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Commutators, eigenvalues, and quantum mechanics on surfaces. Evans Harrell Georgia Tech www.math.gatech.edu/~harrell Tucson and Tours, 2004
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Commutators, eigenvalues and quantum mechanics on surfaces...

Apr 10, 2018

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Commutators,

eigenvalues,and

quantum mechanics

on surfaces.Evans Harrell

Georgia Tech

www.math.gatech.edu/~harrell

Tucson and Tours,

2004

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Dramatis personae

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Dramatis personae

• Commutator [A,B] = AB - BA

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Dramatis personae

• Commutator [A,B] = AB - BA

• The “nano” world

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Dramatis personae

• Commutator [A,B] = AB - BA

• The “nano” world

• Curvature

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Eigenvalues

• H uk = λ uk

• For simplicity, the spectrum will often be

assumed to be discrete. For example, the

operators might be defined on bounded

regions.

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Eigenvalues

• Laplacian - squares of frequencies of 

normal modes of vibration

(acoustics/electromagnetics, etc.)

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Eigenvalues

• Laplacian - squares of frequencies of 

normal modes of vibration

(acoustics/electromagnetics, etc.)

• Schrödinger Operator - energies of an atom

or quantum system.

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The spectral theorem for a general self-

adjoint operator

• The spectrum can be any closed subset of R.

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The spectral theorem for a general self-

adjoint operator

• For each u, there exists a measure µ, such that

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The spectral theorem for a general self-

adjoint operator

• Implication:

 – If f(λ) ≥ g(λ) on the spectrum, then

 – <u, f(H) u>  ≥ <u, g(H) u> 

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The spectrum of H

• For Laplace or Schrödinger not just any old

set of numbers can be the spectrum!

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“Universal” constraints on the spectrum

• H. Weyl, 1910, Laplace, λn ~ n2/d

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“Universal” constraints on the spectrum• H. Weyl, 1910, Laplace, λn ~ n2/d

• W. Kuhn, F. Reiche, W. Thomas, W. Heisenberg,

1925, “sum rules” for atomic energies.

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“Universal” constraints on the spectrum• H. Weyl, 1910, Laplace, λn ~ n2/d

• W. Kuhn, F. Reiche, W. Thomas, W. Heisenberg,1925, “sum rules” for atomic energies.

• L. Payne, G. Pólya, H. Weinberger, 1956: Thegap is controlled by the average of the smallereigenvalues:

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“Universal” constraints on the spectrum• H. Weyl, 1910, Laplace, λn ~ n2/d

• W. Kuhn, F. Reiche, W. Thomas, W. Heisenberg,1925, “sum rules” for atomic energies.

• L. Payne, G. Pólya, H. Weinberger, 1956: Thegap is controlled by the average of the smallereigenvalues:

• E. Lieb and W. Thirring, 1977, P. Li, S.T. Yau,

1983, sums of powers of eigenvalues, in terms of the phase-space volume.

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“Universal” constraints on the spectrum• H. Weyl, 1910, Laplace, λn ~ n2/d

• W. Kuhn, F. Reiche, W. Thomas, W. Heisenberg, 1925,“sum rules” for atomic energies.

• L. Payne, G. Pólya, H. Weinberger, 1956: The gap iscontrolled by the average of the smaller eigenvalues:

• E. Lieb and W. Thirring, 1977, P. Li, S.T. Yau, 1983,sums of powers of eigenvalues, in terms of the phase-spacevolume.

• Hile-Protter, 1980, Like PPW, but morecomplicated.

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PPW vs. HP

• L. Payne, G. Pólya, H. Weinberger, 1956:

• Hile-Protter, 1980:

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The universal industry after PPW

• Ashbaugh-Benguria 1991, proof of the

isoperimetric conjecture of PPW.

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“Universal” constraints on eigenvalues

• Ashbaugh-Benguria 1991, isoperimetric conjecture of 

PPW proved.

• H. Yang 1991-5, unpublished, complicated formulae likePPW, respecting Weyl asymptotics.

• Harrell, Harrell-Michel, Harrell-Stubbe, 1993-present,

commutators.

• Hermi PhD thesis

• Levitin-Parnovsky, 2001?

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In this industry….

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In this industry….

1. The arguments have varied, but always

essentially algebraic.

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In this industry….

1. The arguments have varied, but always

essentially algebraic.

2. Geometry often shows up - isoperimetric

theorems, etc.

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On a (hyper) surface,what object is most like

the Laplacian?

(Δ = the good old flat scalar Laplacian of Laplace)

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• Answer #1 (Beltrami’s answer): Consider

only tangential variations.

• At a fixed point, orient Cartesian x0 with the

normal, then calculate

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Difficulty:

• The Laplace-Beltrami operator is an

intrinsic object, and as such is unaware

that the surface is immersed!

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Answer #2

The nanophysicists’ answer• E.g., Da Costa, Phys. Rev. A 1981

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Answer #2:

- ΔLB + q,

Where the effective potential q responds to

how the surface is immersed in space.

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Nanoelectronics

• Nanoscale = 10-1000 X width of atom

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Nanoelectronics

• Nanoscale = 10-1000 X width of atom

• Foreseen by Feynman in 1960s

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Nanoelectronics

• Nanoscale = 10-1000 X width of atom

• Foreseen by Feynman in 1960s

• Laboratories by 1990.

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Nanoelectronics• Quantum wires - etched semiconductors,

wires of gold in carbon nanotubes.

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Nanoelectronics• Quantum wires

• Quantum waveguides - macroscopic in two

dimensions, nanoscale in the width

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Nanoelectronics• Quantum wires

• Quantum waveguides

• Designer potentials - STM places individual

atoms on a surface

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• Answer #2 (The nanoanswer):

  - ΔLB + q

• Since Da Costa, PRA, 1981: Perform a

singular limit and renormalization toattain the surface as the limit of a thindomain.

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Thin domain of fixed width

variable r= distance from edge

Energy form in separated variables:

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Energy form in separated variables:

First term is the energy form of Laplace-Beltrami.

Conjugate second term so as to replace it by a potential.

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Some subtleties• The limit is singular - change of dimension.

• If the particle is confined e.g. by Dirichlet

boundary conditions, the energies all

diverge to +infinity

• “Renormalization” is performed to separate

the divergent part of the operator.

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The result:

- ΔLB + q,

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Principal curvatures

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The result:

- ΔLB + q,

d=1, q = -κ2/4 ≤ 0 d=2, q = - (κ1-κ2)2/4 ≤ 0

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Consequence of q(x) ≤ 0:

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Consequence of q(x) ≤ 0:• If there is any bending at all, and the wire or

waveguide is large and asymptotically flat,

then there is always a bound state below theconduction level.

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Consequence of q(x) ≤ 0:• If there is any bending at all, and the wire or

waveguide is large and asymptotically flat,

then there is always a bound state below theconduction level.

• By bending or straightening the wire,

current can be switched off or on.

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Difficulty:

• Tied to a particular physical model -

other effective potentials arise from other

physical models or limits.

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Some other answers• In other physical situations, such as

reaction-diffusion, q(x) may be other

quadratic expressions in the curvature,usually q(x) ≤ 0.

• The conformal answer: q(x) is a

multiple of the scalar curvature.

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Heisenberg's Answer(if he had thought about it)

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Heisenberg's Answer(if he had thought about it)

Note: q(x) ≥ 0 !

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Commutators: [A,B] := AB-BA

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Commutators: [A,B] := AB-BA

1. Quantum mechanics is the effect thatobservables do not commute:

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• Canonical commutation:

[Q, P] = i

• Equations of motion, “Heisenberg picture”

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Canonical commutation

[Q, P] = i

= 1

Represented by Q = x, P = - i d/dx

Canonical commutation is then just

the product rule:

Set

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Commutators: [A,B] := AB-BA2. Eigenvalue gaps are connected to commutators:

H uk =λ

k uk , H self-adjoint

Elementary gap formula:

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Commutators: [A,B] := AB-BA

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What do you get whenyou put canonical

commutation togetherwith the gap formula?

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Commutators and gaps

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The fundamental eigenvalue gap

• In quantum mechanics, an excitation energy

• In “spectral geometry” a geometric quantity

small gaps indicate decoupling (dumbbells)

(Cheeger, Yang-Yau, etc.)

large gaps indicate convexity/isoperimetric(Ashbaugh-Benguria)

  Γ := λ2 - λ1

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Gap Lemma

H = your favorite self-adjoint operator, u1 thefundamental eigenfunction, and G is whatever you

want.

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Gap Lemma

H = your favorite self-adjoint operator, u1 thefundamental eigenfunction, and G is whatever you

want. CHOOSE IT WELL!

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Commutators and gaps

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Commutators and gaps

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Commutators and gaps

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But on the spectrum,

(λ - λ1) (λ2 - λ1) ≤ (λ - λ1)2

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Universal Bounds using Commutators

 – Play off canonical commutation relations

against the specific form of the operator:H = p2 + V(x)

 – Insert projections, take traces.

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Universal Bounds using Commutators

• A “sum rule” identity (Harrell-Stubbe, 1997):

Here, H is any Schrödinger operator, p is the gradient

(times -i if you are a physicist and you use atomic units)

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Universal Bounds with Commutators

• Compare with Hile-Protter:

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Universal Bounds with Commutators

• No sum on j - multiply by f(λ j), sum and

symmetrize

• Numerator only kinetic energy - no

potential.

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Among the consequences:

• All gaps: [λn,λn+1] ⊆ [λ-(n),λ+(n)], where

• The constant σ is a bound for the kinetic

energy/total energy. (σ

=1 for Laplace, but1/2 for the harmonic oscillator)

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Among the consequences:

• All gaps: [λn,λn+1] ⊆ [λ-(n),λ+(n)], where

• Dn is a statistical quantity calculated from

the lower eigenvalues.

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Among the consequences:

• All gaps: [λn,λn+1] ⊆ [λ-(n),λ+(n)], where

• Sharp for the harmonic oscillator for all n!

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And now for some completely

different commutators….

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Commutators: [A,B] := AB-BA3. Curvature is the effect that motions do not commute:

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Commutators: [A,B] := AB-BA

• More formally (from, e.g., Chavel, Riemannian Geometry, A Modern

 Introduction: Given vector fields X,Y,Zand a connection ∇, the curvature tensor isgiven by:

R(X,Y) = [∇Y ,∇X ] - ∇[Y,X]

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Commutators: [A,B] := AB-BA3a. The equations of space curves are commutators:

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Commutators: [A,B] := AB-BA3a. The equations of space curves are commutators:

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Commutators: [A,B] := AB-BA3a. The equations of space curves are commutators:

Note: curvature is defined by a second commutator

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The Serret-Frenet equations as

commutator relations:

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Sum on m and integrate. QED

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Sum on m and integrate. QED

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Interpretation:

Algebraically, for quantum mechanics on a

wire, the natural H0

is not

  p2,

but rather

H1/4 := p2 + κ2/4.

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That is, the gap for any H is

controlled by an expectation value

of H1/4.

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Bound is sharp for the circle:

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Gap bounds for (hyper) surfaces

Here h is the sum of the principal curvatures.

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where

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Bound is sharp for the sphere:

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Spinorial Canonical

Commutation

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Spinorial Canonical

Commutation

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Sum Rules

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Corollaries of sum rules

• Sharp universal bounds for all gaps

• Some estimates of partition function

Z(t) = ∑ exp(-t λk)

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Speculations and open problems

• Can one obtain/improve Lieb-Thirring bounds as a

consequence of sum rules?

• Full understanding of spectrum of Hg.

What spectral data needed to determine the curve?

What is the bifurcation value for the minimizer of λ1?

• Physical understanding of Hg and of the spinorial operators

it is related to.

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Sharp universal bound

for all gaps

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Partition function

Z(t) := tr(exp(-tH)).

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Partition function

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which implies