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The kinetic inductance detector (KID) is a versatile and scalable detectortechnology with a wide range of applications. These superconducting detectorsoffer significant advantages: simple and robust fabrication, intrinsicmultiplexing that will allow thousands of detectors to be read out with asingle microwave line, and simple and low cost room temperature electronics.These strengths make KIDs especially attractive for HEP science via mm-wavecosmological studies. Examples of these potential cosmological observationsinclude studying cosmic acceleration (Dark Energy) through measurements of thekinetic Sunyaev-Zeldovich effect, precision cosmology through ultra-deepmeasurements of small-scale CMB anisotropy, and mm-wave spectroscopy to map outthe distribution of cosmological structure at the largest scales and highestredshifts. The principal technical challenge for these kinds of projects is thesuccessful deployment of large-scale high-density focal planes -- a need thatcan be addressed by KID technology. In this paper, we present an overview ofmicrostrip-coupled KIDs for use in mm-wave observations and outline theresearch and development needed to advance this class of technology and enablethese upcoming large-scale experiments.

Large-Format, Transmission-Line-Coupled Kinetic Inductance Detector Arrays for HEP at Millimeter Wavelengths