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1.
Phys Rev Lett ; 96(4): 040405, 2006 Feb 03.
Artigo em Inglês | MEDLINE | ID: mdl-16486796

RESUMO

We propose a physical system allowing one to experimentally observe the distribution of the complex zeros of a random polynomial. We consider a degenerate, rotating, quasi-ideal atomic Bose gas prepared in the lowest Landau level. Thermal fluctuations provide the randomness of the bosonic field and of the locations of the vortex cores. These vortices can be mapped to zeros of random polynomials, and observed in the density profile of the gas.

2.
Phys Rev Lett ; 95(19): 190403, 2005 Nov 04.
Artigo em Inglês | MEDLINE | ID: mdl-16383962

RESUMO

We have observed phase defects in quasi-2D Bose-Einstein condensates close to the condensation temperature. Either a single or several equally spaced condensates are produced by selectively evaporating the sites of a 1D optical lattice. When several clouds are released from the lattice and allowed to overlap, dislocation lines in the interference patterns reveal nontrivial phase defects.

3.
Phys Rev Lett ; 93(18): 180403, 2004 Oct 29.
Artigo em Inglês | MEDLINE | ID: mdl-15525136

RESUMO

We have observed high-contrast matter wave interference between 30 Bose-Einstein condensates with uncorrelated phases. Interferences were observed after the independent condensates were released from a one-dimensional optical lattice and allowed to overlap. This phenomenon is explained with a simple theoretical model, which generalizes the analysis of the interference of two condensates.

4.
Phys Rev Lett ; 92(5): 050403, 2004 Feb 06.
Artigo em Inglês | MEDLINE | ID: mdl-14995289

RESUMO

We study the rotation of a 87Rb Bose-Einstein condensate confined in a quadratic plus quartic potential. This trap configuration allows one to increase the rotation frequency of the gas above the trap frequency. In such a fast rotation regime we observe a dramatic change in the appearance of the quantum gas. The vortices which were easily detectable for a slower rotation become much less visible, and their surface density is well below the value expected for this rotation frequency domain. We discuss some possible tracks to account for this effect.

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