Cited by 99Quantum Mechanics and ApplicationsQuantum Information and CryptographyNoncommutative and Quantum Gravity Theories

Testing Bell’s Inequality with Cosmic Photons: Closing the Setting-Independence Loophole

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Gallicchio, Jason, Friedman, Andrew S., Kaiser, David I.·2014·Physical Review Letters

Abstract

We propose a practical scheme to use photons from causally disconnected cosmic sources to set the detectors in an experimental test of Bell's inequality. In current experiments, with settings determined by quantum random number generators, only a small amount of correlation between detector settings and local hidden variables, established less than a millisecond before each experiment, would suffice to mimic the predictions of quantum mechanics. By setting the detectors using pairs of quasars or patches of the cosmic microwave background, observed violations of Bell's inequality would require any such coordination to have existed for billions of years-an improvement of 20 orders of magnitude.

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Crossref · 10.1103/physrevlett.112.110405

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  • Other random resources, such as independent comic photons, have been proposed for loophole-free Bell's inequality tests.

    “Other random resources have also been proposed for loophole-free Bell ' s inequality tests, such as independent comic photons. 92”

    From Quantum random number generation (2016) · cites this paper as [92]

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Research works printed but not linked: 26

  1. [5]G. Weihs, T. Jennewein, C. Simon, et al., Phys. Rev. Lett. 81 , 5039 (1998), arXiv:quant-ph/9810080. · arXiv
  2. [6]B. F. Toner and D. Bacon, Phys. Rev. Lett. 91 , 187904 (2003), arXiv:quant-ph/0304076. · arXiv
  3. [10]M. Giustina, A. Mech, S. Ramelow, et al., Nature 497 , 227 (2013), arXiv:1212.0533 [quant-ph]. · arXiv
  4. [11]B. G. Christensen, K. T. McCusker, J. Altepeter, et al., Phys. Rev. Lett. 111 , 130406 (2013), arXiv:1306.5772 [quant-ph]. · arXiv
  5. [13]J. Conway and S. Kochen, Found. Phys. 36 , 1441 (2006), arXiv:quant-ph/0604079. · arXiv
  6. [14]G. 't Hooft, ArXiv e-prints (2007), arXiv:quantph/0701097.
  7. [16]M. J. W. Hall, Phys. Rev. Lett. 105 , 250404 (2010), arXiv:1007.5518 [quant-ph]. · arXiv
  8. [17]J. Barrett and N. Gisin, Phys. Rev. Lett. 106 , 100406 (2011), arXiv:1008.3612 [quant-ph]. · arXiv
  9. [19]T. Fritz, New J. Phys. 14 , 103001 (2012), arXiv:1206.5115 [quant-ph]. · arXiv
  10. [20]J.-W. Pan, Z.-B. Chen, C.-Y. Lu, et al., Rev. Mod. Phys. 84 , 777 (2012), arXiv:0805.2853 [quant-ph]. · arXiv
  11. [21]A. S. Friedman, D. I. Kaiser, and J. Gallicchio, Phys. Rev. D 88 , 044038 (2013), arXiv:1305.3943 [astroph.CO]. · arXiv
  12. [23]A. H. Guth and D. I. Kaiser, Science 307 , 884 (2005), arXiv:astro-ph/0502328. · arXiv
  13. [26]D. J. Mortlock, S. J. Warren, B. P. Venemans, et al., Nature 474 , 616 (2011), arXiv:1106.6088 [astro-ph.CO]. · arXiv
  14. [27]J. Cooke, M. Sullivan, E. J. Barton, et al., Nature 460 , 237 (2009), arXiv:0907.1928 [astro-ph.CO]. · arXiv
  15. [28]A. Cucchiara, A. J. Levan, D. B. Fox, et al., Astrophys. J. 736 , 7 (2011), arXiv:1105.4915 [astro-ph.CO]. · arXiv
  16. [29]D. A. Kann, S. Klose, B. Zhang, et al., Astrophys. J. 720 , 1513 (2010), arXiv:0712.2186. · arXiv
  17. [31]I. Pˆ aris, P. Petitjean, ´ E. Aubourg, et al., Astron. & Astro. 548 , A66 (2012), arXiv:1210.5166 [astro-ph.CO]. · arXiv
  18. [32]P. A. R. Ade et al. and (Planck collaboration), ArXiv e-prints (2013), arXiv:1303.5076 [astro-ph.CO]. · arXiv
  19. [35]D. H. Smith, G. Gillett, M. P. de Almeida, et al., Nature Comm. 3 , 625 (2012), arXiv:1111.0829 [quant-ph]. · arXiv
  20. [39]A. de Oliveira-Costa, M. Tegmark, B. M. Gaensler, et al., Mon. Not. R. Astron. Soc. 388 , 247 (2008), arXiv:0802.1525 [astro-ph]. · arXiv
  21. [40]R. Leonardi, B. Williams, M. Bersanelli, et al., New Astron. Rev. 50 , 977 (2006), arXiv:0704.0810. · arXiv
  22. [42]T. Scheidl, E. Wille, and R. Ursin, New J. Phys. 15 , 043008 (2013), arXiv:1211.2111 [quant-ph]. · arXiv
  23. [43]J. Hubmayr, F. Aubin, E. Bissonnette, et al., ArXiv eprints (2009), arXiv:0908.1997 [astro-ph.IM]. · arXiv
  24. [44]P. A. R. Ade et al. and (Planck HFI Core Team), Astron. & Astro. 536 , A4 (2011), arXiv:1101.2039 [astro-ph.IM]. · arXiv
  25. [45]J. F. Mac´ ıas-P´ erez, G. Lagache, B. Maffei, et al., Astron. & Astro. 467 , 1313 (2007), arXiv:astro-ph/0603665. · arXiv
  26. [46]G. 't Hooft, ArXiv e-prints (2009), arXiv:0908.3408 [quant-ph]. · arXiv

Cited by

Sorted by citations

Authors
Gallicchio, J., Friedman, A. S., & Kaiser, D. I.
Affiliations
  • University of Chicago (US)
  • Massachusetts Institute of Technology (US)
Venue
Physical Review Letters
Published
2014-03-18
Volume
112
Issue
11
Pages
110405-110405
ISSN
  • 0031-9007 (ISSN-L)
  • 1079-7114
OpenAlex
W2056597044
Cited by
99
References
48
Citations by year
2026: 2 · 2025: 6 · 2024: 4 · 2023: 3 · 2022: 9 · 2021: 6 · 2020: 6 · 2019: 8 · 2018: 10 · 2017: 11 · 2016: 12 · 2015: 12 · 2014: 8
FWCI
7.13
Type
journal article
Language
en
Open access
Locations
  • Physical Review Letters (publishedVersion)
  • arXiv (Cornell University) (publishedVersion)
  • PubMed (publishedVersion)
  • DSpace@MIT (Massachusetts Institute of Technology) (submittedVersion)
  • arXiv (Cornell University)
Funders
  • U.S. Department of Energy (DE-FG02-05ER41360)
  • National Science Foundation (SES-1056580, ANT-0638937)
Topics
  • Physical Sciences › Physics and Astronomy › Atomic and Molecular Physics, and Optics › Quantum Mechanics and Applications
  • Physical Sciences › Computer Science › Artificial Intelligence › Quantum Information and Cryptography
  • Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
Keywords
Bell inequalities, quasar pairs, cosmic microwave background, quantum randomness, local hidden variable theories, quantum nonlocality

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