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Operator Representations

An operator representation is a concrete coordinate form of an abstract operator. Depending on the chosen basis or representation map, the same operator can appear as a matrix, a multiplication rule, a differential expression, an integral kernel, or a diagonal spectral form.

The abstract operator is the basis-independent object. Its representative is the form used for a particular calculation. A valid change of representation must transform states, operators, inner products, and operator domains consistently.

This distinction is not cosmetic. It explains why momentum is a derivative in position space but a multiplier in momentum space, why a local potential becomes a momentum-mixing kernel, and why diagonal, sparse, or real-looking matrices are generally properties of a representation rather than of the operator itself.

Helpful background. Bases and representations explain state coordinates; change of basis gives the overlap-matrix convention used below.

Let AA be an operator on a Hilbert space H\mathcal H, with domain D(A)D(A) when AA is unbounded. A representation R\mathcal R is implemented by a unitary map

UR:H⟶KR,\mathcal U_{\mathcal R}: \mathcal H\longrightarrow\mathcal K_{\mathcal R},

where KR\mathcal K_{\mathcal R} is a coordinate Hilbert space such as Cn\mathbb C^n, ℓ2\ell^2, or L2(X,dμ)L^2(X,d\mu). Define

ψR=UR∣ψ⟩,AR=URAUR†,D(AR)=URD(A).\begin{aligned} \psi_{\mathcal R} &=\mathcal U_{\mathcal R}\lvert\psi\rangle,\\ A_{\mathcal R} &=\mathcal U_{\mathcal R} A\mathcal U_{\mathcal R}^\dagger,\\ D(A_{\mathcal R}) &=\mathcal U_{\mathcal R}D(A). \end{aligned}

The represented action satisfies

ARψR=URA∣ψ⟩.A_{\mathcal R}\psi_{\mathcal R} = \mathcal U_{\mathcal R} A\lvert\psi\rangle.

This is the master translation rule. A matrix and a differential operator can represent the same AA because they act in different coordinate Hilbert spaces related by a unitary map.

One abstract operator mapped to discrete, position, momentum, and spectral representations

For a self-adjoint particle operator on L2(R)L^2(\mathbb R), these are alternative representations when their bases and domains are specified. A finite-level system instead uses coordinate spaces of its own dimension. Spectra, algebraic identities, and correctly paired predictions agree, while matrix entries and computational form can change.

If R\mathcal R and S\mathcal S are two representations, the unitary map between their coordinate spaces is

WSR=USUR†.W_{\mathcal S\mathcal R} = \mathcal U_{\mathcal S} \mathcal U_{\mathcal R}^\dagger.

Therefore

ψS=WSRψR,AS=WSRARWSR†,D(AS)=WSRD(AR).\begin{aligned} \psi_{\mathcal S} &=W_{\mathcal S\mathcal R} \psi_{\mathcal R},\\ A_{\mathcal S} &=W_{\mathcal S\mathcal R} A_{\mathcal R} W_{\mathcal S\mathcal R}^\dagger,\\ D(A_{\mathcal S}) &=W_{\mathcal S\mathcal R} D(A_{\mathcal R}). \end{aligned}

The detailed passive-basis convention and its alternatives are developed in Change of Basis. The practical rule is simple:

Never transform a state representative without transforming the operator representative and the inner product convention that go with it.

Predictions Are Representation Independent

Section titled “Predictions Are Representation Independent”

Unitarity gives

⟨ϕ∣A∣ψ⟩=⟨ϕR,ARψR⟩KR,∥Aψ∥=∥ARψR∥.\begin{aligned} \langle\phi\rvert A\lvert\psi\rangle &= \langle\phi_{\mathcal R}, A_{\mathcal R}\psi_{\mathcal R}\rangle_{\mathcal K_{\mathcal R}},\\ \lVert A\psi\rVert &= \lVert A_{\mathcal R}\psi_{\mathcal R}\rVert. \end{aligned}

Thus expectation values, transition amplitudes, and probabilities do not depend on the representation when every ingredient is translated consistently. This invariance is a useful error detector: two representations that give different predictions have not been matched correctly.

Let {∣en⟩}\{\lvert e_n\rangle\} be a finite or countably infinite orthonormal basis. To define the matrix elements of an unbounded AA, require each en∈D(A)e_n\in D(A). The state coordinates and operator matrix elements are

cn=⟨en∣ψ⟩,Amn=⟨em∣A∣en⟩.c_n=\langle e_n\vert\psi\rangle, \qquad A_{mn}=\langle e_m\rvert A\lvert e_n\rangle.

In finite dimensions, or for bounded AA in a countable basis, the represented action is matrix multiplication:

(Ac)m=∑nAmncn.(A c)_m = \sum_n A_{mn}c_n.

In finite dimension the operator can be reconstructed as

A=∑m,n∣em⟩Amn⟨en∣.A = \sum_{m,n} \lvert e_m\rangle A_{mn} \langle e_n\rvert.

For bounded AA in an infinite basis, use finite compressions PNAPNP_NAP_N, which converge strongly to AA as PN→IP_N\to I. For unbounded AA, even ψ∈D(A)\psi\in D(A) does not guarantee that arbitrary basis truncations converge in the graph norm ∥ψ∥2+∥Aψ∥2\sqrt{\|\psi\|^2+\|A\psi\|^2}; the domain and convergence must be established separately. This formula makes the distinction precise: AA is the map, while [Amn][A_{mn}] is its coordinate array in the named basis. The underlying linear algebra is reviewed in Matrices as Linear Maps.

For finite matrices in one orthonormal basis,

(AB)mn=∑kAmkBkn,(A†)mn=Anm∗,[A,B]mn=∑k(AmkBkn−BmkAkn).\begin{aligned} (AB)_{mn} &=\sum_k A_{mk}B_{kn},\\ (A^\dagger)_{mn} &=A_{nm}^*,\\ [A,B]_{mn} &=\sum_k \bigl(A_{mk}B_{kn}-B_{mk}A_{kn}\bigr). \end{aligned}

For a finite matrix, self-adjointness becomes Amn=Anm∗A_{mn}=A_{nm}^*, and unitarity becomes A†A=IA^\dagger A=I. These matrix conditions express invariant operator properties in a particular orthonormal basis.

In an infinite basis, formal matrix multiplication can hide convergence and domain issues. A coefficient sequence can represent a vector outside D(A)D(A) even when each basis vector lies in D(A)D(A) and every matrix element is finite.

Let SS be the overlap matrix that sends old state components to new ones:

d=Sc.d=Sc.

With this convention, the operator matrix transforms as

Anew=SAoldS†.A_{\mathrm{new}} = S A_{\mathrm{old}}S^\dagger.

The expectation value remains unchanged:

d†Anewd=c†Aoldc.d^\dagger A_{\mathrm{new}}d = c^\dagger A_{\mathrm{old}}c.

Other books may define the overlap matrix in the opposite direction and write the inverse-looking conjugation. The physics agrees once the state and operator conventions are paired.

A continuous representation uses generalized kets {∣q⟩}\{\lvert q\rangle\} satisfying a distributional completeness relation

∫X∣q⟩⟨q∣ dμ(q)=I.\int_X \lvert q\rangle\langle q\rvert \,d\mu(q)=I.

The state representative is the wavefunction

ψ(q)=⟨q∣ψ⟩.\psi(q)=\langle q\vert\psi\rangle.

The generalized kets need not be normalizable vectors in H\mathcal H. They are distributional tools whose precise setting is explained in Generalized Eigenvectors. The physical state remains the normalizable vector reconstructed from its wavefunction.

The continuous analogue of a matrix element is the kernel

A(q,q′)=⟨q∣A∣q′⟩.A(q,q') = \langle q\rvert A\lvert q'\rangle.

It acts by

(Aψ)(q)=∫XA(q,q′)ψ(q′) dμ(q′).(A\psi)(q) = \int_X A(q,q')\psi(q') \,d\mu(q').

For ordinary kernels and sufficient integrability to interchange integrals, matrix algebra becomes

(AB)(q,q′)=∫XA(q,r)B(r,q′) dμ(r),A†(q,q′)=A(q′,q)∗.\begin{aligned} (AB)(q,q') &=\int_X A(q,r)B(r,q') \,d\mu(r),\\ A^\dagger(q,q') &=A(q',q)^*. \end{aligned}

The identity kernel is the delta distribution appropriate to the measure:

I(q,q′)=δμ(q,q′).I(q,q')=\delta_\mu(q,q').

These formulas are not permission to multiply arbitrary distributions. Kernels need not be ordinary functions. Differential operators are represented by derivatives of delta distributions, and singular interactions may require additional distributional care.

For a spinless particle on the line with canonical momentum and no vector potential,

ψ(x)=⟨x∣ψ⟩.\psi(x)=\langle x\vert\psi\rangle.

The position and momentum operators act as

(Qψ)(x)=xψ(x),(Pψ)(x)=−iℏdψdx.\begin{aligned} (Q\psi)(x)&=x\psi(x),\\ (P\psi)(x)&=-i\hbar\frac{d\psi}{dx}. \end{aligned}

For the common Hamiltonian

H=P22m+V(Q),H=\frac{P^2}{2m}+V(Q),

the position representative is

(Hψ)(x)=[−ℏ22md2dx2+V(x)]ψ(x).(H\psi)(x) = \left[ -\frac{\hbar^2}{2m}\frac{d^2}{dx^2} +V(x) \right]\psi(x).

These differential expressions are incomplete without domains and boundary conditions. For example, the same formal derivative can describe different self-adjoint momentum operators on different configuration spaces.

The preceding actions can be written as kernels:

Q(x,x′)=x δ(x−x′),P(x,x′)=−iℏ ∂xδ(x−x′),V(Q)(x,x′)=V(x)δ(x−x′).\begin{aligned} Q(x,x') &=x\,\delta(x-x'),\\ P(x,x') &=-i\hbar\,\partial_x\delta(x-x'),\\ V(Q)(x,x') &=V(x)\delta(x-x'). \end{aligned}

For the Hamiltonian,

H(x,x′)=[−ℏ22m∂x2+V(x)]δ(x−x′).H(x,x') = \left[ -\frac{\hbar^2}{2m}\partial_x^2 +V(x) \right]\delta(x-x').

The derivative acts on the xx variable. After integration against ψ(x′)\psi(x'), the delta distribution reproduces the familiar differential operator.

Choose the convention

⟨x∣p⟩=12πℏeipx/ℏ.\langle x\vert p\rangle = \frac{1}{\sqrt{2\pi\hbar}} e^{ipx/\hbar}.

The momentum-space wavefunction is ϕ(p)=⟨p∣ψ⟩\phi(p)=\langle p\vert\psi\rangle. In this representation,

(Pϕ)(p)=pϕ(p),(Qϕ)(p)=iℏdϕdp.\begin{aligned} (P\phi)(p)&=p\phi(p),\\ (Q\phi)(p)&=i\hbar\frac{d\phi}{dp}. \end{aligned}

The free Hamiltonian is a multiplication operator:

(H0ϕ)(p)=p22mϕ(p).(H_0\phi)(p) = \frac{p^2}{2m}\phi(p).

The Fourier transform, normalization, and domain details are developed in Momentum-Space Representation.

A Local Potential Becomes Nonlocal in Momentum

Section titled “A Local Potential Becomes Nonlocal in Momentum”

For an integrable potential VV, position-space multiplication has momentum-space kernel

V(p,p′)=⟨p∣V(Q)∣p′⟩=12πℏ∫Re−i(p−p′)x/ℏV(x) dx.\begin{aligned} V(p,p') &=\langle p\rvert V(Q)\lvert p'\rangle\\ &=\frac{1}{2\pi\hbar} \int_{\mathbb R} e^{-i(p-p')x/\hbar}V(x)\,dx. \end{aligned}

Therefore

(Vϕ)(p)=∫RV(p,p′)ϕ(p′) dp′.(V\phi)(p) = \int_{\mathbb R} V(p,p')\phi(p')\,dp'.

For polynomial or other suitable tempered potentials, interpret this Fourier integral distributionally on test functions; for more singular cases define the transformed operator and its domain first. A local potential generally mixes momenta. Conversely, a function of momentum is multiplicative in momentum space but generally nonlocal in position space. This is a concrete demonstration that computational locality depends on the chosen representation.

For spin 1/21/2, choose the SzS_z eigenbasis. Then

Sz=ℏ2(100−1),S_z = \frac{\hbar}{2} \begin{pmatrix} 1&0\\ 0&-1 \end{pmatrix},

while

Sx=ℏ2(0110).S_x = \frac{\hbar}{2} \begin{pmatrix} 0&1\\ 1&0 \end{pmatrix}.

In the SxS_x eigenbasis, SxS_x is diagonal and SzS_z is off-diagonal. Their eigenvalues and commutation relation do not change. The matrix pattern changes because the state-space basis has changed. The physical laboratory spin axes are held fixed in this passive calculation.

The canonical matrix identities are collected in Pauli Matrices.

If a time-independent self-adjoint HH has a complete orthonormal discrete energy eigenbasis,

H∣En⟩=En∣En⟩,H\lvert E_n\rangle=E_n\lvert E_n\rangle,

then

Hmn=Enδmn.H_{mn}=E_n\delta_{mn}.

The Schrödinger equation reduces to independent component equations:

iℏdcndt=Encn,i\hbar\frac{dc_n}{dt}=E_nc_n,

with solution

cn(t)=e−iEnt/ℏcn(0).c_n(t)=e^{-iE_nt/\hbar}c_n(0).

This simplicity is why the energy representation is adapted to a time-independent Hamiltonian. A different observable AA need not be diagonal in the same basis; its off-diagonal matrix elements connect energy sectors.

Degeneracy leaves freedom to rotate the basis inside an energy eigenspace. A complete set of commuting observables can supply additional labels. Continuous energy spectra require delta normalization and possible multiplicity labels rather than a simple list of normalizable vectors.

Worked Example: The Oscillator in Two Representations

Section titled “Worked Example: The Oscillator in Two Representations”

For the one-dimensional harmonic oscillator, position representation gives

(Qψ)(x)=xψ(x),(Hψ)(x)=[−ℏ22md2dx2+12mω2x2]ψ(x).\begin{aligned} (Q\psi)(x)&=x\psi(x),\\ (H\psi)(x) &=\left[ -\frac{\hbar^2}{2m}\frac{d^2}{dx^2} +\frac12m\omega^2x^2 \right]\psi(x). \end{aligned}

In the number basis {∣n⟩}\{\lvert n\rangle\}, the Hamiltonian is diagonal:

Hnm=ℏω(n+12)δnm.H_{nm} = \hbar\omega \left(n+\frac12\right) \delta_{nm}.

Writing q0=ℏ/(2mω)q_0=\sqrt{\hbar/(2m\omega)}, position is instead tridiagonal:

Qnm=q0⟨n∣(a+a†)∣m⟩=q0[m δn,m−1+m+1 δn,m+1].\begin{aligned} Q_{nm} &=q_0 \langle n\rvert(a+a^\dagger)\lvert m\rangle\\ &=q_0 \left[ \sqrt m\,\delta_{n,m-1} +\sqrt{m+1}\,\delta_{n,m+1} \right]. \end{aligned}

The multiplication operator and the infinite tridiagonal matrix are two exact representatives of the same abstract QQ. Truncating the matrix to finitely many number states is a separate approximation.

For a product basis

∣i,α⟩=∣i⟩A⊗∣α⟩B,\lvert i,\alpha\rangle = \lvert i\rangle_A\otimes\lvert\alpha\rangle_B,

a local operator has matrix elements

(XA⊗IB)iα,jβ=(XA)ijδαβ.(X_A\otimes I_B)_{i\alpha,j\beta} = (X_A)_{ij}\delta_{\alpha\beta}.

Changing local bases conjugates the matrix by UA⊗UBU_A\otimes U_B. The abstract tensor-product operator and its locality to subsystem AA remain unchanged. The physical interpretation is developed in Subsystems and Local Observables.

For an unbounded operator, the pair (A,D(A))(A,D(A)) is the operator. Under a unitary representation map,

D(AR)=URD(A).D(A_{\mathcal R}) = \mathcal U_{\mathcal R}D(A).

This condition preserves self-adjointness:

A=A†⟺AR=AR†,A=A^\dagger \quad\Longleftrightarrow\quad A_{\mathcal R}=A_{\mathcal R}^\dagger,

where each adjoint is taken with its correct Hilbert-space inner product and domain.

A formal differential expression without a domain is not a complete representation of an unbounded operator. The canonical domain theory is in Domains of Operators and Hermitian vs Self-Adjoint Operators.

Active Transformations Are a Different Question

Section titled “Active Transformations Are a Different Question”

The conjugation A↦UAU†A\mapsto UAU^\dagger can appear in two conceptually distinct uses:

  • A passive representation change rewrites the same state and operator in new coordinates. Predictions are unchanged because all representatives are transformed together.
  • An active physical transformation changes the state, apparatus, or observable relative to a fixed coordinate description. It can represent a rotation, translation, symmetry operation, or time evolution.

The same matrix algebra can occur in both descriptions. One must state what is held fixed before assigning physical meaning.

Exact Representation Change versus Truncation

Section titled “Exact Representation Change versus Truncation”

A unitary change of representation is exact and preserves the full operator. A finite truncation instead replaces AA by a compression such as

A(N)=PNAPN∣PNH.A^{(N)} = P_NAP_N \big\rvert_{P_N\mathcal H}.

For an unbounded AA, this finite matrix is defined when the retained basis vectors lie in D(A)D(A). It is generally not unitarily equivalent to AA. It can change spectra, domains, commutators, and long-time dynamics. For example, finite matrices cannot satisfy the canonical commutator exactly because

Tr⁡[X,P]=0,\operatorname{Tr}[X,P]=0,

whereas

Tr⁡(iℏIN)=iℏN.\operatorname{Tr}(i\hbar I_N) = i\hbar N.

Numerical basis calculations must therefore be checked for convergence as the truncation grows. The approximation strategy belongs to Discretization.

Unitary equivalence preserves:

  • the spectrum, including multiplicities and spectral type;
  • self-adjointness, positivity, unitarity, and normality;
  • operator norms and trace-class quantities when they are defined;
  • products, adjoints, commutators, and functional identities;
  • expectation values, transition amplitudes, and measurement probabilities;
  • the dimension of kernels and spectral subspaces;
  • the transformed domain structure of unbounded operators.

The following are generally representation dependent:

  • state components and pointwise wavefunction values;
  • individual matrix elements;
  • whether a representative is diagonal, sparse, banded, real, or dense;
  • whether an operator looks multiplicative, differential, or integral;
  • which couplings appear as off-diagonal entries;
  • the computational cost of applying the representative.

An invariant claim should survive unitary translation. A coordinate-dependent claim can still be useful, but its representation must be named.

  • Position representation exposes local spatial potentials, geometry, boundary conditions, and configuration-space probability density.
  • Momentum representation diagonalizes translations and free motion and turns derivatives into multipliers.
  • Energy representation simplifies time evolution under a time-independent Hamiltonian.
  • Spin or angular-momentum bases adapt calculations to a measurement axis or rotational symmetry.
  • Symmetry-adapted bases block-diagonalize operators by conserved quantum numbers.
  • Product bases expose subsystem structure and local operators.
  • Numerical bases are chosen for sparsity, convergence, conditioning, and efficient matrix-vector products.

There is no universally best representation. The best one makes the dominant operator, symmetry, or boundary condition simple without obscuring the quantity being computed.

Translate state and operator together. With d=Scd=Sc, use Anew=SAoldS†A_{\rm new}=SA_{\rm old}S^\dagger. Comparing dd with the old operator usually changes the expectation value because the coordinate conventions no longer match.

Keep the transformed domain. A derivative and a multiplier can represent the same self-adjoint momentum operator only when the Fourier transform also maps their domains. Formal differential expressions alone do not establish unitary equivalence.

Separate basis change from approximation. A finite compression discards components. It may approximate low-energy predictions well while failing exact identities, as the oscillator commutator exercise below illustrates.

For a compact formula comparison, use the Representation Translation Table.

Exercise 1: Matrix action and reconstruction

Section titled “Exercise 1: Matrix action and reconstruction”

Let Amn=⟨em∣A∣en⟩A_{mn}=\langle e_m\rvert A\lvert e_n\rangle in a finite orthonormal basis. Derive both

(Ac)m=∑nAmncn(Ac)_m=\sum_nA_{mn}c_n

and the reconstruction formula for AA.

Solution

Insert completeness between the bra and the state:

⟨em∣A∣ψ⟩=∑n⟨em∣A∣en⟩⟨en∣ψ⟩=∑nAmncn.\begin{aligned} \langle e_m\rvert A\lvert\psi\rangle &=\sum_n \langle e_m\rvert A\lvert e_n\rangle \langle e_n\vert\psi\rangle\\ &=\sum_nA_{mn}c_n. \end{aligned}

Insert completeness on both sides of AA:

A=IAI=∑m,n∣em⟩⟨em∣A∣en⟩⟨en∣=∑m,n∣em⟩Amn⟨en∣.\begin{aligned} A &=IAI\\ &=\sum_{m,n} \lvert e_m\rangle \langle e_m\rvert A\lvert e_n\rangle \langle e_n\rvert\\ &=\sum_{m,n} \lvert e_m\rangle A_{mn}\langle e_n\rvert. \end{aligned}

In the SzS_z basis, let

σz=(100−1),S=12(111−1).\sigma_z= \begin{pmatrix} 1&0\\ 0&-1 \end{pmatrix}, \qquad S=\frac{1}{\sqrt2} \begin{pmatrix} 1&1\\ 1&-1 \end{pmatrix}.

Compute SσzS†S\sigma_zS^\dagger and interpret the result.

Solution

The matrix SS is real, symmetric, and unitary. Direct multiplication gives

SσzS†=(0110)=σx.S\sigma_zS^\dagger = \begin{pmatrix} 0&1\\ 1&0 \end{pmatrix} = \sigma_x.

The old zz-component operator is represented by σx\sigma_x in the basis of σx\sigma_x eigenvectors. Its eigenvalues remain ±1\pm1; only its coordinate matrix has changed.

Starting from

(Aψ)(q)=∫A(q,r)ψ(r) dμ(r),(A\psi)(q) = \int A(q,r)\psi(r)\,d\mu(r),

derive the kernels of ABAB and A†A^\dagger, assuming ordinary kernels and sufficient integrability for each interchange of integrals.

Solution

Apply BB first and substitute:

(ABψ)(q)=∫ ⁣ ⁣∫dμ(r) dμ(q′)×A(q,r)B(r,q′)ψ(q′).(AB\psi)(q) =\int\!\!\int d\mu(r)\,d\mu(q') \times A(q,r)B(r,q')\psi(q').

Therefore

(AB)(q,q′)=∫A(q,r)B(r,q′) dμ(r).(AB)(q,q') = \int A(q,r)B(r,q')\,d\mu(r).

Comparing ⟨ϕ,Aψ⟩\langle\phi,A\psi\rangle with ⟨A†ϕ,ψ⟩\langle A^\dagger\phi,\psi\rangle gives

A†(q,q′)=A(q′,q)∗.A^\dagger(q,q')=A(q',q)^*.

Exercise 4: Canonical commutator in position space

Section titled “Exercise 4: Canonical commutator in position space”

On the Schwartz space of smooth rapidly decreasing functions on the line, verify that Q=xQ=x and P=−iℏ d/dxP=-i\hbar\,d/dx satisfy [Q,P]ψ=iℏψ[Q,P]\psi=i\hbar\psi.

Solution

Compute the two orders:

(QPψ)(x)=−iℏxψ′(x),(PQψ)(x)=−iℏddx(xψ(x))=−iℏ(ψ(x)+xψ′(x)).\begin{aligned} (QP\psi)(x) &=-i\hbar x\psi'(x),\\ (PQ\psi)(x) &=-i\hbar\frac{d}{dx} \bigl(x\psi(x)\bigr)\\ &=-i\hbar\bigl(\psi(x)+x\psi'(x)\bigr). \end{aligned}

Subtracting gives

([Q,P]ψ)(x)=iℏψ(x).([Q,P]\psi)(x)=i\hbar\psi(x).

The calculation is valid on a domain where both compositions are defined. It does not by itself settle self-adjoint boundary conditions.

Using

ϕ(p)=12πℏ∫e−ipx/ℏψ(x) dx,\phi(p) = \frac{1}{\sqrt{2\pi\hbar}} \int e^{-ipx/\hbar}\psi(x)\,dx,

for a Schwartz wavefunction, show that multiplication by xx becomes iℏ d/dpi\hbar\,d/dp.

Solution

Let cℏ=(2πℏ)−1/2c_\hbar=(2\pi\hbar)^{-1/2}. Differentiating the transform gives

ϕ′(p)=−icℏℏ∫xe−ipx/ℏψ(x) dx.\phi'(p) = -\frac{i c_\hbar}{\hbar} \int x e^{-ipx/\hbar}\psi(x)\,dx.

Therefore

iℏϕ′(p)=cℏ∫e−ipx/ℏxψ(x) dx.i\hbar\phi'(p) = c_\hbar \int e^{-ipx/\hbar}x\psi(x)\,dx.

The final expression is the Fourier transform of QψQ\psi. Hence

Qp=iℏddpQ_p=i\hbar\frac{d}{dp}

on the transformed domain.

Use

Q=q0(a+a†),q0=ℏ2mω,Q=q_0(a+a^\dagger), \qquad q_0=\sqrt{\frac{\hbar}{2m\omega}},

to show that the number-basis matrix of QQ is tridiagonal.

Solution

The ladder actions are

a∣m⟩=m∣m−1⟩,a†∣m⟩=m+1∣m+1⟩.\begin{aligned} a\lvert m\rangle &=\sqrt m\lvert m-1\rangle,\\ a^\dagger\lvert m\rangle &=\sqrt{m+1}\lvert m+1\rangle. \end{aligned}

Therefore

Qnm=q0[m δn,m−1+m+1 δn,m+1].Q_{nm} =q_0\left[ \sqrt m\,\delta_{n,m-1} +\sqrt{m+1}\,\delta_{n,m+1} \right].

Only the first off-diagonals are nonzero, so the matrix is tridiagonal.

Exercise 7: Domain under Fourier transformation

Section titled “Exercise 7: Domain under Fourier transformation”

Let F\mathcal F be the unitary position-to-momentum Fourier transform and let Px=−iℏ d/dxP_x=-i\hbar\,d/dx be self-adjoint on its standard real-line domain. State the operator and domain of Pp=FPxF†P_p=\mathcal FP_x\mathcal F^\dagger.

Solution

Fourier transformation turns differentiation into multiplication, so

(Ppϕ)(p)=pϕ(p).(P_p\phi)(p)=p\phi(p).

The transformed domain is

D(Pp)={ϕ∈L2(R) | pϕ∈L2(R)}.D(P_p) = \left\{ \phi\in L^2(\mathbb R) \,\middle|\, p\phi\in L^2(\mathbb R) \right\}.

Equivalently, D(Pp)=FD(Px)D(P_p)=\mathcal F D(P_x). Carrying the domain through the unitary map is what preserves self-adjointness.

Exercise 8: The commutator at a truncation boundary

Section titled “Exercise 8: The commutator at a truncation boundary”

Retain oscillator number states ∣0⟩,…,∣N−1⟩|0\rangle,\ldots,|N-1\rangle. Let aNa_N and aN†a_N^\dagger be the compressed ladder matrices. Show that

[aN,aN†]=IN−N∣N−1⟩⟨N−1∣.[a_N,a_N^\dagger]=I_N-N|N-1\rangle\langle N-1|.

Use this to find [QN,PN][Q_N,P_N], where QN=q0(aN+aN†)Q_N=q_0(a_N+a_N^\dagger) and PN=ip0(aN†−aN)P_N=i p_0(a_N^\dagger-a_N) with q0p0=ℏ/2q_0p_0=\hbar/2.

Solution

For n<N−1n<N-1, both ladder paths are retained, so (aNaN†−aN†aN)∣n⟩=((n+1)−n)∣n⟩=∣n⟩(a_Na_N^\dagger-a_N^\dagger a_N)|n\rangle=((n+1)-n)|n\rangle=|n\rangle. At the top state, aN†∣N−1⟩=0a_N^\dagger|N-1\rangle=0, while aN†aN∣N−1⟩=(N−1)∣N−1⟩a_N^\dagger a_N|N-1\rangle=(N-1)|N-1\rangle. Thus the top diagonal entry is 1−N1-N, giving the stated result.

Consequently,

[QN,PN]=iℏ(IN−N∣N−1⟩⟨N−1∣).[Q_N,P_N]=i\hbar\bigl(I_N-N|N-1\rangle\langle N-1|\bigr).

Its trace is zero, as every finite matrix commutator requires. The correction acts entirely at the truncation boundary: states supported below the top level have the expected commutator expectation, but the full finite matrices do not satisfy the canonical relation.

  • B. C. Hall, Quantum Theory for Mathematicians, Springer, 2013. Publisher.
  • J. J. Sakurai and J. Napolitano, Modern Quantum Mechanics, 3rd ed., Cambridge University Press, 2020, Chapter 1. Publisher.
  • R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994.