Why Professor Richard Feynman was upset solving the Laplace equation for spherical waves? Anzor A. Khelashvili a)

Similar documents
Keywords: Schrödinger equation, radial equation, boundary condition, singular potentials.

Lecture 7: Angular Momentum, Hydrogen Atom

I. CONSTRUCTION OF THE GREEN S FUNCTION

2. Electrostatics. Dr. Rakhesh Singh Kshetrimayum 8/11/ Electromagnetic Field Theory by R. S. Kshetrimayum

Scattering in Three Dimensions

EM Boundary Value Problems

( ) [ ] [ ] [ ] δf φ = F φ+δφ F. xdx.

arxiv: v1 [physics.pop-ph] 3 Jun 2013

Lecture 23. Representation of the Dirac delta function in other coordinate systems

PHYS 301 HOMEWORK #10 (Optional HW)

3D-Central Force Problems I

arxiv: v1 [physics.gen-ph] 18 Aug 2018

PES 3950/PHYS 6950: Homework Assignment 6

4. Electrodynamic fields

Nuclear size corrections to the energy levels of single-electron atoms

2 Lecture 2: The Bohr atom (1913) and the Schrödinger equation (1925)

ON THE TWO-BODY PROBLEM IN QUANTUM MECHANICS

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department Physics 8.07: Electromagnetism II September 15, 2012 Prof. Alan Guth PROBLEM SET 2

Doublet structure of Alkali spectra:

Right-handed screw dislocation in an isotropic solid

Introduction to Nuclear Forces

= e2. = 2e2. = 3e2. V = Ze2. where Z is the atomic numnber. Thus, we take as the Hamiltonian for a hydrogenic. H = p2 r. (19.4)

THE LAPLACE EQUATION. The Laplace (or potential) equation is the equation. u = 0. = 2 x 2. x y 2 in R 2

ON INDEPENDENT SETS IN PURELY ATOMIC PROBABILITY SPACES WITH GEOMETRIC DISTRIBUTION. 1. Introduction. 1 r r. r k for every set E A, E \ {0},

Math 124B February 02, 2012

Review: Electrostatics and Magnetostatics

Appendix B The Relativistic Transformation of Forces

A new approach in classical electrodynamics to protect principle of causality

Energy Levels Of Hydrogen Atom Using Ladder Operators. Ava Khamseh Supervisor: Dr. Brian Pendleton The University of Edinburgh August 2011

Lecture 8 - Gauss s Law

New problems in universal algebraic geometry illustrated by boolean equations

Physics 2A Chapter 10 - Moment of Inertia Fall 2018

-Δ u = λ u. u(x,y) = u 1. (x) u 2. (y) u(r,θ) = R(r) Θ(θ) Δu = 2 u + 2 u. r = x 2 + y 2. tan(θ) = y/x. r cos(θ) = cos(θ) r.

Anyone who can contemplate quantum mechanics without getting dizzy hasn t understood it. --Niels Bohr. Lecture 17, p 1

On the integration of the equations of hydrodynamics

APPENDIX. For the 2 lectures of Claude Cohen-Tannoudji on Atom-Atom Interactions in Ultracold Quantum Gases

Gauss Law. Physics 231 Lecture 2-1

Superluminal Group Velocity of Electromagnetic Near-fields *

3. Electromagnetic Waves II

arxiv:gr-qc/ v2 8 Jun 2006

A Relativistic Electron in a Coulomb Potential

B da = 0. Q E da = ε. E da = E dv

Quantum Mechanics II

POISSON S EQUATION 2 V 0

As is natural, our Aerospace Structures will be described in a Euclidean three-dimensional space R 3.

PHYS 110B - HW #7 Spring 2004, Solutions by David Pace Any referenced equations are from Griffiths Problem statements are paraphrased

Section 8.2 Polar Coordinates

working pages for Paul Richards class notes; do not copy or circulate without permission from PGR 2004/11/3 10:50

Appendix A. Appendices. A.1 ɛ ijk and cross products. Vector Operations: δ ij and ɛ ijk

Multipole Radiation. February 29, The electromagnetic field of an isolated, oscillating source

1 Spherical multipole moments

Physics 505 Homework No. 9 Solutions S9-1

On the radial derivative of the delta distribution

Compactly Supported Radial Basis Functions

Hopefully Helpful Hints for Gauss s Law

PROBLEM SET #1 SOLUTIONS by Robert A. DiStasio Jr.

Green s Identities and Green s Functions

Physics 161 Fall 2011 Extra Credit 2 Investigating Black Holes - Solutions The Following is Worth 50 Points!!!

Conservative Averaging Method and its Application for One Heat Conduction Problem

Vectors, Vector Calculus, and Coordinate Systems

221B Lecture Notes Scattering Theory I

Physics 506 Winter 2006 Homework Assignment #9 Solutions

The Poisson bracket and magnetic monopoles

Problems with Mannheim s conformal gravity program

TheWaveandHelmholtzEquations

Calculation of Quark-antiquark Potential Coefficient and Charge Radius of Light Mesons

12th WSEAS Int. Conf. on APPLIED MATHEMATICS, Cairo, Egypt, December 29-31,

PHY2061 Enriched Physics 2 Lecture Notes. Gauss Law

15 Solving the Laplace equation by Fourier method

Flux. Area Vector. Flux of Electric Field. Gauss s Law

Physics 107 TUTORIAL ASSIGNMENT #8

DonnishJournals

you of a spring. The potential energy for a spring is given by the parabola U( x)

arxiv:gr-qc/ v1 29 Jan 1998

Geometry of the homogeneous and isotropic spaces

Physics 122, Fall October 2012

Gravitational Memory?

ASTR415: Problem Set #6

1.2 Differential cross section

8 Separation of Variables in Other Coordinate Systems

(read nabla or del) is defined by, k. (9.7.1*)

Physics 2B Chapter 22 Notes - Magnetic Field Spring 2018

c n ψ n (r)e ient/ h (2) where E n = 1 mc 2 α 2 Z 2 ψ(r) = c n ψ n (r) = c n = ψn(r)ψ(r)d 3 x e 2r/a0 1 πa e 3r/a0 r 2 dr c 1 2 = 2 9 /3 6 = 0.

IX INDUCTANCE AND MAGNETIC FIELDS

Class 2. Lesson 1 Stationary Point Charges and Their Forces. Basic Rules of Electrostatics. Basic Rules of Electrostatics

DOING PHYSICS WITH MATLAB COMPUTATIONAL OPTICS

Casimir-Polder potential for parallel metallic plates in background of a conical defect

5.111 Lecture Summary #6 Monday, September 15, 2014

11) A thin, uniform rod of mass M is supported by two vertical strings, as shown below.

EELE 3331 Electromagnetic I Chapter 4. Electrostatic fields. Islamic University of Gaza Electrical Engineering Department Dr.

Antennas & Propagation

MATH 415, WEEK 3: Parameter-Dependence and Bifurcations

The Strain Compatibility Equations in Polar Coordinates RAWB, Last Update 27/12/07

Exceptional regular singular points of second-order ODEs. 1. Solving second-order ODEs

The Schwartzchild Geometry

AST 121S: The origin and evolution of the Universe. Introduction to Mathematical Handout 1

7.2. Coulomb s Law. The Electric Force

Dymore User s Manual Two- and three dimensional dynamic inflow models

$ i. !((( dv vol. Physics 8.02 Quiz One Equations Fall q 1 q 2 r 2 C = 2 C! V 2 = Q 2 2C F = 4!" or. r ˆ = points from source q to observer

A Hartree-Fock Example Using Helium

Transcription:

Why Pofesso Richad Feynman was upset solving the Laplace equation fo spheical waves? Anzo A. Khelashvili a) Institute of High Enegy Physics, Iv. Javakhishvili Tbilisi State Univesity, Univesity St. 9, 009, Tbilisi, Geogia and St. Andea the Fist-called Geogian Univesity of Patiachy of Geogia, Chavchavadze Ave. 53a, 06, Tbilisi, Geogia Teimuaz P. Nadaeishvili b) Iv. Javakhishvili Tbilisi State Univesity, Faculty of Exact and Natual Sciences, Chavchavadze Ave. 3, 079, Tbilisi, Geogia and Institute of High Enegy Physics, Iv. Javakhishvili Tbilisi State Univesity, Univesity St. 9, 009, Tbilisi, Geogia Abstact. We take attention to the singula behavio of the Laplace opeato in spheical coodinates, which was established in ou ealie wok. This singulaity has many nontivial consequences. In this aticle we conside only the simplest ones, which ae connected to the solution of Laplace equation in Feynman classical books and Lectues. Feynman was upset looking in his deived solutions, which have a fictitious singula behavio at the oigin. We show how these inconsistencies can be avoided. Keywods: Laplace equation, Spheical and Catesian coodinates, bounday condition. PACS numbes: 03.65.-w, 03.65.Ca, 03.65.Ta I. INTRODUCTION R.Feynman in his Lectues discussed the deivation of spheical waves on the basis of wave equation in spheical coodinates. Deived solution has a singulaity at the oigin = 0. He wote about this solution the following: Ou solution must epesent physically a situation, in which thee is some souce at the oigin. In othe wods, we

have inadvetently made a mistake. We have not solved the fee wave equation eveywhee; we solved it with zeo on the ight eveywhee except at the oigin. Ou mistake cept in because some of the steps in ou deivation ae not legal when = 0.. R. Feynman pobably had meant singula behavio of Laplace opeato at the oigin. Nowadays we know that Laplacian is indeed singula in spheical coodinates,3 and a moe caution teatment is necessay. Ou aim in this aticle will be caeful investigation of Feynman s poblem. This aticle is oganized as follows. In Sec. II we conside the electostatic poblem. In Sec. III we conside the Yukawa potential. Sec. IV we give concluding emaks. II. ElECTROSTATIC PROBLEM Let us begin, follow Feynman, by electostatic poblem, whee the same mistake occus. R.Feynman mentioned: Let s show that it is easy to make the same kind of mistake in an electostatic poblem. Suppose we want a solution of the equation fo an electostatic potential in fee space, ψ = 0. In an explicit fom this equation looks like ψ ( ) = d ψ dψ + = 0 d d () R.Feynman continued: It is often moe convenient to wite this equation in the following fom d ψ = ( ψ ) () d If you cay out the diffeentiation indicated in this equation, you will see that the ight hand side is the same as in pevious equation

We want to emphasis that exactly this statement fails at = 0 4. It was shown in 4 that the coect elation looks like d ψ = d ) (3 ( ψ ) 4πδ ( ) ( ψ ) (3) Theefoe some of elations of Feynman s book will undego elevant coections. If we intoduce the epesentation of 3-dimensional delta function in spheical coodinates, namely, and use taditional shot elation ( ) ( 3 ) δ δ () =, (4) 4π u ( ) ψ ( ) we deive the following fom of Laplace equation = (5) d u δ ()() u = 0 (6) d It seems that afte tansition to function u( ) thee appeas souce-like tem in the Laplace equation δ ()() u = δ ()() u 0. It is caused by singula chaacte of Jacobian of tansfomation fom Catesian to spheical coodinates, J = sinθ at the oigin. (usually the singulaity with espect to θ is avoided by the equiements of discontinuity and uniqueness, which esults in appeaance of spheical hamonics ( θ, ϕ) How can we eject this exta tem fom equation? It depends on value of ( 0) Υ lm 5. u. thee ae thee possibilities: a finite u ( 0) must be excluded, because afte etuning to ψ, thee appeas undesiable / tem, which is not a solution of Laplace equation. The second possibility u ( 0) = must also be ejected, as the pesence of infinite tem in 3

( 0) 0 equation is nonsense. So, thee emains only possibility, u = and if at the same time we take this function to behave as u ε ( ) + 0, ( ε > 0) (7) then this tem kills the delta function and we etun to the standad equation. This consideation shows, that the standad educed adial equation is valid only in cases when the estiction u ( 0 ) = 0 is fulfilled 3. In this case standad equation looks like d d u = 0 (8) and has a solution () = a b u + (9) Taking into account the above estiction, we obtain that b = 0 and, theefoe u ψ = = a = const. While R.Feynman mentioned: found that the following ψ is a solution fo the electostatic potential in fee space b ψ = a + (0) Then R.Feynman continued: Something is evidently wong. In the egion whee thee ae no electic chages, we know the solution fo the electostatic potential: the potential is eveywhee constant. That coesponds to the fist tem in ou solution. But we have also the second tem, which says that thee is a contibution to the potential that vaies as one ove the distance fom the oigin. We know, howeve, that such a potential 4

coesponds to a point chage at the oigin. So, although we thought we wee solving fo the potential in fee space, ou solution also gives the field fo a point souce at the oigin. We see that igoous consideation of adial Laplace equation puts all things on thei own places. The estiction u( 0 ) = 0 has a decisive meaning. The natual question aises: Why does the bounday condition-like estiction aises in the fee equation? This happens because tansfomation to spheical coodinates does not involve = point and the tansition to u () function feels this, because of facto. 0 The second tem in Feynman consideation b / is not a solution at all. Indeed, afte its substitution into Laplace equation we obtain a delta function, instead of zeo. Anothe way to avoid this solution is a compaison to Catesian solution, whee the wave function at the oigin is constant, as it is clea fom the solution of the in this coodinates 6 ψ = 0 equation ψ = e ± iαx e ± iβy e ± α + β z () The same can be demonstated by consideing chaacteistic equation fo (), substituting thee ψ s, it follows s s ( s + ) = 0 integating this equation by the spheical element s s + ( s + ) ( ) = 0 s+ b a d in abitay bounds, we obtain () (3) it follows that we have only one solution s = 0, which coesponds to ψ = const accodance with Catesian behavio., in 5

III. YUKAWA POTENTIAL Anothe place whee R.Feynman made use the elation () is the Yukawa potential (ibid. Chapte 8). It is commonly believed that the Yukawa potential is a spheically symmetic solution of well-known wave equation φ μ φ = 0 (4) Aming with the pevious consideation, R.Feynman wote this equation in the following fom ( φ) μ φ = 0 (5) solution of which is φ = ± Ke μ and theefoe afte a suitable bounday condition at infinity, it follows the Yukawa potential μ e φ = K (6) But we know, that a igoous application of coect elation (3) gives μ e μ e = μ ( 3 ) μ () 4 πδ e, (7) Inteesting enough that this fom was given in the ealie book 7. It follows that the Yukawa potential is not a spheically symmetic solution of Eq. (4) eveywhee, but it is such only ahead of oigin. We see fom Eq. (7) that the Yukawa potential is a solution of nonhomogenious wave equation with a souse tem on the ight-hand side φ μ φ = 4 πk δ 3 ( ) ( ) (8) 6

IV. CONCLUSIONS In conclusion, we have demonstated that caeful consideation of Laplacian opeato nea the oigin emoves all the inconsistencies elated to Feynman s analysis. The only point which must be claified is a igoous detemination of a chaacte of aspiation to zeo of u() function in ode to povide u ( ) δ ( ) = 0, which is a business of the theoy of distibutions. Moeove we note that things will be changed in many applications whee the Laplace opeato is used in spheical coodinates. ACKNOWLEDGEMENTS Authos acknowledges financial suppot of the Shota Rustaveli National Science Foundation (Pojects DI/3/0 and FR//4) a) Electonic mail: anzo.khelashvili@tsu.ge b) Electonic mail: teimuaz.nadaeishvili@tsu.ge 7

R.Feynman, R.Leighton and M.Sands, The Feynman Lectues on Physics (Addison- Wesley Publishing Company,Inc.Reading,Massachusetts, Pablo Alto, London,964) Vol.II, Electomagnetism. Chapte 0. Anzo A.Khelashvili and Teimuaz P. Nadaeishvili, Unexpected delta-function tem in the adial Schodinge equation, e-pint axiv: 00. 78. 3 Anzo A.Khelashvili and Teimuaz P. Nadaeishvili, What is the bounday condition fo adial wave function of the Schödinge equation?, Am. J. Phys. 79 (6), 668-67 (0). 4 Anzo A.Khelashvili and Teimuaz P. Nadaeishvili, Delta-like singulaity in the Radial Laplace Opeato and the Status of the Radial Schodinge Equation, Bulletin of the Geogian National Academy of Sciences (Moambe) 6 (), 68-73 (0). axiv:0.85 5 See, any book on quantum mechanics. 6 J. D. Jackson, Classical Electodynamics, 3d ed. (John Wiley & Sons, New Yok, 999). 7 H.Bethe and F. Hoffmann, Mesons and Fields, (Row Peteson and Company, New Yok, 955). Vol, p. 30. 8