2016
DOI: 10.1088/1367-2630/18/11/113017
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On the observation of nonclassical excitations in Bose–Einstein condensates

Abstract: In the recent experimental and theoretical literature well-established nonclassicality criteria from the field of quantum optics have been directly applied to the case of excitations in matter-waves. Among these are violations of Cauchy-Schwarz inequalities, Glauber-Sudarshan P-nonclassicality, sub-Poissonian number-difference squeezing (also known as the two-mode variance) and the criterion of nonseparability. We review the strong connection of these criteria and their meaning in quantum optics, and point out… Show more

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Cited by 30 publications
(36 citation statements)
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“…vac (k), giving rise to inequality (17). This condition is represented by the dashed vertical line in Fig.…”
Section: Steerabilitymentioning
confidence: 94%
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“…vac (k), giving rise to inequality (17). This condition is represented by the dashed vertical line in Fig.…”
Section: Steerabilitymentioning
confidence: 94%
“…It should be noticed that it crosses the outermost limit of physical states with n 1 = n 2 ≡ n for a finite value of the mean occupation number n. This can be understood from the fact that the realisation of inequality (17) requires sufficiently large oscillations of the G (2) (k, t) with respect to G (2) vac (k). It is interesting to notice that it is the symmetric condition (A.12) that is used in the recent work [46], where the threshold is correctly pointed out.…”
Section: Steerabilitymentioning
confidence: 98%
“…The study of g 2 is of interest because the occurrence of entanglement and the quantum nature of the Hawking process can be tested through the violation of the Cauchy-Schwarz inequality, as recently studied in a similar context in Refs. [32,33,[40][41][42][43][44][45][46]. For instance, the Cauchy-Schwarz inequality is violated along the characteristic Hawking quanta-partner correlation lines u|out-d2|out of Figs.…”
Section: Zero Temperaturementioning
confidence: 99%
“…Note that not transforming the coordinate φ as done in equation (35) would have resulted in obtaining the somewhat more usual diagonal form of oblate spheroidal coordinates (without the dr dφ cross term).…”
Section: The Kerr Spacetimementioning
confidence: 99%