Quantum Mechanics-II Problem Set - 6

Total Page:16

File Type:pdf, Size:1020Kb

Quantum Mechanics-II Problem Set - 6 Quantum Mechanics-II Problem Set - 6 1. Use WKB approximation to determine energy levels of the potential 8 V if 0 < x < a=2 <> 0 V (x) = 0 if a=2 < x < a :>1 otherwise 0 Express your answer in terms of V0 and the energy En of a particle in 0 a box. Assume E1 > V0. Solution: 1 1 Figure 1: Figure for Q.1 This is a problem with two walls and the corresponding quantization R a condition is 0 pdx = nπ~. The momentum of the particle is given by p = p2m[E − V (x)] where V (x) is as given above. Now Z a p Z a=2 p p Z a p pdx = 2m E − V0dx + 2m Edx 0 0 a=2 p p a p a = 2m[ E − V + E ] = 0 2 2 Thus p a p p 2m [ E − V + E] = nπ 2 0 ~ 1 Square both sides ma2 [E − V + E + 2pE(E − V )] = n2π2 2 2 0 0 ~ which simplifies to 2 2E − V − n2π2 2 = −2pE(E − V ) 0 ma2 ~ 0 n2π2 2 Define E = ~ , which is the energy of the n− th state of particle n 2ma2 in a box. The above equation becomes p 2E − V0 − 4En = −2 E(E − V0) square it again 2 2 2 4E + V0 − 4EV0 + 16En − 8En(2E − V0) = 4E(E − V0) which gives E2E E4 E2 n = V 2 + n − n 4 0 256 8 Simplifying, we get, 2 V0 V0 E = En + + 2 16En V The first order perturbation theory gives E = E + 0 . The extra n 2 2 V0 term goes to zero for small V0 (which gives the correct limit for 16En particle in a box) or in the classical limit for which n is very large. 2. Consider a particle in one dimension in the presence of a potential V = αjxj; α > 0. Using WKB approximation find its energy. Solution: V (x) E −c +c x 2 This is a problem with no wall but with two turning points at ±c where E c = . The momentum is given by α r E p(x) = p2m(E − V (x)) = 2mα( − j x j) α Thus we have, using Z +c 1 p(x)dx = (n + )~ −c 2 s s Z +c p Z 0 E p Z +c E pdx = 2mα + x dx + 2mα − x dx −c −c α 0 α " #0 " #+c p 2 E 3=2 p 2 E 3=2 = 2mα + x + 2mα − − x 3 α 3 α −c 0 " # p 2 E 3=2 E 3=2 E 3=2 E 3=2 = 2mα − − c + + − c 3 α α α α p 2 E 3=2 = 2 2mα 3 α Thus we have p 2 E 3=2 1 2 2mα = (n + ) 3 α 2 ~ which simplifies to 1 3 2=3 1 E = ~ α(n + )2=3 (2mα)1=3 8 2 3. Tunneling: Consider a potential barrier of width a and arbitrary shape. A free particle with energy E comes from the left and strikes it at x = 0. Find the probability of its tunnelling to region III. 3 E Region I Region Region III II x = 0 x = a Figure 2: Figure for Q.3 Solution: 2k2 A free particle with energy E = ~ is incident on the barrier from 2m the left and strikes the barrier at x = 0. The wavefunctions in three regions are as follows. Region I : ikx −ikx I (x) = e + rI e where rI is the reflection coefficient at the barrier at x = 0. If tI I is the transmission fraction at x = 0, the wave function in region II : −α(x) II (x) = tII (x)e where we have assumed that the barrier is thick enough so there is no reflection from the other end at x = a and Z x r2m α(x) = 2 (V (x) − E)dx 0 ~ 1 1 tII (x) = tII (0) = tII (0) j p(x) j r2m (V (x) − E) ~2 In the third region, which is to the right of x = a, the wavefunction is once gain a free particle with no reflected component, ikx III (x) = Ae 4 The transmission coefficient is the ratio of the square of the amplitude transmitted into the region III to that incident from region I (which we have taken to be 1). j A j2 T = =j A j2 1 Continuity of the wavefunction at x = 0 gives α(0) I (0) = tII (0)e Thus 1 Z xr2m (x) = (0) exp( (V (x) − E)dx) Ii 2m I 2 [ (V (x) − E)]1=4 0 ~ ~2 Continuity at x = a gives II (a) = III (a) which gives 1 Z ar2m (a) = (0) exp( (V (x) − E)dx) III 2m I 2 [ (V (a) − E)]1=4 0 ~ ~2 The tunnelling probability is given by 2 j III (a) j −2γ(a) T = 2 = Ae j I (0) j where Z x r2m γ(x) = 2 (V (x) − E)dx 0 ~ 4. Assume that the potential function in a metal can be approximated by the following potential V (x) = Θ(x)[V1 − eEx] where E is constant electric field. The metal occupies the space x < 0 with its surface at x = 0. Since applied field does not penetrate inside the metal, the energy of electrons below the surface are unaffected 5 by the field. Find the probability that an electron with an energy 0 < E < V1 can be ejected from the surface of the metal. V = Φ + EF − eEx EF Filled electrons x = 0 x = Φ=eE Figure 3: figure for Q.4 Solution: This problem is a simple application of the tunnelling of the previous problem, known as \cold emission". We know that the electrons which lie below the surface of a metal do not feel the effect of the electric field as the field does not penetrate inside the metal. The electrons near the surface, however, may be regarded as being in a potential well of depth φ (with , where φ is the work function of the metal, which we have come across in photoelectric effect. If the potential just at the surface is V , the electrons would get ejected with an energy E = V − φ. In the presence of an external field, the new potential outside the surface of the metal is (measured from the bottom of the conduction band) V (x) = φ + EF − eEx ≡ V1 − eEx where V1 = φ+EF , Thus the electrons at the Fermi level see a triangular V − E potential barrier extending from x = 0 to x = 1 F . We are 1 2 eE looking for the tunnelling probability of electrons at the Fermi surface 6 which we take to have energy E (in place of EF mentioned above). The tunnelling probability was shown to be given by T = exp(−γ) where r Z x2 2mp γ = 2 2 φ − eEx dx x1 ~ The integral is straight forward and we get r 3 2 2mV1 E 3=2 γ = 2 2 2 [1 − ] 3 ~ e E V1 5. Find the probability of transmission through a parabolic barrier 8 x2 <V 1 − jxj < a V (x) = 0 a2 :0 otherwise V (x) E -a -b 0 b a Figure 4: Figure Q. 5 Solution: Turning points are given by x2 E = V [1 − ] 0 a2 7 which gives p V − E x = ±a 0 = ±b V0 Thus (see Problem 3) Z x r2m γ = 2 (V (x) − E)dx 0 ~ r2m Z b x2 1=2 = 2 V0 1 − 2 − E dx ~ −b a r 2 π 2mV0a E = 2 1 − 2 ~ V0 The tunnelling probability is given by e−2γ. 6. A ball of mass m is acted on by uniform gravity g bouncing up and down an elastic floor. Take the floor to be the zero of the potential energy. Using WKB approximation obtain the quantized energy level of the system. Solution Suppose the ball is dropped from a height z = a above the floor (z = 0). The potential energy is V (z) = mgz. We have one here, one, the floor and the other at z = a. The other turning point depends on the energy of the ball (assume that the coefficient of restitution is unity). If the energy is E, the turning point is E=mg. The quantization condition is Z E=mg 3 pdz = n + π~ 0 4 p2 where, since E = + mgz, we have 2m p r mgz p(z) = 2mE 1 − E Thus Z E=mg p Z E=mg r mgz pdz = 2mE 1 − dz 0 0 E 8 mg E Integral is done by substituting y = 1 − z, so that dz = − dy. E mg The quantization condition then becomes p E Z 1 p p E 2 8E3 1=2 3 2mE ydy = 2mE × = 2 = n + π~ mg 0 mg 3 9mg 4 Thus for the energy levels are given by 9π2 31=3 E = mg2π2 2 n + 8 ~ 4 1 7. A truncated harmonic oscillator has potential m!2(x2 −a2) for jxj < a 2 and is zero outside it. Find the WKB estimate for the bound state. Under what condition (connecting m; ! and a, there is only one bound state? Solution: This is a problem with two turning points. The turning points are symmetric and given by x = ±c 1 E = m!2(c2 − a2) 2 r 2E so that c = + a2. We have m!2 Z +c 1 p(x)dx = n + π~ −c 2 r 2E p Since p(x) = p2m(E − V ) = m! + a2 − x2 = m! c2 − x2 is m!2 even, the integral may be written as Z c p π 1 2 c2 − x2dx = ~ n + 0 m! 2 The integral on the left is πc2=4.
Recommended publications
  • (T/E) the Wkb Approximation for General Matrix
    SLAC-PUB-2481 March 1980 (T/E) * THE WKB APPROXIMATION FOR GENERAL MATRIX HAMILTONIANS James D. Bjorken and Harry S. Orbach Stanford Linear Accelerator Center Stanford University, Stanford, California 94305 ABSTRACT We present a method of obtaining WKB type solutions for generalized .~ Schroedinger equations for which the Hamiltonian is an arbitrary matrix function of any.number of pairs of canonical operators. Our solution reduces the problem to that of finding the matrix which diagonalizes the classical Hamiltonian and determining the scalar WKB wave functions for the diagonalized Hamiltonian's entries (presented explicitly in terms of classical quantities). If the classical Hamiltonian has degenerate eigenvalues, the solution contains a vector in the classically degenerate subspace. This vector satisfies a classical equation and is given explicitly in terms of the classical Hamiltonian as a Dyson series. As an example, we obtain, from the Dirac equation for an electron with anomalous magnetic moment, the relativistic spin-precession equation. Submitted to Physical Review D Work supported by the Department of Energy, contract DE-AC03-76SF00515. -2- 1. INTRODUCTION The WRB approximation' forms a bridge between classical mechanics and quantum mechanics. Classical features of the system are clearly displayed, and the quantum features are introduced in a simple way, with only minimal appearances of %. And while quantum mechanics, at best, is no easier a problem than classical mechanics, a virtue of the WKB approximation is that it makes it not much harder. The WKB approximation is usually presented in the context of a non-relativistic Schroedinger equation for a scalar wave function of a single spatial variable.
    [Show full text]
  • Some Recent Developments in WKB Approximation SOME RECENT DEVELOPMENTS in WKB APPROXIMATION
    Some recent developments in WKB approximation SOME RECENT DEVELOPMENTS IN WKB APPROXIMATION BY AKBAR SAFARI, M.Sc. a thesis submitted to the department of Physics & Astronomy and the school of graduate studies of mcmaster university in partial fulfilment of the requirements for the degree of Master of Science c Copyright by Akbar Safari, August 2013 All Rights Reserved Master of Science (2013) McMaster University (Physics & Astronomy) Hamilton, Ontario, Canada TITLE: Some recent developments in WKB approximation AUTHOR: Akbar Safari M.Sc., (Condensed Matter Physics) IUST, Tehran, Iran SUPERVISOR: Dr. D.W.L. Sprung NUMBER OF PAGES: xiii, 107 ii To my wife, Mobina Abstract WKB theory provides a plausible link between classical mechanics and quantum me- chanics in its semi-classical limit. Connecting the WKB wave function across the turning points in a quantum well, leads to the WKB quantization condition. In this work, I focus on some improvements and recent developments related to the WKB quantization condition. First I discuss how the combination of super-symmetric quan- tum mechanics and WKB, gives the SWKB quantization condition which is exact for a large class of potentials called shape invariant potentials. Next I turn to the fact that there is always a probability of reflection when the potential is not constant and the phase of the wave function should account for this reflection. WKB theory ignores reflection except at turning points. I explain the work of Friedrich and Trost who showed that by including the correct “reflection phase" at a turning point, the WKB quantization condition can be made to give exact bound state energies.
    [Show full text]
  • Copyright C 2020 by Robert G. Littlejohn Physics 221A Fall 2020 Notes 7 the WKB Method† 1. Introduction the WKB Method Is Impo
    Copyright c 2020 by Robert G. Littlejohn Physics 221A Fall 2020 Notes 7 The WKB Method † 1. Introduction The WKB method is important both as a practical means of approximating solutions to the Schr¨odinger equation and as a conceptual framework for understanding the classical limit of quantum mechanics. The initials stand for Wentzel, Kramers and Brillouin, who first applied the method to the Schr¨odinger equation in the 1920’s. The WKB approximation is also called the semiclassical or quasiclassical approximation. The basic idea behind the method can be applied to any kind of wave (in optics, acoustics, etc): it is to expand the solution of the wave equation in the ratio of the wavelength to the scale length of the environment in which the wave propagates, when that ratio is small. In quantum mechanics, this is equivalent to treating ¯h formally as a small parameter. The method itself antedates quantum mechanics by many years, and was used by Liouville and Green in the early nineteenth century. Planck’s constant ¯h has dimensions of action, so its value depends on the units chosen, and it does not make sense to say that ¯h is “small.” However, typical mechanical problems have quantities with dimensions of action that appear in them, for example, an angular momentum, a linear mo- mentum times a distance, etc., and if ¯h is small in comparison to these then it makes sense to treat ¯h formally as a small parameter. This would normally be the case for macroscopic systems, which are well described by classical mechanics.
    [Show full text]
  • University of Groningen Instantons and Cosmologies in String Theory Collinucci, Giulio
    University of Groningen Instantons and cosmologies in string theory Collinucci, Giulio IMPORTANT NOTE: You are advised to consult the publisher's version (publisher's PDF) if you wish to cite from it. Please check the document version below. Document Version Publisher's PDF, also known as Version of record Publication date: 2005 Link to publication in University of Groningen/UMCG research database Citation for published version (APA): Collinucci, G. (2005). Instantons and cosmologies in string theory. s.n. Copyright Other than for strictly personal use, it is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), unless the work is under an open content license (like Creative Commons). The publication may also be distributed here under the terms of Article 25fa of the Dutch Copyright Act, indicated by the “Taverne” license. More information can be found on the University of Groningen website: https://www.rug.nl/library/open-access/self-archiving-pure/taverne- amendment. Take-down policy If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. Downloaded from the University of Groningen/UMCG research database (Pure): http://www.rug.nl/research/portal. For technical reasons the number of authors shown on this cover page is limited to 10 maximum. Download date: 02-10-2021 Chapter 2 Instantons In this chapter we will study the basics of instantons, heavily borrowing material from the classic textbooks by S.
    [Show full text]
  • Modified Airy Function and WKB Solutions to the Wave Equation
    NAT L INST. OF STAND & TECH R.I.C. NIST REFERENCE PUBLICATIONS A11103 VlOVDl NIST Monograph 176 Modified Airy Function and WKB Solutions to the Wave Equation I A. K. Ghataky R. L. GallawUy and 1. C. Goyal - QC- 100 U556 M United States Department of Commerce #176 National Institute of standards and Technology 1991 NIST Monograph 176 QClO mi Modified Airy Function and WKB Solutions to the Wave Equation A. K. Ghatak R. L. Gallawa I. C. Goyal Electromagnetic Technology Division Electronics and Electrical Engineering Laboratory National Institute of Standards and Technology Boulder, CO 80303 This monograph was prepared, in part, under the auspices of the Indo-US Collaborative Program in Materials Sciences. Permanent Affiliation of Professors Ghatak and Goyal is Physics Department, Indian Institute of Technology New Delhi, India. November 1991 U.S. Department of Commerce Robert A. Mosbacher, Secretary National Institute of Standards and Technology John W. Lyons, Director National Institute of Standards and Technology Monograph 176 Natl. Inst. Stand. Technol. Mono. 176, 172 pages (Nov. 1991) CODEN: NIMOEZ U.S. GOVERNMENT PRINTING OFFICE WASHINGTON: 1991 For sale by the Superintendent of Documents, U.S. Government Printing Office, Washington, DC 20402-9325 TABLE OF CONTENTS PREFACE vii 1. INTRODUCTION 1 2. WKB SOLUTIONS TO INITIAL VALUE PROBLEMS 6 2.1 Introduction 6 2.2 The WKB Solutions 6 2.3 An Alternative Derivation 11 2.4 The General WKB Solution 14 Case I: Barrier to the Right 15 Case II: Barrier to the Left 19 2.5 Examples 21 Example 2.1 21 Example 2.2 27 3.
    [Show full text]
  • WKB Approximation - Wikipedia
    WKB approximation - Wikipedia https://en.wikipedia.org/wiki/WKB_approximation WKB approximation From Wikipedia, the free encyclopedia In mathematical physics, the WKB approximation or WKB method is a method for finding approximate solutions to linear differential equations with spatially varying coefficients. It is typically used for a semiclassical calculation in quantum mechanics in which the wavefunction is recast as an exponential function, semiclassically expanded, and then either the amplitude or the phase is taken to be slowly changing. The name is an initialism for Wentzel–Kramers–Brillouin. It is also known as the LG or Liouville–Green method. Other often-used letter combinations include JWKB and WKBJ, where the "J" stands for Jeffreys. Contents 1 Brief history 2 WKB method 3 An example 3.1 Precision of the asymptotic series 4 Application to the Schrödinger equation 5 See also 6 References 6.1 Modern references 6.2 Historical references 7 External links Brief history This method is named after physicists Wentzel, Kramers, and Brillouin, who all developed it in 1926. In 1923, mathematician Harold Jeffreys had developed a general method of approximating solutions to linear, second-order differential equations, which includes the Schrödinger equation. Even though the Schrödinger equation was developed two years later, Wentzel, Kramers, and Brillouin were apparently unaware of this earlier work, so Jeffreys is often neglected credit. Early texts in quantum mechanics contain any number of combinations of their initials, including WBK, BWK, WKBJ, JWKB and BWKJ. An authoritative discussion and critical survey has been given by R B Dingle.[1] Earlier references to the method are: Carlini in 1817, Liouville in 1837, Green in 1837, Rayleigh in 1912 and Gans in 1915.
    [Show full text]
  • Semiclassical Approximation
    Chapter 3 Semiclassical approximation c B. Zwiebach 3.1 The classical limit The WKB approximation provides approximate solutions for linear differential equations with coefficients that have slow spatial variation. The acronym WKB stands for Wentzel, Kramers, Brillouin, who independently discovered it in 1926. It was in fact discovered earlier, in 1923 by the mathematician Jeffreys. When applied to quantum mechanics, it is called the semi-classical approximation, since classical physics then illuminates the main features of the quantum wavefunction. The de Broglie wavelength λ of a particle can help us assess if classical physics is relevant to the physical situation. For a particle with momentum p we have h λ = : (3.1.1) p Classical physics provides useful physical insight when λ is much smaller than the relevant length scale in the problem we are investigating. Alternatively if we take h ! 0 this will formally make λ ! 0, or λ smaller than the length scale of the problem. Being a constant of nature, we cannot really make ~ ! 0, so taking this limit is a thought experiment in which we imagine worlds in which h takes smaller and smaller values making classical physics more and more applicable. The semi-classical approximation studied here will be applicable if a suitable generalization of the de Broglie wavelength discussed below is small and slowly varying. The semi-classical approximation will be set up mathematically by thinking of ~ as a parameter that can be taken to be as small as desired. Our discussion in this chapter will focus on one-dimensional problems. Consider there- fore a particle of mass m and total energy E moving in a potential V (x).
    [Show full text]
  • PHY 305: WKB and Path Integral Formulation of QM in These Notes, We Will Study the Relationship Between Quantum Mechanics and Cl
    PHY 305: WKB and Path Integral Formulation of QM In these notes, we will study the relationship between quantum mechanics and classical mechanics. Any new physical theory that replaces an existing one, has to show that it can reproduce all the old results in the limit where the old theory is accurate. In our case, this limit is ~ → 0. Since ~ is a dimensionful quantity 2 −1 [ ~ ] = kg · m · s . (1) which is the units of angular momentum = momentum × distance, or action = energy × time. This means that the classical description should for systems for which the characteristic mass, size, and velocity are such that its ‘action’ is large compared to ~. This important requirement is known as the correspondence principle, and quantum mechanics satisfies it beautifully. 1. Classical Action For simplicity we consider a non-relativistic particle of mass m moving in one dimension, under influence of a potential V (x). We can describe the classical motion of the particle either via a Hamiltonian or a Lagrangian p2 1 H(x, p) = + V (x); L(x, x˙) = mx˙ 2 − V (x) . (2) 2m 2 The equations of motion are respectively the Hamilton equations or the Euler-Lagrange equations ∂H ∂H d ∂L ∂L x˙ = , p˙ = − ; − = 0 . (3) ∂p ∂x dt ∂x˙ ∂x In our specific example, these equations reduce to the familiar form p ∂V x˙ = , p˙ = − (4) m ∂x ∂V which is just Newton’s equation with a force F (x) = − ∂x . 1 The usual formulation of quantum mechanics, via the Schr¨odinger equation and Heisen- berg equations of motion, is most closely related to the Hamilton formulation of classical mechanics.
    [Show full text]
  • Semiclassical Approximations in Wave Mechanics Semiclassical Limit K E Mount
    Reports on Progress in Physics Related content - Potential scattering cross sections in the Semiclassical approximations in wave mechanics semiclassical limit K E Mount To cite this article: M V Berry and K E Mount 1972 Rep. Prog. Phys. 35 315 - Uniform approximation for potential scattering involving a rainbow M V Berry - Semiclassical techniques for treating the one-dimensional Schrodinger equation: View the article online for updates and enhancements. uniform approximations and oscillatory integrals B J B Crowley Recent citations - ERS approximation for solving Schrödinger’s equation and applications Hichem Eleuch and Michael Hilke - A quantum mechanical insight into SN2 reactions: Semiclassical initial value representation calculations of vibrational features of the ClCH3Cl pre-reaction complex with the VENUS suite of codes Xinyou Ma et al - Semiclassical Treatment of High-Lying Electronic States of H2+ T. J. Price and Chris H. Greene This content was downloaded from IP address 169.228.105.170 on 09/01/2019 at 20:44 Semiclassical approximations in wave mechanics M V BERRY AND K E MOUNT H H Wills Physics Laboratory, Tyndall Avenue, Bristol BS8 1TL Contents Page 1. Introduction , . 316 2. Problems with no classical turning points . 317 2.1. A simple illustrative example . 317 2.2. The basic WKB solutions . 319 2.3. The semiclassical reflected wave. 322 3. The complex method for treating classical turning points , . 325 3.1. The origin of the connection problem . 325 3.2. The connection formulae for the case of one turning point: their reversibility . 328 3.3. More turning points . , 335 4. Uniform approximations for one-dimensional problems .
    [Show full text]
  • Copyright C 2020 by Robert G. Littlejohn Physics 221A Fall 2020
    Copyright c 2020 by Robert G. Littlejohn Physics 221A Fall 2020 Notes 7 The WKB Method † 1. Introduction The WKB method is important both as a practical means of approximating solutions to the Schr¨odinger equation and as a conceptual framework for understanding the classical limit of quantum mechanics. The initials stand for Wentzel, Kramers and Brillouin, who first applied the method to the Schr¨odinger equation in the 1920’s. The WKB approximation is also called the semiclassical or quasiclassical approximation. The basic idea behind the method can be applied to any kind of wave (in optics, acoustics, etc): it is to expand the solution of the wave equation in the ratio of the wavelength to the scale length of the environment in which the wave propagates, when that ratio is small. In quantum mechanics, this is equivalent to treating ¯h formally as a small parameter. The method itself antedates quantum mechanics by many years, and was used by Liouville and Green in the early nineteenth century. Planck’s constant ¯h has dimensions of action, so its value depends on the units chosen, and it does not make sense to say that ¯h is “small.” However, typical mechanical problems have quantities with dimensions of action that appear in them, for example, an angular momentum, a linear mo- mentum times a distance, etc., and if ¯h is small in comparison to these then it makes sense to treat ¯h formally as a small parameter. This would normally be the case for macroscopic systems, which are well described by classical mechanics.
    [Show full text]
  • Arxiv:Hep-Th/9405029V2 5 May 1994 LA-UR-94-569 Supersymmetry and Quantum Mechanics
    LA-UR-94-569 Supersymmetry and Quantum Mechanics Fred Cooper Theoretical Division, Los Alamos National Laboratory, Los Alamos, NM 87545 Avinash Khare Institute of Physics, Bhubaneswar 751005, INDIA Uday Sukhatme Department of Physics, University of Illinois at Chicago, Chicago, IL 60607 February 1, 2008 arXiv:hep-th/9405029v2 5 May 1994 Abstract In the past ten years, the ideas of supersymmetry have been prof- itably applied to many nonrelativistic quantum mechanical problems. In particular, there is now a much deeper understanding of why cer- tain potentials are analytically solvable and an array of powerful new approximation methods for handling potentials which are not exactly solvable. In this report, we review the theoretical formulation of su- persymmetric quantum mechanics and discuss many applications. Ex- actly solvable potentials can be understood in terms of a few basic ideas which include supersymmetric partner potentials, shape invari- ance and operator transformations. Familiar solvable potentials all 1 have the property of shape invariance. We describe new exactly solv- able shape invariant potentials which include the recently discovered self-similar potentials as a special case. The connection between in- verse scattering, isospectral potentials and supersymmetric quantum mechanics is discussed and multi-soliton solutions of the KdV equation are constructed. Approximation methods are also discussed within the framework of supersymmetric quantum mechanics and in particular it is shown that a supersymmetry inspired WKB approximation is exact for a class of shape invariant potentials. Supersymmetry ideas give particularly nice results for the tunneling rate in a double well potential and for improving large N expansions. We also discuss the problem of a charged Dirac particle in an external magnetic field and other potentials in terms of supersymmetric quantum mechanics.
    [Show full text]
  • Tunneling in Cosine Potential with Periodic Boundary Conditions
    Tunneling in cosine potential with periodic boundary conditions. Zbigniew Ambroziński October 29, 2018 Abstract In this paper we discuss three methods to calculate energy splitting in cosine potential on a circle, Bloch waves, semi–classical approximation and restricted basis approach. While the Bloch wave method gives only a qualitative result, with the WKB method we are able to determine its unknown coefficients. The numerical approach is most exact and enables us to extract further corrections to previous results. 1 Introduction In this article we study tunneling in quantum mechanical cosine potential with periodic boundary conditions. Hamiltonian of this system is given by the formula 1 1 p H = P 2 + (1 − cos (2π gX)) (1) 2 4π2g with X 2 (0; g−1=2K) where K is the number of minima and with periodic boundary conditions. For shorter 1 notation we put V (x) = 4π2 (1 − cos(2πx)). Within perturbative calculus vacuum energy of the system is degenerate. Each ground state is localized in different minimum. Tunneling is responsible for splitting of the energies. In general, this effect cannot be studied analytically. One can give a first approximation to the splitting using semiclassical–approximation (or WKB approximation) which was developed by G. Wentzel, H. Kramers and L. Brillouin in 1926. In this approach, one finds that the ground energy is shifted by a quantity which is a nonperturbative function of coupling constant. This classical solution is called an instanton. Validity of the instanton calculus is limited to systems with widely separated minima with a large potential barrier in between. Nevertheless, it has a vast range of applications to modern field theories.
    [Show full text]