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dc.contributor.authorRauch, Dominik
dc.contributor.authorHandsteiner, Johannes
dc.contributor.authorHochrainer, Armin
dc.contributor.authorGallicchio, Jason
dc.contributor.authorFriedman, Andrew S.
dc.contributor.authorLiu, Bo
dc.contributor.authorBulla, Lukas
dc.contributor.authorEcker, Sebastian
dc.contributor.authorSteinlechner, Fabian
dc.contributor.authorUrsin, Rupert
dc.contributor.authorHu, Beili
dc.contributor.authorLeon, David
dc.contributor.authorBenn, Chris
dc.contributor.authorGhedina, Adriano
dc.contributor.authorCecconi, Massimo
dc.contributor.authorScheidl, Thomas
dc.contributor.authorZeilinger, Anton
dc.contributor.authorLeung, Calvin
dc.contributor.authorGuth, Alan
dc.contributor.authorKaiser, David I
dc.date.accessioned2018-08-20T19:07:08Z
dc.date.available2018-08-20T19:07:08Z
dc.date.issued2018-08
dc.date.submitted2018-06
dc.identifier.issn0031-9007
dc.identifier.issn1079-7114
dc.identifier.urihttp://hdl.handle.net/1721.1/117430
dc.description.abstractIn this Letter, we present a cosmic Bell experiment with polarization-entangled photons, in which measurement settings were determined based on real-time measurements of the wavelength of photons from high-redshift quasars, whose light was emitted billions of years ago; the experiment simultaneously ensures locality. Assuming fair sampling for all detected photons and that the wavelength of the quasar photons had not been selectively altered or previewed between emission and detection, we observe statistically significant violation of Bell’s inequality by 9.3 standard deviations, corresponding to an estimated p value of ≲7.4×10^{-21}. This experiment pushes back to at least ∼7.8  Gyr ago the most recent time by which any local-realist influences could have exploited the “freedom-of-choice” loophole to engineer the observed Bell violation, excluding any such mechanism from 96% of the space-time volume of the past light cone of our experiment, extending from the big bang to today.en_US
dc.publisherAmerican Physical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevLett.121.080403en_US
dc.rightsCreative Commons Attributionen_US
dc.rights.urihttp://creativecommons.org/licenses/by/3.0en_US
dc.sourceAmerican Physical Societyen_US
dc.titleCosmic Bell Test Using Random Measurement Settings from High-Redshift Quasarsen_US
dc.typeArticleen_US
dc.identifier.citationRauch, Dominik et al. "Cosmic Bell Test Using Random Measurement Settings from High-Redshift Quasars." Physical Review Letters 121, 8 (August 2018): 080403en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.mitauthorLeung, Calvin
dc.contributor.mitauthorGuth, Alan
dc.contributor.mitauthorKaiser, David I
dc.relation.journalPhysical Review Lettersen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2018-08-20T18:00:24Z
dc.language.rfc3066en
dspace.orderedauthorsRauch, Dominik; Handsteiner, Johannes; Hochrainer, Armin; Gallicchio, Jason; Friedman, Andrew S.; Leung, Calvin; Liu, Bo; Bulla, Lukas; Ecker, Sebastian; Steinlechner, Fabian; Ursin, Rupert; Hu, Beili; Leon, David; Benn, Chris; Ghedina, Adriano; Cecconi, Massimo; Guth, Alan H.; Kaiser, David I.; Scheidl, Thomas; Zeilinger, Antonen_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0003-3802-5206
dc.identifier.orcidhttps://orcid.org/0000-0002-5054-6744
mit.licensePUBLISHER_CCen_US


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