Classical-quantum Interface of a Particle in a Time-dependent Linear Potential

2010 ◽  
Vol 49 (4) ◽  
pp. 936-942 ◽  
Author(s):  
L. Krache ◽  
M. Maamache ◽  
Y. Saadi
2004 ◽  
Vol 70 (2-3) ◽  
pp. 98-100 ◽  
Author(s):  
Mai-Lin Liang ◽  
Zhi-Guo Zhang ◽  
Kai-Sheng Zhong

2018 ◽  
Vol 32 (15) ◽  
pp. 1850184 ◽  
Author(s):  
Emmanuel Kengne ◽  
Ahmed Lakhssassi

To analytically investigate the matter-wave solitons of Bose–Einstein condensates (BECs) in time-dependent complex potential, we consider a cubic-quintic Gross–Pitaevskii (GP) equation with distributed coefficients and a dissipative term. By introducing a suitable ansatz, we establish the criterion of the modulational instability (MI) of the system and present an explicit expression for the growth rate of a purely growing MI. Effects of the parabolic background potential, as well as of the linear potential, the gain/loss parameter, and the two- and three-body interatomic interactions on the MI are investigated. We show how the feeding/loss parameter can be well used to control the instability of the system. The analytical resolution of the considered GP equation leads to exact bright, dark and kink solitary wave solutions which are used to investigate analytically the dynamics of matter-wave solitons in BECs under consideration. These analytical investigations show that the amplitude and the motion of bright, dark and kink solitary waves depend on the strengths of the two- and three-body interatomic interactions, as well as on the strengths of the external trapping potential and the parameter of the gain/loss of atoms in the condensate.


2018 ◽  
Vol 39 (2) ◽  
pp. 025710
Author(s):  
Mahima Chhabra ◽  
Ritwick Das

1971 ◽  
Vol 69 (2) ◽  
pp. 315-318
Author(s):  
H. F. Stoeckli

AbstractIt is shown that the formula for the gravitational red shift predicted by the theory of general relativity can also be derived by classical quantum mechanics combined with relativistic arguments. The agreement between the two derivations is a consequence of the separability of the time-dependent wave function, and of the first-order time differential in the wave equation.


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