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A bioinspired solution for spectrally selective thermochromic VO2 coated intelligent glazing

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Abstract

We present a novel approach towards achieving high visible transmittance for vanadium dioxide (VO2) coated surfaces whilst maintaining the solar energy transmittance modulation required for smart-window applications. Our method deviates from conventional approaches and utilizes subwavelength surface structures, based upon those present on the eyeballs of moths, that are engineered to exhibit broadband, polarization insensitive and wide-angle antireflection properties. The moth-eye functionalised surface is expected to benefit from simultaneous super-hydrophobic properties that enable the window to self-clean. We develop a set of design rules for the moth-eye surface nanostructures and, following this, numerically optimize their dimensions using parameter search algorithms implemented through a series of Finite Difference Time Domain (FDTD) simulations. We select six high-performing cases for presentation, all of which have a periodicity of 130 nm and aspect ratios between 1.9 and 8.8. Based upon our calculations the selected cases modulate the solar energy transmittance by as much as 23.1% whilst maintaining high visible transmittance of up to 70.3%. The performance metrics of the windows presented in this paper are the highest calculated for VO2 based smart-windows.

© 2013 Optical Society of America

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Figures (7)

Fig. 1
Fig. 1 Spectra used to weight the transmittance functions in Eqs. 1. The photopic luminous efficiency of the human eye [23], ȳ(λ), and the AM1.5 solar irradiance spectrum [24].
Fig. 2
Fig. 2 The optical model for VO2 as used in our FDTD simulations.
Fig. 3
Fig. 3 FDTD simulations of planar VO2 window systems with different thin-film thicknesses showing the associated changes in T lum cold and ΔTsol. The transmittance color in both the hot and cold phases are shown in the upper bars.
Fig. 4
Fig. 4 Side (a) and top (b) elevations of a nanotextured surface with hexagonally arranged circular paraboloid cones. Pitch P, base-width W and VO2 coating thickness C. As in (b), when W = P 4 3 2 C both the peak-to-trough height difference and the areal density at the air-VO2 interface are maximized.
Fig. 5
Fig. 5 FDTD parameter search for hexagonally arranged VO2 coated paraboloid nanostructures in which W = 4 3 P 2 C. Contours lines of Tlum are overlaid upon a heat-map of ΔTsol and vice-versa. Six parameter sets are chosen [A–F] (detailed in Table 3)
Fig. 6
Fig. 6 [C] Normal incidence transmittance, absorptance and reflectance spectra for a moth-eye smart-window, case C: H = 700 nm, C = 8 nm, P = 130 nm and W = 134 nm.
Fig. 7
Fig. 7 Wide-angle FDTD simulations of the transmittance through (a) a moth-eye smart-window surface (case C) and (b) a planar 50 nm thick VO2 smart-window with a 40 nm TiO2 antireflection coating applied to the surface.

Tables (3)

Tables Icon

Table 1 A comparison of smart-window transmittance metrics for a variety of VO2 based multilayer smart-window systems. Eqs. 1 and 2 are used to calculate the reported metrics using broadband transmittance data extracted from the cited publications where appropriate. All dimensions are in nanometers, Tsol, Tlum and ΔTsol are all presented as a percentage of energy transmittance.

Tables Icon

Table 2 Calculations of the maximum pitch for moth-eye surface nanostructures that satisfy Eq. 3 over different wavelength intervals and angles of incidence. The moth-eye surface is assumed to be in air (n0 = 1). Values for n1 are calculated as the maximum refractive index for metallic and semiconductor VO2 within the wavelength range. All angles are in degrees, wavelengths and pitches are quoted in nanometers

Tables Icon

Table 3 Smart-window transmittance metrics for selected moth-eye VO2 smart-windows systems. Equations 1 and 2 are used to calculate the reported metrics. All dimensions are in nanometers, Tsol, Tlum and ΔTsol are all presented as a percentage of energy transmittance.

Equations (4)

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T lum σ = λ = 380 nm 780 nm y ¯ ( λ ) T σ ( λ ) d λ λ = 380 nm 780 nm y ¯ ( λ ) d λ T sol σ = λ = 300 nm 2500 nm AM 1.5 ( λ ) T σ ( λ ) d λ λ = 300 nm 2500 nm AM 1.5 ( λ ) d λ
Δ T lum = T lum cold T lum hot Δ T sol = T sol cold T sol hot
P λ min n 1 + n 0 sin ( θ i )
W = P 4 3 2 C
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