Slides from FYS4411 Lectures Morten Hjorth-Jensen & Gustav R. - - PowerPoint PPT Presentation

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Slides from FYS4411 Lectures Morten Hjorth-Jensen & Gustav R. Jansen 1 Department of Physics and Center of Mathematics for Applications University of Oslo, N-0316 Oslo, Norway Spring 2012 1 / 38 Quantum dots What are they? Electrons


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SLIDE 1

Slides from FYS4411 Lectures

Morten Hjorth-Jensen & Gustav R. Jansen

1Department of Physics and Center of Mathematics for Applications

University of Oslo, N-0316 Oslo, Norway

Spring 2012

1 / 38

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SLIDE 2

Quantum dots

What are they?

◮ Electrons confined in an external potential. ◮ What happens in semiconductors? ◮ Coloumb effects and the Pauli principle keeps an excited

electron-hole pair bound.

◮ Modelled by a free particle with an effective mass in an

external potential. Can disregard the crystal lattice.

◮ Have the same properties as atoms, only larger size. Are

discussed as artificial atoms.

◮ Discrete energy levels. ◮ Selfbound. ◮ Relatively long lifetimes. 2 / 38

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SLIDE 3

Quantum dots

What are they?

◮ Electrons confined in an external potential. ◮ What happens in semiconductors? ◮ Coloumb effects and the Pauli principle keeps an excited

electron-hole pair bound.

◮ Modelled by a free particle with an effective mass in an

external potential. Can disregard the crystal lattice.

◮ Have the same properties as atoms, only larger size. Are

discussed as artificial atoms.

◮ Discrete energy levels. ◮ Selfbound. ◮ Relatively long lifetimes. 3 / 38

slide-4
SLIDE 4

Quantum dots

What are they?

◮ Electrons confined in an external potential. ◮ What happens in semiconductors? ◮ Coloumb effects and the Pauli principle keeps an excited

electron-hole pair bound.

◮ Modelled by a free particle with an effective mass in an

external potential. Can disregard the crystal lattice.

◮ Have the same properties as atoms, only larger size. Are

discussed as artificial atoms.

◮ Discrete energy levels. ◮ Selfbound. ◮ Relatively long lifetimes. 4 / 38

slide-5
SLIDE 5

Quantum dots

What are they?

◮ Electrons confined in an external potential. ◮ What happens in semiconductors? ◮ Coloumb effects and the Pauli principle keeps an excited

electron-hole pair bound.

◮ Modelled by a free particle with an effective mass in an

external potential. Can disregard the crystal lattice.

◮ Have the same properties as atoms, only larger size. Are

discussed as artificial atoms.

◮ Discrete energy levels. ◮ Selfbound. ◮ Relatively long lifetimes. 5 / 38

slide-6
SLIDE 6

Quantum dots

What are they?

◮ Electrons confined in an external potential. ◮ What happens in semiconductors? ◮ Coloumb effects and the Pauli principle keeps an excited

electron-hole pair bound.

◮ Modelled by a free particle with an effective mass in an

external potential. Can disregard the crystal lattice.

◮ Have the same properties as atoms, only larger size. Are

discussed as artificial atoms.

◮ Discrete energy levels. ◮ Selfbound. ◮ Relatively long lifetimes. 6 / 38

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SLIDE 7

Quantum dots

Properties

◮ Energylevels depends on the size of the crystal. (Typically

nanometer scale)

◮ Smaller crystals have larger energy gaps. ◮ Effective mass depends on type of semiconductor and

size.

◮ Effective mass much smaller than me. ◮ Large de Broglie wavelength - λ =

h γmov

◮ Quantum effects visible at larger scales.

◮ Emits light when electron recombines with hole. Frequency

depends on energy gap.

◮ There are indications that the shape of the crystal also

affect energy gap.

◮ Can be modelled as particles in a well.

7 / 38

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SLIDE 8

Quantum dots

Properties

◮ Energylevels depends on the size of the crystal. (Typically

nanometer scale)

◮ Smaller crystals have larger energy gaps. ◮ Effective mass depends on type of semiconductor and

size.

◮ Effective mass much smaller than me. ◮ Large de Broglie wavelength - λ =

h γmov

◮ Quantum effects visible at larger scales.

◮ Emits light when electron recombines with hole. Frequency

depends on energy gap.

◮ There are indications that the shape of the crystal also

affect energy gap.

◮ Can be modelled as particles in a well.

8 / 38

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SLIDE 9

Quantum dots

Properties

◮ Energylevels depends on the size of the crystal. (Typically

nanometer scale)

◮ Smaller crystals have larger energy gaps. ◮ Effective mass depends on type of semiconductor and

size.

◮ Effective mass much smaller than me. ◮ Large de Broglie wavelength - λ =

h γmov

◮ Quantum effects visible at larger scales.

◮ Emits light when electron recombines with hole. Frequency

depends on energy gap.

◮ There are indications that the shape of the crystal also

affect energy gap.

◮ Can be modelled as particles in a well.

9 / 38

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SLIDE 10

Quantum dots

Properties

◮ Energylevels depends on the size of the crystal. (Typically

nanometer scale)

◮ Smaller crystals have larger energy gaps. ◮ Effective mass depends on type of semiconductor and

size.

◮ Effective mass much smaller than me. ◮ Large de Broglie wavelength - λ =

h γmov

◮ Quantum effects visible at larger scales.

◮ Emits light when electron recombines with hole. Frequency

depends on energy gap.

◮ There are indications that the shape of the crystal also

affect energy gap.

◮ Can be modelled as particles in a well.

10 / 38

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SLIDE 11

Quantum dots

Properties

◮ Energylevels depends on the size of the crystal. (Typically

nanometer scale)

◮ Smaller crystals have larger energy gaps. ◮ Effective mass depends on type of semiconductor and

size.

◮ Effective mass much smaller than me. ◮ Large de Broglie wavelength - λ =

h γmov

◮ Quantum effects visible at larger scales.

◮ Emits light when electron recombines with hole. Frequency

depends on energy gap.

◮ There are indications that the shape of the crystal also

affect energy gap.

◮ Can be modelled as particles in a well.

11 / 38

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SLIDE 12

Quantum dots

Properties

◮ Energylevels depends on the size of the crystal. (Typically

nanometer scale)

◮ Smaller crystals have larger energy gaps. ◮ Effective mass depends on type of semiconductor and

size.

◮ Effective mass much smaller than me. ◮ Large de Broglie wavelength - λ =

h γmov

◮ Quantum effects visible at larger scales.

◮ Emits light when electron recombines with hole. Frequency

depends on energy gap.

◮ There are indications that the shape of the crystal also

affect energy gap.

◮ Can be modelled as particles in a well.

12 / 38

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SLIDE 13

Quantum dots

Usage

◮ Quantum laboratory. ◮ Improved transistors. ◮ Quantum computers ◮ QLED (light emitting diode) and lasers.

◮ Smaller sizes

◮ Medical imaging techniques and realtime tracking of

molecules/cells.

◮ Improved solar panel efficiency.

13 / 38

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SLIDE 14

Quantum dots

Usage

◮ Quantum laboratory. ◮ Improved transistors. ◮ Quantum computers ◮ QLED (light emitting diode) and lasers.

◮ Smaller sizes

◮ Medical imaging techniques and realtime tracking of

molecules/cells.

◮ Improved solar panel efficiency.

14 / 38

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SLIDE 15

Quantum dots

Usage

◮ Quantum laboratory. ◮ Improved transistors. ◮ Quantum computers ◮ QLED (light emitting diode) and lasers.

◮ Smaller sizes

◮ Medical imaging techniques and realtime tracking of

molecules/cells.

◮ Improved solar panel efficiency.

15 / 38

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SLIDE 16

Quantum dots

Usage

◮ Quantum laboratory. ◮ Improved transistors. ◮ Quantum computers ◮ QLED (light emitting diode) and lasers.

◮ Smaller sizes

◮ Medical imaging techniques and realtime tracking of

molecules/cells.

◮ Improved solar panel efficiency.

16 / 38

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SLIDE 17

Quantum dots

Usage

◮ Quantum laboratory. ◮ Improved transistors. ◮ Quantum computers ◮ QLED (light emitting diode) and lasers.

◮ Smaller sizes

◮ Medical imaging techniques and realtime tracking of

molecules/cells.

◮ Improved solar panel efficiency.

17 / 38

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SLIDE 18

Quantum dots

Usage

◮ Quantum laboratory. ◮ Improved transistors. ◮ Quantum computers ◮ QLED (light emitting diode) and lasers.

◮ Smaller sizes

◮ Medical imaging techniques and realtime tracking of

molecules/cells.

◮ Improved solar panel efficiency.

18 / 38

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SLIDE 19

Quantum dots, the case of our project

We consider a system of electrons confined in a pure isotropic harmonic oscillator potential V(r) = m∗ω2

0r 2/2, where m∗ is the effective mass of the electrons in the host

semiconductor, ω0 is the oscillator frequency of the confining potential, and r = (x, y, z) denotes the position of the particle. The Hamiltonian of a single particle trapped in this harmonic oscillator potential simply reads ˆ H = p2 2m∗ + 1 2m∗ω2

0r2

where p is the canonical momentum of the particle.

19 / 38

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SLIDE 20

Quantum dots

When considering several particles trapped in the same quantum dot, the Coulomb repulsion between those electrons has to be added to the single particle Hamiltonian which gives ˆ H =

Ne

X

i=1

„ pi2 2m∗ + 1 2m∗ω2

0ri 2

« + e2 4πǫ0ǫr X

i<j

1 ri − rj , where Ne is the number of electrons, −e (e > 0) is the charge of the electron, ǫ0 and ǫr are respectively the free space permitivity and the relative permitivity of the host material (also called dielectric constant), and the index i labels the electrons.

20 / 38

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SLIDE 21

Quantum dots

We assume that the magnetic field − → B is static and along the z axis. At first we ignore the spin-dependent terms. The Hamiltonian of these electrons in a magnetic field now reads ˆ H =

Ne

X

i=1

„(pi + eA)2 2m∗ + 1 2 m∗ω2

0ri 2

« + e2 4πǫ0ǫr X

i<j

1 ri − rj , (1) =

Ne

X

i=1

„ pi2 2m∗ + e 2m∗ (A · pi + pi · A) + e2 2m∗ A2 + 1 2m∗ω2

0ri 2

« (2) + e2 4πǫ0ǫr X

i<j

1 ri − rj , (3) where A is the vector potential defined by B = ∇ × A.

21 / 38

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SLIDE 22

Quantum dots

In coordinate space, pi is the operator −i∇i and by applying the Hamiltonian on the total wave function Ψ(r) in the Schr¨

  • dinger equation, we obtain the following operator

acting on Ψ(r) A · pi + pi · A = −i(A · ∇i + ∇i · A) Ψ (4) = −i(A · (∇iΨ) + ∇i · (AΨ)) (5)

22 / 38

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SLIDE 23

Quantum dots

We note that if we use the product rule and the Coulomb gauge ∇ · A = 0 (by choosing the vector potential as A = 1

2B × r), pi and ∇i commute and we obtain

∇i · (AΨ) = A · (∇iΨ) + (∇i · A) | {z } Ψ = A · (∇iΨ)

23 / 38

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SLIDE 24

Quantum dots

This leads us to the following Hamiltonian: ˆ H =

Ne

X

i=1

„ − 2 2m∗ ∇2

i − i e

m∗ A · ∇i + e2 2m∗ A2 + 1 2m∗ω2

0ri 2

« + e2 4πǫ0ǫr X

i<j

1 ri − rj ,

24 / 38

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SLIDE 25

Quantum dots

The linear term in A becomes, in terms of B: −ie m∗ A · ∇i = − ie 2m∗ (B × ri) · ∇i (6) = −ie 2m∗ B · (ri × ∇i) (7) = e 2m∗ B · L (8) where L = −i(ri × ∇i) is the orbital angular momentum operator of the electron i.

25 / 38

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SLIDE 26

Quantum dots

If we assume that the electrons are confined in the xy-plane, the quadratic term in A can be written as e2 2m∗ A2 = e2 8m∗ (B × r)2 = e2 8m∗ B2r 2

i 26 / 38

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SLIDE 27

Quantum dots

Until this point we have neglected the intrinsic magnetic moment of the electrons which is due to the electron spin in the host material. We will now add its effect to the

  • Hamiltonian. This intrinsic magnetic moment is given by Ms = −g∗

s (eS)/(2m∗),

where S is the spin operator of the electron and g∗

s its effective spin gyromagnetic ratio

(or effective g-factor in the host material).We see that the spin magnetic moment Ms gives rise to an additional interaction energy linear in the magnetic field, ˆ Hs = −Ms · B = g∗

s

e 2m∗ B ˆ Sz = g∗

s

ωc 2 ˆ Sz where ωc = eB/m∗ is known as the cyclotron frequency.

27 / 38

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SLIDE 28

Quantum dots

The final Hamiltonian reads ˆ H =

Ne

X

i=1

„ −2 2m∗ ∇2

i + Harmonic ocscillator potential

z }| { 1 2 m∗ω2

0ri 2

« +

Coulomb interactions

z }| { e2 4πǫ0ǫr X

i<j

1 |ri − rj| +

Ne

X

i=1

„1 2m∗ “ωc 2 ”2 ri

2 + 1

2ωcˆ L(i)

z + 1

2g∗

s ωc ˆ

S(i)

z

« | {z }

single particle interactions with the magnetic field

, (9)

28 / 38

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SLIDE 29

Quantum dots

In order to simplify the computation, the Hamiltonian can be rewritten on dimensionless

  • form. For this purpose, we introduce the following constants:

◮ the oscillator frequency ω = ω0 q 1 + ω2

c/(4ω2 0),

◮ a new energy unit ω, ◮ a new length unit, the oscillator length defined by l = p /(m∗ω), also called the characteristic length unit. We rewrite the Hamiltonian in dimensionless units using: r − → r l , ∇ − → l ∇ and ˆ Lz − → ˆ Lz

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SLIDE 30

Quantum dots

It leads to the following Hamiltonian: ˆ H =

Ne

X

i=1

„ − 1 2∇2

i + 1

2r 2

i

« +

Dimensionless confinement strength (λ)

z }| { e2 4πǫ0ǫr 1 ωl X

i<j

1 rij +

Ne

X

i=1

„1 2 ωc ω ˆ L(i)

z + 1

2g∗

s

ωc ω ˆ S(i)

z

« , (10) Lengths are now measured in units of l = p /(m∗ω), and energies in units of ω.

30 / 38

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SLIDE 31

Quantum dots

A new dimensionless parameter λ = l/a∗

0 (where a∗ 0 = 4πǫ0ǫr2/(e2m∗) is the

effective Bohr radius) describes the strength of the electron-electron interaction. Large λ implies strong interaction and/or large quantum dot. Since both ˆ Lz and ˆ Sz commute with the Hamiltonian we can perform the calculations separately in subspaces of given quantum numbers Lz and Sz.

31 / 38

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SLIDE 32

Quantum dots

The simplified dimensionless Hamiltonian becomes ˆ H =

Ne

X

i=1

» − 1 2∇2

i + 1

2r 2

i

– + λ X

i<j

1 rij +

Ne

X

i=1

„ 1 2 ωc ω L(i)

z + 1

2g∗

s

ωc ω S(i)

z

« ,

32 / 38

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SLIDE 33

Quantum dots

The last sum which is proportional to the magnetic field involves only the quantum numbers Lz and Sz and not the operators themselves. Therefore these terms can be put aside during the resolution, the squizzing effect of the magnetic field being included simply in the parameter λ. The contribution of these terms will be added when the other part has been solved. This brings us to the simple and general form of the Hamiltonian: ˆ H =

Ne

X

i=1

„ − 1 2∇2

i + 1

2 r 2

i

« + λ X

i<j

1 rij .

33 / 38

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SLIDE 34

Quantum dots

The form ˆ H =

Ne

X

i=1

„ − 1 2∇2

i + 1

2 r 2

i

« + λ X

i<j

1 rij , is however not so practical since the interaction carries a strength λ. Why?

34 / 38

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SLIDE 35

Quantum dots

We rewrite it as a one-body part ˆ H0 =

Ne

X

i=1

„ − 1 2∇2

i + ω2

2 r 2

i

« , and interacting part ˆ V =

Ne

X

i<j

1 |ri − rj|. Your task till next week is to show this. The unperturbed part of the Hamiltonian yields the single-particle energies ǫi = ω (2n + |m| + 1) , (11) where n = 0, 1, 2, 3, .. and m = 0, ±1, ±2, ... The index i runs from 0, 1, 2, . . . .

35 / 38

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SLIDE 36

Harmonic oscillator in 2D with cartesian coordinates

Hamilton operator

  • H0 =

N

  • i=1
  • −1

2∇2

i + 1

2ω2r 2

i

  • Eigenvalues and eigenfunctions

φnx,ny(x, y) = AHnx(√ωx)Hny(√ωy) exp (−ω(x2 + y2)/2 E = ω(nx + ny + 1) Leads to a shell structure, similar to atomic and nuclear systems.

36 / 38

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SLIDE 37

Hermite polynomials

The Hermite polynomials are the solutions of the following differential equation d2H(x) dx2 − 2x dH(x) dx + (λ − 1)H(x) = 0. (12) The first few polynomials are H0(x) = 1, H1(x) = 2x, H2(x) = 4x2 − 2, H3(x) = 8x3 − 12, and H4(x) = 16x4 − 48x2 + 12. They fulfil the orthogonality relation ∞

−∞

e−x2Hn(x)2dx = 2nn!√π, and the recursion relation Hn+1(x) = 2xHn(x) − 2nHn−1(x).

37 / 38

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SLIDE 38

Tasks for next week

◮ Set up the harmonic oscillator wave function in cartesian coordinates for an electron with nx = ny = 0 and find the oscillator energy. ◮ Use this result to find the unperturbed energy Z Φ∗ ˆ H0Φdτ =

N

X

µ=1

µ|h|µ. for two electrons with the same quantum numbers. Is that possible? ◮ Repeat for six electrons (find the relevant harmonic oscillator quantum numbers) ◮ Read chapter 5 of Lars Eivind Lerv˚ ag’s thesis, it deals with quantum dots and gives a good introduction to the physics of quantum dots. ◮ For the project, finish parts 1a and 1b, including analytical derivatives and the profile analysis.

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