A New Application of the Modal-Hamiltonian Interpretation of Quantum Mechanics: the Problem of Optical Isomerism
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Unit 1 Old Quantum Theory
UNIT 1 OLD QUANTUM THEORY Structure Introduction Objectives li;,:overy of Sub-atomic Particles Earlier Atom Models Light as clectromagnetic Wave Failures of Classical Physics Black Body Radiation '1 Heat Capacity Variation Photoelectric Effect Atomic Spectra Planck's Quantum Theory, Black Body ~diation. and Heat Capacity Variation Einstein's Theory of Photoelectric Effect Bohr Atom Model Calculation of Radius of Orbits Energy of an Electron in an Orbit Atomic Spectra and Bohr's Theory Critical Analysis of Bohr's Theory Refinements in the Atomic Spectra The61-y Summary Terminal Questions Answers 1.1 INTRODUCTION The ideas of classical mechanics developed by Galileo, Kepler and Newton, when applied to atomic and molecular systems were found to be inadequate. Need was felt for a theory to describe, correlate and predict the behaviour of the sub-atomic particles. The quantum theory, proposed by Max Planck and applied by Einstein and Bohr to explain different aspects of behaviour of matter, is an important milestone in the formulation of the modern concept of atom. In this unit, we will study how black body radiation, heat capacity variation, photoelectric effect and atomic spectra of hydrogen can be explained on the basis of theories proposed by Max Planck, Einstein and Bohr. They based their theories on the postulate that all interactions between matter and radiation occur in terms of definite packets of energy, known as quanta. Their ideas, when extended further, led to the evolution of wave mechanics, which shows the dual nature of matter -
Arxiv:Quant-Ph/0105127V3 19 Jun 2003
DECOHERENCE, EINSELECTION, AND THE QUANTUM ORIGINS OF THE CLASSICAL Wojciech Hubert Zurek Theory Division, LANL, Mail Stop B288 Los Alamos, New Mexico 87545 Decoherence is caused by the interaction with the en- A. The problem: Hilbert space is big 2 vironment which in effect monitors certain observables 1. Copenhagen Interpretation 2 of the system, destroying coherence between the pointer 2. Many Worlds Interpretation 3 B. Decoherence and einselection 3 states corresponding to their eigenvalues. This leads C. The nature of the resolution and the role of envariance4 to environment-induced superselection or einselection, a quantum process associated with selective loss of infor- D. Existential Interpretation and ‘Quantum Darwinism’4 mation. Einselected pointer states are stable. They can retain correlations with the rest of the Universe in spite II. QUANTUM MEASUREMENTS 5 of the environment. Einselection enforces classicality by A. Quantum conditional dynamics 5 imposing an effective ban on the vast majority of the 1. Controlled not and a bit-by-bit measurement 6 Hilbert space, eliminating especially the flagrantly non- 2. Measurements and controlled shifts. 7 local “Schr¨odinger cat” states. Classical structure of 3. Amplification 7 B. Information transfer in measurements 9 phase space emerges from the quantum Hilbert space in 1. Action per bit 9 the appropriate macroscopic limit: Combination of einse- C. “Collapse” analogue in a classical measurement 9 lection with dynamics leads to the idealizations of a point and of a classical trajectory. In measurements, einselec- III. CHAOS AND LOSS OF CORRESPONDENCE 11 tion replaces quantum entanglement between the appa- A. Loss of the quantum-classical correspondence 11 B. -
Quantum Theory of the Hydrogen Atom
Quantum Theory of the Hydrogen Atom Chemistry 35 Fall 2000 Balmer and the Hydrogen Spectrum n 1885: Johann Balmer, a Swiss schoolteacher, empirically deduced a formula which predicted the wavelengths of emission for Hydrogen: l (in Å) = 3645.6 x n2 for n = 3, 4, 5, 6 n2 -4 •Predicts the wavelengths of the 4 visible emission lines from Hydrogen (which are called the Balmer Series) •Implies that there is some underlying order in the atom that results in this deceptively simple equation. 2 1 The Bohr Atom n 1913: Niels Bohr uses quantum theory to explain the origin of the line spectrum of hydrogen 1. The electron in a hydrogen atom can exist only in discrete orbits 2. The orbits are circular paths about the nucleus at varying radii 3. Each orbit corresponds to a particular energy 4. Orbit energies increase with increasing radii 5. The lowest energy orbit is called the ground state 6. After absorbing energy, the e- jumps to a higher energy orbit (an excited state) 7. When the e- drops down to a lower energy orbit, the energy lost can be given off as a quantum of light 8. The energy of the photon emitted is equal to the difference in energies of the two orbits involved 3 Mohr Bohr n Mathematically, Bohr equated the two forces acting on the orbiting electron: coulombic attraction = centrifugal accelleration 2 2 2 -(Z/4peo)(e /r ) = m(v /r) n Rearranging and making the wild assumption: mvr = n(h/2p) n e- angular momentum can only have certain quantified values in whole multiples of h/2p 4 2 Hydrogen Energy Levels n Based on this model, Bohr arrived at a simple equation to calculate the electron energy levels in hydrogen: 2 En = -RH(1/n ) for n = 1, 2, 3, 4, . -
Vibrational Quantum Number
Fundamentals in Biophotonics Quantum nature of atoms, molecules – matter Aleksandra Radenovic [email protected] EPFL – Ecole Polytechnique Federale de Lausanne Bioengineering Institute IBI 26. 03. 2018. Quantum numbers •The four quantum numbers-are discrete sets of integers or half- integers. –n: Principal quantum number-The first describes the electron shell, or energy level, of an atom –ℓ : Orbital angular momentum quantum number-as the angular quantum number or orbital quantum number) describes the subshell, and gives the magnitude of the orbital angular momentum through the relation Ll2 ( 1) –mℓ:Magnetic (azimuthal) quantum number (refers, to the direction of the angular momentum vector. The magnetic quantum number m does not affect the electron's energy, but it does affect the probability cloud)- magnetic quantum number determines the energy shift of an atomic orbital due to an external magnetic field-Zeeman effect -s spin- intrinsic angular momentum Spin "up" and "down" allows two electrons for each set of spatial quantum numbers. The restrictions for the quantum numbers: – n = 1, 2, 3, 4, . – ℓ = 0, 1, 2, 3, . , n − 1 – mℓ = − ℓ, − ℓ + 1, . , 0, 1, . , ℓ − 1, ℓ – –Equivalently: n > 0 The energy levels are: ℓ < n |m | ≤ ℓ ℓ E E 0 n n2 Stern-Gerlach experiment If the particles were classical spinning objects, one would expect the distribution of their spin angular momentum vectors to be random and continuous. Each particle would be deflected by a different amount, producing some density distribution on the detector screen. Instead, the particles passing through the Stern–Gerlach apparatus are deflected either up or down by a specific amount. -
Lecture 3: Particle in a 1D Box
Lecture 3: Particle in a 1D Box First we will consider a free particle moving in 1D so V (x) = 0. The TDSE now reads ~2 d2ψ(x) = Eψ(x) −2m dx2 which is solved by the function ψ = Aeikx where √2mE k = ± ~ A general solution of this equation is ψ(x) = Aeikx + Be−ikx where A and B are arbitrary constants. It can also be written in terms of sines and cosines as ψ(x) = C sin(kx) + D cos(kx) The constants appearing in the solution are determined by the boundary conditions. For a free particle that can be anywhere, there is no boundary conditions, so k and thus E = ~2k2/2m can take any values. The solution of the form eikx corresponds to a wave travelling in the +x direction and similarly e−ikx corresponds to a wave travelling in the -x direction. These are eigenfunctions of the momentum operator. Since the particle is free, it is equally likely to be anywhere so ψ∗(x)ψ(x) is independent of x. Incidently, it cannot be normalized because the particle can be found anywhere with equal probability. 1 Now, let us confine the particle to a region between x = 0 and x = L. To do this, we choose our interaction potential V (x) as follows V (x) = 0 for 0 x L ≤ ≤ = otherwise ∞ It is always a good idea to plot the potential energy, when it is a function of a single variable, as shown in Fig.1. The TISE is now given by V(x) V=infinity V=0 V=infinity x 0 L ~2 d2ψ(x) + V (x)ψ(x) = Eψ(x) −2m dx2 First consider the region outside the box where V (x) = . -
The Quantum Mechanical Model of the Atom
The Quantum Mechanical Model of the Atom Quantum Numbers In order to describe the probable location of electrons, they are assigned four numbers called quantum numbers. The quantum numbers of an electron are kind of like the electron’s “address”. No two electrons can be described by the exact same four quantum numbers. This is called The Pauli Exclusion Principle. • Principle quantum number: The principle quantum number describes which orbit the electron is in and therefore how much energy the electron has. - it is symbolized by the letter n. - positive whole numbers are assigned (not including 0): n=1, n=2, n=3 , etc - the higher the number, the further the orbit from the nucleus - the higher the number, the more energy the electron has (this is sort of like Bohr’s energy levels) - the orbits (energy levels) are also called shells • Angular momentum (azimuthal) quantum number: The azimuthal quantum number describes the sublevels (subshells) that occur in each of the levels (shells) described above. - it is symbolized by the letter l - positive whole number values including 0 are assigned: l = 0, l = 1, l = 2, etc. - each number represents the shape of a subshell: l = 0, represents an s subshell l = 1, represents a p subshell l = 2, represents a d subshell l = 3, represents an f subshell - the higher the number, the more complex the shape of the subshell. The picture below shows the shape of the s and p subshells: (notice the electron clouds) • Magnetic quantum number: All of the subshells described above (except s) have more than one orientation. -
Chapter 4 Introduction to Molecular QM
Chapter 4 Introduction to Molecular QM Contents 4.1 Born-Oppenheimer approximation ....................76 4.2 Molecular orbitals .................................. ..77 + 4.3 Hydrogen molecular ion H2 ..........................78 4.4 The structures of diatomic molecules ..................83 Basic Questions A. What is Born-Oppenheimer approximation? B. What are molecular orbitals? C. Is He2 a stable molecule? 75 76 CHAPTER 4. INTRODUCTION TO MOLECULAR QM 4.1 Born-Oppenheimer approximation and electron terms Consider a general many-body Hamiltonian of a molecule Hˆ = Hˆe + Hˆn + Hˆen, where Hˆe is the Hamiltonian of many-electrons in the molecule, Hˆn is that of nuclei, and Hˆen describes the interaction potential between the two subsystems. As nuclear mass is much larger (about 2000 times larger) than electron mass, it is a good ap- proximation to ignore nuclear’s motion and focus on the dynamics of electrons for given nuclear configuration. We use general coordinate x =(x1, x2, ...) for all electrons (spatial and spin coor- dinates) and X = (X1,X2, ...) for all nuclei’s. The total wavefunction of a molecule is separatable as Ψ(x, X)=Ψe(x, X)Ψn(X) . If we approximate HˆnΨe(x, X) Ψe(x, X)Hˆn (the noncommuting kinetic part is proportional to 1/M , where M ≈is nuclear mass), we have separatable Schr¨odinger equations, namely (Hˆe + Hˆen)Ψe(x, X)= EΨe(x, X), E = E(X) for electrons motion with nuclei’s coordinates X as parameters, and [Hˆn + E(X)]Ψn(X)= EnΨn(X) for the nuclei motion. This is called Born-Oppenheimer approximation. Notice that E = E(X) plays a role of potential in the nuclei Schr¨odinger equation. -
Chapter 10 Theories of Electronic Molecular Structure
Chapter 10 Theories of Electronic Molecular Structure Solving the Schrödinger equation for a molecule first requires specifying the Hamiltonian and then finding the wavefunctions that satisfy the equation. The wavefunctions involve the coordinates of all the nuclei and electrons that comprise the molecule. The complete molecular Hamiltonian consists of several terms. The nuclear and electronic kinetic energy operators account for the motion of all of the nuclei and electrons. The Coulomb potential energy terms account for the interactions between the nuclei, the electrons, and the nuclei and electrons. Other terms account for the interactions between all the magnetic dipole moments and the interactions with any external electric or magnetic fields. The charge distribution of an atomic nucleus is not always spherical and, when appropriate, this asymmetry must be taken into account as well as the relativistic effect that a moving electron experiences as a change in mass. This complete Hamiltonian is too complicated and is not needed for many situations. In practice, only the terms that are essential for the purpose at hand are included. Consequently in the absence of external fields, interest in spin- spin and spin-orbit interactions, and in electron and nuclear magnetic resonance spectroscopy (ESR and NMR), the molecular Hamiltonian usually is considered to consist only of the kinetic and potential energy terms, and the Born- Oppenheimer approximation is made in order to separate the nuclear and electronic motion. In general, electronic wavefunctions for molecules are constructed from approximate one-electron wavefunctions. These one-electron functions are called molecular orbitals. The expectation value expression for the energy is used to optimize these functions, i.e. -
Einselection Without Pointer States
Einselection without pointer states Einselection without pointer states - Decoherence under weak interaction Christian Gogolin Universit¨atW¨urzburg 2009-12-16 C. Gogolin j Universit¨atW¨urzburg j 2009-12-16 1 / 26 Einselection without pointer states j Introduction New foundation for Statistical Mechanics X Thermodynamics X Statistical Mechanics Second Law ergodicity equal a priory probabilities Classical Mechanics [2, 3] C. Gogolin j Universit¨atW¨urzburg j 2009-12-16 2 / 26 Einselection without pointer states j Introduction New foundation for Statistical Mechanics X Thermodynamics X Statistical Mechanics Second Law ergodicity ? equal a priory probabilities Classical Mechanics ? [2, 3] C. Gogolin j Universit¨atW¨urzburg j 2009-12-16 2 / 26 Einselection without pointer states j Introduction New foundation for Statistical Mechanics X Thermodynamics X Statistical Mechanics [2, 3] C. Gogolin j Universit¨atW¨urzburg j 2009-12-16 2 / 26 Einselection without pointer states j Introduction New foundation for Statistical Mechanics X Thermodynamics X Statistical Mechanics * Quantum Mechanics X [2, 3] C. Gogolin j Universit¨atW¨urzburg j 2009-12-16 2 / 26 quantum mechanical orbitals discrete energy levels coherent superpositions hopping Einselection without pointer states j Introduction Why do electrons hop between energy eigenstates? C. Gogolin j Universit¨atW¨urzburg j 2009-12-16 3 / 26 discrete energy levels hopping Einselection without pointer states j Introduction Why do electrons hop between energy eigenstates? quantum mechanical orbitals coherent superpositions C. Gogolin j Universit¨atW¨urzburg j 2009-12-16 3 / 26 Einselection without pointer states j Introduction Why do electrons hop between energy eigenstates? quantum mechanical orbitals discrete energy levels coherent superpositions hopping C. -
Eliminating Ground-State Dipole Moments in Quantum Optics
Eliminating ground-state dipole moments in quantum optics via canonical transformation Gediminas Juzeliunas* Luciana Dávila Romero† and David L. Andrews† *Institute of Theoretical Physics and Astronomy, Vilnius University, A. Goštauto 12, 2600 Vilnius, Lithuania †School of Chemical Sciences and Pharmacy, University of East Anglia, Norwich NR4 7TJ, United Kingdom Abstract By means of a canonical transformation it is shown how it is possible to recast the equations for molecular nonlinear optics to completely eliminate ground-state static dipole coupling terms. Such dipoles can certainly play a highly important role in nonlinear optical response – but equations derived by standard methods, in which these dipoles emerge only as special cases of transition moments, prove unnecessarily complex. It has been shown that the elimination of ground-state static dipoles in favor of dipole shifts results in a considerable simplification in form of the nonlinear optical susceptibilities. In a fully quantum theoretical treatment the validity of such a procedure has previously been verified using an expedient algorithm, whose defense was afforded only by a highly intricate proof. In this paper it is shown how a canonical transformation method entirely circumvents such an approach; it also affords new insights into the formulation of quantum field interactions. 2 1. Introduction In recent years it has become increasingly evident that permanent (static) electric dipoles play a highly important role in the nonlinear optical response of molecular systems [1, 2]. Most molecules are intrinsically polar by nature, and calculation of their optical susceptibilities with regard only to transition dipole moments can produce results that are significantly in error [3, 4]. -
A Model-Theoretic Interpretation of Environmentally-Induced
A model-theoretic interpretation of environmentally-induced superselection Chris Fields 815 East Palace # 14 Santa Fe, NM 87501 USA fi[email protected] November 28, 2018 Abstract The question of what constitutes a “system” is foundational to quantum mea- surement theory. Environmentally-induced superselection or “einselection” has been proposed as an observer-independent mechanism by which apparently classical sys- tems “emerge” from physical interactions between degrees of freedom described com- pletely quantum-mechanically. It is shown here that einselection can only generate classical systems if the “environment” is assumed a priori to be classical; einselection therefore does not provide an observer-independent mechanism by which classicality can emerge from quantum dynamics. Einselection is then reformulated in terms of positive operator-valued measures (POVMs) acting on a global quantum state. It is shown that this re-formulation enables a natural interpretation of apparently-classical systems as virtual machines that requires no assumptions beyond those of classical arXiv:1202.1019v2 [quant-ph] 13 May 2012 computer science. Keywords: Decoherence, Einselection, POVMs, Emergence, Observer, Quantum-to-classical transition 1 Introduction The concept of environmentally-induced superselection or “einselection” was introduced into quantum mechanics by W. Zurek [1, 2] as a solution to the “preferred-basis problem,” 1 the problem of selecting one from among the arbitrarily many possible sets of basis vectors spanning the Hilbert space of a system of interest. Zurek’s solution was brilliantly simple: it transferred the preferred basis problem from the observer to the environment in which the system of interest is embedded, and then solved the problem relative to the environment. -
Decoherence and the Transition from Quantum to Classical—Revisited
Decoherence and the Transition from Quantum to Classical—Revisited Wojciech H. Zurek This paper has a somewhat unusual origin and, as a consequence, an unusual structure. It is built on the principle embraced by families who outgrow their dwellings and decide to add a few rooms to their existing structures instead of start- ing from scratch. These additions usually “show,” but the whole can still be quite pleasing to the eye, combining the old and the new in a functional way. What follows is such a “remodeling” of the paper I wrote a dozen years ago for Physics Today (1991). The old text (with some modifications) is interwoven with the new text, but the additions are set off in boxes throughout this article and serve as a commentary on new developments as they relate to the original. The references appear together at the end. In 1991, the study of decoherence was still a rather new subject, but already at that time, I had developed a feeling that most implications about the system’s “immersion” in the environment had been discovered in the preceding 10 years, so a review was in order. While writing it, I had, however, come to suspect that the small gaps in the landscape of the border territory between the quantum and the classical were actually not that small after all and that they presented excellent opportunities for further advances. Indeed, I am surprised and gratified by how much the field has evolved over the last decade. The role of decoherence was recognized by a wide spectrum of practic- 86 Los Alamos Science Number 27 2002 ing physicists as well as, beyond physics proper, by material scientists and philosophers.