Math 2.0

Quantum theory Definition

Faddeev equations

Builds on Scattering theoryHilbert spaceSelf-adjoint operatorResolvent

Definition

Consider three particles with the Hilbert space ℋ=L2(ℝ6)\mathcal{H} = L^2(\R^6) of the relative motion, after removal of the center of mass. Let H0H_0 be the self-adjoint kinetic energy operator. Let V1,V2,V3V_1, V_2, V_3 be the pair potentials, where ViV_i is the interaction of the pair that does not contain particle ii. Let H=H0+V1+V2+V3H = H_0 + V_1 + V_2 + V_3 and V=V1+V2+V3V = V_1 + V_2 + V_3. For z∈ℂ∖ℝz \in \C \setminus \R, let G0(z)=(z−H0)−1G_0(z) = (z - H_0)^{-1} be the free resolvent. Let Ti(z)T_i(z) be the two-body transition operator of the pair ii in the three-body space, defined by Ti(z)=Vi+Vi G0(z) Ti(z).T_i(z) = V_i + V_i\, G_0(z)\, T_i(z). The Faddeev equations are the system for three operators T(1),T(2),T(3)T^{(1)}, T^{(2)}, T^{(3)} T(i)(z)=Ti(z)+Ti(z) G0(z)∑j≠iT(j)(z),i=1,2,3.T^{(i)}(z) = T_i(z) + T_i(z)\, G_0(z) \sum_{j \ne i} T^{(j)}(z), \qquad i = 1, 2, 3. The sum T(z)=T(1)(z)+T(2)(z)+T(3)(z)T(z) = T^{(1)}(z) + T^{(2)}(z) + T^{(3)}(z) then solves the three-body equation T(z)=V+V G0(z) T(z)T(z) = V + V\, G_0(z)\, T(z). For a bound state ψ\psi of energy EE below the spectrum of H0H_0, the wave function form is ψ=ψ1+ψ2+ψ3\psi = \psi_1 + \psi_2 + \psi_3 with ψi=G0(E) Ti(E)∑j≠iψj,i=1,2,3.\psi_i = G_0(E)\, T_i(E) \sum_{j \ne i} \psi_j, \qquad i = 1, 2, 3.

Remarks

Check of the operator form: put T(i)=Vi+ViG0TT^{(i)} = V_i + V_i G_0 T; then T(i)−ViG0T(i)=Vi(1+G0∑j≠iT(j))T^{(i)} - V_i G_0 T^{(i)} = V_i \big(1 + G_0 \sum_{j \ne i} T^{(j)}\big), and (1−ViG0)−1Vi=Ti(1 - V_i G_0)^{-1} V_i = T_i gives the Faddeev equation; summing over ii gives T=V+VG0TT = V + V G_0 T. Check of the wave function form: if Hψ=EψH\psi = E\psi, then ψ=G0(E)Vψ\psi = G_0(E) V \psi, and ψi=G0(E)Viψ\psi_i = G_0(E) V_i \psi satisfies (1−G0Vi)ψi=G0Vi∑j≠iψj(1 - G_0 V_i)\psi_i = G_0 V_i \sum_{j \ne i} \psi_j, which is the stated equation since (1−G0Vi)−1G0Vi=G0Ti(1 - G_0 V_i)^{-1} G_0 V_i = G_0 T_i. Non-example: the three-body Lippmann–Schwinger equation T=V+VG0TT = V + V G_0 T itself has a kernel VG0V G_0 that is not compact, even after iteration. The reason is the terms in which one pair interacts while the third particle moves freely. These terms carry a delta function in the momentum of the spectator particle. The kernel of the Faddeev system has no such disconnected terms after one iteration, and for suitable short-range potentials a power of it is compact on suitable function spaces. The equations were introduced by L. D. Faddeev in 1960.

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Further reading

  1. Web https://en.wikipedia.org/wiki/Faddeev_equations
About this page
Tag3Z6PB686G6
URIm2://3Z6PB686G6
Kinddefinition
WritingW0 stub
MSC81U10
DefinesFaddeev equations
UsesScattering theory, Hilbert space, Self-adjoint operator, Resolvent
Changed3 November 2026

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