Supplemental Material Cosmic Bell Test: Measurement Settings from Milky Way Stars
نویسندگان
چکیده
Johannes Handsteiner1,∗ Andrew S. Friedman2,† Dominik Rauch1, Jason Gallicchio3, Bo Liu1,4, Hannes Hosp1, Johannes Kofler5, David Bricher1, Matthias Fink1, Calvin Leung3, Anthony Mark2, Hien T. Nguyen6, Isabella Sanders2, Fabian Steinlechner1, Rupert Ursin1,7, Sören Wengerowsky1, Alan H. Guth2, David I. Kaiser2, Thomas Scheidl1, and Anton Zeilinger1,7‡ 1Institute for Quantum Optics and Quantum Information (IQOQI), Austrian Academy of Sciences, Boltzmanngasse 3, 1090 Vienna, Austria 2Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139 USA 3Department of Physics, Harvey Mudd College, Claremont, CA 91711 USA 4School of Computer, NUDT, 410073 Changsha, China 5Max Planck Institute of Quantum Optics, Hans-Kopfermann-Straße 1, 85748 Garching, Germany 6NASA Jet Propulsion Laboratory, Pasadena, CA 91109 USA 7Vienna Center for Quantum Science & Technology (VCQ), Faculty of Physics, University of Vienna, Boltzmanngasse 5, 1090 Vienna, Austria
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Cosmic Bell Test: Measurement Settings from Milky Way Stars.
Bell's theorem states that some predictions of quantum mechanics cannot be reproduced by a local-realist theory. That conflict is expressed by Bell's inequality, which is usually derived under the assumption that there are no statistical correlations between the choices of measurement settings and anything else that can causally affect the measurement outcomes. In previous experiments, this "fr...
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