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Expectation Value

For a normalized pure state and an observable AA,

⟨A⟩ψ=⟨ψ∣A∣ψ⟩.\langle A\rangle_\psi = \langle\psi\rvert A \lvert\psi\rangle.

For a density operator,

⟨A⟩ρ=Tr⁡(ρA).\langle A\rangle_\rho = \operatorname{Tr}(\rho A).

The most general spectral statement is

⟨A⟩ρ=∫Rλ dμρA(λ),\langle A\rangle_\rho = \int_{\mathbb R} \lambda\, d\mu_\rho^A(\lambda),

where

μρA(Δ)=Tr⁡[ρPA(Δ)]\mu_\rho^A(\Delta) = \operatorname{Tr} \left[ \rho P^A(\Delta) \right]

is the Born probability measure for the observable AA. The expectation exists as a finite number when the absolute first moment is finite:

∫R∣λ∣ dμρA(λ)<∞.\int_{\mathbb R} \lvert\lambda\rvert\, d\mu_\rho^A(\lambda) <\infty.
SettingExpectation value
Normalized pure state⟨A⟩ψ=⟨ψ∣A∣ψ⟩\langle A\rangle_\psi=\langle\psi\rvert A\lvert\psi\rangle
Density operator⟨A⟩ρ=Tr⁡(ρA)\langle A\rangle_\rho=\operatorname{Tr}(\rho A)
Discrete spectrum⟨A⟩=∑aa p(a)\langle A\rangle=\sum_a a\,p(a)
Continuous density⟨A⟩=∫λpA(λ) dλ\langle A\rangle=\int \lambda p_A(\lambda)\,d\lambda
General spectral measure⟨A⟩=∫λ dμA(λ)\langle A\rangle=\int\lambda\,d\mu^A(\lambda)
Finite-dimensional state vector⟨A⟩=c†Ac\langle A\rangle=\mathbf c^\dagger A\mathbf c
Position representation⟨A⟩=∫ψ∗(x)(Aψ)(x) dx\langle A\rangle=\int\psi^*(x)(A\psi)(x)\,dx
Mixed state in components⟨A⟩=∑i,jρijAji\langle A\rangle=\sum_{i,j}\rho_{ij}A_{ji}

The expectation value is the first moment of the probability distribution for measuring AA in the specified state. If identically prepared systems are measured independently and the first moment exists, their sample mean approaches ⟨A⟩\langle A\rangle in the large-sample limit.

An expectation value is not generally:

  • the result of one measurement;
  • an eigenvalue of AA;
  • the most probable outcome;
  • a value known to have existed before measurement.

For example, a spin component with possible outcomes ±ℏ/2\pm\hbar/2 can have expectation value zero. Zero summarizes the outcome distribution even though it is not an allowed result of that measurement.

If

A=∑aaPa,A = \sum_a aP_a,

then

p(a)=Tr⁡(ρPa)p(a) = \operatorname{Tr}(\rho P_a)

and

⟨A⟩ρ=∑aa p(a).\langle A\rangle_\rho = \sum_a a\,p(a).

The projector PaP_a contains the full eigenspace for eigenvalue aa, so the same formula handles degeneracy. For a normalized pure state with an orthonormal eigenbasis {∣a,r⟩}\{\lvert a,r\rangle\},

⟨A⟩ψ=∑a,ra∣⟨a,r∣ψ⟩∣2.\langle A\rangle_\psi = \sum_{a,r} a \lvert \langle a,r\rvert\psi\rangle \rvert^2.

The degeneracy label rr is summed because the observable reports aa, not an unresolved basis label inside its eigenspace.

If the Born distribution has a density pA(λ)p_A(\lambda) with respect to dλd\lambda,

⟨A⟩=∫−∞∞λpA(λ) dλ.\langle A\rangle = \int_{-\infty}^{\infty} \lambda p_A(\lambda)\,d\lambda.

For one-dimensional position,

⟨X⟩ψ=∫−∞∞x∣ψ(x)∣2 dx.\langle X\rangle_\psi = \int_{-\infty}^{\infty} x \lvert\psi(x)\rvert^2\,dx.

An observable can have both discrete and continuous spectral parts. In a common notation,

⟨A⟩=∑nanwn+∫Rλpac(λ) dλ.\langle A\rangle = \sum_n a_nw_n + \int_{\mathbb R} \lambda p_{\mathrm{ac}}(\lambda)\,d\lambda.

Omitting either occupied part of a mixed spectrum gives the wrong mean. The spectral-measure formula includes all parts without requiring a separate case split.

For a normalized column vector c\mathbf c and Hermitian matrix AA,

⟨A⟩=c†Ac.\langle A\rangle = \mathbf c^\dagger A\mathbf c.

For a density matrix,

⟨A⟩=Tr⁡(ρA)=∑i,jρijAji.\langle A\rangle = \operatorname{Tr}(\rho A) = \sum_{i,j} \rho_{ij}A_{ji}.

The second expression shows that off-diagonal entries can contribute. Only in a basis that diagonalizes AA does the expectation reduce to a weighted sum of diagonal state entries:

⟨A⟩=∑aa ρaa\langle A\rangle = \sum_a a\,\rho_{aa}

for a nondegenerate eigenbasis.

For numerical work, use a conjugate transpose, not an ordinary transpose. A significant imaginary part in the expectation of a Hermitian matrix usually indicates a non-Hermitian input, a missing complex conjugation, inconsistent basis conventions, or numerical error.

In one-dimensional position representation,

⟨A⟩ψ=∫−∞∞ψ∗(x)(Aψ)(x) dx.\langle A\rangle_\psi = \int_{-\infty}^{\infty} \psi^*(x) (A\psi)(x)\,dx.

For a multiplication operator f(x^)f(\hat x),

⟨f(x^)⟩=∫−∞∞f(x)∣ψ(x)∣2 dx.\langle f(\hat x)\rangle = \int_{-\infty}^{\infty} f(x) \lvert\psi(x)\rvert^2\,dx.

For momentum,

⟨p^⟩=∫−∞∞ψ∗(x)(−iℏddx)ψ(x) dx.\langle \hat p\rangle = \int_{-\infty}^{\infty} \psi^*(x) \left( -i\hbar\frac{d}{dx} \right) \psi(x)\,dx.

Apply the differential operator to the wavefunction before multiplying by ψ∗\psi^*. Boundary behavior and the operator domain are part of the formula. Integration by parts can demonstrate reality only when its boundary term is justified.

In several dimensions or curvilinear coordinates, use the correct measure:

⟨A⟩=∫ψ∗(q)(Aψ)(q) dμ(q).\langle A\rangle = \int \psi^*(q) (A\psi)(q) \,d\mu(q).

For spherical coordinates,

dμ=r2sin⁡θ dr dθ dϕ.d\mu = r^2\sin\theta \,dr\,d\theta\,d\phi.

For a nonzero but unnormalized vector ∣ψ~⟩\lvert\widetilde\psi\rangle,

⟨A⟩=⟨ψ~∣A∣ψ~⟩⟨ψ~∣ψ~⟩.\langle A\rangle = \frac{ \langle\widetilde\psi\rvert A \lvert\widetilde\psi\rangle }{ \langle\widetilde\psi \vert \widetilde\psi\rangle }.

For a positive trace-class operator ρ~\widetilde\rho with nonzero trace,

⟨A⟩=Tr⁡(ρ~A)Tr⁡ρ~.\langle A\rangle = \frac{ \operatorname{Tr} (\widetilde\rho A) }{ \operatorname{Tr}\widetilde\rho }.

The denominators are essential. They do not repair a vector outside the relevant operator or form domain, nor an operator that fails positivity.

For a suitable function ff,

⟨f(A)⟩ρ=∫Rf(λ) dμρA(λ).\langle f(A)\rangle_\rho = \int_{\mathbb R} f(\lambda) \,d\mu_\rho^A(\lambda).

The nnth moment is

⟨An⟩ρ=Tr⁡(ρAn),\langle A^n\rangle_\rho = \operatorname{Tr}(\rho A^n),

when it exists. The variance is

(ΔA)2=⟨A2⟩−⟨A⟩2.(\Delta A)^2 = \langle A^2\rangle -\langle A\rangle^2.

The notation ⟨A⟩2\langle A\rangle^2 means the square of the first moment. It is not the same as ⟨A2⟩\langle A^2\rangle.

Expectation is linear:

⟨αA+βB⟩=α⟨A⟩+β⟨B⟩,\langle \alpha A+\beta B \rangle = \alpha\langle A\rangle +\beta\langle B\rangle,

whenever the terms are defined. The operators AA and BB need not commute for this identity.

Linearity does not imply factorization:

⟨AB⟩≠⟨A⟩⟨B⟩\langle AB\rangle \neq \langle A\rangle \langle B\rangle

in general. Products can depend on correlations and operator ordering. If ABAB is not self-adjoint, its expectation may be complex even when AA and BB are individually observables.

For a bipartite state ρAB\rho_{AB} and a local observable AA on subsystem AA,

⟨A⟩=Tr⁡AB[ρAB(A⊗IB)].\langle A\rangle = \operatorname{Tr}_{AB} \left[ \rho_{AB} (A\otimes I_B) \right].

With the reduced state

ρA=Tr⁡BρAB,\rho_A = \operatorname{Tr}_B\rho_{AB},

the same expectation is

⟨A⟩=Tr⁡A(ρAA).\langle A\rangle = \operatorname{Tr}_A(\rho_AA).

The identity on the untouched subsystem is often suppressed. Restoring it prevents dimension and tensor-order mistakes.

For a Schrödinger-picture state evolving under H(t)H(t) and an operator A(t)A(t),

ddt⟨A⟩=iℏ⟨[H,A]⟩+⟨∂A∂t⟩,\frac{d}{dt} \langle A\rangle = \frac{i}{\hbar} \langle[H,A]\rangle + \left\langle \frac{\partial A}{\partial t} \right\rangle,

under the regularity and domain assumptions required for differentiation. If AA has no explicit time dependence and commutes with HH, its expectation is conserved.

This equation concerns evolution of the mean. It does not replace the expectation formula; it is obtained by differentiating that formula using the equation of motion.

SymbolMathematical typeMeaning
AAUsually self-adjoint operatorObservable
ρ\rhoPositive trace-one operatorGeneral quantum state
∣ψ⟩\lvert\psi\rangleNormalized vector up to phasePure state
PaP_aSpectral projectorEvent associated with eigenvalue aa
μρA\mu_\rho^AProbability measureBorn distribution of AA in state ρ\rho
pA(λ)p_A(\lambda)Probability densityDensity of continuous outcomes
⟨A⟩ρ\langle A\rangle_\rhoScalarExpectation of AA in state ρ\rho
ΔA\Delta ANonnegative scalarStandard deviation of AA

The state subscript is often omitted when context makes it unambiguous.

An expectation value has the same physical dimensions as the observable:

[⟨A⟩]=[A].[\langle A\rangle]=[A].

More generally,

[⟨An⟩]=[A]n,[ΔA]=[A].[\langle A^n\rangle]=[A]^n, \qquad [\Delta A]=[A].

In a continuous formula, pA(λ)p_A(\lambda) has inverse units of λ\lambda, so

λpA(λ) dλ\lambda p_A(\lambda)\,d\lambda

has the units of AA. The density matrix and normalized state vector are dimensionless abstract objects, although their coordinate components can carry measure-dependent units.

For bounded AA, every Hilbert-space vector has a finite vector expectation. For unbounded self-adjoint AA, several related conditions must be distinguished:

  • The literal vector expression ⟨ψ∣A∣ψ⟩\langle\psi\rvert A\lvert\psi\rangle requires ψ∈D(A)\psi\in\mathcal D(A).
  • A finite spectral first moment requires
∫R∣λ∣ dμψA(λ)<∞.\int_{\mathbb R} \lvert\lambda\rvert \,d\mu_\psi^A(\lambda) <\infty.

This allows the expectation to be defined as a quadratic-form value under conditions weaker than ψ∈D(A)\psi\in\mathcal D(A).

  • A finite second moment requires
∫Rλ2 dμψA(λ)<∞,\int_{\mathbb R} \lambda^2 \,d\mu_\psi^A(\lambda) <\infty,

which is the condition needed for a finite variance and is equivalent to ψ∈D(A)\psi\in\mathcal D(A) for self-adjoint AA.

  • For a density operator and unbounded AA, a standard sufficient condition for an absolutely defined finite mean is
Tr⁡(ρ∣A∣)<∞.\operatorname{Tr} \left( \rho\lvert A\rvert \right) <\infty.

Formal matrix or integral manipulations do not override these existence conditions.

  • The state and observable refer to the same Hilbert space.
  • The state is normalized, or the displayed normalization denominator is included.
  • AA is self-adjoint when interpreted as a physical observable.
  • The first spectral moment exists.
  • Coordinate representations use the correct measure and operator domain.
  • Trace expressions involving unbounded operators are defined under appropriate trace and domain conditions.
  • Statistical sample-mean interpretations assume repeated comparable preparations and an appropriate independence model.

The expectation formula is exact within standard quantum mechanics. It applies to pure and mixed states and to discrete, continuous, or mixed spectra, provided the relevant moment exists.

For a non-self-adjoint operator BB,

⟨B⟩=Tr⁡(ρB)\langle B\rangle = \operatorname{Tr}(\rho B)

can still be mathematically useful, but it may be complex and is not directly the mean of a sharp real-valued observable.

The expectation value alone does not determine the full outcome distribution. Different distributions can have the same mean but different variances, tails, or higher moments.

  • For self-adjoint AA, the result should be real within numerical tolerance.
  • If the spectrum lies in [amin⁡,amax⁡][a_{\min},a_{\max}], then
amin⁡≤⟨A⟩≤amax⁡.a_{\min} \leq \langle A\rangle \leq a_{\max}.
  • The dimensions of ⟨A⟩\langle A\rangle must match those of AA.
  • A basis change applied consistently to the state and operator must leave the result invariant.
  • In a normalized eigenstate ∣a⟩\lvert a\rangle, the expectation should reduce to aa.
  • For A=IA=I, the expectation must equal one.
  • For a positive operator, the expectation must be nonnegative.
  • In a product state, appropriate product-observable expectations should factorize; entangled and classically correlated states need not.

Let

∣ψ⟩=α∣0⟩+β∣1⟩,∣α∣2+∣β∣2=1,\lvert\psi\rangle = \alpha\lvert0\rangle +\beta\lvert1\rangle, \qquad \lvert\alpha\rvert^2 +\lvert\beta\rvert^2 =1,

and let

Z=(100−1).Z = \begin{pmatrix} 1&0\\ 0&-1 \end{pmatrix}.

Then

⟨Z⟩=∣α∣2−∣β∣2.\langle Z\rangle = \lvert\alpha\rvert^2 -\lvert\beta\rvert^2.

The only measurement outcomes are +1+1 and −1-1. Their Born probabilities are ∣α∣2\lvert\alpha\rvert^2 and ∣β∣2\lvert\beta\rvert^2, and the displayed expectation is their probability-weighted average.

Expectation Values owns the statistical meaning, spectral construction, domain distinctions, and repeated-measurement interpretation. Trace Rule for Expectation Values derives the mixed-state and component forms.

Expectation Values in Wave Mechanics owns coordinate-space calculations and boundary checks.

  • Treating the expectation value as a guaranteed or most likely outcome.
  • Using an ordinary transpose instead of a conjugate transpose.
  • Reading probabilities from diagonal density-matrix entries in the wrong basis.
  • Computing ⟨A⟩2\langle A\rangle^2 when ⟨A2⟩\langle A^2\rangle is required.
  • Assuming ⟨AB⟩=⟨A⟩⟨B⟩\langle AB\rangle=\langle A\rangle\langle B\rangle.
  • Reordering noncommuting factors inside a trace rather than only cycling them.
  • Ignoring the integration measure in curvilinear coordinates.
  • Dropping boundary terms for differential operators without checking the domain.
  • Using the pure-state expression for a mixed state without an ensemble average or trace.
  • Suppressing tensor-product identities until subsystem dimensions become ambiguous.
  • Assuming normalization guarantees that every unbounded-observable moment exists.
  • R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994, chs. 4 and 7.
  • J. J. Sakurai and J. Napolitano, Modern Quantum Mechanics, 3rd ed., Cambridge University Press, 2020, ch. 1.
  • L. E. Ballentine, Quantum Mechanics: A Modern Development, World Scientific, 1998, chs. 2 and 3.
  • M. Reed and B. Simon, Methods of Modern Mathematical Physics I: Functional Analysis, rev. ed., Academic Press, 1980, ch. VIII.