Abstract

How and why could an interacting system of many particles be described as if all particles were independent and identically distributed? This question is at least as old as statistical mechanics itself. Its quantum version has been rejuvenated by the birth of cold atoms physics. In particular, the experimental creation of Bose–Einstein condensates leads to the following variant: why and how can a large assembly of very cold interacting bosons (quantum particles deprived of the Pauli exclusion principle) all populate the same quantum state? In this text I review the various mathematical techniques allowing to prove that the lowest energy state of a bosonic system forms, in a reasonable macroscopic limit of large particle number, a Bose–Einstein condensate. This means that indeed in the relevant limit all particles approximately behave as if independent and identically distributed, according to a law determined by minimizing a non-linear Schrödinger energy functional. This is a particular instance of the justification of the mean-field approximation in statistical mechanics, starting from the basic many-body Schrödinger Hamiltonian.

Highlights

  • We start with the basic mathematical description of N non-relativistic d−dimensional quantum particles in a scalar potential V : Rd → R and a gauge vector potential A : Rd → Rd, interacting via an even pairinteraction potential w : Rd → R

  • Readers already acquainted with quantum statistical mechanics will probably want to skip to Section 1.4 after glancing at Section 1.1, and very briefly at Sections 1.2 and 1.3 to get familiar with the notation1 I use

  • In most of the text our applications will be to cold alkali gases [249, 255, 35, 83, 108, 71, 315], where the particles are neutral atoms, the magnetic field is artificial, the external potential is a magneto-optic trap and interactions are via van der Waals forces

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Summary

Aims and scope

Readers already acquainted with quantum statistical mechanics will probably want to skip to Section 1.4 after glancing at Section 1.1, and very briefly at Sections 1.2 and 1.3 to get familiar with the notation I use. The first three sections are intended as a very basic introduction to newcomers in the field

Introduction
Basic quantum statistical mechanics
Second-quantized formalism
Mean-field approximation and scaling limits
Non-linear Schrodinger functionals
Main theorem
Outline
Connections and further topics
Hamiltonian-based methods
Applying the classical de Finetti theorem
The quantum de Finetti theorem and applications
Localization plus quantum de Finetti
Coherent states method
Better localization in the coherent states method
Conclusion
Moments estimates
Pair correlations and the scattering length
Jastrow-Dyson trial states
Bogoliubov-like trial states
Dyson lemmas
Thermodynamic energy of the homogeneous dilute gas
Local density approximation method
Bogoliubov methods for GP ground states
Full Text
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