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Continuous Variables and Modes

Continuous-variable systems have observables with continuous spectra or modes with unbounded occupation. Their Hilbert spaces are typically infinite-dimensional, but the organizing questions remain the same as for qubits: what is the subsystem decomposition, which states factorize, what information survives a partial trace, and which correlations are genuinely quantum?

The extra care comes from three sources:

  • position and momentum eigenvectors are generalized states rather than normalizable vectors;
  • different particle, mode, and spatial-region decompositions answer different physical questions;
  • covariance matrices completely characterize Gaussian states but not arbitrary non-Gaussian states.

This chapter connects wave mechanics, Fock space, and entanglement without making quantum optics or continuous-variable quantum information duplicate canonical homes.

TaskCanonical pageMain output
identify the infinite-dimensional settingContinuous-Variable Systemstensor products, normalizability, modes, and Gaussian preview
decide which modes define subsystemsMode Decompositionsspatial, momentum, frequency, polarization, and wavepacket modes
analyze elementary mode entanglementTwo-Mode Entanglementsingle-excitation, number-correlated, squeezed, and beam-splitter states
interpret ideal EPR correlations safelyEPR State Previewcommuting collective observables and normalizable approximations
use first and second momentsGaussian States Previewquadratures, covariance matrices, Wigner functions, and Gaussian criteria
connect squeezing to entanglementSqueezed States as Entangled Modestwo-mode squeezing, reduced thermal states, and EPR-like noise suppression
translate wave mechanics into composite-state languagePosition-Space Two-Particle Statesproduct kernels, entangled wavefunctions, reductions, and exchange symmetry

A canonical degree of freedom has operators qq and pp satisfying

[q,p]=iℏI.[q,p]=i\hbar I.

Neither operator has a finite spectrum, and the associated Hilbert space cannot be finite-dimensional. The standard position representation is

H=L2(R,dx),\mathcal H=L^2(\mathbb R,dx),

whose vectors are square-integrable wavefunctions modulo equality almost everywhere. The position kets ∣x⟩\lvert x\rangle are useful generalized eigenvectors, but

⟨x∣x′⟩=δ(x−x′)\langle x|x'\rangle = \delta(x-x')

shows that they are not normalized Hilbert-space vectors.

An oscillator mode is also continuous-variable even though its number basis is discrete:

Hmathrmmode=span⁡{∣0⟩,∣1⟩,…}.\mathcal H_{mathrm{mode}} = \operatorname{span} \{\lvert0\rangle,\lvert1\rangle,\ldots\}.

The unbounded occupation and continuous quadrature spectra, not the notation used for the basis, make it a continuous-variable system.

For two distinguishable particles on a line,

H12=L2(R,dx1)⊗L2(R,dx2)≅L2(R2,dx1dx2).\begin{aligned} \mathcal H_{12} &= L^2(\mathbb R,dx_1) \otimes L^2(\mathbb R,dx_2) \\ &\cong L^2(\mathbb R^2,dx_1dx_2). \end{aligned}

A pure state is represented by Ψ(x1,x2)\Psi(x_1,x_2). It is normalized when

∫R2dx1dx2 ∣Ψ(x1,x2)∣2=1.\int_{\mathbb R^2} dx_1dx_2\, \lvert\Psi(x_1,x_2)\rvert^2 =1.

It is a product state exactly when, up to sets of measure zero,

Ψ(x1,x2)=ψ(x1)ϕ(x2).\Psi(x_1,x_2) = \psi(x_1)\phi(x_2).

For identical particles, the formal coordinate slots do not automatically define operational subsystems. The wavefunction must also obey the appropriate exchange symmetry, and mode or region partitions may be more physical.

Suppose the one-particle space decomposes into orthogonal mode subspaces,

h=hA⊕hB.\mathcal h = \mathcal h_A\oplus\mathcal h_B.

Bosonic or fermionic Fock space then factorizes, after an ordering convention is fixed in the fermionic case, as

F±(h)≅F±(hA)⊗F±(hB).\mathcal F_{\pm}(\mathcal h) \cong \mathcal F_{\pm}(\mathcal h_A) \otimes \mathcal F_{\pm}(\mathcal h_B).

This factorization makes modes AA and BB candidate subsystems. A state can therefore be separable in one mode decomposition and entangled in another. That is not a contradiction: entanglement is a property of a state together with a specified tensor-product structure and observable access.

For a normalized two-particle wavefunction, the pure-state density kernel is

ρ(x1,x2;x1′,x2′)=Ψ(x1,x2)Ψ∗(x1′,x2′).\rho(x_1,x_2;x_1',x_2') = \Psi(x_1,x_2) \Psi^*(x_1',x_2').

Tracing over particle or coordinate slot 2 gives

ρ1(x,x′)=∫Rdy Ψ(x,y)Ψ∗(x′,y).\rho_1(x,x') = \int_{\mathbb R}dy\, \Psi(x,y) \Psi^*(x',y).

The kernel defines an operator through

(ρ1f)(x)=∫Rdx′ ρ1(x,x′)f(x′).(\rho_1 f)(x) = \int_{\mathbb R}dx'\, \rho_1(x,x')f(x').

For a product wavefunction, ρ1\rho_1 has rank one. For a pure entangled state it is mixed. The Position-Space Two-Particle States page owns the full wavefunction analysis and the cautions associated with center-of-mass coordinates and identical-particle symmetry.

Modes Are Chosen, Not Discovered Once and for All

Section titled “Modes Are Chosen, Not Discovered Once and for All”

Let aia_i annihilate an excitation in orthonormal mode ii. A unitary one-particle basis change defines

bα=∑iUαi∗ai,bα†=∑iUαiai†.b_\alpha = \sum_i U_{\alpha i}^*a_i, \qquad b_\alpha^\dagger = \sum_i U_{\alpha i}a_i^\dagger.

For bosons,

[bα,bβ†]=δαβ,[b_\alpha,b_\beta^\dagger] = \delta_{\alpha\beta},

and the analogous fermionic anticommutator is preserved. Spatial, frequency, momentum, polarization, and wavepacket modes are therefore different bases of the same one-particle space when the transformation is unitary and complete.

The physically useful decomposition depends on preparation, dynamics, and measurement. A beam splitter changes the relation between input and output modes; a detector with finite bandwidth selects wavepacket modes; a lattice model privileges local orbitals. Mode Decompositions owns these choices and their operational caveats.

For one bosonic mode, set ℏ=1\hbar=1 and define

q=a+a†2,p=a−a†i2.q = \frac{a+a^\dagger}{\sqrt2}, \qquad p = \frac{a-a^\dagger}{i\sqrt2}.

Then [q,p]=i[q,p]=i. For mm modes, collect the quadratures into

R=(q1,p1,…,qm,pm)T.R = (q_1,p_1,\ldots,q_m,p_m)^{\mathsf T}.

Their commutators are encoded by the symplectic form:

[Rj,Rk]=iΩjk,Ω=⨁r=1m(01−10).[R_j,R_k] = i\Omega_{jk}, \qquad \Omega = \bigoplus_{r=1}^{m} \begin{pmatrix} 0&1\\ -1&0 \end{pmatrix}.

For a state ρ\rho, define the displacement vector and covariance matrix by

dj=Tr⁡(ρRj),d_j = \operatorname{Tr}(\rho R_j),

and

Γjk=12Tr⁡[ρ{ΔRj,ΔRk}],\Gamma_{jk} = \frac12 \operatorname{Tr} \left[ \rho\{\Delta R_j,\Delta R_k\} \right],

where ΔRj=Rj−dj\Delta R_j=R_j-d_j. Every physical covariance matrix obeys

Γ+i2Ω⪰0.\Gamma + \frac{i}{2}\Omega \succeq 0.

With these conventions the vacuum covariance is I/2I/2. Convention changes are common, so factors of two must be checked before importing an uncertainty or entanglement criterion.

A Gaussian state has a Gaussian characteristic function or, equivalently, a Gaussian Wigner function. It is completely determined by dd and Γ\Gamma. This turns many infinite-dimensional questions into finite-dimensional linear algebra.

For non-Gaussian states, the same moments remain useful but are not complete. Distinct states can share the same first and second moments, and a covariance-based test may fail to detect entanglement that is visible in higher moments or in the full density operator.

The Gaussian States Preview page develops purity, symplectic eigenvalues, Wigner functions, and the Gaussian partial-transpose criterion. This chapter uses only the structural lesson:

Gaussian state⟹(d,Γ) is complete,\text{Gaussian state} \Longrightarrow (d,\Gamma)\text{ is complete},

whereas

(d,Γ)⇏ρ.(d,\Gamma) \nRightarrow \rho.

The state

∣Ψ1⟩=α∣1,0⟩+β∣0,1⟩,∣α∣2+∣β∣2=1.\begin{aligned} \lvert\Psi_1\rangle &= \alpha\lvert1,0\rangle + \beta\lvert0,1\rangle, \\ \lvert\alpha\rvert^2+\lvert\beta\rvert^2 &=1. \end{aligned}

is entangled across the mode split when both coefficients are nonzero. Tracing out mode BB gives

ρA=∣α∣2∣1⟩⟨1∣+∣β∣2∣0⟩⟨0∣.\rho_A = \lvert\alpha\rvert^2\lvert1\rangle\langle1\rvert + \lvert\beta\rvert^2\lvert0\rangle\langle0\rvert.

This is mode entanglement, not entanglement between two persistent particle identities. Its operational use can depend on phase references, local number constraints, and which mode operations are available.

A central Gaussian example is

∣TMSV(r)⟩=1−λ2×∑n=0∞λn∣n,n⟩,λ=tanh⁡r.\begin{aligned} \lvert\mathrm{TMSV}(r)\rangle &= \sqrt{1-\lambda^2} \\ &\quad\times \sum_{n=0}^{\infty} \lambda^n\lvert n,n\rangle, \\ \lambda &=\tanh r. \end{aligned}

This is already a Schmidt decomposition. Either mode alone has a geometric number distribution,

ρA=(1−λ2)∑n=0∞λ2n∣n⟩⟨n∣,\rho_A = (1-\lambda^2) \sum_{n=0}^{\infty} \lambda^{2n} \lvert n\rangle\langle n\rvert,

with mean occupation

nˉ=sinh⁡2r.\bar n = \sinh^2 r.

The reduced state is thermal in form, even though the joint two-mode state is pure. Its entanglement entropy is

S=(nˉ+1)ln⁡(nˉ+1)−nˉln⁡nˉ.S = (\bar n+1)\ln(\bar n+1) - \bar n\ln\bar n.

The Squeezed States as Entangled Modes page owns the squeezing transformation and its quantum-optical interpretation.

For a suitable two-mode squeezing phase, the collective quadratures obey

Var⁡(q1−q2)=e−2r,Var⁡(p1+p2)=e−2r.\begin{aligned} \operatorname{Var}(q_1-q_2) &=e^{-2r}, \\ \operatorname{Var}(p_1+p_2) &=e^{-2r}. \end{aligned}

The two collective observables commute:

[q1−q2,p1+p2]=0.[q_1-q_2,p_1+p_2]=0.

As rr increases, their fluctuations become small while conjugate combinations become noisy. The formal r→∞r\to\infty limit has perfect EPR correlations, infinite energy, and no normalizable state vector. Physical experiments and calculations use finite-squeezing states or other normalizable wavepackets.

The EPR State Preview owns this limiting construction. The historical EPR argument and Bell inequalities have separate canonical homes in foundations; strong quadrature correlation alone should not be called a Bell-inequality violation.

State and taskAppropriate first toolLimitation to record
pure bipartite vectorSchmidt decomposition or reduced-state entropyspectra may be infinite and entropy may diverge
mixed finite-mode stateseparability criteria, witnesses, or negativityno single scalar captures all operational resources
Gaussian bipartite statecovariance matrix and Gaussian partial transposeconvention and bipartition must be fixed
non-Gaussian statefull density operator, characteristic function, or tailored witnesssecond moments are generally incomplete
field or spatial-region problemregulated algebra or mode decompositioncontinuum factorization and ultraviolet limits require care

No diagnostic should be applied before the subsystem decomposition is stated. For infinite-dimensional systems, domains, convergence, energy constraints, and regularization may be part of the physical question rather than technical afterthoughts.

1. Specify the physical degrees of freedom

Section titled “1. Specify the physical degrees of freedom”

State whether the objects are particles, oscillator modes, field modes, spatial regions, or effective collective coordinates.

Write the factorization or direct-sum decomposition explicitly. For identical particles, distinguish formal particle slots from accessible modes or regions.

Record the value of ℏ\hbar, quadrature normalization, Fourier-transform convention, covariance ordering, and mode basis.

Verify normalization, trace class, finite moments required by the calculation, and any energy or ultraviolet cutoff. Treat delta-correlated states as idealizations.

Use wavefunction kernels for coordinate questions, number states for occupation structure, and phase-space or covariance methods for Gaussian states.

Trace over the stated subsystem, or transform both states and observables when changing mode bases. Do not change the factorization silently.

7. Match the diagnostic to the state class

Section titled “7. Match the diagnostic to the state class”

Use pure-state spectra, Gaussian criteria, or non-Gaussian witnesses only within their stated assumptions.

Identify the measurements, reference frames, and local controls that make the proposed subsystem correlations accessible.

This chapter owns the composite-system structure shared by continuous coordinates and modes. Detailed homes remain elsewhere:

  • Calling every infinite-dimensional system continuous-variable. State which observables or unbounded mode occupations supply the continuous-variable structure.
  • Treating position eigenstates as normalized vectors. They are distributions used inside a rigged-Hilbert-space framework.
  • Assuming a mode decomposition is unique. Modes depend on basis, apparatus, and accessible observable algebra.
  • Confusing particle entanglement with mode entanglement. Name the tensor factors explicitly.
  • Ignoring exchange symmetry. A two-coordinate wavefunction for identical particles must lie in the physical symmetry sector.
  • Using covariance data as a complete state description without Gaussianity. Higher moments can contain essential information.
  • Mixing quadrature conventions. Vacuum variances and uncertainty inequalities change by factors of two.
  • Calling the ideal EPR state physical. Perfect correlations require a non-normalizable, infinite-energy limit.
  • Inferring Bell nonlocality from entanglement or squeezing alone. Bell violation requires a specified inequality and measurement scenario.
  • Letting a basis change silently redefine locality. Transformations that mix the chosen subsystems can change the entanglement being discussed.

Wave-mechanics route: Continuous-Variable Systems → Position-Space Two-Particle States → Reduced States and Partial Trace.

Mode route: Mode Decompositions → Fock Space and Occupation Number → Two-Mode Entanglement.

Gaussian route: Gaussian States Preview → Squeezed States as Entangled Modes → EPR State Preview.

Field-theory bridge: Mode Expansions → Field Operators → Entanglement in QFT Preview.

Across-fields bridge: Entanglement Across Fields → Entanglement in Quantum Optics or Entanglement in QFT Preview.

Practice bridge: Reference, Problems, and Notebooks → Entanglement Diagnostic Table → Computational Notebooks.

  • L. E. Ballentine, Quantum Mechanics: A Modern Development, 2nd ed., World Scientific, 2014.
  • R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994.
  • B. C. Hall, Quantum Theory for Mathematicians, Springer, 2013.
  • D. F. Walls and G. J. Milburn, Quantum Optics, 2nd ed., Springer, 2008.
  • S. L. Braunstein and P. van Loock, “Quantum information with continuous variables,” Reviews of Modern Physics 77, 513–577, 2005.
  • C. Weedbrook et al., “Gaussian quantum information,” Reviews of Modern Physics 84, 621–669, 2012.
  • A. Serafini, Quantum Continuous Variables: A Primer of Theoretical Methods, CRC Press, 2017.
  • R. Simon, “Peres–Horodecki separability criterion for continuous variable systems,” Physical Review Letters 84, 2726–2729, 2000.
  • S. D. Bartlett, T. Rudolph, and R. W. Spekkens, “Reference frames, superselection rules, and quantum information,” Reviews of Modern Physics 79, 555–609, 2007.

Let Ψ(x,y)=ψ(x)ϕ(y)\Psi(x,y)=\psi(x)\phi(y), where both factors are normalized. Compute the reduced kernel ρ1(x,x′)\rho_1(x,x') and show that the reduced state is pure.

Solution

Substitution into the partial trace gives

ρ1(x,x′)=∫dy ψ(x)ϕ(y)ψ∗(x′)ϕ∗(y)=ψ(x)ψ∗(x′),\begin{aligned} \rho_1(x,x') &= \int dy\, \psi(x)\phi(y) \psi^*(x')\phi^*(y) \\ &= \psi(x)\psi^*(x'), \end{aligned}

because ∫dy ∣ϕ(y)∣2=1\int dy\,\lvert\phi(y)\rvert^2=1. Thus ρ1=∣ψ⟩⟨ψ∣\rho_1=\lvert\psi\rangle\langle\psi\rvert, so

ρ12=ρ1,Tr⁡(ρ12)=1.\rho_1^2=\rho_1, \qquad \operatorname{Tr}(\rho_1^2)=1.

Exercise 2: Mode algebra under a basis change

Section titled “Exercise 2: Mode algebra under a basis change”

Let bα=∑iUαi∗aib_\alpha=\sum_iU_{\alpha i}^*a_i, where UU is unitary and [ai,aj†]=δij[a_i,a_j^\dagger]=\delta_{ij}. Verify the canonical commutator for the bb modes.

Solution

Using linearity,

[bα,bβ†]=∑i,jUαi∗Uβj[ai,aj†]=∑iUαi∗Uβi=δαβ.\begin{aligned} [b_\alpha,b_\beta^\dagger] &= \sum_{i,j} U_{\alpha i}^*U_{\beta j} [a_i,a_j^\dagger] \\ &= \sum_i U_{\alpha i}^*U_{\beta i} \\ &= \delta_{\alpha\beta}. \end{aligned}

The last equality is unitarity. A unitary one-particle basis change therefore preserves the bosonic mode algebra.

Exercise 3: Reduced state of one shared excitation

Section titled “Exercise 3: Reduced state of one shared excitation”

For ∣Ψ1⟩=α∣1,0⟩+β∣0,1⟩\lvert\Psi_1\rangle=\alpha\lvert1,0\rangle+\beta\lvert0,1\rangle, find the eigenvalues of ρA\rho_A and state when the mode state is entangled.

Solution

The two terms contain orthogonal states of mode BB, so their cross terms vanish under the partial trace:

ρA=∣α∣2∣1⟩⟨1∣+∣β∣2∣0⟩⟨0∣.\rho_A = \lvert\alpha\rvert^2 \lvert1\rangle\langle1\rvert + \lvert\beta\rvert^2 \lvert0\rangle\langle0\rvert.

Its nonzero eigenvalues are ∣α∣2\lvert\alpha\rvert^2 and ∣β∣2\lvert\beta\rvert^2. The pure joint state is entangled across the A∣BA|B mode split exactly when both eigenvalues are nonzero.

Exercise 4: Vacuum covariance and uncertainty

Section titled “Exercise 4: Vacuum covariance and uncertainty”

With q=(a+a†)/2q=(a+a^\dagger)/\sqrt2 and p=(a−a†)/(i2)p=(a-a^\dagger)/(i\sqrt2), show that the vacuum covariance is I2/2I_2/2 and saturates the uncertainty relation.

Solution

In the vacuum, ⟨q⟩=⟨p⟩=0\langle q\rangle=\langle p\rangle=0. Using a∣0⟩=0a\lvert0\rangle=0 and [a,a†]=1[a,a^\dagger]=1 gives

⟨q2⟩=⟨p2⟩=12,\langle q^2\rangle = \langle p^2\rangle = \frac12,

while the symmetrized cross covariance vanishes. Hence

Γ0=12(1001).\Gamma_0 = \frac12 \begin{pmatrix} 1&0\\ 0&1 \end{pmatrix}.

Therefore

Var⁡(q)Var⁡(p)=14,\operatorname{Var}(q) \operatorname{Var}(p) = \frac14,

which saturates the Robertson uncertainty bound for [q,p]=i[q,p]=i.

Exercise 5: Marginal of a two-mode squeezed state

Section titled “Exercise 5: Marginal of a two-mode squeezed state”

Starting from the Schmidt coefficients of ∣TMSV(r)⟩\lvert\mathrm{TMSV}(r)\rangle, verify normalization and compute the mean occupation of either reduced mode.

Solution

With λ=tanh⁡r\lambda=\tanh r, normalization follows from the geometric series:

(1−λ2)∑n=0∞λ2n=1.(1-\lambda^2) \sum_{n=0}^{\infty}\lambda^{2n} =1.

The reduced probabilities are pn=(1−λ2)λ2np_n=(1-\lambda^2)\lambda^{2n}. Thus

nˉ=(1−λ2)∑n=0∞nλ2n=λ21−λ2=sinh⁡2r.\begin{aligned} \bar n &= (1-\lambda^2) \sum_{n=0}^{\infty} n\lambda^{2n} \\ &= \frac{\lambda^2}{1-\lambda^2} \\ &= \sinh^2 r. \end{aligned}

The geometric marginal is thermal in form even though the joint state is pure.