Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

Scalar diffraction analysis of the dispersion effect on the focal length of low-index thin flat lenses

Open Access Open Access

Abstract

We analyze the dispersion effect of the focal length of low-index thin lenses by using scalar diffraction and finite difference time domain (FDTD) methods. We compare the dispersion results obtained by using these methods with reported experimental results, and the well-known analytical formula for focal length (f) of diffractive lenses as a function of wavelength $(\lambda ),\; \; f(\lambda )= \frac{{{f_0}{\lambda _0}}}{\lambda }$ where f0 is the designed focal length for wavelength λ0. We show that when the analytical formula is applied to thin flat lenses with low-refractive index, the results are accurate for small numerical aperture (NA) up to 0.2. For larger NA, the error between the analytical approximation and the FDTD analysis remains around 8% over a wide range of NA.

© 2022 Optica Publishing Group under the terms of the Optica Open Access Publishing Agreement

1. Introduction

Thin-flat lenses are important to the miniaturization of optical devices because of their flat geometry and small size [16]. These lenses are more dispersive than traditional lenses and efforts are underway to study the dispersion properties [711]. The numerical aperture (NA) of thin flat lenses can be much higher than that of a traditional lens or a diffraction lens. For instance, an NA of 0.4 is considered to be high for a diffraction lens [12], whereas the NA of a thin flat lens can be close to or even greater than 1 [13]. While lenses with large NA can have novel properties and applications, studying the dispersion of these lenses involves complicated numerical computations [12,14]. The goal of this study is to determine the accuracy of analytical and scalar diffraction methods for the study of dispersion in thin flat lenses with high NA. The study aims at thin flat lenses with low-index materials. Although most thin-lenses use high refractive index materials, low refractive index materials can be an attractive alternative because of their inherently small loss [6,7,15,16]. The results of the study will provide a guideline for focal length calculations in the design of flat lenses with a wide range of NAs.

It has been shown that several approximations of the classical diffraction theory can be used to describe the focal field pattern and dispersion of traditional lenses [12]. These approaches include analytical approximations, scalar diffraction, and vector diffraction theory. They have varying degrees of accuracy and computational complexity. In this work, we employ these methods to study the dispersion effects of the focal length of thin flat lenses. We study an analytical approximation derived for diffractive lenses [17,18], a scalar diffraction approximation [6], and a vector finite difference time domain (FDTD) method. We specifically evaluate the accuracy of a simple analytical approximation for focal length calculation by comparing these results with available experimental data and FDTD results. It should be noted that simple approximating equations are very useful tools in flat lens design because it is impossible to develop perfectly accurate theory for flat lenses over a wide range of NAs, while FDTD numerical computations require terabytes of memory and are always time consuming [5].

2. Lens design

The thin flat lenses for this study consist of low-index subwavelength structures [6]. Once the desired focal length of a focusing lens is known, the subwavelength structure of an equivalent flat lens can be designed in various ways. When using low refractive index transparent materials, the subwavelength structure of the flat lens reduces to the filling factor of the material in an air matrix. This is possible because light interacts weakly with low index material, and the phase change is obtained through propagation only. For instance, to focus the beam into a focal spot at a distance f, the flat lens must impart the following phase [4,6,10]:

$$\begin{array}{{c}} {{\mathbf \Phi }\left( {{\boldsymbol x},{\boldsymbol y}} \right) = \frac{{2{\boldsymbol \pi }}}{{\boldsymbol \lambda }}\left( {\sqrt {{{\boldsymbol x}^\mathbf 2} + {{\boldsymbol y}^\mathbf 2} + {{\boldsymbol f}^\mathbf 2}} - {\boldsymbol f}} \right),\; \mathbf 0 < {\mathbf \Phi } < \mathbf 2\mathbf \pi } \end{array}$$
where $\lambda $ is the operational wavelength and (x, y) are the in-plane spatial coordinates. After discretizing the desired phase profile, the required phase at each unit cell (or pixel) of the flat lens is known. This required phase can be implemented by using propagation phase:
$$\begin{array}{{c}} {{{\mathbf \Phi }_0} = \frac{{\mathbf 2{\boldsymbol \pi }{{\boldsymbol n}_{{\boldsymbol eff}}}({{\boldsymbol x},{\boldsymbol y}} ){\boldsymbol H}}}{{\boldsymbol \lambda }}} \end{array}$$
where ${\mathrm{\Phi }_0}$ is the desired phase at the location (x,y), H is the thickness of the lens, and ${n_{eff}}({x,y} )$ is the required effective refractive index at (x,y).

It is possible to control the effective refractive index of a single pixel of the flat lens by using the filling factor (FF) of the subwavelength structure of the lenses.

$$\begin{array}{{c}} {{{\boldsymbol n}_{{\boldsymbol eff}}} = \sqrt {{\boldsymbol n}_{\boldsymbol s}^\mathbf 2{\boldsymbol {FF}} + 1 - {\boldsymbol {FF}}} } \end{array}.$$

Here, the background material is assumed to be air, ns is the refractive index of inclusion material (ns <1.9) and FF is the inclusion filling factor. Each pixel of the lens might be an arrangement of different inclusions with specific filling factor [6]. To implement a specific filling factor using a fixed ns­, it is sufficient to implement a filling factor profile FF(x, y):

$$\begin{array}{{c}} {\boldsymbol {FF}({x,y} )= \frac{{{\mathbf \Phi }_{{\mathbf {pixel}}}^\mathbf 2({{\boldsymbol x},{\boldsymbol y}} )- \mathbf 2{\mathbf \pi \boldsymbol H}}}{{\mathbf 2{\mathbf \pi \boldsymbol H}({{\boldsymbol n}_{\boldsymbol s}^\mathbf 2 - \mathbf1} )}}} \end{array}.$$

Thus, the subwavelength structure of a flat lens that focuses an incoming beam into a focal spot can be designed once the focal lengths is specified.

We do not include materials dispersion in the study, because most low refractive index materials have low dispersion compared to diffraction dispersion in visible wavelengths.

3. Methods of calculation

3.1 Analytical approximation

For diffractive lenses, a well-known analytic approximation for the focal length (f) as a function of wavelength (λ) is [17,18]:

$$\begin{array}{{c}} {\boldsymbol f({\boldsymbol \lambda } )= \frac{{{{\boldsymbol f}_\mathbf 0}{{\boldsymbol \lambda }_\mathbf 0}}}{{\boldsymbol \lambda }}} \end{array}$$
where f0 is the designed focal length for wavelength λ0. Equation (5) is a good approximation for traditional diffractive lenses with very small NAs. Its applicability to thin flat lenses, especially those with higher NA, has not been explored. Such a simple equation is a very useful tool in flat lens design because it is impossible to develop perfectly accurate theory for flat lenses over a wide range of NAs and FDTD numerical computations require huge computational resources [5].

To assess the accuracy of (5) for flat lenses, we compare its results with those calculated by using the Rayleigh-Sommerfeld (RS) approximation [6] and the FDTD method, as well as experimental measurements.

3.2 Rayleigh-Sommerfeld approximation

In the Rayleigh-Sommerfeld (RS) approximation, the complex amplitude of the light at a plane (x, y) which is a distance D away from the lens edge (xin, yin) along the optical axis can be given as [19]:

$$\begin{array}{{c}} {\mathbf A({{\boldsymbol \lambda },{\boldsymbol x},{\boldsymbol y}} )= \frac{{\mathbf D}}{{{\boldsymbol i \mathbf \lambda }}}\smallint \smallint \left( {\frac{{{\mathbf T}{{\mathbf e}^{ - {\mathbf i}{{\mathbf \Phi }_{{\mathbf {edge}}}}({{{\boldsymbol x}_{{\boldsymbol {in}}}},{{\boldsymbol y}_{{\boldsymbol {in}}}}} )}}{{\boldsymbol e}^{{\boldsymbol {ikr}}}}}}{{\boldsymbol r}}} \right)\mathbf d{{\mathbf x}_{{\mathbf {in}}}}\mathbf d{{\mathbf y}_{{\mathbf {in}}}}} \end{array}$$
where $\lambda $ is the operating wavelength, T is the transmission of the lens, ${\mathrm{\Phi }_{\textrm{edge}}}$ is the imparted phase by the lens, k is the wavenumber of the beam, (${x_{in}},{y_{in}}$) is the coordinate at the lens edge, and r is given as $r = \; \sqrt {{D^2} + {{({x - {x_{in}}} )}^2} + {{({y - {y_{in}}} )}^2}} .$

Note that (6) was used in [6] to calculate the focal properties of a thin lens. It was shown in [6] that for a single wavelength analysis, predictions made using this equation matches well with vector FDTD simulations and experimental results for NAs up to 0.9.

4. Results and discussion

We compare the results obtained by using the analytical approximation in (5) and the results obtained by using the scalar diffraction in (6) with experimental results from [10]. The results are summarized in Fig. 1.

 figure: Fig. 1.

Fig. 1. Comparison of focal lengths shift predicted by using the analytical approximation and the scalar diffraction prediction with experimental results from [10]. The design wavelength (λ0) is 530 nm, and the NA is 0.2.

Download Full Size | PDF

The lens used in [10] has a numerical aperture of 0.2, a thickness of 600 nm, and a period of 400 nm. Though the thin flat lens in [10] do not use low index materials, it relies on geometrical propagation to implement the phase described in (1). The focusing mechanism and the focusing properties of this lens is comparable to the lens we studied in this work.

From Fig. 1, we observe that both the RS approximation and (5) matched the experimental result, with a 2.4% error for the scalar diffraction and a 2.5% error for (1). These results indicate that the scalar diffraction and (5) accurately predicts the dispersion of a thin flat lens if the NA is 0.2 or less.

To study the accuracy of the analytical and scalar diffraction over a large range of NA, we calculated the dispersion of a thin flat lens by using the vector full wave finite different time domain (FDTD) method and perform comparative studies.

Figure 2 shows the dispersion property of the flat lens with NA = 0.2 and ${\lambda _0} = 400nm$, calculated by using the FDTD (a) and the RS (b) methods. This figure shows that for NA = 0.2, the focal length translates linearly as wavelength increases, and the results obtained using the two methods show agreement. The scalar diffraction theory predicts that the focal length smoothly shifts as the operating wavelength changes, with the shape of the intensity profile preserved, as shown in Fig. 2(b). The vector analysis shows similar behavior, shown in Fig. 2(a). This result indicates that the scalar diffraction and vector FDTD methods agree when NA is small.

 figure: Fig. 2.

Fig. 2. The light intensity distribution along the optical axis of a thin flat lens calculated by using (a) the FDTD method and (b) the Rayleigh Sommerfeld approximation.

Download Full Size | PDF

We compared the focal length shift for higher NA by using the analytical formula in (5), the RS approximation described in (6), and the vector full wave FDTD method. The results are summarized in Fig. 3. Results from the scalar RS approximation and (5) matches well even at higher NA. For instance, at NA = 0.45, 0.65, 0.85, the Eqs. (5) and (6) predict the same shift in focal length, as shown in Fig. 3(a), (b), and (c). The focal length shift obtained by using the vector FDTD method shows certain discrepancy. This is because both (5) and (6) are scalar diffraction methods that ignore additional artifacts introduced due to the vector nature of light, such as off-axis peaks [12]. In Fig. 4, the normalized amplitudes of the electric field at the focal plane calculated by using FDTD and the RS method are shown. The off-axis peaks can be seen in the FDTD results.

 figure: Fig. 3.

Fig. 3. The dispersion of focal length with respect to operating wavelength of the lens at (a) NA = 0.450, (b) NA = 0.65 and (c) NA = 0.85. The dispersion is calculated by using the scalar RS diffraction equation in (6), the FDTD method, and the analytical approximation in (1).

Download Full Size | PDF

 figure: Fig. 4.

Fig. 4. Normalized amplitude of the fields (a)Ex, (b)Ey, and (c)Ez calculated by using FDTD. (d) Amplitude of A(x, y) described in (6).

Download Full Size | PDF

In addition, the change in the effective refractive index of neighboring pixels of the thin flat lens is not negligible. Therefore, the scalar diffraction in (6) has limited accuracy compared to an FDTD analysis. These effects lead to a persistent discrepancy between the results from the scalar diffraction in (6) and the vector full-wave FDTD method when studying dispersion.

While the scalar diffraction in (6) and the analytical approximation in (5) show deviations from the vector analysis, this error does not increase at higher NA. Figure 4 shows the errors in the normalized focal length shift for the Eqs. (5) and (6) when compared to the that calculated by using the full wave FDTD method. For each NA, the error is calculated as:

$$\begin{array}{{c}} {\boldsymbol {Error}({\boldsymbol \%} )= \mathbf {100} \times \frac{{\left|{{{\left( {\frac{{\boldsymbol f}}{{{{\boldsymbol f}_0}}}} \right)}_{{\boldsymbol {fdtd}}}} - {\boldsymbol \; }{{\left( {\frac{{\boldsymbol f}}{{{{\boldsymbol f}_0}}}} \right)}_{{\boldsymbol {scalar}}}}} \right|}}{{{{\left( {\frac{{\boldsymbol f}}{{{{\boldsymbol f}_0}}}} \right)}_{{\boldsymbol {fdtd}}}}}}} \end{array}.$$

The errors of the scalar RS approximation in (6) and the analytical approximation in (5) remain around 8% for the NA range 0.3-0.9. These results indicate that (5) is a reasonably accurate approximation to predict the dispersion of thin flat lenses even at high NA. The scalar RS diffraction method has a similar accuracy.

It should be noted that the focal length of a lens shifts from the design focal length as NA increases [20,21]. This effect is included in the FDTD analysis but not in Eqs. (5) and (6). This shift contributes to the errors shown in Fig. 5.

 figure: Fig. 5.

Fig. 5. The error in the scalar and analytical results compared to the FDTD analysis.

Download Full Size | PDF

5. Conclusion

In conclusion, we have studied the dispersive nature of low-index thin flat lenses and compared three methods for calculating the dispersion. We showed that the analytical dispersion Eq. (1) originally derived for diffractive lenses remain accurate for low index thin flat lenses with low NA. When the NA is higher, the error between the analytical approximation and the FDTD analysis remains around 10% over a wide range of NA. Because the analytical approximation is significantly faster in computation and easier to use, it can be sufficient for most applications. Full wave FDTD analyses can be used to design and evaluate focal plane light intensity distribution of flat lenses with high accuracy, at the cost of added computational complexity.

Disclosures

The authors declare no conflict of interest.

Data availability

Data underlying the results presented in this paper are not publicly available at this time but may be obtained from the authors upon reasonable request.

References

1. N. Yu and F. Capasso, “Flat optics with designer metasurfaces,” Nat. Mater. 13(2), 139–150 (2014). [CrossRef]  

2. M. Decker, I. Staude, M. Falkner, J. Dominguez, D. N. Neshev, I. Brener, T. Pertsch, and Y. S. Kivshar, “High-efficiency dielectric Huygens’ surfaces,” Adv. Opt. Mater. 3(6), 813–820 (2015). [CrossRef]  

3. S. J. Byrnes, A. Lenef, F. Aieta, and F. Capasso, “Designing large, high-efficiency, high-numerical-aperture, transmissive meta-lenses for visible light,” Opt. Express 24(5), 5110–5124 (2016). [CrossRef]  

4. M. Khorasaninejad, W. T. Chen, R. C. Devlin, J. Oh, A. Y. Zhu, and F. Capasso, “Metalenses at visible wavelengths: Diffraction-limited focusing and subwavelength resolution imaging,” Science 352(6290), 1190–1194 (2016). [CrossRef]  

5. A. She, S. Zhang, S. Shian, D. R. Clarke, and F. Capasso, “Large area metalenses: design, characterization, and mass manufacturing,” Opt. Express 26(2), 1573–1585 (2018). [CrossRef]  

6. A. A. Siraji and Y. Zhao, “Design and analysis of thin optical lens composed of low-index subwavelength structures,” Appl. Opt. 58(17), 4654–4664 (2019). [CrossRef]  

7. M. Khorasaninejad, Z. Shi, A. Y. Zhu, W.-T. Chen, V. Sanjeev, A. Zaidi, and F. Capasso, “Achromatic metalens over 60 nm bandwidth in the visible and metalens with reverse chromatic dispersion,” Nano Lett. 17(3), 1819–1824 (2017). [CrossRef]  

8. S. Shrestha, A. C. Overvig, M. Lu, A. Stein, and N. Yu, “Broadband achromatic dielectric metalenses,” Light: Sci. Appl. 7(1), 85 (2018). [CrossRef]  

9. M. Ye, V. Ray, and Y. S. Yi, “Achromatic Flat Subwavelength Grating Lens Over Whole Visible Bandwidths,” IEEE Photonics Technol. Lett. 30(10), 955–958 (2018). [CrossRef]  

10. W. T. Chen, A. Y. Zhu, V. Sanjeev, M. Khorasaninejad, Z. Shi, E. Lee, and F. Capasso, “A broadband achromatic metalens for focusing and imaging in the visible,” Nat. Nanotechnol. 13(3), 220–226 (2018). [CrossRef]  

11. L. Li, Q. Yuan, R. Chen, X. Zou, W. Zang, T. Li, G. Zheng, S. Wang, Z. Wang, and S. Zhu, “Chromatic dispersion manipulation based on metasurface devices in the mid-infrared region,” Chin. Opt. Lett. 18(8), 082401 (2020). [CrossRef]  

12. M. Mansuripur, “Distribution of light at and near the focus of high-numerical-aperture objectives,” J. Opt. Soc. Am. A 3(12), 2086–2093 (1986). [CrossRef]  

13. M. Khorasaninejad, A. Y. Zhu, C. Roques-Carmes, W. T. Chen, J. Oh, I. Mishra, R. C. Devlin, and F. Capasso, “Polarization-insensitive metalenses at visible wavelengths,” Nano Lett. 16(11), 7229–7234 (2016). [CrossRef]  

14. Y. Zhang, H. An, D. Zhang, G. Cui, and X. Ruan, “Diffraction theory of high numerical aperture subwavelength circular binary phase Fresnel zone plate,” Opt. Express 22(22), 27425–27436 (2014). [CrossRef]  

15. A. Zhan, S. Colburn, R. Trivedi, T. K. Fryett, C. M. Dodson, and A. Majumdar, “Low-Contrast Dielectric Metasurface Optics,” ACS Photonics 3(2), 209–214 (2016). [CrossRef]  

16. A. A. Siraji and Y. Zhao, “High-sensitivity and high-Q-factor glass photonic crystal cavity and its applications as sensors,” Opt. Lett. 40(7), 1508–1511 (2015). [CrossRef]  

17. E. Arbabi, A. Arbabi, S. M. Kamali, Y. Horie, and A. Faraon, “Controlling the sign of chromatic dispersion in diffractive optics with dielectric metasurfaces,” Optica 4(6), 625–632 (2017). [CrossRef]  

18. M. Born and E. Wolf, Principles of Optics: Electromagnetic Theory of Propagation, Interference and Diffraction of Light, 7th ed. (Cambridge University Press, 1999).

19. D. G. Voelz, Computational Fourier Optics: A MATLAB Tutorial (SPIE press Bellingham, WA, 2011).

20. Y. Li and E. Wolf, “Focal shifts in diffracted converging spherical waves,” Opt. Commun. 39(4), 211–215 (1981). [CrossRef]  

21. Y. Li, “Dependence of the focal shift on Fresnel number and f number,” J. Opt. Soc. Am. 72(6), 770–774 (1982). [CrossRef]  

Data availability

Data underlying the results presented in this paper are not publicly available at this time but may be obtained from the authors upon reasonable request.

Cited By

Optica participates in Crossref's Cited-By Linking service. Citing articles from Optica Publishing Group journals and other participating publishers are listed here.

Alert me when this article is cited.


Figures (5)

Fig. 1.
Fig. 1. Comparison of focal lengths shift predicted by using the analytical approximation and the scalar diffraction prediction with experimental results from [10]. The design wavelength (λ0) is 530 nm, and the NA is 0.2.
Fig. 2.
Fig. 2. The light intensity distribution along the optical axis of a thin flat lens calculated by using (a) the FDTD method and (b) the Rayleigh Sommerfeld approximation.
Fig. 3.
Fig. 3. The dispersion of focal length with respect to operating wavelength of the lens at (a) NA = 0.450, (b) NA = 0.65 and (c) NA = 0.85. The dispersion is calculated by using the scalar RS diffraction equation in (6), the FDTD method, and the analytical approximation in (1).
Fig. 4.
Fig. 4. Normalized amplitude of the fields (a)Ex, (b)Ey, and (c)Ez calculated by using FDTD. (d) Amplitude of A(x, y) described in (6).
Fig. 5.
Fig. 5. The error in the scalar and analytical results compared to the FDTD analysis.

Equations (7)

Equations on this page are rendered with MathJax. Learn more.

Φ ( x , y ) = 2 π λ ( x 2 + y 2 + f 2 f ) , 0 < Φ < 2 π
Φ 0 = 2 π n e f f ( x , y ) H λ
n e f f = n s 2 F F + 1 F F .
F F ( x , y ) = Φ p i x e l 2 ( x , y ) 2 π H 2 π H ( n s 2 1 ) .
f ( λ ) = f 0 λ 0 λ
A ( λ , x , y ) = D i λ ( T e i Φ e d g e ( x i n , y i n ) e i k r r ) d x i n d y i n
E r r o r ( % ) = 100 × | ( f f 0 ) f d t d ( f f 0 ) s c a l a r | ( f f 0 ) f d t d .
Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All rights reserved, including rights for text and data mining and training of artificial technologies or similar technologies.