An Explanation of the Physical Origin of the Extra-ordinary Angular
Tolerance of Cavity Resonator Integrated Grating Filters
Nadège Rassem, Anne-Laure Fehrembach and Evgeni Popov
Université d'Aix-Marseille, CNRS, Centrale Marseille, Institut Fresnel, Marseille, France
Keywords: Gratings, Subwavelength Structures, Bragg Reflectors, Eigenvalues, Resonance Domain.
Abstract: Cavity – resonator - integrated guided - mode resonance filters (CRIGFs) are promising structures that afford
a very fine spectral width less than 1 nm. We study another structure to compare compare it to CRIGF. The
angular acceptance of CRIGF is an order of magnitude greater than in classical gratings, even with complex
pattern. To identify the phenomenon responsible for the extraordinary large angular acceptance of CRIGF,
we study the dispersion curve of the mode excited in the CRIGF.
1 INTRODUCTION
With the increase of applications requiring spectral
filtering, free space optical filters are the focus of
several studies.
Fabry-Perot multilayer filters are the most widely
used free space filters but show limits for narrow band
filtering. To get a narrow spectral width with this type
of filters, one needs a large number of layers thus
increasing the size of the component which becomes
unstable over time and with temperature.
Resonant grating filters are a very promising
alternative relative to conventional multilayer filters.
The resonant grating filter is composed of a stack of
several dielectric layers on top of which a periodic
nanostructure is engraved. The multilayer stack plays
the role of a planar waveguide and the engraved
structure allows to couple and decouple one
eigenmode of the structure to the incident wave
through one diffraction order of the grating. When
the component is illuminated, a resonance peak
occurs in the reflectivity or transmittivity spectrum.
The characteristics of the peak, namely the centering
wavelength and width, are mainly governed by the
grating parameters. Those resonant grating structures
are commonly called GMRF (Guided-mode
Resonance Filters) and are known to have a very
small angular tolerance. However they have a high
quality factor and a very high rate of rejection.
The small angular tolerance is observed especially
when the GMRF is illuminated under oblique
incidence. That is to say when one single mode is
excited through one diffraction order, usually the first
order. In this configuration, it is possible to show
(Evenor et al., 2012).
The spectral and angular width depends on the
same parameters of the grating, namely the height h
of the grating and its 1st Fourier coefficient. A small
angular tolerance leads up to the degradation of the
rate of rejection and to the spreading of the spectrum
when the grating is illuminated with a beam with a
large divergence. But if our grating is illuminated
under normal incidence, two counter propagating
modes are excited. In this configuration, the angular
width depends on the 2nd Fourier coefficient while
the spectral width depends on the first coefficient as
shown in. (Evenor et al., 2012). Resonant grating
filters with complex basic pattern have been proposed
(Fehrembach et al., 2010), leading to an angular width
of 0.5° at 1550nm for a bandwidth of 0.28nm. Yet,
these record performance may be still insufficient for
applications where the component have to be
illuminated with a focused beam. In this optic another
structure called CRIGF was introduced (X. Buet et
al., 2012) and (K. Kintaka et al., 2012). It consists of
a GMRF and a pair of distributed Bragg reflectors
(DBRs) constructing a waveguide cavity resonator.
We inserted a phase section between each DBR and
the GMRF to optimize the reflectivity of the CRIGF.
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Rassem N., Fehrembach A. and Popov E..
An Explanation of the Physical Origin of the Extra-ordinary Angular Tolerance of Cavity Resonator Integrated Grating Filters.
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2015 SCITEPRESS (Science and Technology Publications, Lda.)