engineering Physics - II

- particle with kinetic energy E strikes a barrier with height U 0 > E and width L. - classically the particle cannot overcome the barrier

ENEE 313, Spr 09 Midterm II Solution

UNIT I: INTRFERENCE & DIFFRACTION Div. B Div. D Div. F INTRFERENCE

THE KINETIC THEORY OF GASES

Section 3: Crystal Binding

A. Kinetic Molecular Theory (KMT) = the idea that particles of matter are always in motion and that this motion has consequences.

Multi-electron atoms

Physics Notes Class 11 CHAPTER 2 UNITS AND MEASUREMENTS

Sample Exercise 12.1 Calculating Packing Efficiency

MODERN ATOMIC THEORY AND THE PERIODIC TABLE

KINETIC THEORY AND THERMODYNAMICS

Chapter 18: The Structure of the Atom

3. Derive the partition function for the ideal monoatomic gas. Use Boltzmann statistics, and a quantum mechanical model for the gas.

Measurement of Charge-to-Mass (e/m) Ratio for the Electron

AS COMPETITION PAPER 2008

Gas Laws. Heat and Temperature

TEACHER BACKGROUND INFORMATION THERMAL ENERGY

Electrons in Atoms & Periodic Table Chapter 13 & 14 Assignment & Problem Set

Photons. ConcepTest ) red light 2) yellow light 3) green light 4) blue light 5) all have the same energy. Which has more energy, a photon of:

Unit 12 Practice Test

Chapter Outline. Diffusion - how do atoms move through solids?

Statistical thermodynamics of Solids: Introduction of structured solids

Transcription:

FYS3410 - Vår 2014 (Kondenserte fasers fysikk) http://www.uio.no/studier/emner/matnat/fys/fys3410/v14/index.html Pensum: Solid State Physics by Philip Hofmann (Chapters 1-7 and 11) Andrej Kuznetsov delivery address: Department of Physics, PB 1048 Blindern, 0316 OSLO Tel: +47-22857762, e-post: andrej.kuznetsov@fys.uio.no visiting address: MiNaLab, Gaustadaleen 23c

Lecture schedule (based on P.Hofmann s Solid State Physics, chapters 1-7 and 11) Module I Periodic Structures and Defects 20/1 Introduction. Crystal bonding. Periodicity and lattices, reciprocal space 4h 21/1 Laue condition, Ewald construction, interpretation of a diffraction experiment 2h 22/1 Bragg planes and Brillouin zones (BZ) 2h 23/1 Elastic strain and structural defects 2h 23/1 Atomic diffusion and summary of Module I 2h Module II - Phonons 03/2 Vibrations, phonons, density of states, and Planck distribution 4h 04/2 Lattice heat capacity: Dulong-Petit, Einstien and Debye models 2h 05/2 Comparison of different models 2h 06/2 Thermal conductivity 2h 07/2 Thermal expansion and summary of Module II 2h Module III Free Electron Gas 24/2 Free electron gas (FEG) versus Free electron Fermi gas (FEFG) 4h 25/2 Effect of temperature Fermi- Dirac distribution 2h 26/2 Heat capacity of FEFG 2h 27/2 Electrical and thermal conductivity in metals 2h 28/2 FEFG in nanostructures 2h Module IV Nearly Free Electron Model 10/3 Bragg reflection of electrons at the boundary of BZ, energy bands 4h 11/3 Empty lattice approximation; number of orbitals in a band 2h 12/3 Semiconductors, effective mass method, intrinsic carriers 2h 13/3 Impurity states in semiconductors and carrier statistics 2h 14/3 p-n junctions and optoelectronic devices 2h

Lecture 14: Free electron gas and free electron Fermi gas Free electron gas (FEG) - Drude model - FEG explaing Ohm s law - FEG expaling Hall effect - FEG explaing Wiedemann-Franz law - FEG heat capacity Free electron Fermi gas (FEFG) a gas of electrons subject to Pauli principle One electron system wave functions orbits; FEFG in 1D in ground state FEFG in 3D in ground state Fermi-Dirac distribution and electron occupancy at T>0

Lecture 14: Free electron gas and free electron Fermi gas Free electron gas (FEG) - Drude model - FEG explaing Ohm s law - FEG expaling Hall effect - FEG explaing Wiedemann-Franz law - FEG heat capacity Free electron Fermi gas (FEFG) a gas of electrons subject to Pauli principle One electron system wave functions orbits; FEFG in 1D in ground state FEFG in 3D in ground state Fermi-Dirac distribution and electron occupancy at T>0

Free electron gas (FEG) - Drude model There could be different opinions what particular discovery was the main breakthrough for the acceleration of the condensed matter physics but a very prominent kick-off was by the discovery of the electron by J.J. Thompson in 1897. Soon afterwards (1900) P. Drude used the new concept to postulate a theory of electrical conductivity. Drude was considering why resistivity in different materials ranges from 10 8 m (Ag) to 10 20 m (polystyrene)? Drude was working prior to the development of quantum mechanics, so he began with a classical model, specifically: (i) positive ion cores within an electron gas that follows Maxwell-Boltzmann statistics; (ii) following the kinetic theory of gases - the electrons ae in form of free electron gas (FEG), so that individual electrons move in straight lines and make collisions only with the ion cores; electron-electron interactions are neglected; (iii) Electrons lose energy gained from the electric field in colisions and the mean free path was approximately the inter-atomic spacing. Drude (or FEG) model successfully exlpained Ohm amd Wiedemann-Franz laws, but failed to explain, e.g., electron heat capacity and the magnetic susceptibility of conduction electrons.

Free electron gas (FEG) - Drude model Velocity of electrons in FEG e.g. at room temperature

Free electron gas (FEG) - Drude model #atoms per volume calculate as #valence electrons per atom density atomic mass

FEG explaining Ohm s law Apply an electric field. The equation of motion is integration gives and if is the average time between collisions then the average drift speed is for we get remember:

FEG explaining Ohm s law number of electrons passing in unit time current of negatively charged electrons current density Ohm s law and with we get

FEG explaining Ohm s law

FEG explaining Ohm s law line

FEG explaining Hall effect Accumulation of charge leads to Hall field EH. Hall field proportional to current density and B field is called Hall coefficient

FEG explaining Hall effect for the steady state

FEG explaining Hall effect

FEG explaining Wiedemann-Franz law Wiedemann and Franz found in 1853 that the ratio of thermal and electrical conductivity for ALL METALS is constant at a given temperature (for room temperature and above). constant Later it was found by L. Lorenz that this constant is proportional to temperature

FEG explaining Wiedemann-Franz law estimated thermal conductivity (from a classical ideal gas) the actual quantum mechanical result is this is 3, more or less...

FEG explaining Wiedemann-Franz law at 273 K metal 10-8 Watt Ω K -2 Ag 2.31 Au 2.35 Cd 2.42 Cu 2.23 Mo 2.61 Pb 2.47 Pt 2.51 Sn 2.52 W 3.04 Zn 2.31 L = 2.45 10-8 Watt Ω K -2

FEG heat capacity an average thermal energy of an ideal gas particle, e.g. an electron from FEG, moving in 3D at some temperature T is: E 3 2 k B T Then for a total nr of N electrons the total energy is: Nk And the electronic heat capacity would then be: U 3 2 du dt If FEG approximation is correct this C el should be added to phonon-related heat capacitance, however, if we go out and measure, we find the electronic contribution is only around one percent of this, specifically at high temperature is still Dulong- Petit value,, that is valid. B T 3 Cel 2 Nk B

Free electron gas (FEG) - Drude model Why does the Drude model work so relatively well when many of its assumptions seem so wrong? In particular, the electrons don t seem to be scattered by each other. Why? How do the electrons sneak by the atoms of the lattice? What are mysterious positive charges realed by Hall effect measuremt in semiconductors? Why do the electrons not seem to contribute to the heat capacity?

Lecture 14: Free electron gas and free electron Fermi gas Free electron gas (FEG) - Drude model - FEG explaing Ohm s law - FEG expaling Hall effect - FEG explaing Wiedemann-Franz law - FEG heat capacity Free electron Fermi gas (FEFG) a gas of electrons subject to Pauli principle One electron system wave functions orbits; FEFG in 1D in ground state FEFG in 3D in ground state Fermi-Dirac distribution and electron occupancy at T>0

Free electron Fermi gas a gas of electrons subject to Pauli principle At low temperature, free mean path of a conduction electron in metal can be as long as 1 cm! Why is it not affected by ion cores or other conduction electrons? (30 seconds discussions) Motion of electrons in crystal (matter wave) is not affected by periodic structure such as ion cores. Electron is scattered infrequently by other conduction electrons due to the Pauli exclusion principle

Lecture 14: Free electron gas and free electron Fermi gas Free electron gas (FEG) - Drude model - FEG explaing Ohm s law - FEG expaling Hall effect - FEG explaing Wiedemann-Franz law - FEG heat capacity Free electron Fermi gas (FEFG) a gas of electrons subject to Pauli principle One electron system wave functions orbits; FEFG in 1D in ground state FEFG in 3D in ground state Fermi-Dirac distribution and electron occupancy at T>0

One electron system wave functions - orbits Neglect electron-electron interaction, infinite potential well, simple QM solution Standing wave B. C. n = 1, 2, - The Pauli exclusion principle n: quantum number m(=1/2 and -1/2): magnetic quantum number - degeneracy: # of orbitals with the same energy - Fermi energy (E F ): energy of the topmost filled level in the ground state of the N electron system In this simple system, every quantum state holds 2 electrons => n F = N/2 Fermi energy: Great, if we know the electron density, we know the Fermi energy!

Lecture 14: Free electron gas and free electron Fermi gas Free electron gas (FEG) - Drude model - FEG explaing Ohm s law - FEG expaling Hall effect - FEG explaing Wiedemann-Franz law - FEG heat capacity Free electron Fermi gas (FEFG) a gas of electrons subject to Pauli principle One electron system wave functions orbits; FEFG in 1D in ground state FEFG in 3D in ground state Fermi-Dirac distribution and electron occupancy at T>0

FEFG in 3D Only if we know how much space one k point occupies (dk x dk y dk z = (2π/L) 3 ) Invoking periodic boundary condition instead of the infinite potential wall (standing wave) boundary condition, we get traveling waves as solutions: Due to spin Fermi wave vector Fermi energy Fermi velocity

Lecture 14: Free electron gas and free electron Fermi gas Free electron gas (FEG) - Drude model - FEG explaing Ohm s law - FEG expaling Hall effect - FEG explaing Wiedemann-Franz law - FEG heat capacity Free electron Fermi gas (FEFG) a gas of electrons subject to Pauli principle One electron system wave functions orbits; FEFG in 1D in ground state FEFG in 3D in ground state Fermi-Dirac distribution and electron occupancy at T>0

Fermi-Dirac distribution and electron occupancy at T>0 Describes the probability that an orbit at energy E will be occupied in an ideal electron gas under thermal equilibrium is chemical potential, f( )=0.5; at 0K, F In comparison, High energy tail approximation E E F 3k B T Boltzmann-Maxwell distribution

Fermi-Dirac distribution and electron occupancy at T>0 # of states between E and E+dE Note here: N N( ) D(E) has a unit of ev -1.

FYS3410 - Vår 2014 (Kondenserte fasers fysikk) http://www.uio.no/studier/emner/matnat/fys/fys3410/v14/index.html Pensum: Solid State Physics by Philip Hofmann (Chapters 1-7 and 11) Andrej Kuznetsov delivery address: Department of Physics, PB 1048 Blindern, 0316 OSLO Tel: +47-22857762, e-post: andrej.kuznetsov@fys.uio.no visiting address: MiNaLab, Gaustadaleen 23c

Lecture schedule (based on P.Hofmann s Solid State Physics, chapters 1-7 and 11) Module I Periodic Structures and Defects 20/1 Introduction. Crystal bonding. Periodicity and lattices, reciprocal space 4h 21/1 Laue condition, Ewald construction, interpretation of a diffraction experiment 2h 22/1 Bragg planes and Brillouin zones (BZ) 2h 23/1 Elastic strain and structural defects 2h 23/1 Atomic diffusion and summary of Module I 2h Module II - Phonons 03/2 Vibrations, phonons, density of states, and Planck distribution 4h 04/2 Lattice heat capacity: Dulong-Petit, Einstien and Debye models 2h 05/2 Comparison of different models 2h 06/2 Thermal conductivity 2h 07/2 Thermal expansion and summary of Module II 2h Module III Free Electron Gas 24/2 Free electron gas (FEG) versus Free electron Fermi gas (FEFG) 4h 25/2 Effect of temperature Fermi- Dirac distribution 2h 26/2 Heat capacity of FEFG 2h 27/2 Electrical and thermal conductivity in metals 2h 28/2 FEFG in nanostructures 2h Module IV Nearly Free Electron Model 10/3 Bragg reflection of electrons at the boundary of BZ, energy bands 4h 11/3 Empty lattice approximation; number of orbitals in a band 2h 12/3 Semiconductors, effective mass method, intrinsic carriers 2h 13/3 Impurity states in semiconductors and carrier statistics 2h 14/3 p-n junctions and optoelectronic devices 2h

Repetition of DOS for FEFG Lecture 15: Electrons at T>0: DOS + Fermi-Dirac distribution (i) Repetition of DOS for FEFG (ii) Fermi-Diract distribution (iii)estimate for the FEFG heat capacity

Repetition of DOS for FEFG Lecture 15: Electrons at T>0: DOS + Fermi-Dirac distribution (i) Repetition of DOS for FEFG (ii) Fermi-Diract distribution (iii)estimate for the FEFG heat capacity

Repetition of DOS for FEFG Consider electrons as quantum particles in a box FEFG model means that

Repetition of DOS for FEFG ~ boundary conditions provide restrictions the wavevector k

Repetition of DOS for FEFG

Repetition of DOS for FEFG The volume of k x1 k y1 k z1 = (2π/L) 3 corresponds to only one k-state, accommodating 2 electrons k x1 k y1 k z1 = (2π/L) 3 While k max or k F accommodate N/2!

Repetition of DOS for FEFG For any E

Repetition of DOS for FEFG Lecture 15: Electrons at T>0: DOS + Fermi-Dirac distribution (i) Repetition of DOS for FEFG (ii) Fermi-Diract distribution (iii)estimate for the FEFG heat capacity

The Fermi-Dirac distribution μ At T=0 all the states are filled up to the highest occupied state. This state is called the Fermi energy E F. It is equal to the chemical potential μ at T=0.

The Fermi-Dirac distribution Describes the probability that an orbit at energy E will be occupied in an ideal electron gas under thermal equilibrium is chemical potential, f( )=0.5; at 0K, F High energy tail approximation E E F 3k B T Boltzmann-Maxwell distribution

The Fermi-Dirac distribution ~ k B T

Repetition of DOS for FEFG Lecture 15: Electrons at T>0: DOS + Fermi-Dirac distribution (i) Repetition of DOS for FEFG (ii) Fermi-Diract distribution (iii)estimate for the FEFG heat capacity

Estimate for the heat capacity of FEFG One of the greatest successes of the free electron model and FD statistics is the explanation of the T dependence of the heat capacity of a metal. k B T To calculate the heat capacity, we need to know how the internal energy of the Fermi gas, E t (T), depends on temperature. By heating a Fermi gas, we populate some states above the Fermi energy E F and deplete some states below E F. This modification is significant within a narrow energy range ~ k B T around E F. The fraction of electrons that we transfer to higher energies ~ k B T/E F, the energy increase for these electrons ~ k B T. Thus, the increase of the internal energy with temperature is C dq T V V const dt de T t dt proportional to n (k B T/E F ) (k B T) ~ n (k B T) 2 /E F. Note, E F = k B T F C e 2 nk 2 B kt B E F compare C V 3 2 nk B C for an ideal gas V de T t dt 2 kt B N E F The Fermi gas heat capacity is much smaller (by k B T/E F <<1) than that of a classical ideal gas with the same energy and pressure. The small heat capacity is a direct consequence of the Pauli principle: most of the electrons cannot change their energy, only a small fraction k B T/E F or T/T F of the electrons are excited out of the ground state.

Heat capacity of a metal: lattice + electrons two contributions: lattice and electrons electrons unimportant at high T but dominating and sufficiently low T

FYS3410 - Vår 2014 (Kondenserte fasers fysikk) http://www.uio.no/studier/emner/matnat/fys/fys3410/v14/index.html Pensum: Solid State Physics by Philip Hofmann (Chapters 1-7 and 11) Andrej Kuznetsov delivery address: Department of Physics, PB 1048 Blindern, 0316 OSLO Tel: +47-22857762, e-post: andrej.kuznetsov@fys.uio.no visiting address: MiNaLab, Gaustadaleen 23c

Lecture schedule (based on P.Hofmann s Solid State Physics, chapters 1-7 and 11) Module I Periodic Structures and Defects 20/1 Introduction. Crystal bonding. Periodicity and lattices, reciprocal space 4h 21/1 Laue condition, Ewald construction, interpretation of a diffraction experiment 2h 22/1 Bragg planes and Brillouin zones (BZ) 2h 23/1 Elastic strain and structural defects 2h 23/1 Atomic diffusion and summary of Module I 2h Module II - Phonons 03/2 Vibrations, phonons, density of states, and Planck distribution 4h 04/2 Lattice heat capacity: Dulong-Petit, Einstien and Debye models 2h 05/2 Comparison of different models 2h 06/2 Thermal conductivity 2h 07/2 Thermal expansion and summary of Module II 2h Module III Electrons 24/2 Free electron gas (FEG) versus Free electron Fermi gas (FEFG) 4h 25/2 Effect of temperature Fermi- Dirac distribution 2h 26/2 FEFG in 2D and 1D, and DOS in nanostructures 2h 27/2 Origin of the band gap and nearly free electron model 2h 28/2 Number of orbitals in a band and general form of the electronic states 2h Module IV Applications 10/3 Energy bands in real solids and transport properties 4h 11/3 Calculation of energy bands 2h 12/3 Semiconductors, effective mass method, intrinsic carriers 2h 13/3 Impurity states in semiconductors and carrier statistics 2h 14/3 p-n junctions and optoelectronic devices 2h

Lecture 16 FEFG in 2D and 1D, and DOS in nanostructures (i) Motivation: intriguing carrier recombination in QW resulting in photons with energies above the band gap; (ii) DOS for low-dimentional FEFG (iii) DOS in quantum wells (iv) DOS in nanowires (v) DOS in quantum dots

Motivation: intriguing carrier recombination in QW resulting in photons with energies above the band gap Single quantum well - repetitions of ZnO/ZnCdO/ZnO periods MQWs

DOS for low-dimentional FEFG

DOS in quantum wells

DOS in quantum wells

DOS in nanowires and quantum dots Density of states per unit volume and energy for a 3-D semiconductor (blue curve), a 10 nm quantum well with infinite barriers (red curve) and a 10 nm by 10 nm quantum wire with infinite barriers (green curve).

DOS in nanowires and quantum dots

FYS3410 - Vår 2014 (Kondenserte fasers fysikk) http://www.uio.no/studier/emner/matnat/fys/fys3410/v14/index.html Pensum: Solid State Physics by Philip Hofmann (Chapters 1-7 and 11) Andrej Kuznetsov delivery address: Department of Physics, PB 1048 Blindern, 0316 OSLO Tel: +47-22857762, e-post: andrej.kuznetsov@fys.uio.no visiting address: MiNaLab, Gaustadaleen 23c

Lecture schedule (based on P.Hofmann s Solid State Physics, chapters 1-7 and 11) Module I Periodic Structures and Defects 20/1 Introduction. Crystal bonding. Periodicity and lattices, reciprocal space 4h 21/1 Laue condition, Ewald construction, interpretation of a diffraction experiment 2h 22/1 Bragg planes and Brillouin zones (BZ) 2h 23/1 Elastic strain and structural defects 2h 23/1 Atomic diffusion and summary of Module I 2h Module II - Phonons 03/2 Vibrations, phonons, density of states, and Planck distribution 4h 04/2 Lattice heat capacity: Dulong-Petit, Einstien and Debye models 2h 05/2 Comparison of different models 2h 06/2 Thermal conductivity 2h 07/2 Thermal expansion and summary of Module II 2h Module III Electrons 24/2 Free electron gas (FEG) versus Free electron Fermi gas (FEFG)

Lecture 17 Origin of energy bands and nearly free electron model Recap of the one-electron approximation Intuitive picture Bragg-reflection for nearly free electrons Gap opening for nearly free electrons Solution of the Schrödinger equation

Solving Recap of the one Schrödinger electron approximation equation for an allelectron wave function in a rigid lattice is still hopeless. We assume an effective one electron potential. we know for sure that 58...but not much more

The idea of energy bands: Na consider one atom of Na: 11 electrons 59

The idea of energy bands: Na consider tow Na atoms / a Na 2 molecule: 22 electrons big separation 60 Focus only on the valence (outer) electrons (3s). What happens when we move them

The idea of energy bands: Na consider two Na atoms / a Na 2 molecule: 2 3s electrons molecular energy levels capacity: 2x2=4 electrons Levels split up in bonding and anti bonding molecular orbitals and are occupied according to the Pauli principle. 61 61 The distance between the atoms must be

The idea of energy bands: Na consider many (N) Na atoms (only 3s level) N levels with very similar energies, like in a super-giant molecule. We can speak of a band of levels. 62 62

The idea of energy bands: Si 4 electrons per atom 2 atoms per unit cell sp 3 : 8 states 4 sp 3 per cell 8 states per atom 16 states per unit cell 63

free electron model naive band picture 64

Bragg-reflection for nearly free electrons 65 electron traveling perpendicular to crystal planes

Bragg-reflection for nearly free electrons consider only one direction (x) free electron wave function with a de Broglie wavelength Bragg condition with this gives a Bragg condition for electron waves: 66

Bragg-reflection for nearly free electrons Bragg condition for electron waves: ragg reflection results in standing, not traveling electron waves ombinations of 67

Gap opening for nearly free electrons 68 68

General form of Bloch theory Schrödinger equation for a periodic potential solutions have the form of Bloch waves plane wave lattice-periodic function