heterodyne detectors

Conventional, superconducting niobium nitride (NbN) hot electron bolometers (HEBs) are so far the most sensitive heterodyne detectors for high-resolution spectroscopy at far-infrared frequencies. Heterodyne detectors take advantage of a local oscillator to convert a terahertz line into a gigahertz line. This allows them to measure not only the intensity in great detail but also the frequency. Heterodyne detectors have been successfully applied in balloon and space telescopes and are candidates to serve in future missions. Ground telescopes cannot see far-infrared radiation as it is blocked by the Earth’s atmosphere.

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limited bandwidth

One drawback of such detectors is its bandwidth, that covers a limited spectral line in one measurement. Another restriction comes from the low operating temperature. Cooling down to 4 Kelvin, either by using a vessel with liquid helium or a mechanical pulse tube, is undesirable for a space observatory considering the constraints on mass, volume, electrical power, and cost.

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new superconducting material

Yuner Gan and her colleagues have now developed a far-infrared HEB detector based on a new superconducting material—magnesium diboride (MgB2)—which has a relatively high critical temperature of 39 Kelvin. This allows them to get a higher operating temperature, at 20 Kelvin or more. They have also demonstrated that the novel HEBs have promising sensitivities and a much increased frequency bandwidth.

SRON is responsible for the overall project. The fabrication of the detectors was done at TU Delft, while the MgB2 thin film was developed at Chalmers University.

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Publication

The publication in the Journal of Applied Physics is selected for the Special Collection Recognizing Women in Applied Physics.

Y. Gan, B. Mirzaei, J.R.G. Silva, S. Cherednichenko, F. van der Tak, and J.R. Gao, ‘Heterodyne performance and characteristics of terahertz MgB2 hot electron bolometers’, J. Applied Physics

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