Tunable Magneto-optical Faraday rotation with a five-level atomic system near the plasmonic nanostructure

2021 ◽  
Author(s):  
Azar Vafafard ◽  
Mostafa Sahrai ◽  
seyyed Hossein Asadpour ◽  
Edris Faizabadi
Keyword(s):  
Faraday Rotation ◽  
Atomic System ◽  
Plasmonic Nanostructure

Phase-controlled optical Faraday rotation in a closed-loop atomic system

2014 ◽  
Vol 32 (1) ◽  
pp. 167 ◽  
Author(s):  
Mariye Veisi ◽  
Azar Vafafard ◽  
Mohammad Mahmoudi
Keyword(s):  
Faraday Rotation ◽  
Closed Loop ◽  
Atomic System

scholarly journals Controllable atom-photon entanglement via quantum interference near plasmonic nanostructure

2022 ◽  
Vol 12 (1) ◽  
Author(s):  
Behzad Sangshekan ◽  
Mostafa Sahrai ◽  
Seyyed Hossein Asadpour ◽  
Jafar Poursamad Bonab
Keyword(s):  
Spontaneous Emission ◽  
Laser Field ◽  
Quantum Interference ◽  
Atomic System ◽  
Two Dimensional ◽  
Control Field ◽  
Plasmonic Nanostructure ◽  
Atomic Distance ◽  
Control Laser

AbstractA five-level atomic system is proposed in vicinity of a two-dimensional (2D) plasmonic nanostructure with application in atom-photon entanglement. The behavior of the atom-photon entanglement is discussed with and without a control laser field. The amount of atom-photon entanglement is controlled by the quantum interference created by the plasmonic nanostructure. Thus, the degree of atom-photon entanglement is affected by the atomic distance from the plasmonic nanostructure. In the presence of a control field, maximum entanglement between the atom and its spontaneous emission field is observed.

scholarly journals Controllable Atom-Photon Entanglement Via Quantum Interference Near Plasmonic Nanostructure

2021 ◽  
Author(s):  
Behzad Sangshekan ◽  
Mostafa Sahrai ◽  
Seyyed Hossein Asadpour ◽  
Jafar Poursamad Bonab
Keyword(s):  
Spontaneous Emission ◽  
Laser Field ◽  
Quantum Interference ◽  
Atomic System ◽  
Two Dimensional ◽  
Control Field ◽  
Plasmonic Nanostructure ◽  
Atomic Distance ◽  
Control Laser

Abstract A five-level atomic system is proposed in vicinity of a two-dimensional (2D) plasmonic nanostructure with application in atom-photon entanglement. The behavior of the atom-photon entanglement is discussed with and without a control laser field. The amount of atom-photon entanglement is controlled by the quantum interference created by the plasmonic nanostructure. Thus, the degree of atom-photon entanglement is affected by the atomic distance from the plasmonic nanostructure. In the presence of a control field, maximum entanglement between the atom and its spontaneous emission field is observed.

NEAR IR FARADAY ROTATION ON YIG DOPED WITH TETRAVALENT AND PENTAVALENT ELEMENTS

1988 ◽  
Vol 49 (C8) ◽  
pp. C8-969-C8-970 ◽  
Author(s):  
F. D'Orazio ◽  
F. Giammaria ◽  
F. Lucari ◽  
G. Parone
Keyword(s):  
Faraday Rotation ◽  
Near Ir

YTTERBIUM SUBLATTICE CONTRIBUTION TO THE FARADAY ROTATION OF YTTERBIUM IRON GARNET

1988 ◽  
Vol 49 (C8) ◽  
pp. C8-961-C8-962
Author(s):  
M. Guillot ◽  
H. Le Gall ◽  
A. Marchand ◽  
A. Barlet ◽  
M. Artinian ◽  
...  
Keyword(s):  
Faraday Rotation ◽  
Iron Garnet

scholarly journals An 84-μG Magnetic Field in a Galaxy at Z=0.692?

2008 ◽  
Vol 4 (S254) ◽  
pp. 95-96
Author(s):  
Arthur M. Wolfe ◽  
Regina A. Jorgenson ◽  
Timothy Robishaw ◽  
Carl Heiles ◽  
Jason X. Prochaska
Keyword(s):  
Magnetic Field ◽  
Magnetic Fields ◽  
Faraday Rotation ◽  
Large Scale ◽  
Dynamo Model ◽  
Magnetic Field Generation ◽  
Interstellar Gas ◽  
Splitting Technique ◽  
Average Value ◽  
The Magnetic Field

AbstractThe magnetic field pervading our Galaxy is a crucial constituent of the interstellar medium: it mediates the dynamics of interstellar clouds, the energy density of cosmic rays, and the formation of stars (Beck 2005). The field associated with ionized interstellar gas has been determined through observations of pulsars in our Galaxy. Radio-frequency measurements of pulse dispersion and the rotation of the plane of linear polarization, i.e., Faraday rotation, yield an average value B ≈ 3 μG (Han et al. 2006). The possible detection of Faraday rotation of linearly polarized photons emitted by high-redshift quasars (Kronberg et al. 2008) suggests similar magnetic fields are present in foreground galaxies with redshifts z > 1. As Faraday rotation alone, however, determines neither the magnitude nor the redshift of the magnetic field, the strength of galactic magnetic fields at redshifts z > 0 remains uncertain.Here we report a measurement of a magnetic field of B ≈ 84 μG in a galaxy at z =0.692, using the same Zeeman-splitting technique that revealed an average value of B = 6 μG in the neutral interstellar gas of our Galaxy (Heiles et al. 2004). This is unexpected, as the leading theory of magnetic field generation, the mean-field dynamo model, predicts large-scale magnetic fields to be weaker in the past, rather than stronger (Parker 1970).The full text of this paper was published in Nature (Wolfe et al. 2008).

Giant THz Faraday rotation with stacked magnetized graphene

2021 ◽  
Vol 129 (18) ◽  
pp. 183103
Author(s):  
Minyu Gu ◽  
Krzysztof A. Michalski
Keyword(s):  
Faraday Rotation
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