Two Examples Illustrating the Differences between Classical and Quantum Mechanics

Similar documents
THE ESSENTIAL SELF-ADJOINTNESS OF SCHRÖDINGER OPERATORS WITH OSCILLATING POTENTIALS. Adam D. Ward. In Memory of Boris Pavlov ( )

Matrices A(t) depending on a Parameter t. Jerry L. Kazdan

Molecular propagation through crossings and avoided crossings of electron energy levels

y" + Q(t)y = o, i e /, (l.i)

UNIVERSITY OF SURREY FACULTY OF ENGINEERING AND PHYSICAL SCIENCES DEPARTMENT OF PHYSICS. BSc and MPhys Undergraduate Programmes in Physics LEVEL HE2

Proceedings of the 5th International Conference on Inverse Problems in Engineering: Theory and Practice, Cambridge, UK, 11-15th July 2005

WAVELET MULTIPLIERS AND SIGNALS

Maximum Process Problems in Optimal Control Theory

i=1 β i,i.e. = β 1 x β x β 1 1 xβ d

8. Limit Laws. lim(f g)(x) = lim f(x) lim g(x), (x) = lim x a f(x) g lim x a g(x)

L p Functions. Given a measure space (X, µ) and a real number p [1, ), recall that the L p -norm of a measurable function f : X R is defined by

SOME INEQUALITIES FOR THE EUCLIDEAN OPERATOR RADIUS OF TWO OPERATORS IN HILBERT SPACES

SELF-ADJOINTNESS OF DIRAC OPERATORS VIA HARDY-DIRAC INEQUALITIES

Lp-norms of weak solutions of elliptic equations in the interior of their domain,

Asymptotic Stability by Linearization

WITH SWITCHING ARMS EXACT SOLUTION OF THE BELLMAN EQUATION FOR A / -DISCOUNTED REWARD IN A TWO-ARMED BANDIT

General Lower Bounds for Resonances in One Dimension*

Hadamard and Perron JWR. October 18, On page 23 of his famous monograph [2], D. V. Anosov writes

APPROXIMATE ISOMETRIES ON FINITE-DIMENSIONAL NORMED SPACES

CLASS NOTES FOR APRIL 14, 2000

THE REGULARITY OF MAPPINGS WITH A CONVEX POTENTIAL LUIS A. CAFFARELLI

Nonlinear stabilization via a linear observability

SELF-ADJOINTNESS OF SCHRÖDINGER-TYPE OPERATORS WITH SINGULAR POTENTIALS ON MANIFOLDS OF BOUNDED GEOMETRY

QUALIFYING EXAMINATION Harvard University Department of Mathematics Tuesday August 31, 2010 (Day 1)

Rigidity and Non-rigidity Results on the Sphere

ADJOINTS, ABSOLUTE VALUES AND POLAR DECOMPOSITIONS

1.4 The Jacobian of a map

THE FUNDAMENTAL THEOREM OF ALGEBRA VIA PROPER MAPS

Math Analysis Notes Mrs. Atkinson 1

Spectrum (functional analysis) - Wikipedia, the free encyclopedia

Multiple Choice. 1.(6 pts) Find symmetric equations of the line L passing through the point (2, 5, 1) and perpendicular to the plane x + 3y z = 9.

Existence Theory: Green s Functions

Math 234. What you should know on day one. August 28, You should be able to use general principles like. x = cos t, y = sin t, 0 t π.

x f(x)

ON THE ASYMPTOTIC GROWTH OF SOLUTIONS TO A NONLINEAR EQUATION

x f(x)

To Be (a Circle) or Not to Be?

Arc Length. Philippe B. Laval. Today KSU. Philippe B. Laval (KSU) Arc Length Today 1 / 12

Hamiltonian Mechanics

Our Current Concept of Locality may be Incomplete

b) The system of ODE s d x = v(x) in U. (2) dt

MATH 415, WEEK 11: Bifurcations in Multiple Dimensions, Hopf Bifurcation

FUNCTION BASES FOR TOPOLOGICAL VECTOR SPACES. Yılmaz Yılmaz

("-1/' .. f/ L) I LOCAL BOUNDEDNESS OF NONLINEAR, MONOTONE OPERA TORS. R. T. Rockafellar. MICHIGAN MATHEMATICAL vol. 16 (1969) pp.

UNCERTAINTY PRINCIPLES FOR THE FOCK SPACE

On the concentration of eigenvalues of random symmetric matrices

Math for Economics 1 New York University FINAL EXAM, Fall 2013 VERSION A

A Note on a Model for the Quasilinear Wave Equation

Coordinates, phase space, constraints

Controllability of linear PDEs (I): The wave equation

SPECTRAL THEOREM FOR COMPACT SELF-ADJOINT OPERATORS

8 Periodic Linear Di erential Equations - Floquet Theory

BASIC MATRIX PERTURBATION THEORY

Introduction to Spectral Theory

Roots and Coefficients Polynomials Preliminary Maths Extension 1

Lecture Notes on Metric Spaces

7 Asymptotics for Meromorphic Functions

March Algebra 2 Question 1. March Algebra 2 Question 1

ENGI 4430 Parametric Vector Functions Page dt dt dt

THE FORM SUM AND THE FRIEDRICHS EXTENSION OF SCHRÖDINGER-TYPE OPERATORS ON RIEMANNIAN MANIFOLDS

Sufficiency Conditions for Finite Escape Times in Systems of Quadratic Differential Equations

Heisenberg Uncertainty in Reduced Power Algebras

ON WEAKLY NONLINEAR BACKWARD PARABOLIC PROBLEM

Traces and Duality Lemma

LMI Methods in Optimal and Robust Control

DISCONJUGACY OF SECOND-ORDER LINEAR DIFFERENTIAL EQUATIONS WITH NON- NEGATIVE COEFFICIENTS

Ordinary differential equations with measurable right-hand side and parameters in metric spaces

CHAPTER VIII HILBERT SPACES

Math Ordinary Differential Equations

Solution: It could be discontinuous, or have a vertical tangent like y = x 1/3, or have a corner like y = x.

MATH 117 LECTURE NOTES

Non-linear wave equations. Hans Ringström. Department of Mathematics, KTH, Stockholm, Sweden

A Method of Computing Eigenvectors and Eigenvalues

GRONWALL'S INEQUALITY FOR SYSTEMS OF PARTIAL DIFFERENTIAL EQUATIONS IN TWO INDEPENDENT VARIABLES

Lecture Notes DRE 7007 Mathematics, PhD

(1) F(x,y, yl, ", y.) 0,

Chapter 4 - Motion in 2D and 3D

Determination of f(00) from the asymptotic series for f(x) about x=0

Real Analysis, 2nd Edition, G.B.Folland Elements of Functional Analysis

MAC 2311 Calculus I Spring 2004

A Chebyshev Polynomial Rate-of-Convergence Theorem for Stieltjes Functions

Solution of Additional Exercises for Chapter 4

NON POSITIVELY CURVED METRIC IN THE SPACE OF POSITIVE DEFINITE INFINITE MATRICES

NUMERICAL RADIUS OF A HOLOMORPHIC MAPPING

Optimal control theory with applications to resource and environmental economics

VOYAGER INSIDE ALGEBRA CORRELATED TO THE NEW JERSEY STUDENT LEARNING OBJECTIVES AND CCSS.

BOOK REVIEWS 165. Square integrable eigenfunctions of the Schrodinger equation decay exponentially.

MATH4104: Quantum nonlinear dynamics. Lecture Two. Review of quantum theory.

S(x) Section 1.5 infinite Limits. lim f(x)=-m x --," -3 + Jkx) - x ~

Overview of vector calculus. Coordinate systems in space. Distance formula. (Sec. 12.1)

A LIMIT-POINT CRITERION FOR NONOSCILLATORY STURM-LIOUVTLLE DIFFERENTIAL OPERATORS1

ON PERIODIC SOLUTIONS OF NONLINEAR DIFFERENTIAL EQUATIONS WITH SINGULARITIES

September Math Course: First Order Derivative

The small ball property in Banach spaces (quantitative results)

14 Periodic phenomena in nature and limit cycles

Copyright c 2007 Jason Underdown Some rights reserved. quadratic formula. absolute value. properties of absolute values

Lecture 3. Econ August 12

Example of Indeterminacy in Classical Dynamics

ON THE DIFFERENCE BETWEEN THE CONCEPTS "COMPOUND" AND "COMPOSED" POISSON PROCESSES. CARL PHILIPSON Stockholm, Sweden

Coordinates, phase space, constraints

Transcription:

Commun. math. Phys. 29, 105--111 (1973) by Springer-Vertag 1973 Two Examples Illustrating the Differences between Classical and Quantum Mechanics Jeffrey Rauch* Department of Mathematics, The University of Michigan, Ann Arbor, Michigan Michael Reed Department of Mathematics, Princeton University, Princeton, New Jersey Received August 1, 1972 Abstract. Two examples are presented: The first shows that a potential V(x) can be in the limit circle case at oe even if the classical travel time to oe is infinite. The second shows that V(x) can be in the limit point case at oo even though the classical travel time to infinity is finite. The first example illustrates the reflection of quantum waves at sharp steps. The second example illustrates the tunnel effect. In this paper we give two examples of motion on a half-line which illustrate two physical differences between classical and quantum mechanics. It is useful to study the half-line case since the necessary techniques and estimates are elementary and the complications which arise in higher dimensions are absent. We say that a potential V(x) is classically complete at o~ if the classical travel time to infinity is infinite for all initial conditions. We say that V(x) is quantum mechanically complete at oe if the differential operator 2m dx 2 + V(x) is in the limit point case at oe. At first glance it seems that the two notions of completeness might be the same since 2m dx 2 + V(x) is in the limit point case at oo if one need not specify boundary conditions at oe. In a rough intuitive sense, this should happen if the classical travel time is infinite. But, in fact, this rough intuition is correct only if the derivatives of V(x) are "small" compared to V(x). We present two examples illustrating this fact. In the first example, V(x) is classically incomplete at but quantum mechanically complete; in the second, V(x) is classically complete at oe but quantum mechanically incomplete. The examples * This research was partially supported by the National Science Foundation under Grant GP-34260. For help with the diagrams, the authors thank Bob Johnson. 8 Commun. math. Phys., Vol. 29

106 J, Rauch and M. Reed: were suggested by Nelson in unpublished lectures at Princeton. The two examples are interesting because in both cases the differences arise from quantum phenomena not found in classical mechanics; namely, the reflection of quantum waves at sharp steps in Example 1 and the tunnel effect in Example 2. This illustrates the point that questions which at first appear to be merely technical mathematical problems often turn out to be closely related to the physics of the situation being described. In the following brief discussion we always assume that V(x) is a real-valued continuously differentiable function on (0, oo). If x(t) and v(t) are position and velocity of a classical particle moving in the potential V, the Hamiltonian is H(x, v)= ½my2+ V(x) and the classical equations of motion are: 2(0 = v(t), ij(t) = 1 V'(x(t)). (i) m For each pair (Xo, Vo), standard arguments give the existence and uniqueness of a solution (x(t), v(t)) for It- to] sufficiently small and satisfying X(to) = xo, V(to) = vo. An elementary argument using uniqueness and the conservation of energy shows that if a global solution (i.e., for all t>to) fails to exist, then there is a z>t o so that either Limx(t)=0 or Limx(t) = oo. The second alternative can only occur if sup V(x) < oo and t'-*~: x>=l dx if the classical travel time (from x= 1), 1 l/e--v(x)' is finite for E > sup V(x). If the second alternative holds we say that V(x) is classically x=>l incomplete at oo. In the quantum mechanical case, let H be the linear operator 2m dx z + V defined on the dense set C~(0, co) in /;2(0, oo). H is essentially self-adjoint on C~ (0, oo) if and only if the ordinary differential equation 1 2m c~"(x) + V(x) q$(x) = 0 (ii) is tile limit point case both at 0 and at oo; i.e., if and only if exactly one nontrivial solution (up to scalar multiples) of (ii) is square integrable near 0 and exactly one is square integrable near oo. (For proofs, see [1, Chapter 9] or [2, XIII. 2].) If H is not essentially self-adjoint, one must choose a self-adjoint extension by fixing boundary conditions at 0 or at oo (or both). In the case where exactly one solution of (ii) is square integrable near oo (limit point case) we say that V(x) is quantum mechanically.complete at oo.

Classical and Quantum Mechanics 107 As mentioned above, a rough intuition says that V(x) should be quantum mechanically complete at ~ if and only if the classical travel time to infinity is infinite because then one should not have to specify boundary conditions at ~. The following result shows that this is in fact true if the derivatives of V are small compared to V. Theorem (Wintner [4]). Let V(x) be a twice continuously differentiable function on (0, oo) which satisfies V(x)-~ - oo as x ~ co, and suppose that!1( v)l'v ax < oo I\ (- vp/~ ~(- for some c > O. Then V(x) is quantum mechanically complete at oo if and only if V(x) is classically complete at ~. We now present two examples which show that if V'(x) is not small compared to V(x), then the classical and quantum notions of completeness at ~ are independent. Example 1 (V is classically incomplete but quantum mechanically complete at ~). The potential V(x) will be a sequence of plateaus at heights -~2k4 smoothly connected by steep cliffs on the short intervals dx (~k, ilk) about the points x = k; see Fig. 1. Since o ~- V(x) < oe, the classical motion under this potential is incomplete at oo. However, if the steps are sharp enough the quantum motion will be complete. The reason for this behavior is that part of the quantum wave is reflected at each of the sharp steps and the steps are arranged so that most of the wave never escapes to infinity. I lh 2 3 4 ~I,,I,,h _2!~ 2 I,,,... Fig. 1 8'

108 J. Rauch and M. Reed: What we need to do is to construct V(x) so that there is a solution of (ii) which is not in L 2 near infinity. To understand the idea, consider the case of infinitely sharp steps, i.e. ek = k = ilk. For x ~ (n- 1, n) let q~(x)= cos(n2~cx - re) with c=l//2rn. Then q) satisfies (ii) except at the integers and clearly 4) L2(0, oo). In the following construction we just smooth out the sharp steps on the intervals (e k, fig) in such a way that the corresponding solution 4) remains outside L 2. On each short interval (0~k, fl0, k = 1, 2, 3..., we define V(x) to be any monotone decreasing function so that V(x) is continuously differentiable on (0, Go). We now show how to choose the ek and ilk- Take ~1 = 1 and define ~b(x)=cos(rccx-r 0 on (0,11. At x=l, q~(1)=l and ~b'(1)=0. We want to choose fll so that the solution has not descended much at ill. Since V(x)< 0 the solution q~(x) of (ii) which equals cos (r~x-zr)on (0, 1] will be concave downward between 1 and its next zero, q. On the interval I = (1, min {q, 2}), q~(x) satisfies which implies that c~(x) - l = 2m i (i V(t) dp(t) dt) ds plv(t) sup 14)(t)l (2m) < 24rt 2 (x- 1) 2 (2m). 2 Choose/~, so dose to 1 that 14)(fii) - II- t/4, the point being that this estimate holds no matter how we patch together the steps just as long as V(x) is greater than -24g 2 in (el,/~1). On (ill, e2) the solution has the form q~(x) =A2 cos(22ncx-7) where we must have ]A2t > 1-1 since q~(fll)> 1-¼. Now, choose ea to be the closest point to 2 where A2cos(2encx-7) has a maximum. At ~2, q~(c~2)>l-¼, so using the same idea as above we can choose f12 so that q~ (/32) > 1 - ¼ - -~. Continuing in this manner we construct a solution q~(x) of (ii) so that ~b(x) =Ancos(n2r~cx-y,) on (fi,-1,e~) and such that la,-nl+lfl,-nl~o and [A,] > 1/2 for all n. Thus, q~(x) will not be in L2(0, m), which implies that V(x) is in the limit point case at m, i.e. V(x) is quantum mechanically complete at oe, Example 2 (V(x) is classically complete but quantum mechanically incomplete at m). The potential V(x) will be of the form - x 4 + ~ at(x) where ak(x) is a very narrow smooth spike centered at x = k with radius of support dk- The spikes are chosen so that V(k)= k; see Fig. 2. Since V(x) is not bounded from above near infinity the classical motion is

Classical and Quantum Mechanics 109 Fig. 2 complete at infinity. We will show that if the supports of the spikes are chosen to be narrow enough, then 1 ~, 2m dx 2 + ~- - x4 + ak(x) will not be essentially self-adjoint on C~(0, 09). Since V(x) is in the limit point case at x=0 [2, p. 14151 this shows that V(x) can not be in the limit point case ~, i.e., V(x) is not quantum mechanically complete at ~. The physical reason for this behavior is that if the spikes are narrow enough, the quantum particle can tunnel through even though the classical particle is turned back. Thus to a quantum mechanical particle the potential V is not very different from I"1 =~- 1 -x 4 which, by Wintner's theorem, is not quantum mechanically complete at oo. We will show that if the supports of the spikes are small enough there is an a, 0 = a < 1, so that k=~l ak~t 2 ~a 2-1 "q- t 2 -~-m-m q~ Vlq~ I + b2 lnbll 2 (iii) for all q~ e C~ (0, ~). The symmetric form of the Kato-Rellich theorem [3, Chapter V, Theorem 4.5] then implies that 2m ~ dx + Vx and l d 2 2m ~ dx + VI + a k are either both essentially self-adjoint on

110 J. Rauch and M. Reed: C~(0, oe) or both not essentially self-adjoint. Since 2m dx 2 + V1 is not essentially self-adjoint, it follows that 2ml dx 2d 2 + V1 + ~ 6k is not essentially self-adjoint, k= To prove (iii) we use a simple a priori estimate. For each positive integer m and each xo ~ IR, let I,~ = {x [ lx - Xol < 1/m}. Then, there is a constant C (independent of xo) such that sup 1412 ~. m m xe1~co (iv) for all q5 ~ C~(IR). To prove (iv), let q be a C oo function with support 1 1 in the interval ( - ½, ½) which is indentically one on (- ~, ¼). We have xo-~ xo-½ and (iv) follows by carrying out the differentiations, integrating by parts in the ~/' ~b' term, and then using the Schwarz inequality. Let ak(x) be a non-negative C ~ function with support in the interval (k--dk, k+dk) with d k < 1/4. Furthermore let a k reach a maximum 1 value of - - 7- + k4 + k = M k at x = k. Then for all q~ e C; (0, oe) II~k~ll 2 ~ 2Mk2dk (sup [q~[:) < 2M ff dk C(11~'112=(,~)+ 11~1122@ <2i~dkC = (2m) 2 ---~-1 qt,+ 2m +(2m)211V~ 4~IIL:@ 2 Now choose d k so that 2M~ dk C(2m) 2 <- ½ and so that Then 2M 2 dk C(2m) 2 sup II'] [2 < 1. < _ + + 2114~[12=(i~) =~=T +V141 +2H~blt 2-

Classical and Quantum Mechanics 111 This proves the estimate (iii) which implies as discussed above that V(x) is not in the limit point case at oe. As an interesting exercise, the reader is invited to work Example 1 using the technique of Example 2 and Example 2 with the technique of Example 1. References t. Coddington, E., Levinson, N. : Theory of ordinary differential equations. New York: McGraw-Hill, t955. 2. Dunford, N., Schwartz, J.T.: Linear operators, II. New York: Interscience 1963. 3. Kato, T.: Perturbation theory for linear operators. Berlin-Heidelberg-New York: Springer 1966. 4. Wintner, A. : On the normalization of characteristic differentials in continuous spectra. Phys. Rev. 72, 516--517 (1947). Jeffrey Rauch Department of Mathematics The University of Michigan Ann Arbor, Mich. 48104 USA Michael Reed Department of Mathematics Princeton University Princeton, N. J. 08540 USA