Wigner Function Non-Classicality Induced in a Charge Qubit Interacting with a Dissipative Field Cavity
We explore a superconducting charge qubit interacting with a dissipative microwave cavity field. Wigner distribution and its non-classicality are investigated analytically under the effects of the qubit–cavity interaction, the qubit–cavity detuning, and the dissipation. As the microwave cavity field...
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2021-05-01
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doaj-e684390366a649638552c1a17b95d1a62021-05-31T23:12:06ZengMDPI AGSymmetry2073-89942021-05-011380280210.3390/sym13050802Wigner Function Non-Classicality Induced in a Charge Qubit Interacting with a Dissipative Field CavityAbdel-Baset A. Mohamed0Eied M. Khalil1Afrah Y. AL-Rezami2Hichem Eleuch3Department of Mathematics, College of Science and Humanities in Al-Aflaj, Prince Sattam bin Abdulaziz University, Al-Aflaj 11942, Saudi ArabiaDepartment of Mathematics, College of Science, Taif University, P.O. Box 11099, Taif 21944, Saudi ArabiaDepartment of Mathematics, College of Science and Humanities in Al-Aflaj, Prince Sattam bin Abdulaziz University, Al-Aflaj 11942, Saudi ArabiaDepartment of Applied Physics and Astronomy, University of Sharjah, Sharjah 27272, United Arab EmiratesWe explore a superconducting charge qubit interacting with a dissipative microwave cavity field. Wigner distribution and its non-classicality are investigated analytically under the effects of the qubit–cavity interaction, the qubit–cavity detuning, and the dissipation. As the microwave cavity field is initially in an even coherent state, we investigate the non-classicality of the Wigner distributions. Partially and maximally frozen entanglement are produced by the qubit–cavity interaction, depending on detuning and cavity dissipation. It is found that the amplitudes and frequency of the Wigner distribution can be controlled by the phase space parameters, the qubit–cavity interaction and the detuning, as well as by the dissipation. The cavity dissipation reduces the non-classicality; this process can be accelerated by the detuning.https://www.mdpi.com/2073-8994/13/5/802charge–qubit systemquasi-probability wigner functionentanglement |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Abdel-Baset A. Mohamed Eied M. Khalil Afrah Y. AL-Rezami Hichem Eleuch |
spellingShingle |
Abdel-Baset A. Mohamed Eied M. Khalil Afrah Y. AL-Rezami Hichem Eleuch Wigner Function Non-Classicality Induced in a Charge Qubit Interacting with a Dissipative Field Cavity Symmetry charge–qubit system quasi-probability wigner function entanglement |
author_facet |
Abdel-Baset A. Mohamed Eied M. Khalil Afrah Y. AL-Rezami Hichem Eleuch |
author_sort |
Abdel-Baset A. Mohamed |
title |
Wigner Function Non-Classicality Induced in a Charge Qubit Interacting with a Dissipative Field Cavity |
title_short |
Wigner Function Non-Classicality Induced in a Charge Qubit Interacting with a Dissipative Field Cavity |
title_full |
Wigner Function Non-Classicality Induced in a Charge Qubit Interacting with a Dissipative Field Cavity |
title_fullStr |
Wigner Function Non-Classicality Induced in a Charge Qubit Interacting with a Dissipative Field Cavity |
title_full_unstemmed |
Wigner Function Non-Classicality Induced in a Charge Qubit Interacting with a Dissipative Field Cavity |
title_sort |
wigner function non-classicality induced in a charge qubit interacting with a dissipative field cavity |
publisher |
MDPI AG |
series |
Symmetry |
issn |
2073-8994 |
publishDate |
2021-05-01 |
description |
We explore a superconducting charge qubit interacting with a dissipative microwave cavity field. Wigner distribution and its non-classicality are investigated analytically under the effects of the qubit–cavity interaction, the qubit–cavity detuning, and the dissipation. As the microwave cavity field is initially in an even coherent state, we investigate the non-classicality of the Wigner distributions. Partially and maximally frozen entanglement are produced by the qubit–cavity interaction, depending on detuning and cavity dissipation. It is found that the amplitudes and frequency of the Wigner distribution can be controlled by the phase space parameters, the qubit–cavity interaction and the detuning, as well as by the dissipation. The cavity dissipation reduces the non-classicality; this process can be accelerated by the detuning. |
topic |
charge–qubit system quasi-probability wigner function entanglement |
url |
https://www.mdpi.com/2073-8994/13/5/802 |
work_keys_str_mv |
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