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Thermal and squeezed vacuum Jaynes-Cummings models with a Kerr medium

机译:带有Kerr介质的热真空和压缩真空Jaynes-Cummings模型

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The dynamics of the Jaynes-Cummings (JCM) model with a nonlinear Kerr medium at initially thermal and squeezed vacuum fields is discussed. At a special choice of the detuning the Rabi frequency can have a minimum at the initial mean photon number n-bar. Then the situation becomes especially interesting and instead of the first-order 'usual' revivals resembling those manifested by the standard coherent JCM, the nonlinear JCM exhibits second-order revivals, also for initially thermal and squeezed vacuum fields, at least for not too large n-bar. The revival times are highly sensitive to the nature of n-bar. In the first case the revival period of the oscillations is dependent on whether n-bar is integer or non-integer (situation similar to an initially coherent field) while in the latter case it depends additionally on the parity of the integer n-bar. Moreover, for the squeezed vacuum model appearance of the revivals at an integer n-bar is accelerated when compared to coherent and thermal models.
机译:讨论了带有非线性Kerr介质的Jaynes-Cummings(JCM)模型在初始热场和压缩真空场下的动力学。通过特殊的失谐选择,拉比频率可以在初始平均光子数n-bar处达到最小值。然后,情况变得特别有趣,非线性JCM代替了由标准相干JCM表现出的一阶“正常”恢复,而对最初的热场和压缩真空场也表现出了二阶恢复,至少在没有太大影响的情况下如此n条。复兴时期对n-bar的性质高度敏感。在第一种情况下,振荡的恢复周期取决于n-bar是整数还是非整数(类似于初始相干场的情况),而在后一种情况下,它还取决于整数n-bar的奇偶性。此外,与相干模型和热模型相比,对于压缩的真空模型,在整数n条下的恢复速度加快。

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