Degenerate Electron Gas Unrealistic model: Uniform positive charge density n L Very large volume V=L 3 Eventually take limit: System is neutral Positive.

Slides:



Advertisements
Similar presentations
Free Electron Fermi Gas
Advertisements

Electric Flux Density, Gauss’s Law, and Divergence
Energy is absorbed and emitted in quantum packets of energy related to the frequency of the radiation: Planck constant h= 6.63  10 −34 J·s Planck constant.
The electromagnetic (EM) field serves as a model for particle fields
January 23, 2001Physics 8411 Elastic Scattering of Electrons by Nuclei We want to consider the elastic scattering of electrons by nuclei to see (i) how.
Degenerate Fermi Gas.
Lecture Notes # 3 Understanding Density of States
The electromagnetic (EM) field serves as a model for particle fields  = charge density, J = current density.
Review Three Pictures of Quantum Mechanics Simple Case: Hamiltonian is independent of time 1. Schrödinger Picture: Operators are independent of time; state.
Stellar Structure Section 5: The Physics of Stellar Interiors Lecture 10 – Relativistic and quantum effects for electrons Completely degenerate electron.
Green’s Functions From Heisenberg to Interaction Picture Useful once we have it, but since we need to know the full ground state and the field operators.
Lecture 18: The Hydrogen Atom
3D Schrodinger Equation
Lecture 17: The Hydrogen Atom
Prof. Reinisch, EEAS / Simple Collision Parameters (1) There are many different types of collisions taking place in a gas. They can be grouped.
Lesson 8 Beta Decay. Beta -decay Beta decay is a term used to describe three types of decay in which a nuclear neutron (proton) changes into a nuclear.
Lecture 19: The Hydrogen Atom Reading: Zuhdahl Outline –The wavefunction for the H atom –Quantum numbers and nomenclature –Orbital shapes and.
 -decay theory. The decay rate Fermi’s Golden Rule density of final states (b) transition (decay) rate (c) transition matrix element (a) Turn off any.
Physics 452 Quantum mechanics II Winter 2012 Karine Chesnel.
Lecture 14 Today Orthogonal coordinate systems 1.The Cartesian (rectangular) coordinate system 2.The cylindrical coordinate system 3.The spherical.
LECTURE 16 THE SCHRÖDINGER EQUATION. GUESSING THE SE.
P460 - many particles1 Many Particle Systems can write down the Schrodinger Equation for a many particle system with x i being the coordinate of particle.
Nuclear Astrophysics 1 Lecture 2 Thurs. Oct. 27, 2011 Prof. Shawn Bishop, Office 2013, Ex
Many-body Green’s Functions
12.3 Assembly of distinguishable particles
Cross section for potential scattering
P D S.E.1 3D Schrodinger Equation Simply substitute momentum operator do particle in box and H atom added dimensions give more quantum numbers. Can.
Lecture 19: The deuteron 13/11/2003 Basic properties: mass: mc 2 = MeV binding energy: (measured via  -ray energy in n + p  d +  ) RMS.
Lecture 16: Beta Decay Spectrum 29/10/2003 (and related processes...) Goals: understand the shape of the energy spectrum total decay rate sheds.
Quantum Two 1. 2 Evolution of Many Particle Systems 3.
Statistical mechanics How the overall behavior of a system of many particles is related to the Properties of the particles themselves. It deals with the.
Four-potential of a field Section 16. For a given field, the action is the sum of two terms S = S m + S mf – Free-particle term – Particle-field interaction.
Advanced Higher Physics Electric Potential. Electric Potential 1 V = work done / q(measured in J C -1 ) Defined as ‘the work done per unit positive charge.
Why is energy extensive? So Hirata Department of Chemistry.
Quantum Mechanical Cross Sections In a practical scattering experiment the observables we have on hand are momenta, spins, masses, etc.. We do not directly.
Introduction to Time dependent Time-independent methods: Kap. 7-lect2 Methods to obtain an approximate eigen energy, E and wave function: perturbation.
Chapter 13 Gravitation Newton’s Law of Gravitation Here m 1 and m 2 are the masses of the particles, r is the distance between them, and G is the.
Plan for Mon, 3 Nov 08 Exam 2, Quiz 5, and Quiz 4 regrades returned Wednesday Bring a USB drive to lab on Wednesday Lecture Cheer up, it’s only quantum.
Atomic Structure The theories of atomic and molecular structure depend on quantum mechanics to describe atoms and molecules in mathematical terms.
Lecture 21: On to Finite Nuclei! 20/11/2003 Review: 1. Nuclear isotope chart: (lecture 1) 304 isotopes with t ½ > 10 9 yrs (age of the earth) 177.
A. Ambrosetti, F. Pederiva and E. Lipparini
Physical Chemistry III (728342) The Schrödinger Equation
Vibrational Motion Harmonic motion occurs when a particle experiences a restoring force that is proportional to its displacement. F=-kx Where k is the.
Lecture 6: Cross Section for Electron Scattering 23/9/2003 Recall from last time: where V n is the normalization volume for the plane wave electron.
The Hydrogen Atom The only atom that can be solved exactly.
ELECTROMAGNETIC PARTICLE: MASS, SPIN, CHARGE, AND MAGNETIC MOMENT Alexander A. Chernitskii.
1 Electric Potential Reading: Chapter 29 Chapter 29.
Quantum Two 1. 2 Time-Dependent Perturbations 3.
Syed Ali Raza Supervisor: Dr. Pervez Hoodbhoy. A brief Overview of Quantum Hall Effect Spinning Disk Spinning Disk with magnetic Field Kubo’s Formula.
Lecture 2 - Feynman Diagrams & Experimental Measurements
Ring Disk Last Time Infinite Plane + Two Infinite Planes FIELD OF RING ALONG AXIS +- FIELD OF DISK ALONG AXIS 1.
The Hydrogen Atom The only atom that can be solved exactly.
Chapter 13 Gravitation.
Chapter V Interacting Fields Lecture 1 Books Recommended:
Concept test 15.1 Suppose at time
The Vector Operator Ñ and The Divergence Theorem
Virial Theorem LL2 Section 34.
Announcements Exam Details: Today: Problems 6.6, 6.7
Concept test 15.1 Suppose at time
Quantum Two.
Consider the He atom. The Hamiltonian is
Adaptive Perturbation Theory: QM and Field Theory
Ψ
Chapter 13 Gravitation.
Chapter 29 Electric Potential Reading: Chapter 29.
Scattering Theory: Revised and corrected
Spin-triplet molecule inside carbon nanotube
LECTURE 15.
Consider a PIB with a sloped bottom. You want to try perturbation
Cooper Pairs In the 1950s it was becoming clear that the superelectrons were paired ie there must be a positive interaction that holds a pair of electrons.
Presentation transcript:

Degenerate Electron Gas Unrealistic model: Uniform positive charge density n L Very large volume V=L 3 Eventually take limit: System is neutral Positive charge is a uniform background – not quantum mechanical. Wave functions of electrons: Particle in a box

Total Hamiltonian Electron piece Background piece Electron-background piece We will need a convergence factor to handle infinities. At end, need to take limit:

Background Pieces Background piece Electron-background piece Translational invariance Note: last term is infinite when we go to desired limits.

Electron Piece All of the physical effects are in H e. Evaluate in second quantization form. Kinetic Piece:

Kinetic Energy Operator Number operator

Now Start on P.E. Momentum conservation Helicity conservation Coulomb interaction does not flip spins

Potential Operator Let Conservation of momentum automatically

No Scattering Term Number Operators Anticommutation relations Cancels remaining N 2 /V piece Still an infinity as μ→0, but it’s just a number and and we can redefine zero of energy.

New Hamiltonian Define dimensionless parameters: Perturbation in high density limit (r 0 << a 0 ).

Notes on High Density Perturbation Expansion In high density limit: See problems 5 & 6 Term diverges as r s →0. Have to handle carefully at second order. We will evaluate a (kinetic energy term) and b (potential energy term) and leave the rest to more powerful machinery that we develop later (I hope). In high density limit: Kinetic energy of ground state plane waves. “Exchange” perturbation

Ground State – Fermi Level In ground state, two electron (one spin up, on spin down) fill each momentum state starting at the lowest and going up until all of the electrons are used up. The energy where they stop is call the “Fermi level.” Fermi Level

Sum over states below Fermi level Note: we are still integrating in rectangular coordinates. Fermi Level – Number Operator Spherical integral Sum over λ

Ground state energy – First Term

Ground state energy – Second Term Makes vacancy in two states Must fill the same two vacancies Thus, either: This is the non-scattering case q=0 Already subtracted.

Working on the Matrix Element Intersection of two spheres

Important Integral Volume of Integration Take zero of coordinate system at k and z along q; do k integral first in cylindrical coordinates for half of volume (then double).

Finish the Integration

Expansion – First Two Terms Kinetic Term Exchange Term Minimum at 4.82 a 0