| Literature DB >> 30333576 |
Dennis Becker1, Maike D Lachmann1, Stephan T Seidel1,2, Holger Ahlers1, Aline N Dinkelaker3, Jens Grosse4,5, Ortwin Hellmig6, Hauke Müntinga4, Vladimir Schkolnik3, Thijs Wendrich1, André Wenzlawski7, Benjamin Weps8, Robin Corgier1,9, Tobias Franz8, Naceur Gaaloul1, Waldemar Herr1, Daniel Lüdtke8, Manuel Popp1, Sirine Amri9, Hannes Duncker6, Maik Erbe10, Anja Kohfeldt10, André Kubelka-Lange4, Claus Braxmaier4,5, Eric Charron9, Wolfgang Ertmer1, Markus Krutzik3, Claus Lämmerzahl4, Achim Peters3, Wolfgang P Schleich11,12,13,14, Klaus Sengstock6, Reinhold Walser15, Andreas Wicht10, Patrick Windpassinger7, Ernst M Rasel16.
Abstract
Owing to the low-gravity conditions in space, space-borne laboratories enable experiments with extended free-fall times. Because Bose-Einstein condensates have an extremely low expansion energy, space-borne atom interferometers based on Bose-Einstein condensation have the potential to have much greater sensitivity to inertial forces than do similar ground-based interferometers. On 23 January 2017, as part of the sounding-rocket mission MAIUS-1, we created Bose-Einstein condensates in space and conducted 110 experiments central to matter-wave interferometry, including laser cooling and trapping of atoms in the presence of the large accelerations experienced during launch. Here we report on experiments conducted during the six minutes of in-space flight in which we studied the phase transition from a thermal ensemble to a Bose-Einstein condensate and the collective dynamics of the resulting condensate. Our results provide insights into conducting cold-atom experiments in space, such as precision interferometry, and pave the way to miniaturizing cold-atom and photon-based quantum information concepts for satellite-based implementation. In addition, space-borne Bose-Einstein condensation opens up the possibility of quantum gas experiments in low-gravity conditions1,2.Year: 2018 PMID: 30333576 DOI: 10.1038/s41586-018-0605-1
Source DB: PubMed Journal: Nature ISSN: 0028-0836 Impact factor: 49.962