Aluminium Kinetic Inductance Detectors at 1.54 THz limited by photon noise and generation-recombination noise Pieter de Visser, Jochem Baselmans, Juan.

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Presentation transcript:

Aluminium Kinetic Inductance Detectors at 1.54 THz limited by photon noise and generation-recombination noise Pieter de Visser, Jochem Baselmans, Juan Bueno, Nuria Llombart, Teun Klapwijk SRON TU Delft, Faculty of Applied Sciences TU Delft, Faculty of Electrical Engineering Mathematics and Computer Siences

Optical Noise Equivalent 1.54 THz GR - Noise Photon Noise

Operation principle Day et al, Nature 425, 817 (2003) 2Δ2Δ Cooper Pairs Quasiparticles h Photons break Cooper pairs => quasiparticles Higher resistance and kinetic inductance Dip depth / amplitude: resistance Resonant frequency / phase: inductance

Anticipated fundamental limits KID is a pair breaking detector: fluctuations in the quasiparticle number Photon noise (= generation noise) Recombination noise Generation-recombination noise Prediction from dark experiments: NEP of 2 x W/Hz 1/2 limited by the presence of excess quasiparticles

Design All Aluminium KID Central Line: 50 nm Al Groundplane: 100 nm Al Halfwave resonator with isolated central strip X-slot Antenna, broad band around 1.54 THz 2 mm silicon elliptical lenses Design suitable for higher frequencies >1.54 THz

Controlled optical setup 8 optical filters! Box-in-box setup Baselmans et al. JLTP 167, 360 (2012) J. Bueno, Poster 106 (Thursday)

Large range in optical power

Fundamental limit: Photon Noise Optical Power (fW) Random arrival rate of the optical photons + recombination noise

Generation-recombination noise De Visser et al. PRL 106, (2011) Wilson & Prober, PRL, 87, (2001) Quasiparticle fluctuations

Optical Noise Equivalent Power GR - Noise Photon Noise Photon noise limited NEP => Measure of optical efficiency: 48%

Optical responsivity + lifetime: Microwave readout power dependent De Visser et al. APL 100, (2012) Goldie, SuST, 26, (2013)

Microwave readout power: Excess quasipartilces AND nonlinear reponse due to redistribution of quasiparticles arXiv: Poster 104 (Monday)

Summary Kinetic Inductance Detector at 1.54 THz – Fundamental noise sources for pair breaking detectors revealed: Photon noise limited Generation-recombination noise => excess quasiparticles – NEP 3.8 x W/Hz 1/2, 48% optical efficiency Well controlled optical setup, large power range 1.54 THz experiment - arXiv: Microwave response - arXiv:

KID at 1.54 THz GR - Noise Photon Noise Optical efficiency: 48% arXiv: