Handout 3 Free Electron Gas in 2D and 1D Electron Gases in 2D

Total Page:16

File Type:pdf, Size:1020Kb

Handout 3 Free Electron Gas in 2D and 1D Electron Gases in 2D Handout 3 Free Electron Gas in 2D and 1D In this lecture you will learn: • Free electron gas in two dimensions and in one dimension • Density of States in k-space and in energy in lower dimensions ECE 407 – Spring 2009 – Farhan Rana – Cornell University Electron Gases in 2D • In several physical systems electron are confined to move in just 2 dimensions STM micrograph • Examples, discussed in detail later in the course, are shown below: Semiconductor Quantum Wells: Graphene: InGaAs GaAs quantum well (1-10 nm) GaAs Semiconductor quantum wells can be composed of Graphene is a single atomic layer pretty much any of carbon atoms arranged in a semiconductor from the TEM honeycomb lattice groups II, III, IV, V, and VI of micrograph the periodic table ECE 407 – Spring 2009 – Farhan Rana – Cornell University 1 Electron Gases in 1D • In several physical systems electron are confined to move in just 1 dimension • Examples, discussed in detail later in the course, are shown below: Semiconductor Quantum Semiconductor Quantum Carbon Nanotubes Wires (or Nanowires): Point Contacts (Rolled Graphene (Electrostatic Gating): Sheets): GaAs metal metal InGaAs InGaAs Nanowire Quantum well GaAs GaAs ECE 407 – Spring 2009 – Farhan Rana – Cornell University Electrons in 2D Metals: The Free Electron Model The quantum state of an electron is described by the time-independent Schrodinger equation: 2 2 r V r r E r 2m Consider a large metal sheet of area A= Lx Ly : A LxLy Use the Sommerfeld model: Ly • The electrons inside the sheet are confined in a Lx two-dimensional infinite potential well with zero potential inside the sheet and infinite potential outside the sheet V r 0 for r inside the sheet V r for r outside the sheet free electrons • The electron states inside the sheet are given (experience no by the Schrodinger equation potential when inside the sheet) ECE 407 – Spring 2009 – Farhan Rana – Cornell University 2 Born Von Karman Periodic Boundary Conditions in 2D 2 Solve: 2 r E r 2m Use periodic boundary conditions: y A LxLy These imply that each x L ,y,z x, y,z x L x edge of the sheet is y L x, y Ly ,z x, y,z folded and joined to x the opposite edge 1 i k . r 1 i k x x ky y Solution is: r e e A A The boundary conditions dictate that the allowed values of kx , and ky are such that: i kxLx 2 e 1 kx n n = 0, ±1, ±2, ±3,……. Lx i ky Ly 2 e 1 ky m m = 0, ±1, ±2, ±3,……. Ly ECE 407 – Spring 2009 – Farhan Rana – Cornell University Born Von Karman Periodic Boundary Conditions in 2D Labeling Scheme: All electron states and energies can be labeled by the corresponding k-vector 2 2 1 i k . r k r e Ek k A 2 m 2 2 Normalization: The wavefunction is properly normalized: d r k r 1 Orthogonality: Wavefunctions of two different states are orthogonal: i k k'. r 2 * 2 e d r r r d r k' k A k' , k Momentum Eigenstates: Another advantage of using the plane-wave energy eigenstates (as opposed to the “sine” energy eigenstates) is that the plane-wave states are also momentum eigenstates Momentum operator: pˆ pˆ r r k r i k i k k Velocity: k 1 Velocity of eigenstates is: vk k Ek m ECE 407 – Spring 2009 – Farhan Rana – Cornell University 3 States in 2D k-Space ky 2 k-space Visualization: Lx The allowed quantum states states can be visualized as a 2D grid of points in the entire “k-space” 2 2 kx n ky m Lx Ly kx 2 n, m = 0, ±1, ±2, ±3, ……. Ly Density of Grid Points in k-space: Looking at the figure, in k-space there is only one grid point in every small area of size: 2 2 2 2 Lx Ly A A There are grid points per unit area of k-space Very important 2 2 result ECE 407 – Spring 2009 – Farhan Rana – Cornell University The Electron Gas in 2D at Zero Temperature - I • Suppose we have N electrons in the sheet. • Then how do we start filling the allowed quantum states? N y A LxLy • Suppose T~0K and we are interested in a filling scheme x Ly that gives the lowest total energy. Lx The energy of a quantum state is: ky 2 2 2 2 2 kx ky k Ek 2 m 2 m Strategy: • Each grid-point can be occupied by two electrons (spin up and spin down) • Start filling up the grid-points (with two electrons kx each) in circular regions of increasing radii until k you have a total of N electrons F • When we are done, all filled (i.e. occupied) quantum states correspond to grid-points that are inside a circular region of radius kF ECE 407 – Spring 2009 – Farhan Rana – Cornell University 4 The Electron Gas in 2D at Zero Temperature - II ky • Each grid-point can be occupied by two electrons (spin up and spin down) kF • All filled quantum states correspond to grid-points that are inside a circular region of radius kF kx 2 Area of the circular region = kF Fermi circle A 2 Number of grid-points in the circular region = kF 2 2 Number of quantum states (including A 2 A 2 spin) in the circular region = 2 kF kF 2 2 2 But the above must equal the total number N of electrons inside the box: A N k 2 2 F 2 N kF Units of the electron n electron density 2 A 2 density n are #/cm 1 2 kF 2 n ECE 407 – Spring 2009 – Farhan Rana – Cornell University The Electron Gas in 2D at Zero Temperature - III k • All quantum states inside the Fermi circle are filled (i.e. y occupied by electrons) • All quantum states outside the Fermi circle are empty kF Fermi Momentum: kx The largest momentum of the electrons is: kF This is called the Fermi momentum Fermi momentum can be found if one knows the electron density: 1 Fermi circle 2 kF 2 n Fermi Energy: 2 2 The largest energy of the electrons is: kF 2m 2k2 This is called the Fermi energy E : E F F F 2m 2 n m Also: E or n E F m 2 F Fermi Velocity: k The largest velocity of the electrons is called the Fermi velocity v : v F F F m ECE 407 – Spring 2009 – Farhan Rana – Cornell University 5 The Electron Gas in 2D at Non-Zero Temperature - I ky dkx A Recall that there are grid points per unit area of k- dk 2 y space 2 kx So in area d k x d k y of k-space the number of grid points is: A A 2 dkx dky d k 2 2 2 2 The summation over all grid points in k-space can be replaced by an area integral d 2k A 2 all k 2 Therefore: d 2k N 2 f k 2 A f k 2 all k 2 f k is the occupation probability of a quantum state ECE 407 – Spring 2009 – Farhan Rana – Cornell University The Electron Gas in 2D at Non-Zero Temperature - II The probability f k that the quantum state of wavevector k is occupied by an electron is given by the Fermi-Dirac distribution function: 1 2 2 2 2 2 kx ky k f k Where: Ek 1 eEk Ef KT 2 m 2 m Therefore: d 2k d 2k 1 N 2 A f k 2 A 2 2 2 2 1 eEk Ef KT Density of States: The k-space integral is cumbersome. We need to convert into a simpler form – an energy space integral – using the following steps: 2 2k2 2k d k 2 k dk and E dE dk 2 m m Therefore: d 2k k dk m 2 A 2 A A 2 dE 2 0 0 ECE 407 – Spring 2009 – Farhan Rana – Cornell University 6 The Electron Gas in 2D at Non-Zero Temperature - III d 2k 1 1 N 2 A A dE g E 2 E k E KT 2D E E KT 2 1 e f 0 1 e f m Where: g2D E 2 Density of states function is constant (independent of energy) in 2D 2 g2D(E) has units: # / Joule-cm ky The product g(E) dE represents the number of quantum states available in the energy interval between E and (E+dE) per cm2 of the metal Suppose E corresponds to the inner circle from the relation: k 2k 2 x E 2 m And suppose (E+dE) corresponds to the outer circle, then g2D(E) dE corresponds to twice the number of the grid points between the two circles ECE 407 – Spring 2009 – Farhan Rana – Cornell University The Electron Gas in 2D at Non-Zero Temperature - IV 1 N A dE g E A dE g E f E E 2D E E KT 2D f 0 1 e f 0 g2D E m Where: g2D E 2 f E E The expression for N can be visualized as the f integration over the product of the two functions: Ef E Check: Suppose T=0K: Ef N A dE g2D E f E Ef A dE g2D E f E Ef 0 0 1 m T = 0K A 2 Ef 0 Ef E m n 2 Ef Compare with the previous result at T=0K: m n E At T=0K (and only at T=0K) the Fermi level 2 F E is the same as the Fermi energy E f F ECE 407 – Spring 2009 – Farhan Rana – Cornell University 7 The Electron Gas in 2D at Non-Zero Temperature - V For T ≠ 0K: Since the carrier density is known, and does not change with temperature, the Fermi level at temperature T is found from the expression Ef 1 m n dE g E K T log1 eK T 2D E E KT 2 0 1 e f In general, the Fermi level Ef is a function of temperature and decreases from EF as the temperature increases.
Recommended publications
  • Fermi- Dirac Statistics
    Prof. Surajit Dhara Guest Teacher, Dept. Of Physics, Narajole Raj College GE2T (Thermal physics and Statistical Mechanics) , Topic :- Fermi- Dirac Statistics Fermi- Dirac Statistics Basic features: The basic features of the Fermi-Dirac statistics: 1. The particles are all identical and hence indistinguishable. 2. The fermions obey (a) the Heisenberg’s uncertainty relation and also (b) the exclusion principle of Pauli. 3. As a consequence of 2(a), there exists a number of quantum states for a given energy level and because of 2(b) , there is a definite a priori restriction on the number of fermions in a quantum state; there can be simultaneously no more than one particle in a quantum state which would either remain empty or can at best contain one fermion. If , again, the particles are isolated and non-interacting, the following two additional condition equations apply to the system: ∑ ; Thermodynamic probability: Consider an isolated system of N indistinguishable, non-interacting particles obeying Pauli’s exclusion principle. Let particles in the system have energies respectively and let denote the degeneracy . So the number of distinguishable arrangements of particles among eigenstates in the ith energy level is …..(1) Therefore, the thermodynamic probability W, that is, the total number of s eigenstates of the whole system is the product of ……(2) GE2T (Thermal physics and Statistical Mechanics), Topic :- Fermi- Dirac Statistics: Circulated by-Prof. Surajit Dhara, Dept. Of Physics, Narajole Raj College FD- distribution function : Most probable distribution : From eqn(2) above , taking logarithm and applying Stirling’s theorem, For this distribution to represent the most probable distribution , the entropy S or klnW must be maximum, i.e.
    [Show full text]
  • Solid State Physics II Level 4 Semester 1 Course Content
    Solid State Physics II Level 4 Semester 1 Course Content L1. Introduction to solid state physics - The free electron theory : Free levels in one dimension. L2. Free electron gas in three dimensions. L3. Electrical conductivity – Motion in magnetic field- Wiedemann-Franz law. L4. Nearly free electron model - origin of the energy band. L5. Bloch functions - Kronig Penney model. L6. Dielectrics I : Polarization in dielectrics L7 .Dielectrics II: Types of polarization - dielectric constant L8. Assessment L9. Experimental determination of dielectric constant L10. Ferroelectrics (1) : Ferroelectric crystals L11. Ferroelectrics (2): Piezoelectricity L12. Piezoelectricity Applications L1 : Solid State Physics Solid state physics is the study of rigid matter, or solids, ,through methods such as quantum mechanics, crystallography, electromagnetism and metallurgy. It is the largest branch of condensed matter physics. Solid-state physics studies how the large-scale properties of solid materials result from their atomic- scale properties. Thus, solid-state physics forms the theoretical basis of materials science. It also has direct applications, for example in the technology of transistors and semiconductors. Crystalline solids & Amorphous solids Solid materials are formed from densely-packed atoms, which interact intensely. These interactions produce : the mechanical (e.g. hardness and elasticity), thermal, electrical, magnetic and optical properties of solids. Depending on the material involved and the conditions in which it was formed , the atoms may be arranged in a regular, geometric pattern (crystalline solids, which include metals and ordinary water ice) , or irregularly (an amorphous solid such as common window glass). Crystalline solids & Amorphous solids The bulk of solid-state physics theory and research is focused on crystals.
    [Show full text]
  • Lecture 3: Fermi-Liquid Theory 1 General Considerations Concerning Condensed Matter
    Phys 769 Selected Topics in Condensed Matter Physics Summer 2010 Lecture 3: Fermi-liquid theory Lecturer: Anthony J. Leggett TA: Bill Coish 1 General considerations concerning condensed matter (NB: Ultracold atomic gasses need separate discussion) Assume for simplicity a single atomic species. Then we have a collection of N (typically 1023) nuclei (denoted α,β,...) and (usually) ZN electrons (denoted i,j,...) interacting ∼ via a Hamiltonian Hˆ . To a first approximation, Hˆ is the nonrelativistic limit of the full Dirac Hamiltonian, namely1 ~2 ~2 1 e2 1 Hˆ = 2 2 + NR −2m ∇i − 2M ∇α 2 4πǫ r r α 0 i j Xi X Xij | − | 1 (Ze)2 1 1 Ze2 1 + . (1) 2 4πǫ0 Rα Rβ − 2 4πǫ0 ri Rα Xαβ | − | Xiα | − | For an isolated atom, the relevant energy scale is the Rydberg (R) – Z2R. In addition, there are some relativistic effects which may need to be considered. Most important is the spin-orbit interaction: µ Hˆ = B σ (v V (r )) (2) SO − c2 i · i × ∇ i Xi (µB is the Bohr magneton, vi is the velocity, and V (ri) is the electrostatic potential at 2 3 2 ri as obtained from HˆNR). In an isolated atom this term is o(α R) for H and o(Z α R) for a heavy atom (inner-shell electrons) (produces fine structure). The (electron-electron) magnetic dipole interaction is of the same order as HˆSO. The (electron-nucleus) hyperfine interaction is down relative to Hˆ by a factor µ /µ 10−3, and the nuclear dipole-dipole SO n B ∼ interaction by a factor (µ /µ )2 10−6.
    [Show full text]
  • Quantum Mechanics Electromotive Force
    Quantum Mechanics_Electromotive force . Electromotive force, also called emf[1] (denoted and measured in volts), is the voltage developed by any source of electrical energy such as a batteryor dynamo.[2] The word "force" in this case is not used to mean mechanical force, measured in newtons, but a potential, or energy per unit of charge, measured involts. In electromagnetic induction, emf can be defined around a closed loop as the electromagnetic workthat would be transferred to a unit of charge if it travels once around that loop.[3] (While the charge travels around the loop, it can simultaneously lose the energy via resistance into thermal energy.) For a time-varying magnetic flux impinging a loop, theElectric potential scalar field is not defined due to circulating electric vector field, but nevertheless an emf does work that can be measured as a virtual electric potential around that loop.[4] In a two-terminal device (such as an electrochemical cell or electromagnetic generator), the emf can be measured as the open-circuit potential difference across the two terminals. The potential difference thus created drives current flow if an external circuit is attached to the source of emf. When current flows, however, the potential difference across the terminals is no longer equal to the emf, but will be smaller because of the voltage drop within the device due to its internal resistance. Devices that can provide emf includeelectrochemical cells, thermoelectric devices, solar cells and photodiodes, electrical generators,transformers, and even Van de Graaff generators.[4][5] In nature, emf is generated whenever magnetic field fluctuations occur through a surface.
    [Show full text]
  • Phys 446: Solid State Physics / Optical Properties Lattice Vibrations
    Solid State Physics Lecture 5 Last week: Phys 446: (Ch. 3) • Phonons Solid State Physics / Optical Properties • Today: Einstein and Debye models for thermal capacity Lattice vibrations: Thermal conductivity Thermal, acoustic, and optical properties HW2 discussion Fall 2007 Lecture 5 Andrei Sirenko, NJIT 1 2 Material to be included in the test •Factors affecting the diffraction amplitude: Oct. 12th 2007 Atomic scattering factor (form factor): f = n(r)ei∆k⋅rl d 3r reflects distribution of electronic cloud. a ∫ r • Crystalline structures. 0 sin()∆k ⋅r In case of spherical distribution f = 4πr 2n(r) dr 7 crystal systems and 14 Bravais lattices a ∫ n 0 ∆k ⋅r • Crystallographic directions dhkl = 2 2 2 1 2 ⎛ h k l ⎞ 2πi(hu j +kv j +lw j ) and Miller indices ⎜ + + ⎟ •Structure factor F = f e ⎜ a2 b2 c2 ⎟ ∑ aj ⎝ ⎠ j • Definition of reciprocal lattice vectors: •Elastic stiffness and compliance. Strain and stress: definitions and relation between them in a linear regime (Hooke's law): σ ij = ∑Cijklε kl ε ij = ∑ Sijklσ kl • What is Brillouin zone kl kl 2 2 C •Elastic wave equation: ∂ u C ∂ u eff • Bragg formula: 2d·sinθ = mλ ; ∆k = G = eff x sound velocity v = ∂t 2 ρ ∂x2 ρ 3 4 • Lattice vibrations: acoustic and optical branches Summary of the Last Lecture In three-dimensional lattice with s atoms per unit cell there are Elastic properties – crystal is considered as continuous anisotropic 3s phonon branches: 3 acoustic, 3s - 3 optical medium • Phonon - the quantum of lattice vibration. Elastic stiffness and compliance tensors relate the strain and the Energy ħω; momentum ħq stress in a linear region (small displacements, harmonic potential) • Concept of the phonon density of states Hooke's law: σ ij = ∑Cijklε kl ε ij = ∑ Sijklσ kl • Einstein and Debye models for lattice heat capacity.
    [Show full text]
  • Chapter 3 Bose-Einstein Condensation of an Ideal
    Chapter 3 Bose-Einstein Condensation of An Ideal Gas An ideal gas consisting of non-interacting Bose particles is a ¯ctitious system since every realistic Bose gas shows some level of particle-particle interaction. Nevertheless, such a mathematical model provides the simplest example for the realization of Bose-Einstein condensation. This simple model, ¯rst studied by A. Einstein [1], correctly describes important basic properties of actual non-ideal (interacting) Bose gas. In particular, such basic concepts as BEC critical temperature Tc (or critical particle density nc), condensate fraction N0=N and the dimensionality issue will be obtained. 3.1 The ideal Bose gas in the canonical and grand canonical ensemble Suppose an ideal gas of non-interacting particles with ¯xed particle number N is trapped in a box with a volume V and at equilibrium temperature T . We assume a particle system somehow establishes an equilibrium temperature in spite of the absence of interaction. Such a system can be characterized by the thermodynamic partition function of canonical ensemble X Z = e¡¯ER ; (3.1) R where R stands for a macroscopic state of the gas and is uniquely speci¯ed by the occupa- tion number ni of each single particle state i: fn0; n1; ¢ ¢ ¢ ¢ ¢ ¢g. ¯ = 1=kBT is a temperature parameter. Then, the total energy of a macroscopic state R is given by only the kinetic energy: X ER = "ini; (3.2) i where "i is the eigen-energy of the single particle state i and the occupation number ni satis¯es the normalization condition X N = ni: (3.3) i 1 The probability
    [Show full text]
  • Chapter 4: Bonding in Solids and Electronic Properties
    Chapter 4: Bonding in Solids and Electronic Properties Free electron theory Consider free electrons in a metal – an electron gas. •regards a metal as a box in which electrons are free to move. •assumes nuclei stay fixed on their lattice sites surrounded by core electrons, while the valence electrons move freely through the solid. •Ignoring the core electrons, one can treat the outer electrons with a quantum mechanical description. •Taking just one electron, the problem is reduced to a particle in a box. Electron is confined to a line of length a. Schrodinger equation 2 2 2 d d 2me E 2 (E V ) 2 2 2me dx dx Electron is not allowed outside the box, so the potential is ∞ outside the box. Energy is quantized, with quantum numbers n. 2 2 2 n2h2 h2 n n n In 1d: E In 3d: E a b c 2 8m a2 b2 c2 8mea e 1 2 2 2 2 Each set of quantum numbers n , n , h n n n a b a b c E 2 2 2 and nc will give rise to an energy level. 8me a b c •In three dimensions, there are multiple combination of energy levels that will give the same energy, whereas in one-dimension n and –n are equal in energy. 2 2 2 2 2 2 na/a nb/b nc/c na /a + nb /b + nc /c 6 6 6 108 The number of states with the 2 2 10 108 same energy is known as the degeneracy. 2 10 2 108 10 2 2 108 When dealing with a crystal with ~1020 atoms, it becomes difficult to work out all the possible combinations.
    [Show full text]
  • High Pressure Band Structure, Density of States, Structural Phase Transition and Metallization in Cds
    Chemical and Materials Engineering 5(1): 8-13, 2017 http://www.hrpub.org DOI: 10.13189/cme.2017.050102 High Pressure Band Structure, Density of States, Structural Phase Transition and Metallization in CdS J. Jesse Pius1, A. Lekshmi2, C. Nirmala Louis2,* 1Rohini College of Engineering, Nagercoil, Kanyakumari District, India 2Research Center in Physics, Holy Cross College, India Copyright©2017 by authors, all rights reserved. Authors agree that this article remains permanently open access under the terms of the Creative Commons Attribution License 4.0 International License Abstract The electronic band structure, density of high pressure studies due to the development of different states, metallization and structural phase transition of cubic designs of diamond anvil cell (DAC). With a modern DAC, zinc blende type cadmium sulphide (CdS) is investigated it is possible to reach pressures of 2 Mbar (200 GPa) using the full potential linear muffin-tin orbital (FP-LMTO) routinely and pressures of 5 Mbar (500 GPa) or higher is method. The ground state properties and band gap values achievable [3]. At such pressures, materials are reduced to are compared with the experimental results. The fractions of their original volumes. With this reduction in equilibrium lattice constant, bulk modulus and its pressure inter atomic distances; significant changes in bonding and derivative and the phase transition pressure at which the structure as well as other properties take place. The increase compounds undergo structural phase transition from ZnS to of pressure means the significant decrease in volume, which NaCl are predicted from the total energy calculations. The results in the change of electronic states and crystal structure.
    [Show full text]
  • Lecture 24. Degenerate Fermi Gas (Ch
    Lecture 24. Degenerate Fermi Gas (Ch. 7) We will consider the gas of fermions in the degenerate regime, where the density n exceeds by far the quantum density nQ, or, in terms of energies, where the Fermi energy exceeds by far the temperature. We have seen that for such a gas μ is positive, and we’ll confine our attention to the limit in which μ is close to its T=0 value, the Fermi energy EF. ~ kBT μ/EF 1 1 kBT/EF occupancy T=0 (with respect to E ) F The most important degenerate Fermi gas is 1 the electron gas in metals and in white dwarf nε()(),, T= f ε T = stars. Another case is the neutron star, whose ε⎛ − μ⎞ exp⎜ ⎟ +1 density is so high that the neutron gas is ⎝kB T⎠ degenerate. Degenerate Fermi Gas in Metals empty states ε We consider the mobile electrons in the conduction EF conduction band which can participate in the charge transport. The band energy is measured from the bottom of the conduction 0 band. When the metal atoms are brought together, valence their outer electrons break away and can move freely band through the solid. In good metals with the concentration ~ 1 electron/ion, the density of electrons in the electron states electron states conduction band n ~ 1 electron per (0.2 nm)3 ~ 1029 in an isolated in metal electrons/m3 . atom The electrons are prevented from escaping from the metal by the net Coulomb attraction to the positive ions; the energy required for an electron to escape (the work function) is typically a few eV.
    [Show full text]
  • Lecture Notes for Quantum Matter
    Lecture Notes for Quantum Matter MMathPhys c Professor Steven H. Simon Oxford University July 24, 2019 Contents 1 What we will study 1 1.1 Bose Superfluids (BECs, Superfluid He, Superconductors) . .1 1.2 Theory of Fermi Liquids . .2 1.3 BCS theory of superconductivity . .2 1.4 Special topics . .2 2 Introduction to Superfluids 3 2.1 Some History and Basics of Superfluid Phenomena . .3 2.2 Landau and the Two Fluid Model . .6 2.2.1 More History and a bit of Physics . .6 2.2.2 Landau's Two Fluid Model . .7 2.2.3 More Physical Effects and Their Two Fluid Pictures . .9 2.2.4 Second Sound . 12 2.2.5 Big Questions Remaining . 13 2.3 Curl Free Constraint: Introducing the Superfluid Order Parameter . 14 2.3.1 Vorticity Quantization . 15 2.4 Landau Criterion for Superflow . 17 2.5 Superfluid Density . 20 2.5.1 The Andronikoshvili Experiment . 20 2.5.2 Landau's Calculation of Superfluid Density . 22 3 Charged Superfluid ≈ Superconductor 25 3.1 London Theory . 25 3.1.1 Meissner-Ochsenfeld Effect . 27 3 3.1.2 Quantum Input and Superfluid Order Parameter . 29 3.1.3 Superconducting Vortices . 30 3.1.4 Type I and Type II superconductors . 32 3.1.5 How big is Hc ............................... 33 4 Microscopic Theory of Bosons 37 4.1 Mathematical Preliminaries . 37 4.1.1 Second quantization . 37 4.1.2 Coherent States . 38 4.1.3 Multiple orbitals . 40 4.2 BECs and the Gross-Pitaevskii Equation . 41 4.2.1 Noninteracting BECs as Coherent States .
    [Show full text]
  • Chapter 13 Ideal Fermi
    Chapter 13 Ideal Fermi gas The properties of an ideal Fermi gas are strongly determined by the Pauli principle. We shall consider the limit: k T µ,βµ 1, B � � which defines the degenerate Fermi gas. In this limit, the quantum mechanical nature of the system becomes especially important, and the system has little to do with the classical ideal gas. Since this chapter is devoted to fermions, we shall omit in the following the subscript ( ) that we used for the fermionic statistical quantities in the previous chapter. − 13.1 Equation of state Consider a gas ofN non-interacting fermions, e.g., electrons, whose one-particle wave- functionsϕ r(�r) are plane-waves. In this case, a complete set of quantum numbersr is given, for instance, by the three cartesian components of the wave vector �k and thez spin projectionm s of an electron: r (k , k , k , m ). ≡ x y z s Spin-independent Hamiltonians. We will consider only spin independent Hamiltonian operator of the type ˆ 3 H= �k ck† ck + d r V(r)c r†cr , �k � where thefirst and the second terms are respectively the kinetic and th potential energy. The summation over the statesr (whenever it has to be performed) can then be reduced to the summation over states with different wavevectork(p=¯hk): ... (2s + 1) ..., ⇒ r � �k where the summation over the spin quantum numberm s = s, s+1, . , s has been taken into account by the prefactor (2s + 1). − − 159 160 CHAPTER 13. IDEAL FERMI GAS Wavefunctions in a box. We as- sume that the electrons are in a vol- ume defined by a cube with sidesL x, Ly,L z and volumeV=L xLyLz.
    [Show full text]
  • Inorganic Chemistry for Dummies® Published by John Wiley & Sons, Inc
    Inorganic Chemistry Inorganic Chemistry by Michael L. Matson and Alvin W. Orbaek Inorganic Chemistry For Dummies® Published by John Wiley & Sons, Inc. 111 River St. Hoboken, NJ 07030-5774 www.wiley.com Copyright © 2013 by John Wiley & Sons, Inc., Hoboken, New Jersey Published by John Wiley & Sons, Inc., Hoboken, New Jersey Published simultaneously in Canada No part of this publication may be reproduced, stored in a retrieval system or transmitted in any form or by any means, electronic, mechanical, photocopying, recording, scanning or otherwise, except as permitted under Sections 107 or 108 of the 1976 United States Copyright Act, without either the prior written permis- sion of the Publisher, or authorization through payment of the appropriate per-copy fee to the Copyright Clearance Center, 222 Rosewood Drive, Danvers, MA 01923, (978) 750-8400, fax (978) 646-8600. Requests to the Publisher for permission should be addressed to the Permissions Department, John Wiley & Sons, Inc., 111 River Street, Hoboken, NJ 07030, (201) 748-6011, fax (201) 748-6008, or online at http://www.wiley. com/go/permissions. Trademarks: Wiley, the Wiley logo, For Dummies, the Dummies Man logo, A Reference for the Rest of Us!, The Dummies Way, Dummies Daily, The Fun and Easy Way, Dummies.com, Making Everything Easier, and related trade dress are trademarks or registered trademarks of John Wiley & Sons, Inc. and/or its affiliates in the United States and other countries, and may not be used without written permission. All other trade- marks are the property of their respective owners. John Wiley & Sons, Inc., is not associated with any product or vendor mentioned in this book.
    [Show full text]