Strong resonant mode coupling of Fabry–Perot and grating resonances in stacked two-layer systems

Author(s):  
Thomas Weiss ◽  
Nikolay A. Gippius ◽  
Gérard Granet ◽  
Sergei G. Tikhodeev ◽  
Richard Taubert ◽  
...  
2021 ◽  
Vol 11 (1) ◽  
Author(s):  
Michał Dudek ◽  
Rafał Kowerdziej ◽  
Alessandro Pianelli ◽  
Janusz Parka

AbstractGraphene-based hyperbolic metamaterials provide a unique scaffold for designing nanophotonic devices with active functionalities. In this work, we have theoretically demonstrated that the characteristics of a polarization-dependent tunable hyperbolic microcavity in the mid-infrared frequencies could be realized by modulating the thickness of the dielectric layers, and thus breaking periodicity in a graphene-based hyperbolic metamaterial stack. Transmission of the tunable microcavity shows a Fabry–Perot resonant mode with a Q-factor > 20, and a sixfold local enhancement of electric field intensity. It was found that by varying the gating voltage of graphene from 2 to 8 V, the device could be self-regulated with respect to both the intensity (up to 30%) and spectrum (up to 2.1 µm). In addition, the switching of the device was considered over a wide range of incident angles for both the transverse electric and transverse magnetic modes. Finally, numerical analysis indicated that a topological transition between elliptic and type II hyperbolic dispersion could be actively switched. The proposed scheme represents a remarkably versatile platform for the mid-infrared wave manipulation and may find applications in many multi-functional architectures, including ultra-sensitive filters, low-threshold lasers, and photonic chips.


2010 ◽  
Author(s):  
Thomas Weiss ◽  
Nikolay A. Gippius ◽  
Richard Taubert ◽  
Gérard Granet ◽  
Sergei G. Tikhodeev ◽  
...  

1987 ◽  
Author(s):  
G. Francis ◽  
A. Bers ◽  
A. K. Ram

1995 ◽  
Vol 155 ◽  
pp. 331-332
Author(s):  
G. Handler ◽  
D. O’Donoghue ◽  
D. A. H. Buckley ◽  
O. Giovannini ◽  
S. O. Kepler ◽  
...  

The variability of CD-24 7599 (V=11.48 mag) was discovered by JCC during observing run XCOV7 of the Whole Earth Telescope (WET, Nather et al. 1990) network in February, 1992. The star was observed as an additional target and 117 hours of high-quality temporal spectroscopic observations were obtained.Our analysis of these data revealed the presence of 7 independent pulsation modes between 27.0 and 38.1 cycles per day (313 – 441 μHz) with semiamplitudes of 2.1 – 10.2 milli-modulation amplitudes (mma). We showed that peaks at linear combination frequencies detected in the power spectra were not due to eigenmodes excited to visible amplitude by resonant mode coupling.


2015 ◽  
Vol 579 ◽  
pp. A133 ◽  
Author(s):  
S. Barceló Forteza ◽  
E. Michel ◽  
T. Roca Cortés ◽  
R. A. García

ACS Photonics ◽  
2015 ◽  
Vol 2 (10) ◽  
pp. 1460-1467 ◽  
Author(s):  
B. S. Simpkins ◽  
Kenan P. Fears ◽  
Walter J. Dressick ◽  
Bryan T. Spann ◽  
Adam D. Dunkelberger ◽  
...  

1977 ◽  
Vol 19 (9) ◽  
pp. 811-816 ◽  
Author(s):  
M Gros ◽  
P Bertrand ◽  
G Baumann

1979 ◽  
Vol 53 ◽  
pp. 359-373 ◽  
Author(s):  
W. Dziembowski

AbstractAttention is focused on those aspects of the theory that may be relevant in understanding the nature of ZZ Ceti-type variable white dwarfs. Recent calculations show that the opacity mechanism can drive a large variety of oscillation modes, including the ones that fit observed periods. An estimate of nonlinear effects shows that resonant mode coupling plays a dominant role in determining the finite amplitude behaviour of oscillations and is also probably responsible for rapid amplitude changes observed in these variables.


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