Spin-orbit splitting in semiconductor quantum dots with a parabolic confinement potential

2001 ◽  
Vol 63 (16) ◽  
Author(s):  
O. Voskoboynikov ◽  
C. P. Lee ◽  
O. Tretyak
1996 ◽  
Vol 53 (11) ◽  
pp. 7287-7298 ◽  
Author(s):  
Tristan Richard ◽  
Pierre Lefebvre ◽  
Henry Mathieu ◽  
Jacques Allègre

Author(s):  
Oscar A. Negrete ◽  
Francisco J. Peña ◽  
Patricio Vargas

In this work, we report the magnetocaloric effect (MCE) in a quantum dot corresponding to an electron interacting with an antidot, under the effect of an Aharonov-Bohm flux subjected to a parabolic confinement potential. We use the Bogachek and Landman model, which additionally allows the study of quantum dots with Fock-Darwin energy levels for vanishing antidot radius and flux. We find that the Aharonov-Bohm flux (AB-flux) strongly controls the oscillatory behaviour of the MCE, thus acting as a control parameter for the cooling or heating of the magnetocaloric effect. We propose a way to detect AB-flux by measuring temperature differences.


Entropy ◽  
2018 ◽  
Vol 20 (11) ◽  
pp. 888 ◽  
Author(s):  
Oscar Negrete ◽  
Francisco Peña ◽  
Patricio Vargas

In this work, we report the magnetocaloric effect (MCE) for an electron interacting with an antidot, under the effect of an Aharonov-Bohm flux (AB-flux) subjected to a parabolic confinement potential. We use the Bogachek and Landman model, which additionally allows the study of quantum dots with Fock-Darwin energy levels for vanishing antidot radius and AB-flux. We find that AB-flux strongly controls the oscillatory behaviour of the MCE, thus acting as a control parameter for the cooling or heating of the magnetocaloric effect. We propose a way to detect AB-flux by measuring temperature differences.


1999 ◽  
Vol 571 ◽  
Author(s):  
H. W. H. Lee ◽  
C. A. Smith ◽  
V. J. Leppert ◽  
S. H. Risbud

ABSTRACTWe observed the quantum confined bandedge emission from ZnSe quantum dots and the size dependence of the energy states, spin-orbit interaction, and Stokes shift. The bandedge emission occurs in the UV-blue. The energy gap = Eg + C/dn where d is the diameter and n is 1. 19 ± 0.13 and 1.21 ± 0.13 for the first and second electron-hole transitions, respectively. The separation between these transitions approaches the bulk spin-orbit splitting, while the Stokes shift decreases with particle size. Effective mass theories can not explain these results. Trap emission is observed in some samples in the green and red, resulting from Se-related traps.


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