Second quantization: where quantization and particles come from?

Similar documents
2 Canonical quantization

Angular momentum. Quantum mechanics. Orbital angular momentum

Rotations in Quantum Mechanics

Quantization of a Scalar Field

The Klein-Gordon equation

Quantum Mechanics II

Problem Set No. 3: Canonical Quantization Due Date: Wednesday October 19, 2018, 5:00 pm. 1 Spin waves in a quantum Heisenberg antiferromagnet

Postulates of Quantum Mechanics

where P a is a projector to the eigenspace of A corresponding to a. 4. Time evolution of states is governed by the Schrödinger equation

Electric and Magnetic Forces in Lagrangian and Hamiltonian Formalism

Generators for Continuous Coordinate Transformations

Time-Independent Perturbation Theory

Quantum Mechanics I Physics 5701

1 Quantum field theory and Green s function

Physics 342 Lecture 27. Spin. Lecture 27. Physics 342 Quantum Mechanics I

Physics 5153 Classical Mechanics. Canonical Transformations-1

1 The Quantum Anharmonic Oscillator

Lecture 9: Eigenvalues and Eigenvectors in Classical Mechanics (See Section 3.12 in Boas)

Problems and Multiple Choice Questions

3. Quantum Mechanics in 3D

Lecture 5. Hartree-Fock Theory. WS2010/11: Introduction to Nuclear and Particle Physics

Summary of free theory: one particle state: vacuum state is annihilated by all a s: then, one particle state has normalization:

Massachusetts Institute of Technology Physics Department

Quantum field theory and Green s function

ψ s a ˆn a s b ˆn b ψ Hint: Because the state is spherically symmetric the answer can depend only on the angle between the two directions.

Statistical Interpretation

in terms of the classical frequency, ω = , puts the classical Hamiltonian in the form H = p2 2m + mω2 x 2

PHY 407 QUANTUM MECHANICS Fall 05 Problem set 1 Due Sep

Path integral in quantum mechanics based on S-6 Consider nonrelativistic quantum mechanics of one particle in one dimension with the hamiltonian:

Total Angular Momentum for Hydrogen

Vector Fields. It is standard to define F µν = µ ϕ ν ν ϕ µ, so that the action may be written compactly as

Representation theory and quantum mechanics tutorial Spin and the hydrogen atom

Quantum Theory and Group Representations

Angular Momentum. Classically the orbital angular momentum with respect to a fixed origin is. L = r p. = yp z. L x. zp y L y. = zp x. xpz L z.

Topological insulator with time-reversal symmetry

Lecture 1: Introduction to QFT and Second Quantization

HAMILTON S PRINCIPLE

Maxwell s equations. based on S-54. electric field charge density. current density

M2A2 Problem Sheet 3 - Hamiltonian Mechanics

Topological insulator part II: Berry Phase and Topological index

Sample Quantum Chemistry Exam 2 Solutions

Canonical transformations (Lecture 4)

Lecture-XXVI. Time-Independent Schrodinger Equation

The Hamiltonian operator and states

Lecture #1. Review. Postulates of quantum mechanics (1-3) Postulate 1

Notes on x-ray scattering - M. Le Tacon, B. Keimer (06/2015)

( r) = 1 Z. e Zr/a 0. + n +1δ n', n+1 ). dt ' e i ( ε n ε i )t'/! a n ( t) = n ψ t = 1 i! e iε n t/! n' x n = Physics 624, Quantum II -- Exam 1

Quantum Mechanics in Three Dimensions

Lecture 11 Spin, orbital, and total angular momentum Mechanics. 1 Very brief background. 2 General properties of angular momentum operators

Simple Harmonic Oscillator

4.3 Lecture 18: Quantum Mechanics

Conservation of Linear Momentum : If a force F is acting on particle of mass m, then according to Newton s second law of motion, we have F = dp /dt =

Harmonic Oscillator I

CHAPTER 1. SPECIAL RELATIVITY AND QUANTUM MECHANICS

Attempts at relativistic QM

Lectures 21 and 22: Hydrogen Atom. 1 The Hydrogen Atom 1. 2 Hydrogen atom spectrum 4

Lecture 4: Equations of motion and canonical quantization Read Sakurai Chapter 1.6 and 1.7

ECE 487 Lecture 6 : Time-Dependent Quantum Mechanics I Class Outline:

Chemistry 532 Practice Final Exam Fall 2012 Solutions

3 Quantization of the Dirac equation

Theoretical physics. Deterministic chaos in classical physics. Martin Scholtz

The quantum state as a vector

Magnets, 1D quantum system, and quantum Phase transitions

Quantization of Scalar Field

Phys 622 Problems Chapter 5

Page 404. Lecture 22: Simple Harmonic Oscillator: Energy Basis Date Given: 2008/11/19 Date Revised: 2008/11/19

PY 351 Modern Physics - Lecture notes, 3

Lecture 6. Fermion Pairing. WS2010/11: Introduction to Nuclear and Particle Physics

Lecture 19 (Nov. 15, 2017)

Department of Physics PRELIMINARY EXAMINATION 2014 Part I. Short Questions

Eigenmodes for coupled harmonic vibrations. Algebraic Method for Harmonic Oscillator.

Quantization of the Spins

Lecture notes for QFT I (662)

Physics 342 Lecture 26. Angular Momentum. Lecture 26. Physics 342 Quantum Mechanics I

Symmetries and particle physics Exercises

Physics 741 Graduate Quantum Mechanics 1 Solutions to Midterm Exam, Fall x i x dx i x i x x i x dx

Physics 828 Problem Set 7 Due Wednesday 02/24/2010

Columbia University Department of Physics QUALIFYING EXAMINATION

Waves and the Schroedinger Equation

( ) in the interaction picture arises only

1 Quantum fields in Minkowski spacetime

5.4 Given the basis e 1, e 2 write the matrices that represent the unitary transformations corresponding to the following changes of basis:

Quantization of scalar fields

3.15. Some symmetry properties of the Berry curvature and the Chern number.

ΑΒΓΔΕΖΗΘΙΚΛΜΝΞΟΠΡΣΤΥΦΧΨΩ αβγδεζηθικλμνξοπρςστυφχψω +<=>± ħ

Lecture 12. The harmonic oscillator

which implies that we can take solutions which are simultaneous eigen functions of

Quantization of the open string on exact plane waves and non-commutative wave fronts

Physics 70007, Fall 2009 Answers to Final Exam

Quantum Mechanics Solutions. λ i λ j v j v j v i v i.

129 Lecture Notes Relativistic Quantum Mechanics

Newton s laws. Chapter 1. Not: Quantum Mechanics / Relativistic Mechanics

Curves in the configuration space Q or in the velocity phase space Ω satisfying the Euler-Lagrange (EL) equations,

1 Mathematical preliminaries

Quantum field theory and Green s function

We can then linearize the Heisenberg equation for in the small quantity obtaining a set of linear coupled equations for and :

( ) /, so that we can ignore all

5 Topological insulator with time-reversal symmetry

General Exam Part II, Fall 1998 Quantum Mechanics Solutions

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department 8.323: Relativistic Quantum Field Theory I PROBLEM SET 2

Transcription:

110 Phys460.nb 7 Second quantization: where quantization and particles come from? 7.1. Lagrangian mechanics and canonical quantization Q: How do we quantize a general system? 7.1.1.Lagrangian Lagrangian mechanics is a reformulation of classical mechanics. L = T - V (7.1) Here, the quantity L is called the Lagrangian, where T is the kinetic energy and V is the potential energy. For example, for a pendulum as shown in the figure, the kinetic energy is T = 1 m r dθ dt = 1 m r θ (7.) where θ represents time derivative of θ V = - m g r cos θ (7.3) And thus L θ, θ = 1 m r θ + m g r cos θ (7.4) Here, the Lagrangian depends on θ and the time derivative of θ. In Lagrangian mechanics, θ is called a coordinate. In this example, we have only one single coordinate, but in general, a more complicated system can have multiple coordinates. And in general, L depends on the coordinates and the time derivatives of these coordinates, e.g. L(q 1, q q n; q 1, q q n ) (7.5) where q i are coordinates. 7.1.. Equation(s) of motion The equation of motion in Lagrangian mechanics: d dt q i = q i (7.6) For the pendulum example discussed above,

Phys460.nb 111 So d dt d θ = θ T dt θ = d dt θ = d d t 1 m r θ θ = d d t m r θ = m r θ.. (7.7) (7.8) and θ = - V θ = m g r cos θ = -m g r sinθ θ (7.9) As a result, the EOM is m r θ.. = -m g r sin θ m r θ.. = -m g sin θ (7.10) (7.11) which is the same as the second law of Newton: m a = F (7.1) 7.1.3. Hamiltonian, canonical coordinates and canonical momenta From the Lagrangian, we can define a canonical momentum for every coordinate: p i = q i (7.13) If the system has n coordinates, we will have n canonical momenta. If the coordinates we used are real space coordinates, these momenta coincide with the momentum we usually used in Newton s theory. If the coordinates that we used here are angles, then the momenta will be angular momenta L. Hamiltonian: H = p i q i - L = T + V (7.14) H is a function of p i and q i For the pendulum example, p = θ = θ = T 1 m r θ θ = θ = m r θ (7.15) Notice that θ is just the angular velocity ω. Here, this p is in fact m r ω, i.e. the angular momentum. H = p θ - L = p θ - 1 m r θ - m g r cos θ (7.16) Because p = m r θ, we can replace all θ by p/m r p H = p m r - 1 m p p r - m g r cos θ = m r m r - p p - m g r cos θ = m r m r - m g r cos θ (7.17) This Hamiltonian is indeed a function of p and θ 7.1.4. Canonical quantization In a quantum system, all physical observable becomes quantum operators, including H, q i and p i. The relation between them remains the same as in classical mechanics. The only ingredient that we need to add here is the uncertainty relation : [q i, p j ] = i δ i, j (7.18)

11 Phys460.nb [q i, q j ] = [p i, p j ] = 0 (7.19) i.e., we request a coordinate NOT to commute with its canonical momentum. The commutator is assumed to be a constant, i for any canonical pair p i and q i. 7.1.5. Summary Step 1: starting from classical mechanics Step : define coordinates Step 3: find the canonical momenta for each coordinate Step 4: write down the Hamiltonian Step 5: require canonical commutation relation Example: for the example we considered above, we have only one coordinate and one momentum, and the Hamiltonian looks like p H = m r - m g r cos q When we quantize this system, we turn everything into quantum operators H = p - m g r cos q m r (7.0) (7.1) And we request [q, p ] = i. Q: What is a cos function of a quantum operator? A: We use Taylor expansions cos x = 1 - x + x4 4 + (7.) So cos q = 1 - q 4 + q 4 + (7.3) And thus H = p m r - m g r cos q = p m r - m g r + m g r q - m g r 4 q 4 + (7.4) We know that a constant in energy is not important, so we can drop the constant part -m g r H = p m r - m g r cos q = p m r + m g r q - m g r 4 q 4 + (7.5) The first two terms here are the Hamiltonian of a harmonic oscillator. And the rest part of the Hamiltonian is known as the non-harmonic part of the potential. 7.. Creation and annihilation operators Q: How do we handle such a quantum system? A: By defining creation and annihilation operators. 7..1. Creation and annihilation operators. Define:

Phys460.nb 113 a i = x q i - (7.6) a i = x q i + (7.7) where x is some arbitrary (positive) real number. It is easy to prove that a i and a i are conjugate of each other, a = a (7.8) and it is easy to verify that a i, a i = 1 a i a i - a i a i = a i, a i = x q i + x [qi, q i ] + i [pi, q i ] - i [qi, p i ] + 1 More generally, we can prove that a i, a j = δ ij = 1 if i = j 0 if i j, x q i - = x [pi, p i ] = - i [qi, p i ] = -i*i = 1 (7.9) (7.30) For the example that we considered above, there is only one coordinate and one momentum, q and p, and thus, we only have one creation operator and one annihilation operator a = x q - (7.31) a = x q + (7.3) 7... Vacuum For simplicity, from now on, we will only focus on the example that discussed above, but please keep in mind that all conclusions can be generalized easily to more complicated Hamiltonians. Here we make two assumptions: Assumption #1: there is one (and only one) quantum state such that a 0 = 0 (7.33) We call this state the vacuum state. Assumption #: The states 0, a 0, a a 0, a a a 0 form a complete basis of the Hilbert space. Comment: These assumptions turn out to be true for most cases that we study in quantum mechanics. 7..3. particle number operator Define particle number operator n = a a (7.34) We can easily prove that this operator is a Hermitian operator, n = n n = a a = a a = a a = n (7.35)

114 Phys460.nb So this operator has real eigenvalues (which could be a physics measurable quantity). We can further prove that n 0 = a a 0 = a (a 0 = a 0 = 0 (7.36) i.e. the vacuum state 0 is an eigenstate of n with eigenvalue 0 n a 0 = a a a 0 = a a a - a a + a a 0 = a a, a + a a 0 = a 1 + a a 0 = a 0 + a a a 0 = a 0 (7.37) The last term is 0, because a 0 = 0 by definition. In other words, we find that a 0 is also an eigenstate of n with eigenvalue 1. We can keep doing the same thing and prove that a m 0 is an eigenstate for the number operator n, and the eigenvalue is m. Bottom line #1: the eigenvalues of the operator n is a non-negative integer 0, 1,, Notice that number of particles are also nonnegative integers, so it makes sense to call this operator the particle number operator. Here, the operator n measures the number of some fictitious particles Bottom line #: a m is an eigenstate of n. 7..4. Hamiltonian: the harmonic part H = p 0 with m being 0, 1,, for a complete basis of the Hilbert space (as assumed above). Each state in this basis m r - m g r cos q = p m r + m g r Lets keep only the first two terms, and ignore all higher order terms of q H 0 = p m r + m g r q q - m g r 4 q 4 + (7.38) (7.39) The part that we ignored are δ H = - m g r 4 q 4 + (7.40) and H = H 0 + δ H For the harmonic part H 0 H 0 = p m r + m g r q (7.41) Because a = x q - (7.4) a = x q + (7.43) we know that q = x a + a (7.44) p = i a - a (7.45)

Phys460.nb 115 Thus, H 0 = p m r + m g r q = i a - a + m g r m r x a + a = - 4 m r a - a + m g r 4 x a + a (7.46) Here a - a = a - a a - a = a a - a a - a a + a a (7.47) and a + a = a + a a + a = a a + a a + a a + a a (7.48) So H 0 = - 4 x a a + a a + 4 x a a + a a (7.49) Now, we choose the value of x, such that the first term vanish - 4 x = 0 (7.50) i.e. x = m g r 3 x = m g r 3 = m r g r And thus H 0 = - 4 x = a a + a a + m g r 4 m r m r g r + g r a a + a a 4 m r g r 4 x a a + a a = 4 g r a a + a a = + g 4 r a a + a a (7.51) (7.5) (7.53) Because a, a = a a - a a = 1, a a = a a + 1 and thus H 0 = g/r a a + a a = g/r a a + a a + 1 = g/r a a + 1 = g/r a a + 1 (7.54) Notice that above g/r = ω is actually the angular frequency of the harmonic oscillator, and a a is in fact the particle number operator n we defined H 0 = ω n + 1 (7.55) We can understand this Hamiltonian as the following: (1) each of our fictitious particle has energy ω. () The system also have an zero point energy (energy of the vacuum) ω. So the total energy of the system is H 0 = ω n + 1 (7.56) Because the energy is carried by these fictitious particles, the total energy is proportional to particle number (up to the zero point energy ω/). Because particle number are quantized integers, the energy is quantized. This is the origin of quantization

116 Phys460.nb 7..5. Hamiltonian: the non-harmonic part How about the terms that we ignored? We can treat them as interactions between particles (i.e. scatterings). The bottom line: (1) for a harmonic oscillator, we can treat it as non-interacting particles (each has energy ω) () for non-harmonic terms, we can treat term as interactions between these particles 7..6. How about waves? For a harmonic oscillator, we know that we can think about it using these fictitious particles. This fictitious particles cannot move (they are confined spatially at the oscillator). This is a bit different from a real particle, which can move in space. How can we have a real particle? Using waves, instead of a single oscillator. Waves is nothing but couple harmonic oscillators (we put a harmonic oscillator at each position x, and couple them together). For each position x, we have one harmonic oscillator, and thus we can define a creation operator at this point a (x) and also an annihilation operator a(x) at this point. We can also ask what is the particle number for each oscillator n (x) = a (x) a(x) The coupling between harmonic oscillators allows the particle at x to move to y (i.e. motion of a particle). Non-harmonic parts gives interactions between this particles. This is the foundation of particle wave duality.