2009
DOI: 10.48550/arxiv.0901.0636
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Cold Bosons in Optical Lattices

V. I. Yukalov

Abstract: Basic properties of cold Bose atoms in optical lattices are reviewed. The main principles of correct self-consistent description of arbitrary systems with Bose-Einstein condensate are formulated. Theoretical methods for describing regular periodic lattices are presented. A special attention is paid to the discussion of Bose-atom properties in the frame of the boson Hubbard model. Optical lattices with arbitrary strong disorder, induced by random potentials, are treated. Possible applications of cold atoms in o… Show more

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Cited by 1 publication
(3 citation statements)
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“…( 11) describes processes where no photons are lost from the system, either because none are emitted, or because one is emitted but is reabsorbed before time ∆t [16,17]. As it appears in the master equation (11) in a similar form to the − i [H, ρ] of a Hamiltonian, but describes only evolution under the condition of no photon loss, this term is called the conditional Hamiltonian. Unlike a normal Hamiltonian, it is not Hermitian, but norm decreasing; this represents the decreasing probability that this condition will continue to hold, and in the master equation is balanced by R(ρ).…”
Section: The No-photon Time Evolutionmentioning
confidence: 99%
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“…( 11) describes processes where no photons are lost from the system, either because none are emitted, or because one is emitted but is reabsorbed before time ∆t [16,17]. As it appears in the master equation (11) in a similar form to the − i [H, ρ] of a Hamiltonian, but describes only evolution under the condition of no photon loss, this term is called the conditional Hamiltonian. Unlike a normal Hamiltonian, it is not Hermitian, but norm decreasing; this represents the decreasing probability that this condition will continue to hold, and in the master equation is balanced by R(ρ).…”
Section: The No-photon Time Evolutionmentioning
confidence: 99%
“…Under the master equation (11), the density matrix converges to a steady state, and for cooling we would like it to converge within a reasonable time to a state with the lowest possible temperature, or equivalently phonon number. In this section, we calculate this steady state using an open system version of Feynman diagrams.…”
Section: Steady State Density Matrixmentioning
confidence: 99%
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