Clarendon Laboratory, Department of Physics, University of Oxford, Parks Road, Oxford, OX1 3PU, United Kingdom.
Department of Mathematics, National University of Singapore, Singapore, Singapore.
Sci Rep. 2017 May 15;7(1):1891. doi: 10.1038/s41598-017-01113-8.
In the study of non-equilibrium polariton condensates it is usually assumed that the dispersion relation of polaritons is parabolic in nature. We show that considering the true non-parabolic kinetic energy of polaritons leads to significant changes in the behaviour of the condensate due to the curvature of the dispersion relation and the possibility of transfer of energy to high wavenumber components in the condensate spatial profile. We present explicit solutions for plane waves and linear excitations, and identify the differences in the theoretical predictions between the parabolic and non-parabolic mean-field models, showing the possibility of symmetry breaking in the latter. We then consider the evolution of wavepackets and show that self-localisation effects may be observed due to the curvature of the dispersion relation. Finally, we revisit the dynamics of dark soliton trains and show that additional localized density excitations may emerge in the dynamics due to the excitation of high frequency components, mimicking the appearance of near-bright solitary waves over short timescales.
在非平衡极化激元凝聚体的研究中,通常假设极化激元的色散关系在本质上是抛物线型的。我们表明,考虑到极化激元的真实非抛物线型动能会导致凝聚体的行为发生显著变化,这是由于色散关系的曲率以及在凝聚体空间分布中能量向高波数分量转移的可能性。我们给出了平面波和线性激发的显式解,并确定了抛物线和非抛物线平均场模型之间的理论预测的差异,表明后者存在对称破缺的可能性。然后,我们考虑了波包的演化,并表明由于色散关系的曲率,可能会观察到自局域化效应。最后,我们重新研究了暗孤子列的动力学,并表明由于高频分量的激发,动力学中可能会出现额外的局域密度激发,在短时间尺度上模拟近亮孤子波的出现。