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Bulletin of the American Physical Society

Quantum Gases on the ISS Capabilities of the BECCAL facility

Lisa Wörner, Christian Schubert, Jens Große, Claus Braxmaier, Ernst Maria Rasel, Wolfgang P. Schleich

Published Jun 5, 2020• 0 citations
OpenAlex

Abstract

BECCAL (Bose-Einstein-Condensate - Cold Atom Laboratory) is an experiment designed to be housed on the International Space Station (ISS) within a bilateral collaboration between DLR and NASA. The payload's design and operation are based on the previous quantum experiments under microgravity, QUANTUS (drop tower), MAIUS (sounding rocket), and CAL (NASA operated ISS experiment). The scienti�c capabilities, outlined here, cover a wide range of cold atom manipulation and observation. Additionally, the payload strives to pave the road for future microgravity missions housing cold atom ensembles.

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IEEE Aerospace Conference (AERO)•Mar 1, 2014•6 citations
BECCAL (Bose-Einstein-Condensate - Cold Atom Laboratory) is an experiment designed to be
housed on the International Space Station (ISS) within a bilateral collaboration between DLR and
NASA. The payload's design and operation are based on the previous quantum experiments under
microgravity, QUANTUS (drop tower), MAIUS (sounding rocket), and CAL (NASA operated ISS
experiment). The scienti�c capabilities, outlined here, cover a wide range of cold atom manipulation
and observation. Additionally, the payload strives to pave the road for future microgravity missions
housing cold atom ensembles.
The Bose-Einstein Condensate and Cold Atom Laboratory (BECCAL) is a DLR-NASA collaboration targeting the operation of a multi-user facility aboard the International Space Station (ISS). BECCAL will be a pathfinder mission to test concepts of future quantum sensors with applications in e.g. gravity missions for earth observation and search for a violation of the universality of free fall. It will feature various capabilities for quantum-optical, atom-optical, and atom-interferometric manipulation methods of laser-cooled atoms and notably Bose-Einstein condensates. The persistent microgravity condition aboard the ISS opens the opportunity for enhanced free-fall times, overlapping multi-species trap configurations impossible on earth thanks to the lack of gravitational sag, and repeatability for detailed statistical analysis. In this contribution the design implementation of these capabilities will be presented and derived performance estimates will be discussed. The BECCAL payload is designed and constructed by the BECCAL Collaboration comprising the DLR Institute of Quantum Technology, the DLR Institute for Satellite Geodesy and Inertial Sensing, the DLR Institute for Software Technology, the Leibniz Universität Hannover, the Humboldt-Universität zu Berlin, the Johannes Gutenberg-Universität Mainz, the Ferdinand Braun Institut für Höchstfrequenztechnik, the Universität Bremen, the Universtität Hamburg, the Universität Ulm, and OHB System AG, with funding support by the DLR Space Agency.
Ultra-cold quantum gases in space promise to boost the sensitivity of matter-wave interferometers. Applications of the latter extend from fundamental physics over the use in navigation to interdisciplinary applications such as geodesy, e.g. satellite gravimetry [1, 2]. Exploiting quantum gases for high-precision interferometry places high demands on their control and manipulation. We take benefit of various microgravity platforms such as the Bremen drop tower [3], the Einstein elevator in Hannover [4], sounding rockets [5,6] and the international space station [7] to advance the necessary methods. The DLR-mission MAIUS-1 demonstrated Bose-Einstein condensation and performed first interferometry experiments [4]. NASA’s Cold Atom Laboratory continues this research in orbit on the ISS [7]. In addition, atom interferometry is pursued in highly dynamic environments such as parabolic flights [8]. Starting from a rubidium Bose-Einstein condensate, recently lowest expansion energies have been achieved by us in the Bremen drop tower as required for extending atom interferometry over several seconds [9]. Extending these methods to quantum mixtures not only opens up new physics in the absence of buoyancy, but also faces challenges regarding their use for interferometry. Interferometers based on two chemical elements have been proposed for quantum tests of the equivalence principle on the ISS as well as on satellites. Currently we prepare a sounding rocket mission to investigate the simultaneous generation and manipulation of potassium and rubidium condensates [10]. Together with CAL [7], these experiments will prepare the DLR-NASA multi-user facility BECCAL for research on quantum gas mixtures and interferometry [11] as well as enhance the readiness level of methods required for STE-QUEST [12], a proposal for a satellite mission currently studied in an modified version within ESA’s VOYAGE 2050 program [13].
Abstract Microgravity eases several constraints limiting experiments with ultracold and condensed atoms on ground. It enables extended times of flight without suspension and eliminates the gravitational sag for trapped atoms. These advantages motivated numerous initiatives to adapt and operate experimental setups on microgravity platforms. We describe the design of the payload, motivations for design choices, and capabilities of the Bose-Einstein Condensate and Cold Atom Laboratory (BECCAL), a NASA-DLR collaboration. BECCAL builds on the heritage of previous devices operated in microgravity, features rubidium and potassium, multiple options for magnetic and optical trapping, different methods for coherent manipulation, and will offer new perspectives for experiments on quantum optics, atom optics, and atom interferometry in the unique microgravity environment on board the International Space Station.
The BECCAL (Bose-Einstein-Condensate – Cold Atom Laboratory) apparatus is a high precision quantum optics experiment which will fly on the International Space Station (ISS). It shall be constructed and operated within a bilateral collaboration between the German Aerospace Center (DLR) and the National Aeronautics and Space Administration (NASA). As a multi user facility, BECCAL shall satisfy the needs of both the American and German scientific community concerning cold atom physics. Various needs are expressed for the functionalities of the scientific apparatus extended by the requirements for operation of an instrument aboard the ISS. For installation into the dedicated accommodation the complex systems have to be mechanically and thermally designed to meet these requirements. Additionally BECCAL has to fit into the Size Weight and Power (SWaP) budget given by the launcher and the ISS rack. This paper gives a summary of the project BECCAL and its environment. Furthermore, the mechanical design of the system is presented. A preliminary approach for the Thermal Control System (TCS) of BECCAL is pointed out afterwards. The paper closes with a conclusion and an outlook on the future work for BECCAL.
This presentation introduces the projects BECCAL and CARIOQA-PMP. BECCAL (Bose-Einstein-Condensate and Cold Atom Laboratory) is a NASA-DLR project for operating a payload for experiments on cold atoms, atom optics and atom interferometry on board of the International Space Station. CARIOQA-PMP (Cold Atom Rubidium Interferometry for Quantum Accelerometry - Pathfinder Mission Preparation) aims for the development of hardware and a mission concept for demonstrating atom-interferometric accelerometry onboard of dedicated satellite. The background is to use such sensors e.g. in future missions for earth observation.
Cold Atom Laboratory (CAL) is a multi-user facility that will provide the ability to study ultra-cold quantum gases in a microgravity environment. The laboratory is an internal payload that will operate on the International Space Station (ISS) in 2016. Principal Investigators from various universities will trade off in designing experiment sequences that vary different parameters, such as magnetic field strength or timing. The primary science data consists of two images of the cold atoms captured successively at the end of each experiment.