Physical Review A · 2008 · 358 citations · 54 references
Numerical AnalysisMany-body DynamicsQuantum DynamicBosonic SystemsEngineeringPhysicsIdentical BosonsMany-body Quantum PhysicQuantum Field TheoryComputational ChemistryPropagation ProcessComputational MechanicsTime-dependent OrbitalsIntegrable SystemGross-pitaevskii EquationBose-einstein CondensationMany-body Problem
The evolution of Bose‑Einstein condensates is typically described by the time‑dependent Gross‑Pitaevskii mean‑field theory, which assumes all bosons occupy a single time‑dependent one‑particle state. The study develops an essentially exact many‑body theory for propagating the time‑dependent Schrödinger equation of \(N\) interacting identical bosons, thereby going beyond mean‑field approximations. The method represents the many‑boson wave function as a time‑dependent linear combination of permanents built from orthogonal orbitals, with both coefficients and orbitals determined by a time‑dependent variational principle that yields coupled first‑order differential equations for orbitals and coefficients, defining the multiconfigurational time‑dependent Hartree for bosons (MCTDHB\((M)\)). Numerical implementation demonstrates convergence as the number of orbitals increases, with illustrative examples of trapped Bose‑Einstein condensate dynamics and a four‑boson double‑well case confirming the method’s accuracy.
The evolution of Bose-Einstein condensates is amply described by the time-dependent Gross-Pitaevskii mean-field theory which assumes all bosons to reside in a single time-dependent one-particle state throughout the propagation process. In this work, we go beyond mean field and develop an essentially exact many-body theory for the propagation of the time-dependent Schr\"odinger equation of $N$ interacting identical bosons. In our theory, the time-dependent many-boson wave function is written as a sum of permanents assembled from orthogonal one-particle functions, or orbitals, where both the expansion coefficients and the permanents (orbitals) themselves are time-dependent and fully determined according to a standard time-dependent variational principle. By employing either the usual Lagrangian formulation or the Dirac-Frenkel variational principle we arrive at two sets of coupled equations of motion, one for the orbitals and one for the expansion coefficients. The first set comprises of first-order differential equations in time and nonlinear integrodifferential equations in position space, whereas the second set consists of first-order differential equations with time-dependent coefficients. We call our theory multiconfigurational time-dependent Hartree for bosons, or $\text{MCTDHB}(M)$, where $M$ specifies the number of time-dependent orbitals used to construct the permanents. Numerical implementation of the theory is reported and illustrative numerical examples of many-body dynamics of trapped Bose-Einstein condensates are provided and discussed. The convergence of the method with a growing number $M$ of orbitals is demonstrated in a specific example of four interacting bosons in a double well.
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Observation of Bose-Einstein Condensation in a Dilute Atomic Vapor
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