Module I, Lecture 05: Quantum Mechanical Theory of Spin Ψ Ψ
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Path Integrals in Quantum Mechanics
Path Integrals in Quantum Mechanics Dennis V. Perepelitsa MIT Department of Physics 70 Amherst Ave. Cambridge, MA 02142 Abstract We present the path integral formulation of quantum mechanics and demon- strate its equivalence to the Schr¨odinger picture. We apply the method to the free particle and quantum harmonic oscillator, investigate the Euclidean path integral, and discuss other applications. 1 Introduction A fundamental question in quantum mechanics is how does the state of a particle evolve with time? That is, the determination the time-evolution ψ(t) of some initial | i state ψ(t ) . Quantum mechanics is fully predictive [3] in the sense that initial | 0 i conditions and knowledge of the potential occupied by the particle is enough to fully specify the state of the particle for all future times.1 In the early twentieth century, Erwin Schr¨odinger derived an equation specifies how the instantaneous change in the wavefunction d ψ(t) depends on the system dt | i inhabited by the state in the form of the Hamiltonian. In this formulation, the eigenstates of the Hamiltonian play an important role, since their time-evolution is easy to calculate (i.e. they are stationary). A well-established method of solution, after the entire eigenspectrum of Hˆ is known, is to decompose the initial state into this eigenbasis, apply time evolution to each and then reassemble the eigenstates. That is, 1In the analysis below, we consider only the position of a particle, and not any other quantum property such as spin. 2 D.V. Perepelitsa n=∞ ψ(t) = exp [ iE t/~] n ψ(t ) n (1) | i − n h | 0 i| i n=0 X This (Hamiltonian) formulation works in many cases. -
Quantum Field Theory*
Quantum Field Theory y Frank Wilczek Institute for Advanced Study, School of Natural Science, Olden Lane, Princeton, NJ 08540 I discuss the general principles underlying quantum eld theory, and attempt to identify its most profound consequences. The deep est of these consequences result from the in nite number of degrees of freedom invoked to implement lo cality.Imention a few of its most striking successes, b oth achieved and prosp ective. Possible limitation s of quantum eld theory are viewed in the light of its history. I. SURVEY Quantum eld theory is the framework in which the regnant theories of the electroweak and strong interactions, which together form the Standard Mo del, are formulated. Quantum electro dynamics (QED), b esides providing a com- plete foundation for atomic physics and chemistry, has supp orted calculations of physical quantities with unparalleled precision. The exp erimentally measured value of the magnetic dip ole moment of the muon, 11 (g 2) = 233 184 600 (1680) 10 ; (1) exp: for example, should b e compared with the theoretical prediction 11 (g 2) = 233 183 478 (308) 10 : (2) theor: In quantum chromo dynamics (QCD) we cannot, for the forseeable future, aspire to to comparable accuracy.Yet QCD provides di erent, and at least equally impressive, evidence for the validity of the basic principles of quantum eld theory. Indeed, b ecause in QCD the interactions are stronger, QCD manifests a wider variety of phenomena characteristic of quantum eld theory. These include esp ecially running of the e ective coupling with distance or energy scale and the phenomenon of con nement. -
5 the Dirac Equation and Spinors
5 The Dirac Equation and Spinors In this section we develop the appropriate wavefunctions for fundamental fermions and bosons. 5.1 Notation Review The three dimension differential operator is : ∂ ∂ ∂ = , , (5.1) ∂x ∂y ∂z We can generalise this to four dimensions ∂µ: 1 ∂ ∂ ∂ ∂ ∂ = , , , (5.2) µ c ∂t ∂x ∂y ∂z 5.2 The Schr¨odinger Equation First consider a classical non-relativistic particle of mass m in a potential U. The energy-momentum relationship is: p2 E = + U (5.3) 2m we can substitute the differential operators: ∂ Eˆ i pˆ i (5.4) → ∂t →− to obtain the non-relativistic Schr¨odinger Equation (with = 1): ∂ψ 1 i = 2 + U ψ (5.5) ∂t −2m For U = 0, the free particle solutions are: iEt ψ(x, t) e− ψ(x) (5.6) ∝ and the probability density ρ and current j are given by: 2 i ρ = ψ(x) j = ψ∗ ψ ψ ψ∗ (5.7) | | −2m − with conservation of probability giving the continuity equation: ∂ρ + j =0, (5.8) ∂t · Or in Covariant notation: µ µ ∂µj = 0 with j =(ρ,j) (5.9) The Schr¨odinger equation is 1st order in ∂/∂t but second order in ∂/∂x. However, as we are going to be dealing with relativistic particles, space and time should be treated equally. 25 5.3 The Klein-Gordon Equation For a relativistic particle the energy-momentum relationship is: p p = p pµ = E2 p 2 = m2 (5.10) · µ − | | Substituting the equation (5.4), leads to the relativistic Klein-Gordon equation: ∂2 + 2 ψ = m2ψ (5.11) −∂t2 The free particle solutions are plane waves: ip x i(Et p x) ψ e− · = e− − · (5.12) ∝ The Klein-Gordon equation successfully describes spin 0 particles in relativistic quan- tum field theory. -
The Critical Casimir Effect in Model Physical Systems
University of California Los Angeles The Critical Casimir Effect in Model Physical Systems A dissertation submitted in partial satisfaction of the requirements for the degree Doctor of Philosophy in Physics by Jonathan Ariel Bergknoff 2012 ⃝c Copyright by Jonathan Ariel Bergknoff 2012 Abstract of the Dissertation The Critical Casimir Effect in Model Physical Systems by Jonathan Ariel Bergknoff Doctor of Philosophy in Physics University of California, Los Angeles, 2012 Professor Joseph Rudnick, Chair The Casimir effect is an interaction between the boundaries of a finite system when fluctua- tions in that system correlate on length scales comparable to the system size. In particular, the critical Casimir effect is that which arises from the long-ranged thermal fluctuation of the order parameter in a system near criticality. Recent experiments on the Casimir force in binary liquids near critical points and 4He near the superfluid transition have redoubled theoretical interest in the topic. It is an unfortunate fact that exact models of the experi- mental systems are mathematically intractable in general. However, there is often insight to be gained by studying approximations and toy models, or doing numerical computations. In this work, we present a brief motivation and overview of the field, followed by explications of the O(2) model with twisted boundary conditions and the O(n ! 1) model with free boundary conditions. New results, both analytical and numerical, are presented. ii The dissertation of Jonathan Ariel Bergknoff is approved. Giovanni Zocchi Alex Levine Lincoln Chayes Joseph Rudnick, Committee Chair University of California, Los Angeles 2012 iii To my parents, Hugh and Esther Bergknoff iv Table of Contents 1 Introduction :::::::::::::::::::::::::::::::::::::: 1 1.1 The Casimir Effect . -
Kinematic Relativity of Quantum Mechanics: Free Particle with Different Boundary Conditions
Journal of Applied Mathematics and Physics, 2017, 5, 853-861 http://www.scirp.org/journal/jamp ISSN Online: 2327-4379 ISSN Print: 2327-4352 Kinematic Relativity of Quantum Mechanics: Free Particle with Different Boundary Conditions Gintautas P. Kamuntavičius 1, G. Kamuntavičius 2 1Department of Physics, Vytautas Magnus University, Kaunas, Lithuania 2Christ’s College, University of Cambridge, Cambridge, UK How to cite this paper: Kamuntavičius, Abstract G.P. and Kamuntavičius, G. (2017) Kinema- tic Relativity of Quantum Mechanics: Free An investigation of origins of the quantum mechanical momentum operator Particle with Different Boundary Condi- has shown that it corresponds to the nonrelativistic momentum of classical tions. Journal of Applied Mathematics and special relativity theory rather than the relativistic one, as has been uncondi- Physics, 5, 853-861. https://doi.org/10.4236/jamp.2017.54075 tionally believed in traditional relativistic quantum mechanics until now. Taking this correspondence into account, relativistic momentum and energy Received: March 16, 2017 operators are defined. Schrödinger equations with relativistic kinematics are Accepted: April 27, 2017 introduced and investigated for a free particle and a particle trapped in the Published: April 30, 2017 deep potential well. Copyright © 2017 by authors and Scientific Research Publishing Inc. Keywords This work is licensed under the Creative Commons Attribution International Special Relativity, Quantum Mechanics, Relativistic Wave Equations, License (CC BY 4.0). Solutions -
Relativistic Quantum Mechanics 1
Relativistic Quantum Mechanics 1 The aim of this chapter is to introduce a relativistic formalism which can be used to describe particles and their interactions. The emphasis 1.1 SpecialRelativity 1 is given to those elements of the formalism which can be carried on 1.2 One-particle states 7 to Relativistic Quantum Fields (RQF), which underpins the theoretical 1.3 The Klein–Gordon equation 9 framework of high energy particle physics. We begin with a brief summary of special relativity, concentrating on 1.4 The Diracequation 14 4-vectors and spinors. One-particle states and their Lorentz transforma- 1.5 Gaugesymmetry 30 tions follow, leading to the Klein–Gordon and the Dirac equations for Chaptersummary 36 probability amplitudes; i.e. Relativistic Quantum Mechanics (RQM). Readers who want to get to RQM quickly, without studying its foun- dation in special relativity can skip the first sections and start reading from the section 1.3. Intrinsic problems of RQM are discussed and a region of applicability of RQM is defined. Free particle wave functions are constructed and particle interactions are described using their probability currents. A gauge symmetry is introduced to derive a particle interaction with a classical gauge field. 1.1 Special Relativity Einstein’s special relativity is a necessary and fundamental part of any Albert Einstein 1879 - 1955 formalism of particle physics. We begin with its brief summary. For a full account, refer to specialized books, for example (1) or (2). The- ory oriented students with good mathematical background might want to consult books on groups and their representations, for example (3), followed by introductory books on RQM/RQF, for example (4). -
A Peek Into Spin Physics
A Peek into Spin Physics Dustin Keller University of Virginia Colloquium at Kent State Physics Outline ● What is Spin Physics ● How Do we Use It ● An Example Physics ● Instrumentation What is Spin Physics The Physics of exploiting spin - Spin in nuclear reactions - Nucleon helicity structure - 3D Structure of nucleons - Fundamental symmetries - Spin probes in beyond SM - Polarized Beams and Targets,... What is Spin Physics What is Spin Physics ● The Physics of exploiting spin : By using Polarized Observables Spin: The intrinsic form of angular momentum carried by elementary particles, composite particles, and atomic nuclei. The Spin quantum number is one of two types of angular momentum in quantum mechanics, the other being orbital angular momentum. What is Spin Physics What Quantum Numbers? What is Spin Physics What Quantum Numbers? Internal or intrinsic quantum properties of particles, which can be used to uniquely characterize What is Spin Physics What Quantum Numbers? Internal or intrinsic quantum properties of particles, which can be used to uniquely characterize These numbers describe values of conserved quantities in the dynamics of a quantum system What is Spin Physics But a particle is not a sphere and spin is solely a quantum-mechanical phenomena What is Spin Physics Stern-Gerlach: If spin had continuous values like the classical picture we would see it What is Spin Physics Stern-Gerlach: Instead we see spin has only two values in the field with opposite directions: or spin-up and spin-down What is Spin Physics W. Pauli (1925) -
1. Dirac Equation for Spin ½ Particles 2
Advanced Particle Physics: III. QED III. QED for “pedestrians” 1. Dirac equation for spin ½ particles 2. Quantum-Electrodynamics and Feynman rules 3. Fermion-fermion scattering 4. Higher orders Literature: F. Halzen, A.D. Martin, “Quarks and Leptons” O. Nachtmann, “Elementarteilchenphysik” 1. Dirac Equation for spin ½ particles ∂ Idea: Linear ansatz to obtain E → i a relativistic wave equation w/ “ E = p + m ” ∂t r linear time derivatives (remove pr = −i ∇ negative energy solutions). Eψ = (αr ⋅ pr + β ⋅ m)ψ ∂ ⎛ ∂ ∂ ∂ ⎞ ⎜ ⎟ i ψ = −i⎜α1 ψ +α2 ψ +α3 ψ ⎟ + β mψ ∂t ⎝ ∂x1 ∂x2 ∂x3 ⎠ Solutions should also satisfy the relativistic energy momentum relation: E 2ψ = (pr 2 + m2 )ψ (Klein-Gordon Eq.) U. Uwer 1 Advanced Particle Physics: III. QED This is only the case if coefficients fulfill the relations: αiα j + α jαi = 2δij αi β + βα j = 0 β 2 = 1 Cannot be satisfied by scalar coefficients: Dirac proposed αi and β being 4×4 matrices working on 4 dim. vectors: ⎛ 0 σ ⎞ ⎛ 1 0 ⎞ σ are Pauli α = ⎜ i ⎟ and β = ⎜ ⎟ i 4×4 martices: i ⎜ ⎟ ⎜ ⎟ matrices ⎝σ i 0 ⎠ ⎝0 − 1⎠ ⎛ψ ⎞ ⎜ 1 ⎟ ⎜ψ ⎟ ψ = 2 ⎜ψ ⎟ ⎜ 3 ⎟ ⎜ ⎟ ⎝ψ 4 ⎠ ⎛ ∂ r ⎞ i⎜ β ψ + βαr ⋅ ∇ψ ⎟ − m ⋅1⋅ψ = 0 ⎝ ∂t ⎠ ⎛ 0 ∂ r ⎞ i⎜γ ψ + γr ⋅ ∇ψ ⎟ − m ⋅1⋅ψ = 0 ⎝ ∂t ⎠ 0 i where γ = β and γ = βα i , i = 1,2,3 Dirac Equation: µ i γ ∂µψ − mψ = 0 ⎛ψ ⎞ ⎜ 1 ⎟ ⎜ψ 2 ⎟ Solutions ψ describe spin ½ (anti) particles: ψ = ⎜ψ ⎟ ⎜ 3 ⎟ ⎜ ⎟ ⎝ψ 4 ⎠ Extremely 4 ⎛ µ ∂ ⎞ compressed j = 1...4 : ∑ ⎜∑ i ⋅ (γ ) jk µ − mδ jk ⎟ψ k description k =1⎝ µ ∂x ⎠ U. -
Class 2: Operators, Stationary States
Class 2: Operators, stationary states Operators In quantum mechanics much use is made of the concept of operators. The operator associated with position is the position vector r. As shown earlier the momentum operator is −iℏ ∇ . The operators operate on the wave function. The kinetic energy operator, T, is related to the momentum operator in the same way that kinetic energy and momentum are related in classical physics: p⋅ p (−iℏ ∇⋅−) ( i ℏ ∇ ) −ℏ2 ∇ 2 T = = = . (2.1) 2m 2 m 2 m The potential energy operator is V(r). In many classical systems, the Hamiltonian of the system is equal to the mechanical energy of the system. In the quantum analog of such systems, the mechanical energy operator is called the Hamiltonian operator, H, and for a single particle ℏ2 HTV= + =− ∇+2 V . (2.2) 2m The Schrödinger equation is then compactly written as ∂Ψ iℏ = H Ψ , (2.3) ∂t and has the formal solution iHt Ψ()r,t = exp − Ψ () r ,0. (2.4) ℏ Note that the order of performing operations is important. For example, consider the operators p⋅ r and r⋅ p . Applying the first to a wave function, we have (pr⋅) Ψ=−∇⋅iℏ( r Ψ=−) i ℏ( ∇⋅ rr) Ψ− i ℏ( ⋅∇Ψ=−) 3 i ℏ Ψ+( rp ⋅) Ψ (2.5) We see that the operators are not the same. Because the result depends on the order of performing the operations, the operator r and p are said to not commute. In general, the expectation value of an operator Q is Q=∫ Ψ∗ (r, tQ) Ψ ( r , td) 3 r . -
Question 1: Kinetic Energy Operator in 3D in This Exercise We Derive 2 2 ¯H ¯H 1 ∂2 Lˆ2 − ∇2 = − R +
ExercisesQuantumDynamics,week4 May22,2014 Question 1: Kinetic energy operator in 3D In this exercise we derive 2 2 ¯h ¯h 1 ∂2 lˆ2 − ∇2 = − r + . (1) 2µ 2µ r ∂r2 2µr2 The angular momentum operator is defined by ˆl = r × pˆ, (2) where the linear momentum operator is pˆ = −i¯h∇. (3) The first step is to work out the lˆ2 operator and to show that 2 2 ˆl2 = −¯h (r × ∇) · (r × ∇)=¯h [−r2∇2 + r · ∇ + (r · ∇)2]. (4) A convenient way to work with cross products, a = b × c, (5) is to write the components using the Levi-Civita tensor ǫijk, 3 3 ai = ǫijkbjck ≡ X X ǫijkbjck, (6) j=1 k=1 where we introduced the Einstein summation convention: whenever an index appears twice one assumes there is a sum over this index. 1a. Write the cross product in components and show that ǫ1,2,3 = ǫ2,3,1 = ǫ3,1,2 =1, (7) ǫ3,2,1 = ǫ2,1,3 = ǫ1,3,2 = −1, (8) and all other component of the tensor are zero. Note: the tensor is +1 for ǫ1,2,3, it changes sign whenever two indices are permuted, and as a result it is zero whenever two indices are equal. 1b. Check this relation ǫijkǫij′k′ = δjj′ δkk′ − δjk′ δj′k. (9) (Remember the implicit summation over index i). 1c. Use Eq. (9) to derive Eq. (4). 1d. Show that ∂ r = r · ∇ (10) ∂r 1e. Show that 1 ∂2 ∂2 2 ∂ r = + (11) r ∂r2 ∂r2 r ∂r 1f. Combine the results to derive Eq. -
2 Quantum Theory of Spin Waves
2 Quantum Theory of Spin Waves In Chapter 1, we discussed the angular momenta and magnetic moments of individual atoms and ions. When these atoms or ions are constituents of a solid, it is important to take into consideration the ways in which the angular momenta on different sites interact with one another. For simplicity, we will restrict our attention to the case when the angular momentum on each site is entirely due to spin. The elementary excitations of coupled spin systems in solids are called spin waves. In this chapter, we will introduce the quantum theory of these excita- tions at low temperatures. The two primary interaction mechanisms for spins are magnetic dipole–dipole coupling and a mechanism of quantum mechanical origin referred to as the exchange interaction. The dipolar interactions are of importance when the spin wavelength is very long compared to the spacing between spins, and the exchange interaction dominates when the spacing be- tween spins becomes significant on the scale of a wavelength. In this chapter, we focus on exchange-dominated spin waves, while dipolar spin waves are the primary topic of subsequent chapters. We begin this chapter with a quantum mechanical treatment of a sin- gle electron in a uniform field and follow it with the derivations of Zeeman energy and Larmor precession. We then consider one of the simplest exchange- coupled spin systems, molecular hydrogen. Exchange plays a crucial role in the existence of ordered spin systems. The ground state of H2 is a two-electron exchange-coupled system in an embryonic antiferromagnetic state. -
Quantum Physics (UCSD Physics 130)
Quantum Physics (UCSD Physics 130) April 2, 2003 2 Contents 1 Course Summary 17 1.1 Problems with Classical Physics . .... 17 1.2 ThoughtExperimentsonDiffraction . ..... 17 1.3 Probability Amplitudes . 17 1.4 WavePacketsandUncertainty . ..... 18 1.5 Operators........................................ .. 19 1.6 ExpectationValues .................................. .. 19 1.7 Commutators ...................................... 20 1.8 TheSchr¨odingerEquation .. .. .. .. .. .. .. .. .. .. .. .. .... 20 1.9 Eigenfunctions, Eigenvalues and Vector Spaces . ......... 20 1.10 AParticleinaBox .................................... 22 1.11 Piecewise Constant Potentials in One Dimension . ...... 22 1.12 The Harmonic Oscillator in One Dimension . ... 24 1.13 Delta Function Potentials in One Dimension . .... 24 1.14 Harmonic Oscillator Solution with Operators . ...... 25 1.15 MoreFunwithOperators. .. .. .. .. .. .. .. .. .. .. .. .. .... 26 1.16 Two Particles in 3 Dimensions . .. 27 1.17 IdenticalParticles ................................. .... 28 1.18 Some 3D Problems Separable in Cartesian Coordinates . ........ 28 1.19 AngularMomentum.................................. .. 29 1.20 Solutions to the Radial Equation for Constant Potentials . .......... 30 1.21 Hydrogen........................................ .. 30 1.22 Solution of the 3D HO Problem in Spherical Coordinates . ....... 31 1.23 Matrix Representation of Operators and States . ........... 31 1.24 A Study of ℓ =1OperatorsandEigenfunctions . 32 1.25 Spin1/2andother2StateSystems . ...... 33 1.26 Quantum