Fractional Quantum Mechanics, Relativistic Quantum Mechanics, Fractional Schrödinger Equation, Relativistic Schrödinger Equation

Total Page:16

File Type:pdf, Size:1020Kb

Fractional Quantum Mechanics, Relativistic Quantum Mechanics, Fractional Schrödinger Equation, Relativistic Schrödinger Equation International Journal of Theoretical and Mathematical Physics 2015, 5(4): 58-65 DOI: 10.5923/j.ijtmp.20150504.02 The Infinite Square Well Problem in the Standard, Fractional, and Relativistic Quantum Mechanics Yuchuan Wei1,2 1International Center of Quantum Mechanics, Three Gorges University, China 2Department of Radiation Oncology, Wake Forest University, NC Abstract There has been a continuous argument on the correctness of the Laskin‟s solution for the infinite square well problem in the fractional quantum mechanics. In this paper, we prove that the Laskin‟s functions are not amathematical solution to the fractional Schrödinger equation and the equation does not have any nonzero solutions at all in the sense of mathematics. As in the standard quantum mechanics, we view the infinite square well problem as the limit of the finite well problem, and define the solution for the infinite square well problem as the limit of the solution for the finite square well problem. Using the simple property of the infinite operators, we show that Laskin‟s function can be the limit solution for the infinite square well problem. The single-sided well problem and the 3 dimensional well problem are included. This operator method works for the same problems in the relativistic quantum mechanicsas well. Keywords Fractional quantum mechanics, Relativistic quantum mechanics, Fractional Schrödinger equation, Relativistic Schrödinger equation standard Schrödinger equation either, and it is nothing but 1. Introduction the limit of the solution to the finite square problem. Without a mathematical definition of the eigenvalues and In 2000, Laskin introduced the fractional quantum eigenfunctions of a Hamiltonian operator with local infinity, mechanics [1-3]. As an example he solved the infinite square the argument will be endless. Therefore, in this paper we well problem in a piecewise fashion [3]. However, in 2010 mathematically define the infinite square well problem as a Jeng, et al [4] criticized that it was meaningless to solve a limit of the finite well. This viewpoint is also useful for other nonlocal equation in a piecewise fashion and they potentials with infinity, such as the coulomb potential in the demonstrated that it was impossible for the ground state hydrogen atom, the single-sided harmonic oscillator, etc. function to satisfy the fractional Schrödinger equation near Since it is difficult to solve the fractional Schrödinger‟s the boundary inside the well. In a series of papers [5-8], equation with a finite square well potential, we wish a direct Bayin insisted that he explicitly completed the calculation in way to find the solution of the infinite square well problem. Jeng‟s paper and the wave functions did satisfy the fractional Fortunately, we can express the fractional Hamiltonian in Schrödinger equation inside the well. Hawkins and Schwarz terms of the standard Hamiltonian. In the same way, we can [9] claimed that the Bayin‟s calculation contained serious mistakes. Luchko [10] provided some evidence that the also solve the infinite square well problem in the relativistic solution did not satisfy the equation outside the well. On the quantum mechanics, since the fractional and relativistic other hand, Dong [11] re-obtained the Laskin‟s solution by quantum mechanics are closely related. We acknowledge solving the fractional Schrödinger equation with the path that these solutions need to be verified when the solutions to integral method. It is not easy for readers to judge their the finite square well problem are reported later. mathematical argument [12, 13], but weagree with Jeng‟s We first recall the infinite square well problem in standard opinion, including that the piecewise way to solve the quantum mechanics, and then solve the problem in the equation is wrong, and that the solution does not satisfy the fractional quantum mechanics and in the relativistic quantum fractional Schrödinger equation, since we will inarguably mechanics. show that the Laskin‟s functions do not satisfy the fractional Schrödinger equation ( 1) anywhere on the x-axis. However, in fact, this solution does not satisfy the 2. Definition of the Infinite Well Problem * Corresponding author: In this section we will recall the relation between the finite [email protected] (Yuchuan Wei) Published online at http://journal.sapub.org/ijtmp and infinite square well problems in the standard quantum Copyright © 2015 Scientific & Academic Publishing. All Rights Reserved mechanics, and accordingly define the infinite square well International Journal of Theoretical and Mathematical Physics 2015, 5(4): 58-65 59 problem in the fractional quantum mechanics. 0 xa , . Vxi (8) 2.1. The Finite and Infinite Potential Wells in the xa Standard Quantum Mechanics At xa , the potential has two infinite jumps. The In the standard quantum mechanics [14], the one subscript imeans the infinite square well. dimensional time-independent Schrödinger equationis Obviously the potential Vi is not real in physics and not H x E x , (1) well-defined in mathematics, since we do not know how to determine the value of the multiplication V x() x where x is a wave function defined on the x-axis, and i outside the well, even if the wave function outside the well is E is an energy. The Hamiltonian operator zero. (Does 0 equal 0,1, or ?) In physics this H T V x (2) potential is used as a simplified model for „a very deep finite square well‟. is the summation of the kinetic energy and the Conventionally the Schrödinger equation potentialenergy of a particle. 22d The standard kinetic energy operator is V x x E x (9) 2m dx2 i pd2 2 2 , (3) T 2 is solved in a piecewise way again [15]. The wave function 22mmdx outside the well is zero because the potential is infinite and where p is the one dimensional momentum operator the wavefunction inside the well is a sine or cosine function. The revised continuity condition for this case is that the wave d functions must be continuous but their derivative should not pi . (4) dx be. The infinite square well problem has the simple and well-known solution As usual, m is the mass of the particle and ℏ is the reduced Plank constant. 1 n A finite square well [15] is defined as sin x a x a (), n x a 2a (10) 0 xa 0,xa , , Vx (5) f V x a 0 n2 2 2 (11) En 2 where V0 0 is the depth of the well and 2a is the width of 8ma the well. The subscript f means the finite square well. for n 1,2,3, . The eigenequation of the finite square well problem is However, we emphasize that this solution does not satisfy the Schrödinger Equations (9). Take the ground state as an 22d V x x E x . (6) example, we have 2m dx2 f 22d This equation can be solved separately in three regions V x x 2m dx2 11i first and then the piecewise solutions are connected by the . (12) continuity condition that the wave function and its derivative 2 must be continuous. This process generates the eigenvalues E11 x ()() x a x a 4ma a Exfn ()and eigenstates fn ()x , with n 1,2,3 . The The wave function satisfies the Schrödinger equation state with n=1 is the ground state [15]. everywhere except at x=a and x=-a. This is not a small flaw One can easily verify that the explicit solutions satisfy the for a differential equation, and we have to say that the wave eigenequation at every point on the whole x-axis functions in (10) are not the solution of the Schrödinger 22d equation at all. The extra terms in the above equation comes , (7) from the discontinuity of the derivative of the wave function, 2 fn V f x fn x E fn x 2m dx but if we keep the derivative of the wavefunction continuous, which convinces us that the continuity condition we use is we can only get a trivial solution x 0 , which is suitable. In fact this continuity condition comes from the meaningless in physics. We have to say that the Schrödinger Schrödinger equation. equation with the infinite square well potential does not have The infinite square well potential is defined as solutions in mathematics. (See the appendix if one feels 60 Yuchuan Wei: The Infinite Square Well Problem in the Standard, Fractional, and Relativistic Quantum Mechanics surprised.) where the coefficient D mc2 /() mc with χ a Since the infinite square well is a limit of the finite square well, conventionally we call the limit of the solutions of the positive real number, and c is the speed of the light. When finite square well problem 2 , taking 1/ 2 and hence Dm 1/ (2 ) , the fractional kinetic energy recovers the standard kinetic energy, limfn (x ) n ( x ), lim E fn ( x ) E n , (13) VV 2 00 i.e. T2 p/ (2 m ) T . Originally Laskin [1-3] required the solution of the infinite square well, and symbolically the fractional parameter 12 , but in this paper we write allow 02 . The fractional Schrödinger equation is 22d n V i x n x E n n x . (14) 2m dx2 HxE x (17) The piecewise way to solve the Schrödinger equation for HTV. (18) the infinite square well, together with the aforementioned revised continuity condition, is nothing but an easy and For the infinite square well problem, we have direct way to get the limit of the finite square well solution d 2 2 . (19) without solving the finite square well problem. D()()2 x Vi x x E x This definition for the infinity potential is applicable for dx several important cases in quantum mechanics.
Recommended publications
  • 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.
    [Show full text]
  • Key Concepts for Future QIS Learners Workshop Output Published Online May 13, 2020
    Key Concepts for Future QIS Learners Workshop output published online May 13, 2020 Background and Overview On behalf of the Interagency Working Group on Workforce, Industry and Infrastructure, under the NSTC Subcommittee on Quantum Information Science (QIS), the National Science Foundation invited 25 researchers and educators to come together to deliberate on defining a core set of key concepts for future QIS learners that could provide a starting point for further curricular and educator development activities. The deliberative group included university and industry researchers, secondary school and college educators, and representatives from educational and professional organizations. The workshop participants focused on identifying concepts that could, with additional supporting resources, help prepare secondary school students to engage with QIS and provide possible pathways for broader public engagement. This workshop report identifies a set of nine Key Concepts. Each Concept is introduced with a concise overall statement, followed by a few important fundamentals. Connections to current and future technologies are included, providing relevance and context. The first Key Concept defines the field as a whole. Concepts 2-6 introduce ideas that are necessary for building an understanding of quantum information science and its applications. Concepts 7-9 provide short explanations of critical areas of study within QIS: quantum computing, quantum communication and quantum sensing. The Key Concepts are not intended to be an introductory guide to quantum information science, but rather provide a framework for future expansion and adaptation for students at different levels in computer science, mathematics, physics, and chemistry courses. As such, it is expected that educators and other community stakeholders may not yet have a working knowledge of content covered in the Key Concepts.
    [Show full text]
  • A Study of Fractional Schrödinger Equation-Composed Via Jumarie Fractional Derivative
    A Study of Fractional Schrödinger Equation-composed via Jumarie fractional derivative Joydip Banerjee1, Uttam Ghosh2a , Susmita Sarkar2b and Shantanu Das3 Uttar Buincha Kajal Hari Primary school, Fulia, Nadia, West Bengal, India email- [email protected] 2Department of Applied Mathematics, University of Calcutta, Kolkata, India; 2aemail : [email protected] 2b email : [email protected] 3 Reactor Control Division BARC Mumbai India email : [email protected] Abstract One of the motivations for using fractional calculus in physical systems is due to fact that many times, in the space and time variables we are dealing which exhibit coarse-grained phenomena, meaning that infinitesimal quantities cannot be placed arbitrarily to zero-rather they are non-zero with a minimum length. Especially when we are dealing in microscopic to mesoscopic level of systems. Meaning if we denote x the point in space andt as point in time; then the differentials dx (and dt ) cannot be taken to limit zero, rather it has spread. A way to take this into account is to use infinitesimal quantities as ()Δx α (and ()Δt α ) with 01<α <, which for very-very small Δx (and Δt ); that is trending towards zero, these ‘fractional’ differentials are greater that Δx (and Δt ). That is()Δx α >Δx . This way defining the differentials-or rather fractional differentials makes us to use fractional derivatives in the study of dynamic systems. In fractional calculus the fractional order trigonometric functions play important role. The Mittag-Leffler function which plays important role in the field of fractional calculus; and the fractional order trigonometric functions are defined using this Mittag-Leffler function.
    [Show full text]
  • Configuration Interaction Study of the Ground State of the Carbon Atom
    Configuration Interaction Study of the Ground State of the Carbon Atom María Belén Ruiz* and Robert Tröger Department of Theoretical Chemistry Friedrich-Alexander-University Erlangen-Nürnberg Egerlandstraße 3, 91054 Erlangen, Germany In print in Advances Quantum Chemistry Vol. 76: Novel Electronic Structure Theory: General Innovations and Strongly Correlated Systems 30th July 2017 Abstract Configuration Interaction (CI) calculations on the ground state of the C atom are carried out using a small basis set of Slater orbitals [7s6p5d4f3g]. The configurations are selected according to their contribution to the total energy. One set of exponents is optimized for the whole expansion. Using some computational techniques to increase efficiency, our computer program is able to perform partially-parallelized runs of 1000 configuration term functions within a few minutes. With the optimized computer programme we were able to test a large number of configuration types and chose the most important ones. The energy of the 3P ground state of carbon atom with a wave function of angular momentum L=1 and ML=0 and spin eigenfunction with S=1 and MS=0 leads to -37.83526523 h, which is millihartree accurate. We discuss the state of the art in the determination of the ground state of the carbon atom and give an outlook about the complex spectra of this atom and its low-lying states. Keywords: Carbon atom; Configuration Interaction; Slater orbitals; Ground state *Corresponding author: e-mail address: [email protected] 1 1. Introduction The spectrum of the isolated carbon atom is the most complex one among the light atoms. The ground state of carbon atom is a triplet 3P state and its low-lying excited states are singlet 1D, 1S and 1P states, more stable than the corresponding triplet excited ones 3D and 3S, against the Hund’s rule of maximal multiplicity.
    [Show full text]
  • Lecture 16 Matter Waves & Wave Functions
    LECTURE 16 MATTER WAVES & WAVE FUNCTIONS Instructor: Kazumi Tolich Lecture 16 2 ¨ Reading chapter 34-5 to 34-8 & 34-10 ¤ Electrons and matter waves n The de Broglie hypothesis n Electron interference and diffraction ¤ Wave-particle duality ¤ Standing waves and energy quantization ¤ Wave function ¤ Uncertainty principle ¤ A particle in a box n Standing wave functions de Broglie hypothesis 3 ¨ In 1924 Louis de Broglie hypothesized: ¤ Since light exhibits particle-like properties and act as a photon, particles could exhibit wave-like properties and have a definite wavelength. ¨ The wavelength and frequency of matter: # & � = , and � = $ # ¤ For macroscopic objects, de Broglie wavelength is too small to be observed. Example 1 4 ¨ One of the smallest composite microscopic particles we could imagine using in an experiment would be a particle of smoke or soot. These are about 1 µm in diameter, barely at the resolution limit of most microscopes. A particle of this size with the density of carbon has a mass of about 10-18 kg. What is the de Broglie wavelength for such a particle, if it is moving slowly at 1 mm/s? Diffraction of matter 5 ¨ In 1927, C. J. Davisson and L. H. Germer first observed the diffraction of electron waves using electrons scattered from a particular nickel crystal. ¨ G. P. Thomson (son of J. J. Thomson who discovered electrons) showed electron diffraction when the electrons pass through a thin metal foils. ¨ Diffraction has been seen for neutrons, hydrogen atoms, alpha particles, and complicated molecules. ¨ In all cases, the measured λ matched de Broglie’s prediction. X-ray diffraction electron diffraction neutron diffraction Interference of matter 6 ¨ If the wavelengths are made long enough (by using very slow moving particles), interference patters of particles can be observed.
    [Show full text]
  • 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.
    [Show full text]
  • Motion and Time Study the Goals of Motion Study
    Motion and Time Study The Goals of Motion Study • Improvement • Planning / Scheduling (Cost) •Safety Know How Long to Complete Task for • Scheduling (Sequencing) • Efficiency (Best Way) • Safety (Easiest Way) How Does a Job Incumbent Spend a Day • Value Added vs. Non-Value Added The General Strategy of IE to Reduce and Control Cost • Are people productive ALL of the time ? • Which parts of job are really necessary ? • Can the job be done EASIER, SAFER and FASTER ? • Is there a sense of employee involvement? Some Techniques of Industrial Engineering •Measure – Time and Motion Study – Work Sampling • Control – Work Standards (Best Practices) – Accounting – Labor Reporting • Improve – Small group activities Time Study • Observation –Stop Watch – Computer / Interactive • Engineering Labor Standards (Bad Idea) • Job Order / Labor reporting data History • Frederick Taylor (1900’s) Studied motions of iron workers – attempted to “mechanize” motions to maximize efficiency – including proper rest, ergonomics, etc. • Frank and Lillian Gilbreth used motion picture to study worker motions – developed 17 motions called “therbligs” that describe all possible work. •GET G •PUT P • GET WEIGHT GW • PUT WEIGHT PW •REGRASP R • APPLY PRESSURE A • EYE ACTION E • FOOT ACTION F • STEP S • BEND & ARISE B • CRANK C Time Study (Stopwatch Measurement) 1. List work elements 2. Discuss with worker 3. Measure with stopwatch (running VS reset) 4. Repeat for n Observations 5. Compute mean and std dev of work station time 6. Be aware of allowances/foreign element, etc Work Sampling • Determined what is done over typical day • Random Reporting • Periodic Reporting Learning Curve • For repetitive work, worker gains skill, knowledge of product/process, etc over time • Thus we expect output to increase over time as more units are produced over time to complete task decreases as more units are produced Traditional Learning Curve Actual Curve Change, Design, Process, etc Learning Curve • Usually define learning as a percentage reduction in the time it takes to make a unit.
    [Show full text]
  • Exercises in Classical Mechanics 1 Moments of Inertia 2 Half-Cylinder
    Exercises in Classical Mechanics CUNY GC, Prof. D. Garanin No.1 Solution ||||||||||||||||||||||||||||||||||||||||| 1 Moments of inertia (5 points) Calculate tensors of inertia with respect to the principal axes of the following bodies: a) Hollow sphere of mass M and radius R: b) Cone of the height h and radius of the base R; both with respect to the apex and to the center of mass. c) Body of a box shape with sides a; b; and c: Solution: a) By symmetry for the sphere I®¯ = I±®¯: (1) One can ¯nd I easily noticing that for the hollow sphere is 1 1 X ³ ´ I = (I + I + I ) = m y2 + z2 + z2 + x2 + x2 + y2 3 xx yy zz 3 i i i i i i i i 2 X 2 X 2 = m r2 = R2 m = MR2: (2) 3 i i 3 i 3 i i b) and c): Standard solutions 2 Half-cylinder ϕ (10 points) Consider a half-cylinder of mass M and radius R on a horizontal plane. a) Find the position of its center of mass (CM) and the moment of inertia with respect to CM. b) Write down the Lagrange function in terms of the angle ' (see Fig.) c) Find the frequency of cylinder's oscillations in the linear regime, ' ¿ 1. Solution: (a) First we ¯nd the distance a between the CM and the geometrical center of the cylinder. With σ being the density for the cross-sectional surface, so that ¼R2 M = σ ; (3) 2 1 one obtains Z Z 2 2σ R p σ R q a = dx x R2 ¡ x2 = dy R2 ¡ y M 0 M 0 ¯ 2 ³ ´3=2¯R σ 2 2 ¯ σ 2 3 4 = ¡ R ¡ y ¯ = R = R: (4) M 3 0 M 3 3¼ The moment of inertia of the half-cylinder with respect to the geometrical center is the same as that of the cylinder, 1 I0 = MR2: (5) 2 The moment of inertia with respect to the CM I can be found from the relation I0 = I + Ma2 (6) that yields " µ ¶ # " # 1 4 2 1 32 I = I0 ¡ Ma2 = MR2 ¡ = MR2 1 ¡ ' 0:3199MR2: (7) 2 3¼ 2 (3¼)2 (b) The Lagrange function L is given by L('; '_ ) = T ('; '_ ) ¡ U('): (8) The potential energy U of the half-cylinder is due to the elevation of its CM resulting from the deviation of ' from zero.
    [Show full text]
  • 1 the LOCALIZED QUANTUM VACUUM FIELD D. Dragoman
    1 THE LOCALIZED QUANTUM VACUUM FIELD D. Dragoman – Univ. Bucharest, Physics Dept., P.O. Box MG-11, 077125 Bucharest, Romania, e-mail: [email protected] ABSTRACT A model for the localized quantum vacuum is proposed in which the zero-point energy of the quantum electromagnetic field originates in energy- and momentum-conserving transitions of material systems from their ground state to an unstable state with negative energy. These transitions are accompanied by emissions and re-absorptions of real photons, which generate a localized quantum vacuum in the neighborhood of material systems. The model could help resolve the cosmological paradox associated to the zero-point energy of electromagnetic fields, while reclaiming quantum effects associated with quantum vacuum such as the Casimir effect and the Lamb shift; it also offers a new insight into the Zitterbewegung of material particles. 2 INTRODUCTION The zero-point energy (ZPE) of the quantum electromagnetic field is at the same time an indispensable concept of quantum field theory and a controversial issue (see [1] for an excellent review of the subject). The need of the ZPE has been recognized from the beginning of quantum theory of radiation, since only the inclusion of this term assures no first-order temperature-independent correction to the average energy of an oscillator in thermal equilibrium with blackbody radiation in the classical limit of high temperatures. A more rigorous introduction of the ZPE stems from the treatment of the electromagnetic radiation as an ensemble of harmonic quantum oscillators. Then, the total energy of the quantum electromagnetic field is given by E = åk,s hwk (nks +1/ 2) , where nks is the number of quantum oscillators (photons) in the (k,s) mode that propagate with wavevector k and frequency wk =| k | c = kc , and are characterized by the polarization index s.
    [Show full text]
  • The Heisenberg Uncertainty Principle*
    OpenStax-CNX module: m58578 1 The Heisenberg Uncertainty Principle* OpenStax This work is produced by OpenStax-CNX and licensed under the Creative Commons Attribution License 4.0 Abstract By the end of this section, you will be able to: • Describe the physical meaning of the position-momentum uncertainty relation • Explain the origins of the uncertainty principle in quantum theory • Describe the physical meaning of the energy-time uncertainty relation Heisenberg's uncertainty principle is a key principle in quantum mechanics. Very roughly, it states that if we know everything about where a particle is located (the uncertainty of position is small), we know nothing about its momentum (the uncertainty of momentum is large), and vice versa. Versions of the uncertainty principle also exist for other quantities as well, such as energy and time. We discuss the momentum-position and energy-time uncertainty principles separately. 1 Momentum and Position To illustrate the momentum-position uncertainty principle, consider a free particle that moves along the x- direction. The particle moves with a constant velocity u and momentum p = mu. According to de Broglie's relations, p = }k and E = }!. As discussed in the previous section, the wave function for this particle is given by −i(! t−k x) −i ! t i k x k (x; t) = A [cos (! t − k x) − i sin (! t − k x)] = Ae = Ae e (1) 2 2 and the probability density j k (x; t) j = A is uniform and independent of time. The particle is equally likely to be found anywhere along the x-axis but has denite values of wavelength and wave number, and therefore momentum.
    [Show full text]
  • 8 the Variational Principle
    8 The Variational Principle 8.1 Approximate solution of the Schroedinger equation If we can’t find an analytic solution to the Schroedinger equation, a trick known as the varia- tional principle allows us to estimate the energy of the ground state of a system. We choose an unnormalized trial function Φ(an) which depends on some variational parameters, an and minimise hΦ|Hˆ |Φi E[a ] = n hΦ|Φi with respect to those parameters. This gives an approximation to the wavefunction whose accuracy depends on the number of parameters and the clever choice of Φ(an). For more rigorous treatments, a set of basis functions with expansion coefficients an may be used. The proof is as follows, if we expand the normalised wavefunction 1/2 |φ(an)i = Φ(an)/hΦ(an)|Φ(an)i in terms of the true (unknown) eigenbasis |ii of the Hamiltonian, then its energy is X X X ˆ 2 2 E[an] = hφ|iihi|H|jihj|φi = |hφ|ii| Ei = E0 + |hφ|ii| (Ei − E0) ≥ E0 ij i i ˆ where the true (unknown) ground state of the system is defined by H|i0i = E0|i0i. The inequality 2 arises because both |hφ|ii| and (Ei − E0) must be positive. Thus the lower we can make the energy E[ai], the closer it will be to the actual ground state energy, and the closer |φi will be to |i0i. If the trial wavefunction consists of a complete basis set of orthonormal functions |χ i, each P i multiplied by ai: |φi = i ai|χii then the solution is exact and we just have the usual trick of expanding a wavefunction in a basis set.
    [Show full text]
  • 1 the Principle of Wave–Particle Duality: an Overview
    3 1 The Principle of Wave–Particle Duality: An Overview 1.1 Introduction In the year 1900, physics entered a period of deep crisis as a number of peculiar phenomena, for which no classical explanation was possible, began to appear one after the other, starting with the famous problem of blackbody radiation. By 1923, when the “dust had settled,” it became apparent that these peculiarities had a common explanation. They revealed a novel fundamental principle of nature that wascompletelyatoddswiththeframeworkofclassicalphysics:thecelebrated principle of wave–particle duality, which can be phrased as follows. The principle of wave–particle duality: All physical entities have a dual character; they are waves and particles at the same time. Everything we used to regard as being exclusively a wave has, at the same time, a corpuscular character, while everything we thought of as strictly a particle behaves also as a wave. The relations between these two classically irreconcilable points of view—particle versus wave—are , h, E = hf p = (1.1) or, equivalently, E h f = ,= . (1.2) h p In expressions (1.1) we start off with what we traditionally considered to be solely a wave—an electromagnetic (EM) wave, for example—and we associate its wave characteristics f and (frequency and wavelength) with the corpuscular charac- teristics E and p (energy and momentum) of the corresponding particle. Conversely, in expressions (1.2), we begin with what we once regarded as purely a particle—say, an electron—and we associate its corpuscular characteristics E and p with the wave characteristics f and of the corresponding wave.
    [Show full text]