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http://hdl.handle.net/2289/7272
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DC Field | Value | Language |
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dc.contributor.author | Sadana, Simanraj | - |
dc.contributor.author | Ghosh, Debadrita | - |
dc.contributor.author | Joarder, Kaushik | - |
dc.contributor.author | Lakshmi, A. Naga | - |
dc.contributor.author | Sanders, Barry C | - |
dc.contributor.author | Sinha, Urbasi | - |
dc.date.accessioned | 2019-08-13T17:50:19Z | - |
dc.date.available | 2019-08-13T17:50:19Z | - |
dc.date.issued | 2019-07 | - |
dc.identifier.citation | Physical Review A, 2019, Vol.100, p013839 | en_US |
dc.identifier.issn | 2469-9926 | - |
dc.identifier.issn | 2469-9934 (online) | - |
dc.identifier.uri | http://hdl.handle.net/2289/7272 | - |
dc.description | Open Access | en_US |
dc.description.abstract | The Hong-Ou-Mandel effect is considered a signature of the quantumness of light, as the dip in coincidence probability using semi-classical theories has an upper bound of 50%. Here we show, theoretically and experimentally, that, with proper phase control of the signals, classical pulses can mimic a Hong-Ou Mandel-like dip. We demonstrate a dip of 99.635 +/- 0.002% with classical microwave fields. Quantumness manifests in wave-particle complementarity of the two-photon state. We construct quantum and classical interferometers for the complementarity test and show that while the two-photon state shows wave particle complementarity, the classical pulses do not. | en_US |
dc.language.iso | en | en_US |
dc.publisher | American Physical Society | en_US |
dc.relation.uri | https://arxiv.org/abs/1810.01297 | en_US |
dc.relation.uri | https://doi.org/10.1103/PhysRevA.100.013839 | en_US |
dc.relation.uri | https://ui.adsabs.harvard.edu/abs/2018arXiv181001297S/abstract | en_US |
dc.rights | 2019 American Physical Society | en_US |
dc.title | Near-100% two-photon-like coincidence-visibility dip with classical light and the role of complementarity | en_US |
dc.type | Article | en_US |
Appears in Collections: | Research Papers (LAMP) |
Files in This Item:
File | Description | Size | Format | |
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2019_PhysRevA_Vol.100_p013839.pdf | Open Access | 1.18 MB | Adobe PDF | View/Open |
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