Broadband refractive optics realized from high index materials provide compelling design solutions for the next generation of observatories for the Cosmic Microwave Background (CMB), and for sub-millimeter astronomy. In this paper, work is presented which extends the state of the art in silicon lenses with metamaterial antireflection (AR) coatings towards larger bandwidth and higher frequency operation. Examples presented include octave bandwidth coatings with less than 0.5% reflection, a prototype 4:1 bandwidth coating, and a coating optimized for 1.4 THz. For these coatings the detailed design, fabrication and testing processes are described as well as the inherent performance trade offs.
Keywords Optics, Metamaterials
IntroductionCurrent and planned ground-based CMB experiments [1-5] and sub-millimeter observatories [6, 7] use photon noise limited detectors. Improving the sensitivity of these instruments requires deploying a greater number of detectors. The two approaches being pursued are development of optical systems with large fields of view, and multichroic detectors. The former usually requires lenses fabricated from high index of refraction materials. The latter requires optical systems operating over broad bandwidths. Simultaneously meeting these design requirements necessitates the realization of high performance AR coatings.Silicon lenses with metamaterial AR coatings represent a rapidly maturing technology that can meet these needs. These coatings offer excellent optical performance (low reflection, low dielectric losses, and low scattering [8]), are robust to thermal cycling, and can be