Dispersion laws of some two-dimensional cavity magnetoexciton-polariton branches
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PODLESNY, Igor, MOSKALENKO, Sveatoslav, DUMANOV, Evgheni, RUSU, Spiridon. Dispersion laws of some two-dimensional cavity magnetoexciton-polariton branches. In: Materials Science and Condensed Matter Physics, Ed. 8-th Edition, 12-16 septembrie 2016, Chişinău. Chişinău: Institutul de Fizică Aplicată, 2016, Editia 8, p. 72. ISBN 978-9975-9787-1-2.
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Materials Science and Condensed Matter Physics
Editia 8, 2016
Conferința "International Conference on Materials Science and Condensed Matter Physics"
8-th Edition, Chişinău, Moldova, 12-16 septembrie 2016

Dispersion laws of some two-dimensional cavity magnetoexciton-polariton branches


Pag. 72-72

Podlesny Igor, Moskalenko Sveatoslav, Dumanov Evgheni, Rusu Spiridon
 
Institute of Applied Physics, Academy of Sciences of Moldova
 
 
Disponibil în IBN: 19 iulie 2019


Rezumat

The energy spectrum of the 2D cavity magnetoexciton-polaritons has been investigated previously, using exact solutions for the Landau quantization of conduction electrons and heavy holes provided by the Rashba method [1]. Two lowest Landau quantization levels for electrons and three lowest Landau levels for heavy-holes, lead to the construction of the six lowest magnetoexciton states. They consist of two dipole-active, two quadrupole-active, and two forbidden quantum transitions from the ground state of the crystal to the magnetoexciton states. The interaction of the four opticalactive magnetoexciton states with the cavity mode photons with a given circular polarization and with well-defined incidence direction leads to the creation of five magnetoexciton-polariton branches. The fifth order dispersion equation is examined by using numerical calculations and the second order dispersion equation in the point k=0 is solved analytically, taking into account only one dipole-active magnetoexciton state. The effective polariton mass (Fig. 1) on the lower polariton branch, the Rabi frequency and the corresponding Hopfield coefficients (Fig. 2) are determined in dependence on the magnetic field strength, the Rashba spin-orbit coupling parameters and the electron and hole g-factors [2].