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Expectation Values

The expectation value of an observable is the first moment of its Born-rule probability distribution. Operationally, it is the average approached by many measurements on independently and identically prepared systems, provided the relevant expectation exists.

For a normalized pure state ∣ψ⟩|\psi\rangle and a self-adjoint observable AA, the familiar operator formula is

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

For a density operator ρ\rho, the corresponding formula is

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

For an unbounded observable, this notation presupposes a finite absolute first spectral moment, Tr⁡(ρ∣A∣)<∞\operatorname{Tr}(\rho |A|)<\infty; the trace is then understood through the spectral integral. Without that condition, the mean need not exist.

These compact expressions are consequences of the Born rule. They do not say that a single measurement will return ⟨A⟩\langle A\rangle, nor that the system possesses this number before measurement. This page owns the quantum measurement meaning and operator formulation of expectation values. Generic probability facts are developed at Expectation Values in Probability, while detailed mixed-state trace calculations belong to Trace Rule for Expectation Values.

Required background. The Born Rule supplies the outcome distribution whose first moment is taken.

Helpful background. Spectral Decomposition supplies the observable’s spectral events; Expectation Values in Probability reviews discrete and continuous means.

Let μρA\mu_\rho^A be the Born probability measure of AA in the state ρ\rho:

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

The expectation value is

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

when the integral is well defined. This definition makes the statistical content explicit: each possible outcome λ\lambda is weighted by its Born probability.

The notation ⟨A⟩\langle A\rangle suppresses the state. That shorthand is safe only when the state is clear from context. The same observable can have very different expectations in different states.

Prepare NN independent systems in the same state ρ\rho, measure AA once on each, and denote the outcomes by a1,…,aNa_1,\ldots,a_N. The empirical mean is

A‾N=1N∑j=1Naj.\overline A_N = \frac{1}{N}\sum_{j=1}^{N}a_j.

If the outcome distribution has a finite absolute first moment, the law of large numbers gives

A‾N⟶⟨A⟩ρ\overline A_N \longrightarrow \langle A\rangle_\rho

with probability one as N→∞N\to\infty. Thus expectation values are testable ensemble predictions, not merely algebraic decorations on operators.

For finite NN, the sample mean fluctuates. If the variance is finite and the trials are independent, its standard deviation is

ΔA‾N=ΔAN.\Delta\overline A_N = \frac{\Delta A}{\sqrt N}.

This N−1/2N^{-1/2} statistical uncertainty is distinct from calibration errors, state-preparation drift, and detector systematics. The intrinsic spread ΔA\Delta A is treated canonically at Variance and Standard Deviation.

Expectation is not the most likely outcome

Section titled “Expectation is not the most likely outcome”

The mean, mode, and median answer different questions:

  • The expectation value is a probability-weighted average.
  • A mode is an outcome with maximal probability or density.
  • A median divides the probability into two halves.

They need not coincide. The expectation need not even be a possible individual outcome.

Three discrete outcome probabilities with a mean marked between the outcomes

For outcomes −3-3, 11, and 66 with probabilities 0.500.50, 0.300.30, and 0.200.20, the expectation is 00. It is neither an allowed outcome nor the most likely outcome, which is −3-3.

For this example,

⟨A⟩=(−3)(0.50)+(1)(0.30)+(6)(0.20)=0.\begin{aligned} \langle A\rangle &= (-3)(0.50)+(1)(0.30)\\ &\qquad{} +(6)(0.20)=0. \end{aligned}

The value zero summarizes the distribution’s first moment. It does not predict that any trial will produce zero.

Suppose AA has a finite or countable spectral decomposition

A=∑aaPa,A = \sum_a aP_a,

where PaP_a projects onto the full eigenspace with eigenvalue aa. The Born probability is

pρ(a)=Tr⁡(ρPa),p_\rho(a) = \operatorname{Tr}(\rho P_a),

and the expectation is

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

For a pure state,

pψ(a)=⟨ψ∣Pa∣ψ⟩,p_\psi(a) = \langle\psi|P_a|\psi\rangle,

so

⟨A⟩ψ=∑aa ⟨ψ∣Pa∣ψ⟩.\langle A\rangle_\psi = \sum_a a\, \langle\psi|P_a|\psi\rangle.

Degeneracy requires no extra probability rule: PaP_a already includes every orthogonal state in the eigenspace. If a basis ∣a,r⟩|a,r\rangle resolves a degeneracy label rr, then

pψ(a)=∑r∣⟨a,r∣ψ⟩∣2.p_\psi(a) = \sum_r |\langle a,r|\psi\rangle|^2.

The canonical probability calculation is at Born Rule for Discrete Spectra.

If the state-dependent spectral measure admits a density pA(λ)p_A(\lambda) with respect to dλd\lambda, then

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

For one-dimensional position in a pure state,

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

The density has inverse-outcome units, so the integrand times dλd\lambda has the units of the observable. The full treatment of densities, atoms, and coordinate changes is at Born Rule for Continuous Spectra.

An observable may have atomic weights wnw_n at eigenvalues ana_n and an absolutely continuous density pac(λ)p_{\mathrm{ac}}(\lambda). Its expectation is

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

One must include both parts. Integrating only the continuum omits occupied bound-state components; summing only eigenvalues omits scattering outcomes. The measure expression

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

handles discrete, continuous, singular, and mixed spectral measures in one line.

The spectral theorem represents a self-adjoint operator as

A=∫Rλ PA(dλ).A = \int_{\mathbb R}\lambda\,P^A(d\lambda).

For a pure state, taking the quadratic form gives

⟨ψ∣A∣ψ⟩=∫Rλ ⟨ψ∣PA(dλ)∣ψ⟩=∫Rλ dμψA(λ).\begin{aligned} \langle\psi|A|\psi\rangle &= \int_{\mathbb R}\lambda\, \langle\psi|P^A(d\lambda)|\psi\rangle\\ &= \int_{\mathbb R}\lambda\, d\mu_\psi^A(\lambda). \end{aligned}

This is exactly the probability-theory expectation. The operator expression and the weighted-outcome expression are not separate postulates; they are two representations of the same Born-rule statistic.

The practical spectral construction is developed at Spectral Decomposition.

Because AA is self-adjoint,

⟨ψ∣A∣ψ⟩∗=⟨Aψ∣ψ⟩=⟨ψ∣Aψ⟩.\begin{aligned} \langle\psi|A|\psi\rangle^* &= \langle A\psi|\psi\rangle\\ &= \langle\psi|A\psi\rangle. \end{aligned}

Hence

⟨A⟩ψ∈R.\langle A\rangle_\psi\in\mathbb R.

In a finite-dimensional numerical calculation, a significant imaginary part usually signals that the matrix is not Hermitian, the state or inner-product convention was implemented incorrectly, or rounding errors are poorly controlled. For differential operators, bad boundary conditions or a domain mismatch can produce the same symptom.

For a density operator ρ\rho with Tr⁡(ρ∣A∣)<∞\operatorname{Tr}(\rho|A|)<\infty, the expectation is

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

In any orthonormal basis {∣n⟩}\{|n\rangle\},

Tr⁡(ρA)=∑n⟨n∣ρA∣n⟩.\operatorname{Tr}(\rho A) = \sum_n\langle n|\rho A|n\rangle.

If

ρ=∑jqj∣ψj⟩⟨ψj∣,\rho = \sum_j q_j|\psi_j\rangle\langle\psi_j|,

then

⟨A⟩ρ=∑jqj⟨ψj∣A∣ψj⟩.\langle A\rangle_\rho = \sum_j q_j \langle\psi_j|A|\psi_j\rangle.

The result depends only on ρ\rho, not on which ensemble decomposition is used to represent it. The cyclicity, basis independence, local-observable formulas, and unbounded-operator cautions of the trace expression are developed at Trace Rule for Expectation Values.

Expectation is linear in the observable. For real α\alpha and β\beta,

⟨αA+βB⟩ρ=α⟨A⟩ρ+β⟨B⟩ρ,\langle\alpha A+\beta B\rangle_\rho = \alpha\langle A\rangle_\rho + \beta\langle B\rangle_\rho,

whenever the required expectations and operator domains are well defined. The observables AA and BB need not commute. This is a statement about ensemble means, not about the existence of a joint sharp measurement.

Linearity does not imply factorization:

⟨AB⟩ρ≠⟨A⟩ρ⟨B⟩ρ\langle AB\rangle_\rho \ne \langle A\rangle_\rho\langle B\rangle_\rho

in general. Correlations, operator ordering, and noncommutativity matter for products.

The functional calculus gives

f(A)=∫Rf(λ) PA(dλ).f(A) = \int_{\mathbb R}f(\lambda)\,P^A(d\lambda).

Therefore

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

provided the expectation exists. Taking f(λ)=λnf(\lambda)=\lambda^n produces the moments

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

In particular,

(ΔA)2=⟨A2⟩ρ−⟨A⟩ρ2.(\Delta A)^2 = \langle A^2\rangle_\rho - \langle A\rangle_\rho^2.

Knowing only ⟨A⟩\langle A\rangle does not determine the distribution. Many different Born distributions share the same first moment.

If

A∣a⟩=a∣a⟩,A|a\rangle=a|a\rangle,

then

⟨A⟩a=a,⟨A2⟩a=a2,ΔA=0.\langle A\rangle_a=a, \qquad \langle A^2\rangle_a=a^2, \qquad \Delta A=0.

Every measurement of AA in that state returns aa in the ideal projective model.

The converse requires the zero-spread condition. Merely finding ⟨A⟩=a\langle A\rangle=a does not prove that the state is an eigenstate, even if aa happens to be an eigenvalue. Contributions above and below aa can average to the same number.

If a bounded observable satisfies

mI≤A≤MI,mI\le A\le MI,

then every state obeys

m≤⟨A⟩ρ≤M.m\le\langle A\rangle_\rho\le M.

For a finite spectrum, the expectation is a convex combination of eigenvalues and lies in their convex hull. For a two-outcome observable with eigenvalues a−a_- and a+a_+,

⟨A⟩=a−p−+a+p+,p−+p+=1,\langle A\rangle = a_-p_-+a_+p_+, \qquad p_-+p_+=1,

so the mean lies between the two outcomes. It need not equal either one.

These bounds are valuable sanity checks. A computed spin expectation outside the operator’s spectral interval is necessarily wrong.

Choose an orthonormal basis and represent the normalized state by a column vector c\mathbf c. Then

⟨A⟩ψ=c†Ac.\langle A\rangle_\psi = \mathbf c^\dagger A\mathbf c.

Under a unitary basis change,

c′=U†c,A′=U†AU.\mathbf c' = U^\dagger\mathbf c, \qquad A' = U^\dagger A U.

The scalar is unchanged:

c′†A′c′=c†Ac.\mathbf c'^{\dagger}A'\mathbf c' = \mathbf c^\dagger A\mathbf c.

An expectation value is representation independent even though the state components and operator matrix change.

Write a qubit state and Hermitian observable as

ρ=12(I+r⋅σ),A=a0I+a⋅σ.\rho = \frac12\bigl(I+\mathbf r\cdot\boldsymbol\sigma\bigr), \qquad A = a_0I+\mathbf a\cdot\boldsymbol\sigma.

Using Tr⁡(σi)=0\operatorname{Tr}(\sigma_i)=0 and Tr⁡(σiσj)=2δij\operatorname{Tr}(\sigma_i\sigma_j)=2\delta_{ij} gives

⟨A⟩ρ=a0+r⋅a.\langle A\rangle_\rho = a_0+\mathbf r\cdot\mathbf a.

For A=σzA=\sigma_z and ∣ψ⟩=α∣0⟩+β∣1⟩|\psi\rangle=\alpha|0\rangle+\beta|1\rangle,

⟨σz⟩ψ=∣α∣2−∣β∣2.\langle\sigma_z\rangle_{\psi} = |\alpha|^2-|\beta|^2.

The outcomes are +1+1 and −1-1. Any expectation in [−1,1][-1,1] is possible, even though values strictly between the endpoints are not single-shot outcomes.

Let H∣En⟩=En∣En⟩H|E_n\rangle=E_n|E_n\rangle and

∣ψ⟩=∑ncn∣En⟩.|\psi\rangle = \sum_n c_n|E_n\rangle.

Then

⟨H⟩ψ=∑n∣cn∣2En.\langle H\rangle_{\psi} = \sum_n |c_n|^2E_n.

Relative phases among the cnc_n do not affect the energy probabilities because HH is diagonal in this basis. For an observable BB that is not diagonal in the energy basis,

⟨B⟩ψ=∑m,ncm∗cnBmn,\langle B\rangle_{\psi} = \sum_{m,n}c_m^*c_n B_{mn},

and off-diagonal terms can make relative phases observable.

In a position representation, a pure-state expectation is formally

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

For position,

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

For momentum in the standard coordinate representation,

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

The second expression is real only when the state lies in the relevant self-adjoint domain and the boundary terms are controlled. The page Expectation Values in Wave Mechanics owns coordinate-space calculations, integration by parts, radial measures, and numerical quadrature.

Normalization of the state does not guarantee that every expectation is finite. The measure-theoretic expectation exists as a finite number when

∫R∣λ∣ dμρA(λ)<∞.\int_{\mathbb R}|\lambda|\, d\mu_\rho^A(\lambda) <\infty.

For a pure state and unbounded AA, the operator expression ⟨ψ∣A∣ψ⟩\langle\psi|A|\psi\rangle is certainly defined when ∣ψ⟩|\psi\rangle lies in the operator domain D(A)D(A). The expectation can also be handled through the associated quadratic form under the appropriate weaker integrability condition. Domain claims should therefore accompany formal differential-operator manipulations.

Higher moments require stronger conditions. A state can have finite ⟨∣A∣⟩\langle|A|\rangle but infinite ⟨A2⟩\langle A^2\rangle, so its mean exists while its variance does not.

Consider the normalized even density

p(x)=12(1+∣x∣)2.p(x) = \frac{1}{2(1+|x|)^2}.

The positive and negative tails appear to cancel in a symmetric principal value, but

∫−∞∞∣x∣p(x) dx=∞.\int_{-\infty}^{\infty}|x|p(x)\,dx =\infty.

Therefore the ordinary expectation of XX is undefined, not zero. Assigning a value by symmetric cancellation confuses a Cauchy principal value with a Lebesgue expectation. This distinction matters whenever outcome distributions have heavy tails.

For a discrete POVM with numerical outcomes yy and effects EyE_y,

p(y)=Tr⁡(ρEy),∑yEy=I.p(y) = \operatorname{Tr}(\rho E_y), \qquad \sum_y E_y=I.

Its expectation is

E[Y]=∑yy Tr⁡(ρEy)=Tr⁡(ρM1),\begin{aligned} \mathbb E[Y] &= \sum_y y\,\operatorname{Tr}(\rho E_y)\\ &= \operatorname{Tr}(\rho M_1), \end{aligned}

where

M1=∑yyEyM_1 = \sum_y yE_y

is the POVM’s first-moment operator. Different POVMs can share the same M1M_1 while having different full distributions and higher moments. Measuring the sharp observable M1M_1 is therefore not generally equivalent to performing the original POVM.

See POVMs: First Encounter for generalized measurement probabilities and effects.

Time dependence and classical-looking motion

Section titled “Time dependence and classical-looking motion”

In the Schrödinger picture, both the state and an explicitly time-dependent observable may contribute to the evolution of an expectation. Under the usual domain assumptions,

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.

This equation does not turn an ensemble mean into a classical trajectory, but for position and momentum it leads to equations resembling classical mechanics under suitable conditions. The interpretation and approximation limits are at Ehrenfest Theorem Overview.

An expectation is an ensemble statistic. A single projective measurement returns a spectral outcome, not generally the mean.

The most probable outcome can differ sharply from the mean. For a continuous law, the mode concerns density height, whereas the expectation depends on the entire weighted tail structure.

⟨A⟩\langle A\rangle is incomplete notation unless the state is understood. The observable alone does not determine its expectation.

Probabilities must be summed over every unresolved degeneracy label and over all atomic and continuous spectral components.

For a nonzero but unnormalized vector ∣ϕ⟩|\phi\rangle, the normalized expression is

⟨A⟩ϕ=⟨ϕ∣A∣ϕ⟩⟨ϕ∣ϕ⟩.\langle A\rangle_{\phi} = \frac{\langle\phi|A|\phi\rangle} {\langle\phi|\phi\rangle}.

The denominator cannot be silently omitted.

Square-integrability of a wavefunction does not ensure a finite expectation for every unbounded observable. Check operator domains, boundary conditions, and absolute moment convergence.

In general ⟨AB⟩≠⟨A⟩⟨B⟩\langle AB\rangle\ne\langle A\rangle\langle B\rangle. Factorization requires additional statistical or state structure.

Inferring the distribution from one moment

Section titled “Inferring the distribution from one moment”

A mean alone does not determine probabilities, variance, skewness, tails, or whether the spectrum is discrete or continuous.

The Born rule defines the state-dependent spectral measure μρA\mu_\rho^A. Its first moment is the expectation value:

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

Equivalent operator formulas are

⟨A⟩ψ=⟨ψ∣A∣ψ⟩,⟨A⟩ρ=Tr⁡(ρA),\langle A\rangle_\psi = \langle\psi|A|\psi\rangle, \qquad \langle A\rangle_\rho = \operatorname{Tr}(\rho A),

under the appropriate domain and convergence assumptions. The expectation is real, linear in the observable, basis independent, and constrained by the spectral range for bounded observables. It is estimated by repeated measurements, need not be an allowed single-shot outcome, and need not exist for a normalized state with sufficiently heavy spectral tails.

  • P. Busch, P. J. Lahti, J.-P. Pellonpää, and K. Ylinen, Quantum Measurement, Springer, 2016, Chapters 3–5.
  • P. A. M. Dirac, The Principles of Quantum Mechanics, 4th ed., Oxford University Press, 1958, Chapters II–III.
  • B. C. Hall, Quantum Theory for Mathematicians, Springer, 2013, Chapters 7–10.
  • M. Reed and B. Simon, Methods of Modern Mathematical Physics, Vol. I: Functional Analysis, revised and enlarged ed., Academic Press, 1980, Sections VII.1–VII.3 and VIII.3.
  • J. J. Sakurai and J. Napolitano, Modern Quantum Mechanics, 3rd ed., Cambridge University Press, 2020, Chapters 1–2.
  • R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994, Chapters 1 and 4.
  • J. von Neumann, Mathematical Foundations of Quantum Mechanics, Princeton University Press, 1955, Chapters II–III.

An observable has outcomes −2-2, 11, and 44 with probabilities 1/41/4, 1/21/2, and 1/41/4. Compute its expectation. Is the expectation an allowed outcome?

Solution

The expectation is

⟨A⟩=(−2)14+(1)12+(4)14=1.\begin{aligned} \langle A\rangle &= (-2)\frac14+(1)\frac12+(4)\frac14\\ &=1. \end{aligned}

Here the expectation happens to equal the allowed outcome 11. That coincidence does not imply that every measurement returns 11; the other outcomes still have total probability 1/21/2.

A two-outcome observable returns 00 with probability 0.90.9 and 2020 with probability 0.10.1. Find the mean and the mode. Explain why neither alone fully describes the experiment.

Solution

The mean is

E[A]=(0)(0.9)+(20)(0.1)=2,\mathbb E[A] = (0)(0.9)+(20)(0.1) =2,

while the unique mode is 00. The mean 22 is not a possible outcome, and the mode omits the rare but large result 2020. The full probability distribution is needed to predict all frequencies.

Let

A=(2i−i−1),∣ψ⟩=15(12).A = \begin{pmatrix} 2 & i\\ -i & -1 \end{pmatrix}, \qquad |\psi\rangle = \frac{1}{\sqrt5} \begin{pmatrix} 1\\ 2 \end{pmatrix}.

Compute ⟨A⟩ψ\langle A\rangle_\psi. Why must the answer be real despite the complex matrix entries?

Solution

First,

A∣ψ⟩=15(2+2i−i−2).A|\psi\rangle = \frac{1}{\sqrt5} \begin{pmatrix} 2+2i\\ -i-2 \end{pmatrix}.

Therefore

⟨A⟩ψ=15(12)(2+2i−i−2)=−25.\begin{aligned} \langle A\rangle_\psi &= \frac15 \begin{pmatrix}1&2\end{pmatrix} \begin{pmatrix}2+2i\\-i-2\end{pmatrix}\\ &= -\frac25. \end{aligned}

The imaginary terms cancel because A=A†A=A^\dagger. A simultaneous unitary change of the state components and operator matrix would leave this scalar unchanged.

For

∣ψ⟩=cos⁡θ2∣0⟩+eiφsin⁡θ2∣1⟩,|\psi\rangle = \cos\frac{\theta}{2}|0\rangle + e^{i\varphi}\sin\frac{\theta}{2}|1\rangle,

compute ⟨σx⟩\langle\sigma_x\rangle. Which relative phase gives the largest value at fixed θ\theta?

Solution

Because

σx=∣0⟩⟨1∣+∣1⟩⟨0∣,\sigma_x = |0\rangle\langle1|+|1\rangle\langle0|,

the expectation is the sum of the two cross terms:

⟨σx⟩=2cos⁡θ2sin⁡θ2cos⁡φ=sin⁡θcos⁡φ.\begin{aligned} \langle\sigma_x\rangle &= 2\cos\frac{\theta}{2} \sin\frac{\theta}{2}\cos\varphi\\ &= \sin\theta\cos\varphi. \end{aligned}

At fixed θ\theta with sin⁡θ≥0\sin\theta\ge0, this is largest for φ=0\varphi=0 modulo 2π2\pi. The example shows that relative phase can affect an expectation when the observable is not diagonal in the preparation basis.

Let p(x)p(x) be a normalized, even position density with a finite absolute first moment. Show that ⟨X⟩=0\langle X\rangle=0. Why is the integrability assumption essential?

Solution

Since p(−x)=p(x)p(-x)=p(x), the function xp(x)xp(x) is odd. Absolute integrability permits the positive and negative halves to be combined legitimately:

⟨X⟩=∫−∞∞xp(x) dx=∫0∞x[p(x)−p(−x)] dx=0.\begin{aligned} \langle X\rangle &= \int_{-\infty}^{\infty}xp(x)\,dx\\ &= \int_0^\infty x[p(x)-p(-x)]\,dx =0. \end{aligned}

Without ∫∣x∣p(x)dx<∞\int |x|p(x)dx<\infty, the two half-line integrals may diverge. A symmetric principal value can then vanish even though the ordinary expectation does not exist.

6. A normalized state with no position mean

Section titled “6. A normalized state with no position mean”

Verify that

p(x)=12(1+∣x∣)2p(x)=\frac{1}{2(1+|x|)^2}

is normalized, and show that E[∣X∣]\mathbb E[|X|] diverges.

Solution

Evenness gives

∫−∞∞p(x) dx=∫0∞dx(1+x)2=1.\int_{-\infty}^{\infty}p(x)\,dx = \int_0^\infty\frac{dx}{(1+x)^2} =1.

For the absolute first moment,

E[∣X∣]=∫0∞x(1+x)2 dx.\mathbb E[|X|] = \int_0^\infty\frac{x}{(1+x)^2}\,dx.

The integrand behaves as 1/x1/x for large xx, so the integral diverges logarithmically. The probability law is normalized, but its position expectation is undefined.

Let

∣ψ⟩=12(∣E1⟩+eiϕ∣E2⟩),|\psi\rangle = \frac{1}{\sqrt2} \left(|E_1\rangle+e^{i\phi}|E_2\rangle\right),

where H∣Ej⟩=Ej∣Ej⟩H|E_j\rangle=E_j|E_j\rangle and E1≠E2E_1\ne E_2. Find ⟨H⟩\langle H\rangle. Does it depend on ϕ\phi?

Solution

Orthogonality and diagonal action of HH give

⟨H⟩=E1+E22.\langle H\rangle = \frac{E_1+E_2}{2}.

It is independent of ϕ\phi because the energy probabilities are both 1/21/2. The relative phase can still affect expectations of observables with nonzero off-diagonal matrix elements between ∣E1⟩|E_1\rangle and ∣E2⟩|E_2\rangle.

An observable has standard deviation ΔA=3\Delta A=3 in a fixed state. Assuming independent preparations and negligible systematics, how many measurements are needed to make the standard deviation of the sample mean at most 0.030.03?

Solution

The sample-mean standard deviation is

ΔA‾N=3N.\Delta\overline A_N = \frac{3}{\sqrt N}.

Requiring this to be at most 0.030.03 gives

3N≤0.03,N≥100,\frac{3}{\sqrt N}\le0.03, \qquad \sqrt N\ge100,

so N≥104N\ge10^4. This quantifies statistical precision only; systematic errors do not generally decrease as N−1/2N^{-1/2}.