2016
DOI: 10.1364/oe.24.00a925
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Nanophotonic resonators for InP solar cells

Abstract: We describe high efficiency thin-film InP solar cells that utilize a periodic array of TiO2 nanocylinders. These nanophotonic resonators are found to reduce the solar-weighted average reflectivity of an InP solar cell to ~1.3%, outperforming the best double-layer antireflection coatings. The coupling between Mie scattering resonances and thin-film interference effects accurately describes the optical enhancement provided by the nanocylinders. The spectrally resolved reflectivity and J-V characterist… Show more

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Cited by 20 publications
(7 citation statements)
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“…The occurring Mie resonance results in forward scattering into the substrate. [4][5][6][7][8][9][40][41][42][43][44] In hexagonal arrays, reflectance dips due to a grating effect (Wood-Rayleigh anomaly) occur at 'p/2′ and '(p/2)•(3) 1/2 ′, where 'p' is the period. In the investigated wavelength range, for the hexagonal period spacing of ~ 550 nm the dip appears at a wavelength of ~ 480 nm.…”
Section: Solar-weighted Reflectance Of Structured Tio 2 Np-based Optimentioning
confidence: 99%
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“…The occurring Mie resonance results in forward scattering into the substrate. [4][5][6][7][8][9][40][41][42][43][44] In hexagonal arrays, reflectance dips due to a grating effect (Wood-Rayleigh anomaly) occur at 'p/2′ and '(p/2)•(3) 1/2 ′, where 'p' is the period. In the investigated wavelength range, for the hexagonal period spacing of ~ 550 nm the dip appears at a wavelength of ~ 480 nm.…”
Section: Solar-weighted Reflectance Of Structured Tio 2 Np-based Optimentioning
confidence: 99%
“…The obtained J sc enhancement agrees well with data reported in a simulation study for a similar type of structuring on InP solar cells. 44 .…”
Section: Solar-weighted Reflectance Of Structured Tio 2 Np-based Optimentioning
confidence: 99%
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“…The spectral response of short-wave infrared (SWIR) In 0.53 Ga 0.47 As/InP focal plane arrays (FPAs) typically covers the wavelength range of 0.9–1.7 μm. For the visible–SWIR (vis–SWIR) In 0.53 Ga 0.47 As (hereafter referred to as InGaAs), it is extended to 0.5–1.7 μm via a substrate removing process. Apart from applications in space remote sensing, the vis–SWIR InGaAs FPAs are emerging as a very powerful technology for novel applications such as medical diagnostics and polarization imaging. However, the sensitivities of the commercial vis–SWIR InGaAs FPAs are currently inferior to that of the silicon cameras in the wavelength range of 0.5–0.9 μm. , Because of the lower surface recombination velocity among III–V semiconductors, InP has been demonstrated to be an ideal substrate to integrate with Mie resonator arrays. , Improved light absorption and photoelectric conversion in the photocathodes for solar hydrogen production have been observed . For the backside-illuminated InGaAs PIN FPAs with a spectral response of 1–1.7 μm, periodically arranged InP Mie resonators can restrain the deleterious multiple reflection of scattered light and enhance the light absorption in the InGaAs absorber, from which enhanced quantum efficiencies and image quality can be expected.…”
Section: Introductionmentioning
confidence: 99%
“…Due to technological progress in nano-fabrication during the last decades, in terms of control of features at subwavelength scales implemented on various materials, of devices based on light trapping in standard p/n diodes, as, e.g. based on InP with improvements above that of standard antireflection coatings [35] or in nanowires of various sorts were proposed by several research groups. For example, silicon nanowires with p-n radial junction [7,9], InP nanowire array [8,10], or nanowire based dye-sensitized solar cell [11].…”
Section: Introductionmentioning
confidence: 99%