7. <strong>Quantum</strong> simulations <strong>of</strong> evaporatively cooled <strong>Bose</strong> condensateslength scales. In fact the presence <strong>of</strong> interparticle interactions means that the atom densityshould be anticorrelated at short distances. There have been indirect local measurementsthat demonstrate the existence <strong>of</strong> some forms <strong>of</strong> higher-order coherence[18, 26, 84, 122],but a complete description or confirmation <strong>of</strong> all the coherence properties <strong>of</strong> the condensateis not yet available. Indeed, it has been pointed out[135] that these experiments donot measure the true second-order correlation function, and that anticorrelation effectsdue to interatomic repulsion extend over longer distances than the scattering length a 0 .Thus a lack <strong>of</strong> second-order coherence over short length scales should be measurable inthe laboratory.Possession <strong>of</strong> coherence implies the existence <strong>of</strong> a phase. Can a phase be ascribedto a condensate in isolation or only in relation to other condensates? Such issues wereaddressed in Ch. 3, in the context <strong>of</strong> measurements <strong>of</strong> relative phase. There it was shownthat even if a condensate in isolation was in a number state, interaction with a secondcondensate induced a relative phase, thus breaking the symmetry. In contrast, in othercondensed-matter systems, such as superfluids and superconductors, which contain manymore particles (by a factor <strong>of</strong> 10 20 or more), the symmetry-breaking processes occur duringthe formation <strong>of</strong> the order parameter when quantum fluctuations are important. Duringthe early stages <strong>of</strong> order-parameter formation, the condensed part <strong>of</strong> the system is smalland subject to quantum fluctuations. As <strong>Bose</strong> stimulation populates the condensate, thesefluctuations freeze out, to become macroscopic properties <strong>of</strong> an essentially classical system.In the case <strong>of</strong> condensates in atom traps, if and how the symmetry breaks during theformation remains an open question. Is there sufficient decoherence that the environmentcan couple to the condensate order parameter and break the symmetry, or are thesecondensates closer to number states, in which phase remains undetermined until an actualmeasurement or other intervention? This process <strong>of</strong> symmetry breaking has much widerimplications than for <strong>Bose</strong>-condensed systems; it aids the understanding <strong>of</strong> cosmologicalevolution and the formation <strong>of</strong> structure in the early universe[81, 104, 190, 191].To address important issues such as these about the nature <strong>of</strong> the condensate, a quantummechanical simulation <strong>of</strong> the evaporative cooling process that leads to condensationmust be undertaken. The final ground state <strong>of</strong> this many-body system is the result <strong>of</strong>a quantum dynamical process which is far from thermal equilibrium. This problem hasbeen approached by many authors using various approximate methods. But to provide a141
7. <strong>Quantum</strong> simulations <strong>of</strong> evaporatively cooled <strong>Bose</strong> condensatesbenchmark for these treatments, and to precisely determine coherence properties, all thequantum effects must be included without approximation.7.1.2 Evaporative coolingThe production <strong>of</strong> atomic <strong>Bose</strong> condensates in recent years has relied upon the development<strong>of</strong> efficient atom trapping and cooling techniques. In particular, it is the amazing success<strong>of</strong> evaporative cooling techniques that has enabled condensation in atom traps. Atomevaporation cools far below recoil limit <strong>of</strong> laser cooling and reduces the temperature bymany orders <strong>of</strong> magnitude without diluting the gas. In this process, the gas is loaded into amagnetic or magneto-optical trap, perhaps at first undergoing some laser cooling[145]. Thegas will approximately obey a <strong>Bose</strong>-<strong>Einstein</strong> distribution. Atoms in the high-temperaturetail <strong>of</strong> the distribution have enough energy to escape from the trap, and do so takingaway more than the average energy per atom. The remaining atoms rethermalise throughelastic interatomic collisions, thereby repopulating the upper levels. The temperature isthus lowered, and there is always a supply <strong>of</strong> hot atoms which can take away more energy.The evaporative cooling procedure was first developed to cool hydrogen atoms[41, 82]in attempts to produce <strong>Bose</strong> condensation, but was more successfully applied to alkalimetalgases[37, 103, 143], leading to condensation in rubidium ( 87 Rb)[3] sodium ( 23 Na)[35],and lithium ( 7 Na)[16]. These alkali gases have a larger effective scattering cross sectionfor elastic collisions and so rethermalise at the faster rate necessary to overcome atomloss processes, such as three-body recombination. Evaporative cooling is now a commonprocedure, with <strong>Bose</strong> condensates being produced in approximately twenty laboratoriesworldwide at the time <strong>of</strong> writing, mainly in 87 Rb and including one in hydrogen[59].This chapter presents the results <strong>of</strong> using phase-space methods to directly simulate thequantum dynamics <strong>of</strong> evaporatively cooled condensates. The method enables calculation<strong>of</strong> the time evolution <strong>of</strong> system properties. We will review the results for several physicalsituations, which reveal interesting transient behaviours and also evidence for the spontaneousformation <strong>of</strong> additional structures, including the evidence for vortices as reportedin [46]. This thesis does not attempt to provide conclusive answers to all the issues raisedabove or to completely characterise the condensate ground state, but rather it summarisesthe progress that has been made using phase-space techniques. These first attempts <strong>of</strong>such multimode quantum calculations constitute only the first steps <strong>of</strong> a comprehensive142
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AbstractThe properties of an atomic
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. . . but this book is already too