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Project

Thin perfect absorbers on top of CMOS

Classical imagers for visible light use silicon as the absorbing semiconductor. But the absorption length in silicon for the visible is rather long, e.g. more than 6 microns for red light. The pixel dimensions of advance imagers are much smaller, going down to even 0.7 microns. As a consequence, it is a huge technological challenge to avoid crosstalk in those structures. However, recent work [1-4] indicates that new meta-materials can be engineered such that perfect absorption can be obtained in layers of only a few nanometers thick. It is clear that such stacks, when integrated in an imager stack on top of CMOS can avoid the crosstalk problems and enable further downscaling of CMOS imagers. This PhD topic focusses on the engineering and the experimental verification of those stacks for use on top of CMOS. Applications are obviously broader than only imagers. Also, amongst others photovoltaics can benefit from these metamaterial stacks. [1] A. Ghobadi, et al.,, “Strong Light–Matter Interaction in Lithography-Free Planar Metamaterial Perfect Absorbers,” ACS Photonics 5, p. 4203, Nov. 2018. [2] M.R.S. Dias, et al., “Lithography-Free, Omnidirectional, CMOS-Compatible AlCu Alloys for Thin-Film Superabsorbers,” Advanced Optical Materials 6, p. 1700830, Jan. 2018. [3] J. Rensberg et al., “Epsilon-Near-Zero Substrate Engineering for Ultrathin-Film Perfect Absorbers,” Phys. Rev. Applied 8, p. 014009, Jul. 2017. [4 ] V. Steenhoff, et al., “Ultrathin Resonant-Cavity-Enhanced Solar Cells with Amorphous Germanium Absorbers,” Advanced Optical Materials 3, p 182, 2015.

Date:25 Nov 2020  →  Today
Keywords:CMOS technology, image sensors, perovskites
Disciplines:Nanophotonics, Photodetectors, optical sensors and solar cells
Project type:PhD project