With the recent production of Bose-Einstein condensates using NASA's Cold Atom Laboratory (CAL) aboard the International Space Station, research is underway focusing on the extent to which quantum mechanics can be studied in a microgravity environment. These condensates have the potential to be the coldest ever studied in experiment and in free-fall their place in orbit allows us to observe them in long time-of-flights. This thesis reports fitting analyses and trap frequency characterization of imaging data from condensates in conventional magnetic potentials. This information will be used for the calibration and design of future experiments with CAL, regarding both conventional and radio-frequency dressed traps. Of particular interest to further study are ellipsoidal shell condensates and the quasi-two-dimensional condensate that exists on its surface in the limit of low shell thickness.
With the recent production of Bose-Einstein condensates using NASA's Cold Atom Laboratory (CAL) aboard the International Space Station, research is underway focusing on the extent to which quantum mechanics can be studied in a microgravity environment. These condensates have the potential to be the coldest ever studied in experiment and in free-fall their place in orbit allows us to observe them in long time-of-flights. This thesis reports fitting analyses and trap frequency characterization of imaging data from condensates in conventional magnetic potentials. This information will be used for the calibration and design of future experiments with CAL, regarding both conventional and radio-frequency dressed traps. Of particular interest to further study are ellipsoidal shell condensates and the quasi-two-dimensional condensate that exists on its surface in the limit of low shell thickness.
Extending the understanding of Bose-Einstein condensate (BEC) physics to new geometries and topologies has a long and varied history in ultracold atomic physics. One such new geometry is that of a bubble, where a condensate would be confined to the surface of an ellipsoidal shell. Study of this geometry would give insight into new collective modes, self-interference effects, topology-dependent vortex behavior, dimensionality crossovers from thick to thin shells, and the properties of condensates pushed into the ultradilute limit. Here we propose to implement a realistic experimental framework for generating shell-geometry BEC using radiofrequency dressing of magnetically trapped samples. Such a tantalizing state of matter is inaccessible terrestrially due to the distorting effect of gravity on experimentally feasible shell potentials. The debut of an orbital BEC machine (NASA Cold Atom Laboratory, aboard the International Space Station) has enabled the operation of quantum-gas experiments in a regime of perpetual freefall, and thus has permitted the planning of microgravity shell-geometry BEC experiments. We discuss specific experimental configurations, applicable inhomogeneities and other experimental challenges, and outline potential experiments.
Abstract We report the status of the Cold Atom Lab (CAL) instrument to be operated aboard the International Space Station (ISS). Utilizing a compact atom chip-based system to create ultracold mixtures and degenerate samples of 87 Rb, 39 K, and 41 K, CAL is a multi-user facility developed by NASA’s Jet Propulsion Laboratory to provide the first persistent quantum gas platform in the microgravity conditions of space. Within this unique environment, atom traps can be decompressed to arbitrarily weak confining potentials, producing a new regime of picokelvin temperatures and ultra-low densities. Further, the complete removal of these confining potential allows the free fall evolution of ultracold clouds to be observed on unprecedented timescales compared to earthbound instruments. This unique facility will enable novel ultracold atom research to be remotely performed by an international group of principle investigators with broad applications in fundamental physics and inertial sensing. Here, we describe the development and validation of critical CAL technologies, including demonstration of the first on-chip Bose–Einstein condensation (BEC) of 87 Rb with microwave-based evaporation and the generation of ultracold dual-species quantum gas mixtures of 39 K/ 87 Rb and 41 K/ 87 Rb in an atom chip trap via sympathetic cooling.
Inspired by investigations of Bose-Einstein condensates (BECs) produced in the Cold Atom Laboratory (CAL) aboard the International Space Station, we present a study of thermodynamic properties of shell-shaped BECs. Within the context of a spherically symmetric ``bubble trap'' potential, we study the evolution of the system from small filled spheres to hollow, large, thin shells via the tuning of trap parameters. We analyze the bubble trap spectrum and states and track the distinct changes in spectra between radial and angular modes across the evolution. This separation of the excitation spectrum provides a basis for quantifying dimensional crossover to quasi-2D physics at a given temperature. Using the spectral data, for a range of trap parameters, we compute the critical temperature for a fixed number of particles to form a BEC. For a set of initial temperatures, we also evaluate the change in temperature that would occur in adiabatic expansion from small filled sphere to large thin shell were the trap to be dynamically tuned. We show that the system cools during this expansion but that the decrease in critical temperature occurs more rapidly, thus resulting in depletion of any initial condensate. We contrast our spectral methods with standard semiclassical treatments, which we find must be used with caution in the thin-shell limit. With regard to interactions, using energetic considerations and corroborated through Bogoliubov treatments, we demonstrate that they would be less important for thin shells due to reduced density but vortex physics would become more predominant. Finally, we apply our treatments to traps that realistically model CAL experiments and borrow from the thermodynamic insights found in the idealized bubble case during adiabatic expansion.
Cold Atom Laboratory (CAL) is a facility that will enable scientists to study ultra-cold quantum gases in a microgravity environment on the International Space Station (ISS) beginning in 2016. The primary science data for each experiment consists of two images taken in quick succession. The first image is of the trapped cold atoms and the second image is of the background. The two images are subtracted to obtain optical density. These raw Level 0 atom and background images are processed into the Level 1 optical density data product, and then into the Level 2 data products: atom number, Magneto-Optical Trap (MOT) lifetime, magnetic chip-trap atom lifetime, and condensate fraction. These products can also be used as diagnostics of the instrument health. With experiments being conducted for 8 hours every day, the amount of data being generated poses many technical challenges, such as downlinking and managing the required data volume. A parallel processing design is described, implemented, and benchmarked. In addition to optimizing the data pipeline, accuracy and speed in producing the Level 1 and 2 data products is key. Algorithms for feature recognition are explored, facilitating image cropping and accurate atom number calculations.
The Cold Atom Laboratory is a multipurpose ultracold gas experiment currently being developed for operation on the international space station. It will have the ability to demonstrate proof-of-principle atom interferometry experiments in space. By using microgravity, atom interferometry has the potential to achieve extremely good performance in sensing and navigation applications. Terrestrial experiments can be used to explore potential challenges and prior to launch. One issue of concern is the release of cold atoms from a magnetic trap into free space. Although the atoms will not fall, they can acquire relatively large velocities due to technical limitations such as stray magnetic fields. This can limit the time available for measurements and thus the atom interferometer performance.
A growing subfield of atomic physics is focused on the miniaturization of Bose-Einstein condensate (BEC)-producing apparatus. Perhaps the largest step forward in this area was the development of the so-called “atom chip.” These microfabricated devices can create tight traps for neutral atoms. In 2018, NASA’s Cold Atom Laboratory (CAL) was launched and installed aboard the International Space Station (ISS). It utilizes a modified miniature atom chip apparatus produced by ColdQuanta called the RuBECi. In this thesis, we present progress towards achieving BEC in a Bates-owned RuBECi, particularly focusing on the laser cooling and magneto-optical trapping stages of the BEC process.