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Em vista de recentes determinações experimentais do perfil de Compton (Eisenberger, Phys. Rev., A2, 1678(1970); Wellenstein e Bonham, Phys. Rev., A7, 1568(1973}, procuramos efetuar um estudo comparativo de cálculos teóricos do perfil de Compton para o átomo de hélio (1S). Para tal, o conjunto de funções de onda elaboradas por Shull e L6wdin (J.Chem.Phy., 23, 1362(1955); 23, 1565(1955}; 30, 617(1959} mostrou-se bastante adequado, visto que permitiu observar a influência da função de onda no cálculo de perfil de Compton. Nossos resultados mostram em contraste à idéia geralmente aceita, que mesmo funções de onda igualmente boas para o cálculo da energia podem fornecer perfis de Compton com um erro maior que o experimental. Alem disso, apresentamos um conjunto de novos dados para o perfil de Compton e para a distribuição radial de momentum. Procuramos, também explicar essas discrepâncias relacionando-as com a transformada de Fourier da função de onda no espaço de configuração. / In view of the recent experimental determination of the Compton profile (Eisenberger, Phys., Rev., A2,1678(1970); Wellenstein and Bonham, Phys, Rev., A7, 1568(1973), we have performed a comparative study of theoretical calcu1ation of the Compton profile for the helium atom (1S). For such, the set of wave functions elaborated by Shull and Löwdin (J.Chem. Phys., 23, 1362(1955); 23, 1565(1955); 30, 617(1959) show itself specially suftable since it was possible to observe the influence af the wave functions on the calculated profile. Our results show in, contrast to general accepted idea, that even equally good wave functions in the energy sense may give theoretical profiles in error greater than the experimental one. Besides, we have presented a set of new data for the Compton profile and radial momentum distribution. A1so we have tried to explain the source of these discrepancies relating them to the Fourier transformation of the wave function in the configuration space.

Em vista de recentes determinações experimentais do perfil de Compton (Eisenberger, Phys. Rev., A2, 1678(1970); Wellenstein e Bonham, Phys. Rev., A7, 1568(1973}, procuramos efetuar um estudo comparativo de cálculos teóricos do perfil de Compton para o átomo de hélio (1S). Para tal, o conjunto de funções de onda elaboradas por Shull e L6wdin (J.Chem.Phy., 23, 1362(1955); 23, 1565(1955}; 30, 617(1959} mostrou-se bastante adequado, visto que permitiu observar a influência da função de onda no cálculo de perfil de Compton. Nossos resultados mostram em contraste à idéia geralmente aceita, que mesmo funções de onda igualmente boas para o cálculo da energia podem fornecer perfis de Compton com um erro maior que o experimental. Alem disso, apresentamos um conjunto de novos dados para o perfil de Compton e para a distribuição radial de momentum. Procuramos, também explicar essas discrepâncias relacionando-as com a transformada de Fourier da função de onda no espaço de configuração. / In view of the recent experimental determination of the Compton profile (Eisenberger, Phys., Rev., A2,1678(1970); Wellenstein and Bonham, Phys, Rev., A7, 1568(1973), we have performed a comparative study of theoretical calcu1ation of the Compton profile for the helium atom (1S). For such, the set of wave functions elaborated by Shull and Löwdin (J.Chem. Phys., 23, 1362(1955); 23, 1565(1955); 30, 617(1959) show itself specially suftable since it was possible to observe the influence af the wave functions on the calculated profile. Our results show in, contrast to general accepted idea, that even equally good wave functions in the energy sense may give theoretical profiles in error greater than the experimental one. Besides, we have presented a set of new data for the Compton profile and radial momentum distribution. A1so we have tried to explain the source of these discrepancies relating them to the Fourier transformation of the wave function in the configuration space.

Ce travail de thèse démontre une technique de détection capable de mesurer, avec une sensibilité à l'atome unique, l'espace des impulsions d'un gaz ultrafroid chargé dans un réseau optique 3D. Nous avons développé un détecteur basé sur des galettes de micro-canaux, capable de sonder électroniquement des nuages d'Hélium-4 métastable. Le gaz est détecté après un temps de vol de 325ms, suffisamment long pour atteindre l'expansion de champ lointain, où la distribution spatiale du gaz coïncide avec la distribution d'impulsion asymptotique. En se plac{c}ant dans un régime proche du remplissage unitaire du réseau, les effets de collisions entre atomes aux premiers instants de l'expansion deviennent négligeables, et donc la distribution d'impulsion asymptotique est égale à la distribution d'impulsion in situ. Nous démontrons expérimentalement cette égalité en comparant nos mesures en champ lointain avec la distribution d'impulsion calculée à partir de l'Hamiltonien de Bose-Hubbard, gr^ace à des simulations Monte Carlo Quantique. Nous observons un bon accord avec la théorie sur plus de 3 ordres de grandeur en densité. Ces simulations sont calculées à partir de nos paramètres expérimentaux, la température étant la seule variable ajustable. Nous utilisons ensuite cette comparaison pour réaliser une thermométrie précise du gaz sur réseau, permettant une exploration de la transition superfluide-gaz normal à travers la mesure directe de différentes quantités, comme la fraction condensée ou la fonction de corrélation à deux particules. / In this thesis, we report the demonstration of a detection technique able to probe, with a single-atom sensitivity, the momentum distribution of an ultracold gas loaded inside a 3D optical lattice. We have developed a micro-channel plate detector, able to electronically probe clouds of metastable Helium-4. The gas is detected after a time-of-flight of 325ms, long enough to reach the far-field expansion, where the spatial distribution of the cloud can be mapped to the asymptotic momentum distribution. By putting ourselves in a regime where the lattice filling is close to unity, the atomic collisions in the first instant of the expansion become negligible, so that the asymptotic momentum distribution is equal to the in situ momentum distribution. We experimentally demonstrate this equality, by comparing our far-field measurements with the momentum distribution calculated from the Bose-Hubbard Hamiltonian, thanks to ab initio quantum Monte Carlo simulations. We show a good agreement with the theory over more than 3 orders of magnitude in density. Those simulations are calculated with our experimental parameters, the temperature being the only adjustable variable. We then use this comparison to perform a precise thermometry of the lattice gas, allowing us to explore the superfluid-normal gas transition through a direct measurement of different quantities, like the condensed fraction or the two-particles correlation function.