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Interactions and Coupling Terms

An interaction term is the part of a composite Hamiltonian that couples tensor factors. For a bipartite system,

H=HA⊗IB+IA⊗HB+Hint,H = H_A\otimes I_B + I_A\otimes H_B + H_{\mathrm{int}},

the interaction term HintH_{\mathrm{int}} is responsible for dynamics that cannot be reduced to independent evolution on AA and BB.

This page focuses on the mechanism: how couplings convert product evolution into entangling evolution, how coupling constants set scales, and how the same pattern appears in spin systems, oscillators, light-matter models, Coulomb interactions, and controlled-phase gates. The broader Hamiltonian structure is developed in Composite Hamiltonians.

Helpful background. Composite Hamiltonians develops local and interaction terms; product states gives the factorization criterion used below.

Noninteracting evolution factors as UA(t)⊗UB(t)U_A(t)\otimes U_B(t), so local unitaries preserve product states. An interaction can instead entangle a product input. The useful test asks how it changes that particular state; failure of the full unitary to factor does not imply that every input becomes entangled.

For a finite-dimensional system, move to the interaction picture to remove the local evolution. At very short times, starting from ∣ψ⟩A∣ϕ⟩B\lvert\psi\rangle_A\lvert\phi\rangle_B,

∣Ψ(t)⟩=∣ψ⟩A∣ϕ⟩B−itℏHint∣ψ⟩A∣ϕ⟩B+O(t2),\lvert\Psi(t)\rangle = \lvert\psi\rangle_A\lvert\phi\rangle_B - \frac{i t}{\hbar} H_{\mathrm{int}} \lvert\psi\rangle_A\lvert\phi\rangle_B + O(t^2),

Here HintH_{\mathrm{int}} is evaluated at the initial time. Terms that change only one factor describe changes of local states. An entangling first-order component is detected by

(I−∣ψ⟩⟨ψ∣)⊗(I−∣ϕ⟩⟨ϕ∣)Hint∣ψ,ϕ⟩≠0.\bigl(I-|\psi\rangle\langle\psi|\bigr)\otimes\bigl(I-|\phi\rangle\langle\phi|\bigr) H_{\mathrm{int}}|\psi,\phi\rangle\ne0.

This projection removes both purely local changes. If it vanishes, entanglement can still appear at higher order. For unbounded Hamiltonians, a norm expansion with an O(t2)O(t^2) remainder requires an appropriate domain, such as D(H2)D(H^2).

From an entangling amplitude to reduced purity

Section titled “From an entangling amplitude to reduced purity”

For a normalized product input, take a finite-dimensional, time-independent Hamiltonian and define

QA=IA−∣ψ⟩⟨ψ∣,QB=IB−∣ϕ⟩⟨ϕ∣,∣χ⟩=(QA⊗QB)Hint∣ψ,ϕ⟩.Q_A=I_A-|\psi\rangle\langle\psi|,\qquad Q_B=I_B-|\phi\rangle\langle\phi|,\qquad |\chi\rangle=(Q_A\otimes Q_B)H_{\mathrm{int}}|\psi,\phi\rangle.

The norm of this component sets the initial loss of reduced-state purity:

1−Tr⁡ρA(t)2=2t2ℏ2∥χ∥2+O(t3).1-\operatorname{Tr}\rho_A(t)^2 =\frac{2t^2}{\hbar^2}\lVert\chi\rVert^2+O(t^3).

To see the coefficient, choose local bases beginning with ∣ψ⟩|\psi\rangle and ∣ϕ⟩|\phi\rangle. First-order amplitudes that change only one index can be removed by local basis rotations, which preserve purity. The remaining block has entries −itχij/ℏ-it\chi_{ij}/\hbar, with both indices orthogonal to the initial factors. Its squared norm is ϵ=t2∥χ∥2/ℏ2\epsilon=t^2\lVert\chi\rVert^2/\hbar^2 to leading order. The largest reduced-state eigenvalue is then 1−ϵ+O(t3)1-\epsilon+O(t^3), while the others have total weight ϵ+O(t3)\epsilon+O(t^3). Squaring the eigenvalues gives Tr⁡ρA2=1−2ϵ+O(t3)\operatorname{Tr}\rho_A^2=1-2\epsilon+O(t^3). Equivalently, differentiating the reduced density operator gives zero first derivative of purity and second derivative −4∥χ∥2/ℏ2-4\lVert\chi\rVert^2/\hbar^2; see Yang, Eqs. (14)–(19).

For a single coupling Hint=gA⊗BH_{\mathrm{int}}=gA\otimes B, with Hermitian A,BA,B and real gg,

∣χ⟩=g(A−⟨A⟩)∣ψ⟩⊗(B−⟨B⟩)∣ϕ⟩,∥χ∥2=g2Var⁡ψ(A)Var⁡ϕ(B).|\chi\rangle =g(A-\langle A\rangle)|\psi\rangle\otimes(B-\langle B\rangle)|\phi\rangle, \qquad \lVert\chi\rVert^2=g^2\operatorname{Var}_{\psi}(A)\operatorname{Var}_{\phi}(B).

Both input fluctuations therefore matter. A zero variance makes this quadratic coefficient vanish; local Hamiltonians can still rotate an input and allow entanglement at higher order. For several coupling terms, their projected amplitudes add before the norm is squared, so interference between terms matters. This is a local expansion near t=0t=0, not a prediction of indefinite purity loss or an entangling time for every input.

The product-operator expansion writes a finite-dimensional coupling as Hint=∑μgμAμ⊗BμH_{\mathrm{int}}=\sum_\mu g_\mu A_\mu\otimes B_\mu. Each term acts jointly on the two factors. The units of gμg_\mu depend on the normalization and units of Aμ,BμA_\mu,B_\mu: dimensionless Pauli matrices take an energy coefficient, while angular-momentum operators require the corresponding powers of ℏ\hbar.

Do not read this product-operator expansion as locality. A term such as Z⊗ZZ\otimes Z is a joint operator: it assigns phases or energies according to both subsystem labels. It is not a sum of one-subsystem Hamiltonians.

The same physical interaction can be represented differently after basis changes, rotating-frame transformations, normal-mode transformations, or effective-Hamiltonian approximations. The key question is not whether the formula contains tensor-product symbols, but whether the full evolution factors as local dynamics for the chosen subsystem split.

Whether a coupling entangles a state depends on the input. A particularly useful exception occurs when one factor has a definite value of the coupling observable.

If

Hint=g A⊗BH_{\mathrm{int}} = g\,A\otimes B

and ∣ψ⟩A\lvert\psi\rangle_A is an eigenstate of AA with eigenvalue aa, then on that input the interaction acts as an effective local Hamiltonian on BB:

Hint(∣ψ⟩A⊗∣ϕ⟩B)=∣ψ⟩A⊗(gaB∣ϕ⟩B).H_{\mathrm{int}} \bigl( \lvert\psi\rangle_A\otimes\lvert\phi\rangle_B \bigr) = \lvert\psi\rangle_A\otimes \bigl(g a B\lvert\phi\rangle_B\bigr).

Under this interaction alone, the full exponential preserves the product form. The same conclusion holds with local terms if the local evolution preserves the relevant eigenspace. Otherwise a local term can rotate the state away from that eigenspace, and later evolution can entangle it. The corresponding statement applies when BB has a definite value in the initial state.

An Ising interaction JZ⊗ZJZ\otimes Z, with JJ in energy units, changes phases according to the two ZZ labels. Its entangling action on ∣++⟩|++\rangle is calculated in composite Hamiltonians. A chain of such couplings with local transverse fields gives the transverse-field Ising model.

Consider two qubits with

H=ℏωA2Z⊗I+ℏωB2I⊗Z+JX⊗X,H=\frac{\hbar\omega_A}{2}Z\otimes I +\frac{\hbar\omega_B}{2}I\otimes Z +JX\otimes X,

where X,Y,ZX,Y,Z are Pauli matrices and the real coupling JJ has energy units. Set ωA=ωB=0\omega_A=\omega_B=0 to isolate the interaction. Since (X⊗X)2=IAB(X\otimes X)^2=I_{AB},

e−iJtX⊗X/ℏ=cos⁡(Jt/ℏ)IAB−isin⁡(Jt/ℏ)X⊗X.e^{-iJtX\otimes X/\hbar} =\cos(Jt/\hbar)I_{AB} -i\sin(Jt/\hbar)X\otimes X.

Starting from ∣00⟩|00\rangle, the state therefore becomes

∣Ψ(t)⟩=cos⁡(Jt/ℏ)∣00⟩−isin⁡(Jt/ℏ)∣11⟩.|\Psi(t)\rangle =\cos(Jt/\hbar)|00\rangle -i\sin(Jt/\hbar)|11\rangle.

When both coefficients are nonzero, the state has Schmidt rank two. Their squared magnitudes are the reduced-state eigenvalues, so equal magnitudes give maximal entanglement. For J≠0J\ne0, the first positive times are

tent=πℏ4∣J∣,∣Ψ(tent)⟩=∣00⟩−i sgn⁡(J)∣11⟩2,tprod=πℏ2∣J∣,∣Ψ(tprod)⟩=−i sgn⁡(J)∣11⟩,treturn=πℏ∣J∣,∣Ψ(treturn)⟩=−∣00⟩.\begin{aligned} t_{\mathrm{ent}}&=\frac{\pi\hbar}{4|J|}, &|\Psi(t_{\mathrm{ent}})\rangle &=\frac{|00\rangle-i\,\operatorname{sgn}(J)|11\rangle}{\sqrt2},\\ t_{\mathrm{prod}}&=\frac{\pi\hbar}{2|J|}, &|\Psi(t_{\mathrm{prod}})\rangle &=-i\,\operatorname{sgn}(J)|11\rangle,\\ t_{\mathrm{return}}&=\frac{\pi\hbar}{|J|}, &|\Psi(t_{\mathrm{return}})\rangle &=-|00\rangle. \end{aligned}

The first return to a product state is a transfer to ∣11⟩|11\rangle up to phase. Returning to the initial ray takes twice as long. The J=0J=0 state remains ∣00⟩|00\rangle. Local ZZ terms generally change this evolution and cannot be discarded without the stated zero-frequency assumption.

Excitation exchange from equal XX and YY couplings

Section titled “Excitation exchange from equal XX and YY couplings”

A different mechanism preserves the total excitation number. Set

Hex=J(X⊗X+Y⊗Y),J∈R.H_{\mathrm{ex}}=J(X\otimes X+Y\otimes Y),\qquad J\in\mathbb R.

In the one-excitation subspace,

Hex∣01⟩=2J∣10⟩,Hex∣10⟩=2J∣01⟩.H_{\mathrm{ex}}|01\rangle=2J|10\rangle,\qquad H_{\mathrm{ex}}|10\rangle=2J|01\rangle.

The terms cancel on ∣00⟩|00\rangle and ∣11⟩|11\rangle. Exponentiating the resulting two-by-two matrix gives

e−iHext/ℏ∣01⟩=cos⁡(2Jt/ℏ)∣01⟩−isin⁡(2Jt/ℏ)∣10⟩.e^{-iH_{\mathrm{ex}}t/\hbar}|01\rangle =\cos(2Jt/\hbar)|01\rangle-i\sin(2Jt/\hbar)|10\rangle.

The state is maximally entangled when both amplitudes have magnitude 1/21/\sqrt2. For J≠0J\ne0, the first such time is πℏ/(8∣J∣)\pi\hbar/(8|J|); complete excitation transfer occurs at πℏ/(4∣J∣)\pi\hbar/(4|J|), when the state is product again. Thus entanglement grows and then decreases during a coherent exchange.

The equality of the XXXX and YYYY coefficients matters. With coefficients Jx,JyJ_x,J_y, the matrix element between ∣00⟩|00\rangle and ∣11⟩|11\rangle is Jx−JyJ_x-J_y, so excitation number is generally no longer conserved. In the one-excitation subspace the equal XXXX and YYYY contributions instead add to 2J2J. This doubles the oscillation rate relative to the XX-only pair flip at the same JJ and halves the first entangling and product-transfer times.

For spin-1/21/2 angular-momentum operators sα=ℏσα/2s_\alpha=\hbar\sigma_\alpha/2, an isotropic coupling can be written

Hiso=Jℏ2∑α=x,y,zs1,α⊗s2,α=J4(X⊗X+Y⊗Y+Z⊗Z).H_{\mathrm{iso}}=\frac{J}{\hbar^2}\sum_{\alpha=x,y,z}s_{1,\alpha}\otimes s_{2,\alpha} =\frac J4(X\otimes X+Y\otimes Y+Z\otimes Z).

Here s1,αs_{1,\alpha} and s2,αs_{2,\alpha} act on their individual spaces and JJ still has energy units. The singlet and triplet energies are −3J/4-3J/4 and J/4J/4, respectively.

For two stable distinguishable oscillators with k≥0k\ge0, the spring potential k(x1−x2)2/2k(x_1-x_2)^2/2 contains the joint coupling −kx1x2-kx_1x_2 and two local frequency shifts. The coupled-oscillator example displays this decomposition.

Normal-mode coordinates can diagonalize the quadratic Hamiltonian. That does not mean the original oscillators were never coupled. It means a new set of collective degrees of freedom has been chosen. The ground state may be simple in the normal-mode variables and entangled relative to the original oscillator split.

The Jaynes–Cummings model describes a two-level system coupled to a single oscillator or cavity mode after a rotating-wave approximation. Its interaction has the form

HJC,int=ℏg(a σ++a†σ−).H_{\mathrm{JC,int}} = \hbar g \left( a\,\sigma_+ + a^\dagger\sigma_- \right).

Choose real gg with units of angular frequency and order the factors as atom, then mode. The products abbreviate aσ+=σ+⊗aa\sigma_+=\sigma_+\otimes a and a†σ−=σ−⊗a†a^\dagger\sigma_-=\sigma_-\otimes a^\dagger. Here aa annihilates a mode excitation, a†a^\dagger creates one, and σ+,σ−\sigma_+,\sigma_- raise and lower the two-level system. The coupling exchanges one excitation between the mode and the two-level system:

a†σ−∣e,n⟩=n+1 ∣g,n+1⟩,a^\dagger\sigma_-\lvert e,n\rangle = \sqrt{n+1}\,\lvert g,n+1\rangle,

while

aσ+∣g,n+1⟩=n+1 ∣e,n⟩.a\sigma_+\lvert g,n+1\rangle = \sqrt{n+1}\,\lvert e,n\rangle.

The total excitation number is conserved by the interaction:

N=a†a+σ+σ−.N = a^\dagger a + \sigma_+\sigma_-.

The approximation assumes near resonance and coupling matrix elements ∣g∣n+1|g|\sqrt{n+1} small compared with the rapidly oscillating counter-rotating frequency scale; see the Rotating-Wave Approximation for the method behind that simplification.

For two distinguishable charged particles, the nonrelativistic Coulomb interaction is

VC(x1,x2)=q1q24πϵ0∣x1−x2∣.V_C(\mathbf x_1,\mathbf x_2) = \frac{q_1q_2} {4\pi\epsilon_0\lvert\mathbf x_1-\mathbf x_2\rvert}.

It is not a sum of a function of x1\mathbf x_1 and a function of x2\mathbf x_2. It couples the coordinates through their separation. The full Hamiltonian

H=p122m1+p222m2+VC(x1,x2)H = \frac{\mathbf p_1^2}{2m_1} + \frac{\mathbf p_2^2}{2m_2} + V_C(\mathbf x_1,\mathbf x_2)

can be transformed to center-of-mass and relative coordinates for an isolated two-body problem. That transformation simplifies the problem, but it does not make the Coulomb potential a local one-particle term in the original particle split.

In many-particle language the same interaction becomes a two-body operator in field or mode variables. The detailed second-quantized form belongs to Two-Body Operators, and scattering from a long-range Coulomb potential belongs to Coulomb Scattering.

In quantum-circuit language, a controlled-phase gate is a unitary that applies a phase only to one joint basis state. A simple Hamiltonian that generates such a phase is

HCP=ℏχ ∣11⟩⟨11∣.H_{\mathrm{CP}} = \hbar\chi\, \lvert11\rangle\langle11\rvert.

For real χ\chi in angular-frequency units, its time evolution is

U(t)=diag⁡(1,1,1,e−iχt)U(t) = \operatorname{diag} \left( 1,1,1,e^{-i\chi t} \right)

in the basis ∣00⟩,∣01⟩,∣10⟩,∣11⟩\lvert00\rangle,\lvert01\rangle,\lvert10\rangle,\lvert11\rangle. For χt=π\chi t=\pi, this is the controlled-ZZ gate:

CZ=diag⁡(1,1,1,−1).CZ = \operatorname{diag}(1,1,1,-1).

Applied to ∣++⟩\lvert++\rangle, it produces

CZ∣++⟩=12(∣00⟩+∣01⟩+∣10⟩−∣11⟩),CZ\lvert++\rangle = \frac12 \bigl( \lvert00\rangle+\lvert01\rangle +\lvert10\rangle-\lvert11\rangle \bigr),

which is entangled. This is the same algebra behind the edge operation in Graph States.

The identity

∣11⟩⟨11∣=14(I−Z)⊗(I−Z)|11\rangle\langle11|=\frac14(I-Z)\otimes(I-Z)

shows exactly how a controlled phase can be generated from a Z⊗ZZ\otimes Z interaction together with local ZZ rotations and a global phase. These extra phases matter when comparing matrices.

A coupling strength is not meaningful without its units and frame. One often sees:

  • JJ as an energy scale in spin Hamiltonians;
  • gg as a field-theory, oscillator, or cavity coupling;
  • χ\chi as an angular-frequency scale for phase accumulation;
  • UU as an on-site Hubbard interaction energy;
  • q1q2/(4πϵ0)q_1q_2/(4\pi\epsilon_0) as the Coulomb strength before the distance dependence is included.

The relevant dimensionless quantity is often a phase or ratio:

θ=Jtℏ,gΔ,VΔE.\theta = \frac{Jt}{\hbar}, \qquad \frac{g}{\Delta}, \qquad \frac{V}{\Delta E}.

In the second ratio, gg and the detuning Δ\Delta must both be angular frequencies; in the third, VV denotes an energy scale. Small couplings can dominate near resonance or over long times. Large couplings can sometimes be simplified by diagonalizing a different zeroth-order Hamiltonian. The words “weak” and “strong” are therefore relative to the timescale, detuning, temperature, bandwidth, or energy gap in the problem.

A coupling constant needs units. Replacing Pauli matrices by spin operators introduces factors of ℏ/2\hbar/2. Writing an explicit normalization prevents a wrong energy or timescale.

A product operator is not a product unitary. Although A⊗BA\otimes B maps a product vector to another product vector, its exponential is generally a sum of such actions and can entangle a superposition.

A change of subsystem variables changes the entanglement question. Normal-mode coordinates can simplify a coupled Hamiltonian while its state remains entangled relative to the original oscillator factors.

  • Michael A. Nielsen and Isaac L. Chuang, Quantum Computation and Quantum Information, 10th anniversary ed., Cambridge University Press, 2010, chapters 2 and 4.
  • J. J. Sakurai and Jim Napolitano, Modern Quantum Mechanics, 3rd ed., Cambridge University Press, 2020, angular momentum and time evolution. Publisher.
  • Marlan O. Scully and M. Suhail Zubairy, Quantum Optics, Cambridge University Press, 1997, atom–field interaction. Publisher.
  • I-Sheng Yang, “The Entanglement Timescale,” Physical Review D 97, 066008 (2018), doi:10.1103/PhysRevD.97.066008, arXiv:1707.05792, Sections II–III, especially Eqs. (14)–(19) — initial purity loss and fluctuations of the coupling.
  1. Let A,BA,B be finite-dimensional Hermitian operators, gg real, Hint=gA⊗BH_{\mathrm{int}}=gA\otimes B, and suppose A∣a⟩=a∣a⟩A\lvert a\rangle=a\lvert a\rangle. Show that this interaction alone cannot entangle an initial state ∣a⟩⊗∣ϕ⟩\lvert a\rangle\otimes\lvert\phi\rangle.
Solution

On this input,

Hint(∣a⟩⊗∣ϕ⟩)=∣a⟩⊗(gaB∣ϕ⟩).H_{\mathrm{int}} (\lvert a\rangle\otimes\lvert\phi\rangle) = \lvert a\rangle\otimes (g a B\lvert\phi\rangle).

The time-evolution operator generated by this interaction acts as

e−igtA⊗B/ℏ(∣a⟩⊗∣ϕ⟩)=∣a⟩⊗e−igaBt/ℏ∣ϕ⟩.e^{-igt A\otimes B/\hbar} (\lvert a\rangle\otimes\lvert\phi\rangle) = \lvert a\rangle\otimes e^{-i g a B t/\hbar}\lvert\phi\rangle.

The result remains a product state.

  1. Factor the controlled-phase unitary into a ZZZZ evolution, two local ZZ rotations, and a global phase. Write ϕ=χt\phi=\chi t.
Solution

All four terms in the projector expansion commute, so

UCP(ϕ)=e−iϕ/4(eiϕZ/4⊗eiϕZ/4)e−iϕZ⊗Z/4.U_{\mathrm{CP}}(\phi)=e^{-i\phi/4} \bigl(e^{i\phi Z/4}\otimes e^{i\phi Z/4}\bigr) e^{-i\phi Z\otimes Z/4}.

For the three basis states other than ∣11⟩|11\rangle, the phases cancel. For ∣11⟩|11\rangle, they multiply to e−iϕe^{-i\phi}. At ϕ=π\phi=\pi this gives CZCZ exactly, including the displayed global phase.

  1. Let H=JZ⊗ZH=JZ\otimes Z and start from (3∣0⟩+∣1⟩)A/2⊗∣+⟩B(\sqrt3|0\rangle+|1\rangle)_A/2\otimes|+\rangle_B. Find the leading loss of AA‘s purity and check it against the exact reduced state. What changes if AA instead starts in ∣0⟩|0\rangle?
Solution

Initially ⟨ZA⟩=1/2\langle Z_A\rangle=1/2, so Var⁡(ZA)=3/4\operatorname{Var}(Z_A)=3/4, while Var⁡(ZB)=1\operatorname{Var}(Z_B)=1. With θ=Jt/ℏ\theta=Jt/\hbar, the leading purity loss is therefore 3θ2/23\theta^2/2.

Evolving each computational-basis amplitude and tracing out BB gives

ρA(t)=(3/43cos⁡(2θ)/43cos⁡(2θ)/41/4),1−Tr⁡ρA(t)2=38sin⁡2(2θ)=32θ2+O(θ4).\rho_A(t)=\begin{pmatrix} 3/4&\sqrt3\cos(2\theta)/4\\ \sqrt3\cos(2\theta)/4&1/4 \end{pmatrix},\qquad 1-\operatorname{Tr}\rho_A(t)^2 =\frac38\sin^2(2\theta) =\frac32\theta^2+O(\theta^4).

The exact answer also shows recoherence at θ=nπ/2\theta=n\pi/2; the short-time term alone cannot describe that return. For the input ∣0⟩A∣+⟩B|0\rangle_A|+\rangle_B, the AA variance is zero and this interaction alone leaves the state product for every time: ∣0⟩A⊗e−iθZ∣+⟩B|0\rangle_A\otimes e^{-i\theta Z}|+\rangle_B.

  1. Let H=JxX⊗X+JyY⊗YH=J_xX\otimes X+J_yY\otimes Y. Find its action on ∣00⟩|00\rangle and state when total excitation number is conserved.
Solution

Since X∣0⟩=∣1⟩X|0\rangle=|1\rangle and Y∣0⟩=i∣1⟩Y|0\rangle=i|1\rangle,

H∣00⟩=(Jx−Jy)∣11⟩.H|00\rangle=(J_x-J_y)|11\rangle.

Likewise, H∣11⟩=(Jx−Jy)∣00⟩H|11\rangle=(J_x-J_y)|00\rangle. These transitions change excitation number by two. They vanish exactly when Jx=JyJ_x=J_y, leaving only transitions within the one-excitation subspace (including the zero-coupling case).