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Electric Dipoles in Atoms and Molecules and the Stark Effect Publicação IF – 1663/2011
Electric Dipoles in Atoms and Molecules and the Stark Effect Instituto de Física, Universidade de São Paulo, CP 66.318 05315-970, São Paulo, SP, Brasil Publicação IF – 1663/2011 21/06/2011 Electric Dipoles of Atoms and Molecules and the Stark Effect M. Cattani Instituto de Fisica, Universidade de S. Paulo, C.P. 66318, CEP 05315−970 S. Paulo, S.P. Brazil . E−mail: [email protected] Abstract. This article was written for undergraduate and postgraduate students of physics. We analyze the electric dipole moments (EDM) of atoms and molecules when they are isolated and when are placed in a uniform static electric field. This was done this because usually in text books and articles this separation is not clearly displayed. Key words: Electric dipole moments of atoms and molecules; Stark effect . (I) Introduction . Our goal is to write an article for undergraduate and postgraduate students of physics to study the electric dipole moments (EDM) of atoms and molecules when they are isolated and when they are placed in a uniform static electric field . We have done this because many times in text books and articles this separation is not clearly displayed. The dipole of an isolated system will be named natural or permanent EDM and that one which is generated by an external field will be named induced EDM. So, we begin recalling the definition of EDM adopted in basic physics courses 1−4 for an isolated aggregate of charges. If in a given system positive charges + q and negative −q are concentrated at different points we say that it has an EDM. -
Atom-Light Interaction and Basic Applications
ICTP-SAIFR school 16.-27. of September 2019 on the Interaction of Light with Cold Atoms Lecture on Atom-Light Interaction and Basic Applications Ph.W. Courteille Universidade de S~aoPaulo Instituto de F´ısicade S~aoCarlos 07/01/2021 2 . 3 . 4 Preface The following notes have been prepared for the ICTP-SAIFR school on 'Interaction of Light with Cold Atoms' held 2019 in S~aoPaulo. They are conceived to support an introductory course on 'Atom-Light Interaction and Basic Applications'. The course is divided into 5 lectures. Cold atomic clouds represent an ideal platform for studies of basic phenomena of light-matter interaction. The invention of powerful cooling and trapping techniques for atoms led to an unprecedented experimental control over all relevant degrees of freedom to a point where the interaction is dominated by weak quantum effects. This course reviews the foundations of this area of physics, emphasizing the role of light forces on the atomic motion. Collective and self-organization phenomena arising from a cooperative reaction of many atoms to incident light will be discussed. The course is meant for graduate students and requires basic knowledge of quan- tum mechanics and electromagnetism at the undergraduate level. The lectures will be complemented by exercises proposed at the end of each lecture. The present notes are mostly extracted from some textbooks (see below) and more in-depth scripts which can be consulted for further reading on the website http://www.ifsc.usp.br/∼strontium/ under the menu item 'Teaching' −! 'Cursos 2019-2' −! 'ICTP-SAIFR pre-doctoral school'. The following literature is recommended for preparation and further reading: Ph.W. -
22.51 Course Notes, Chapter 11: Perturbation Theory
11. Perturbation Theory 11.1 Time-independent perturbation theory 11.1.1 Non-degenerate case 11.1.2 Degenerate case 11.1.3 The Stark effect 11.2 Time-dependent perturbation theory 11.2.1 Review of interaction picture 11.2.2 Dyson series 11.2.3 Fermi’s Golden Rule 11.1 Time-independent perturbation theory Because of the complexity of many physical problems, very few can be solved exactly (unless they involve only small Hilbert spaces). In particular, to analyze the interaction of radiation with matter we will need to develop approximation methods36 . 11.1.1 Non-degenerate case We have an Hamiltonian = + ǫV H H0 where we know the eigenvalue of the unperturbed Hamiltonian and we want to solve for the perturbed case H0 = 0 + ǫV , in terms of an expansion in ǫ (with ǫ varying between 0 and 1). The solution for ǫ 1 is the desired Hsolution. H → We assume that we know exactly the energy eigenkets and eigenvalues of : H0 k = E(0) k H0 | ) k | ) As is hermitian, its eigenkets form a complete basis k k = 11. We assume at first that the energy spectrum H0 k | )( | is not degenerate (that is, all the E(0) are different, in the next section we will study the degenerate case). The k L eigensystem for the total hamiltonian is then ( + ǫV ) ϕ = E (ǫ) ϕ H0 | k)ǫ k | k)ǫ where ǫ = 1 is the case we are interested in, but we will solve for a general ǫ as a perturbation in this parameter: (0) (1) 2 (2) (0) (1) 2 (2) ϕ = ϕ + ǫ ϕ + ǫ ϕ + ..., E = E + ǫE + ǫ E + .. -
Taxonomy of Belarusian Educational and Research Portal of Nuclear Knowledge
Taxonomy of Belarusian Educational and Research Portal of Nuclear Knowledge S. Sytova� A. Lobko, S. Charapitsa Research Institute for Nuclear Problems, Belarusian State University Abstract The necessity and ways to create Belarusian educational and research portal of nuclear knowledge are demonstrated. Draft tax onomy of portal is presented. 1 Introduction President Dwight D. Eisenhower in December 1953 presented to the UN initiative "Atoms for Peace" on the peaceful use of nuclear technology. Today, many countries have a strong nuclear program, while other ones are in the process of its creation. Nowadays there are about 440 nuclear power plants operating in 30 countries around the world. Nuclear reac tors are used as propulsion systems for more than 400 ships. About 300 research reactors operate in 50 countries. Such reactors allow production of radioisotopes for medical diagnostics and therapy of cancer, neutron sources for research and training. Approximately 55 nuclear power plants are under construction and 110 ones are planned. Belarus now joins the club of countries that have or are building nu clear power plant. Our country has a large scientific potential in the field of atomic and nuclear physics. Hence it is obvious the necessity of cre ation of portal of nuclear knowledge. The purpose of its creation is the accumulation and development of knowledge in the nuclear field as well as popularization of nuclear knowledge for the general public. *E-mail:[email protected] 212 Wisdom, enlightenment Figure 1: Knowledge management 2 Nuclear knowledge Since beginning of the XXI century the International Atomic Energy Agen cy (IAEA) gives big attention to the nuclear knowledge management (NKM) [1]-[3] . -
Canadian-Built Laser Chills Antimatter to Near Absolute Zero for First Time Researchers Achieve World’S First Manipulation of Antimatter by Laser
UNDER EMBARGO UNTIL 8:00 AM PT ON WED MARCH 31, 2021 DO NOT DISTRIBUTE BEFORE EMBARGO LIFT Canadian-built laser chills antimatter to near absolute zero for first time Researchers achieve world’s first manipulation of antimatter by laser Vancouver, BC – Researchers with the CERN-based ALPHA collaboration have announced the world’s first laser-based manipulation of antimatter, leveraging a made-in-Canada laser system to cool a sample of antimatter down to near absolute zero. The achievement, detailed in an article published today and featured on the cover of the journal Nature, will significantly alter the landscape of antimatter research and advance the next generation of experiments. Antimatter is the otherworldly counterpart to matter; it exhibits near-identical characteristics and behaviours but has opposite charge. Because they annihilate upon contact with matter, antimatter atoms are exceptionally difficult to create and control in our world and had never before been manipulated with a laser. “Today’s results are the culmination of a years-long program of research and engineering, conducted at UBC but supported by partners from across the country,” said Takamasa Momose, the University of British Columbia (UBC) researcher with ALPHA’s Canadian team (ALPHA-Canada) who led the development of the laser. “With this technique, we can address long-standing mysteries like: ‘How does antimatter respond to gravity? Can antimatter help us understand symmetries in physics?’. These answers may fundamentally alter our understanding of our Universe.” Since its introduction 40 years ago, laser manipulation and cooling of ordinary atoms have revolutionized modern atomic physics and enabled several Nobel-winning experiments. -
Atomic Physicsphysics AAA Powerpointpowerpointpowerpoint Presentationpresentationpresentation Bybyby Paulpaulpaul E.E.E
ChapterChapter 38C38C -- AtomicAtomic PhysicsPhysics AAA PowerPointPowerPointPowerPoint PresentationPresentationPresentation bybyby PaulPaulPaul E.E.E. Tippens,Tippens,Tippens, ProfessorProfessorProfessor ofofof PhysicsPhysicsPhysics SouthernSouthernSouthern PolytechnicPolytechnicPolytechnic StateStateState UniversityUniversityUniversity © 2007 Objectives:Objectives: AfterAfter completingcompleting thisthis module,module, youyou shouldshould bebe ableable to:to: •• DiscussDiscuss thethe earlyearly modelsmodels ofof thethe atomatom leadingleading toto thethe BohrBohr theorytheory ofof thethe atom.atom. •• DemonstrateDemonstrate youryour understandingunderstanding ofof emissionemission andand absorptionabsorption spectraspectra andand predictpredict thethe wavelengthswavelengths oror frequenciesfrequencies ofof thethe BalmerBalmer,, LymanLyman,, andand PashenPashen spectralspectral series.series. •• CalculateCalculate thethe energyenergy emittedemitted oror absorbedabsorbed byby thethe hydrogenhydrogen atomatom whenwhen thethe electronelectron movesmoves toto aa higherhigher oror lowerlower energyenergy level.level. PropertiesProperties ofof AtomsAtoms ••• AtomsAtomsAtoms areareare stablestablestable andandand electricallyelectricallyelectrically neutral.neutral.neutral. ••• AtomsAtomsAtoms havehavehave chemicalchemicalchemical propertiespropertiesproperties whichwhichwhich allowallowallow themthemthem tototo combinecombinecombine withwithwith otherotherother atoms.atoms.atoms. ••• AtomsAtomsAtoms emitemitemit andandand absorbabsorbabsorb -
Manipulating Atoms with Photons
Manipulating Atoms with Photons Claude Cohen-Tannoudji and Jean Dalibard, Laboratoire Kastler Brossel¤ and Coll`ege de France, 24 rue Lhomond, 75005 Paris, France ¤Unit¶e de Recherche de l'Ecole normale sup¶erieure et de l'Universit¶e Pierre et Marie Curie, associ¶ee au CNRS. 1 Contents 1 Introduction 4 2 Manipulation of the internal state of an atom 5 2.1 Angular momentum of atoms and photons. 5 Polarization selection rules. 6 2.2 Optical pumping . 6 Magnetic resonance imaging with optical pumping. 7 2.3 Light broadening and light shifts . 8 3 Electromagnetic forces and trapping 9 3.1 Trapping of charged particles . 10 The Paul trap. 10 The Penning trap. 10 Applications. 11 3.2 Magnetic dipole force . 11 Magnetic trapping of neutral atoms. 12 3.3 Electric dipole force . 12 Permanent dipole moment: molecules. 12 Induced dipole moment: atoms. 13 Resonant dipole force. 14 Dipole traps for neutral atoms. 15 Optical lattices. 15 Atom mirrors. 15 3.4 The radiation pressure force . 16 Recoil of an atom emitting or absorbing a photon. 16 The radiation pressure in a resonant light wave. 17 Stopping an atomic beam. 17 The magneto-optical trap. 18 4 Cooling of atoms 19 4.1 Doppler cooling . 19 Limit of Doppler cooling. 20 4.2 Sisyphus cooling . 20 Limits of Sisyphus cooling. 22 4.3 Sub-recoil cooling . 22 Subrecoil cooling of free particles. 23 Sideband cooling of trapped ions. 23 Velocity scales for laser cooling. 25 2 5 Applications of ultra-cold atoms 26 5.1 Atom clocks . 26 5.2 Atom optics and interferometry . -
Qualification Exam: Quantum Mechanics
Qualification Exam: Quantum Mechanics Name: , QEID#43228029: July, 2019 Qualification Exam QEID#43228029 2 1 Undergraduate level Problem 1. 1983-Fall-QM-U-1 ID:QM-U-2 Consider two spin 1=2 particles interacting with one another and with an external uniform magnetic field B~ directed along the z-axis. The Hamiltonian is given by ~ ~ ~ ~ ~ H = −AS1 · S2 − µB(g1S1 + g2S2) · B where µB is the Bohr magneton, g1 and g2 are the g-factors, and A is a constant. 1. In the large field limit, what are the eigenvectors and eigenvalues of H in the "spin-space" { i.e. in the basis of eigenstates of S1z and S2z? 2. In the limit when jB~ j ! 0, what are the eigenvectors and eigenvalues of H in the same basis? 3. In the Intermediate regime, what are the eigenvectors and eigenvalues of H in the spin space? Show that you obtain the results of the previous two parts in the appropriate limits. Problem 2. 1983-Fall-QM-U-2 ID:QM-U-20 1. Show that, for an arbitrary normalized function j i, h jHj i > E0, where E0 is the lowest eigenvalue of H. 2. A particle of mass m moves in a potential 1 kx2; x ≤ 0 V (x) = 2 (1) +1; x < 0 Find the trial state of the lowest energy among those parameterized by σ 2 − x (x) = Axe 2σ2 : What does the first part tell you about E0? (Give your answers in terms of k, m, and ! = pk=m). Problem 3. 1983-Fall-QM-U-3 ID:QM-U-44 Consider two identical particles of spin zero, each having a mass m, that are con- strained to rotate in a plane with separation r. -
Chapter 8 Perturbation Theory, Zeeman Effect, Stark Effect
Chapter 8 Perturbation Theory, Zeeman Effect, Stark Effect Unfortunately, apart from a few simple examples, the Schr¨odingerequation is generally not exactly solvable and we therefore have to rely upon approximative methods to deal with more realistic situations. Such methods include perturbation theory, the variational method and the WKB1-approximation. In our Scriptum we, however, just cope with perturbation theory in its simplest version. It is a systematic procedure for obtaining approximate solutions to the unperturbed problem which is assumed to be known exactly. 8.1 Time{Independent Perturbation Theory The method of perturbation theory is that we deform slightly { perturb { a known Hamil- tonian H0 by a new Hamiltonian HI, some potential responsible for an interaction of the system, and try to solve the Schr¨odingerequation approximately since, in general, we will be unable to solve it exactly. Thus we start with a Hamiltonian of the following form H = H0 + λ HI where λ 2 [0; 1] ; (8.1) where the Hamiltonian H0 is perturbed by a smaller term, the interaction HI with λ small. The unperturbed Hamiltonian is assumed to be solved and has well-known eigenfunctions and eigenvalues, i.e. 0 (0) 0 H0 n = En n ; (8.2) where the eigenfunctions are chosen to be normalized 0 0 m n = δmn : (8.3) The superscript " 0 " denotes the eigenfunctions and eigenvalues of the unperturbed system H0 , and we furthermore require the unperturbed eigenvalues to be non-degenerate (0) (0) Em 6= En ; (8.4) 1, named after Wentzel, Kramers and Brillouin. 151 152CHAPTER 8. PERTURBATION THEORY, ZEEMAN EFFECT, STARK EFFECT otherwise we would use a different method leading to the so-called degenerate perturbation theory. -
22. Atomic Physics and Quantum Mechanics
22. Atomic Physics and Quantum Mechanics S. Teitel April 14, 2009 Most of what you have been learning this semester and last has been 19th century physics. Indeed, Maxwell's theory of electromagnetism, combined with Newton's laws of mechanics, seemed at that time to express virtually a complete \solution" to all known physical problems. However, already by the 1890's physicists were grappling with certain experimental observations that did not seem to fit these existing theories. To explain these puzzling phenomena, the early part of the 20th century witnessed revolutionary new ideas that changed forever our notions about the physical nature of matter and the theories needed to explain how matter behaves. In this lecture we hope to give the briefest introduction to some of these ideas. 1 Photons You have already heard in lecture 20 about the photoelectric effect, in which light shining on the surface of a metal results in the emission of electrons from that surface. To explain the observed energies of these emitted elec- trons, Einstein proposed in 1905 that the light (which Maxwell beautifully explained as an electromagnetic wave) should be viewed as made up of dis- crete particles. These particles were called photons. The energy of a photon corresponding to a light wave of frequency f is given by, E = hf ; where h = 6:626×10−34 J · s is a new fundamental constant of nature known as Planck's constant. The total energy of a light wave, consisting of some particular number n of photons, should therefore be quantized in integer multiples of the energy of the individual photon, Etotal = nhf. -
Lorentz's Electromagnetic Mass: a Clue for Unification?
Lorentz’s Electromagnetic Mass: A Clue for Unification? Saibal Ray Department of Physics, Barasat Government College, Kolkata 700 124, India; Inter-University Centre for Astronomy and Astrophysics, Pune 411 007, India; e-mail: [email protected] Abstract We briefly review in the present article the conjecture of electromagnetic mass by Lorentz. The philosophical perspectives and historical accounts of this idea are described, especially, in the light of Einstein’s special relativistic formula E = mc2. It is shown that the Lorentz’s elec- tromagnetic mass model has taken various shapes through its journey and the goal is not yet reached. Keywords: Lorentz conjecture, Electromagnetic mass, World view of mass. 1. Introduction The Nobel Prize in Physics 2004 has been awarded to D. J. Gross, F. Wilczek and H. D. Politzer [1,2] “for the discovery of asymptotic freedom in the theory of the strong interaction” which was published three decades ago in 1973. This is commonly known as the Standard Model of mi- crophysics (must not be confused with the other Standard Model of macrophysics - the Hot Big Bang!). In this Standard Model of quarks, the coupling strength of forces depends upon distances. Hence it is possible to show that, at distances below 10−32 m, the strong, weak and electromagnetic interactions are “different facets of one universal interaction”[3,4]. This instantly reminds us about another Nobel Prize award in 1979 when S. Glashow, A. Salam and S. Weinberg received it “for their contributions to the theory of the unified weak and electro- magnetic interaction between elementary particles, including, inter alia, the prediction of the arXiv:physics/0411127v4 [physics.hist-ph] 31 Jul 2007 weak neutral current”. -
Lectures on Atomic Physics
Lectures on Atomic Physics Walter R. Johnson Department of Physics, University of Notre Dame Notre Dame, Indiana 46556, U.S.A. January 4, 2006 Contents Preface xi 1 Angular Momentum 1 1.1 Orbital Angular Momentum - Spherical Harmonics . 1 1.1.1 Quantum Mechanics of Angular Momentum . 2 1.1.2 Spherical Coordinates - Spherical Harmonics . 4 1.2 Spin Angular Momentum . 7 1.2.1 Spin 1=2 and Spinors . 7 1.2.2 In¯nitesimal Rotations of Vector Fields . 9 1.2.3 Spin 1 and Vectors . 10 1.3 Clebsch-Gordan Coe±cients . 11 1.3.1 Three-j symbols . 15 1.3.2 Irreducible Tensor Operators . 17 1.4 Graphical Representation - Basic rules . 19 1.5 Spinor and Vector Spherical Harmonics . 21 1.5.1 Spherical Spinors . 21 1.5.2 Vector Spherical Harmonics . 23 2 Central-Field SchrÄodinger Equation 25 2.1 Radial SchrÄodinger Equation . 25 2.2 Coulomb Wave Functions . 27 2.3 Numerical Solution to the Radial Equation . 31 2.3.1 Adams Method (adams) . 33 2.3.2 Starting the Outward Integration (outsch) . 36 2.3.3 Starting the Inward Integration (insch) . 38 2.3.4 Eigenvalue Problem (master) . 39 2.4 Quadrature Rules (rint) . 41 2.5 Potential Models . 44 2.5.1 Parametric Potentials . 45 2.5.2 Thomas-Fermi Potential . 46 2.6 Separation of Variables for Dirac Equation . 51 2.7 Radial Dirac Equation for a Coulomb Field . 52 2.8 Numerical Solution to Dirac Equation . 57 2.8.1 Outward and Inward Integrations (adams, outdir, indir) 57 i ii CONTENTS 2.8.2 Eigenvalue Problem for Dirac Equation (master) .