English

Optical Response of Strained- and Unstrained-Silicon Cold-Electron Bolometers

Instrumentation and Methods for Astrophysics 2016-03-11 v1 Instrumentation and Detectors

Abstract

We describe the optical characterisation of two silicon cold-electron bolometers each consisting of a small (32×14 μm32 \times 14~\mathrm{\mu m}) island of degenerately doped silicon with superconducting aluminium contacts. Radiation is coupled into the silicon absorber with a twin-slot antenna designed to couple to 160-GHz radiation through a silicon lens.The first device has a highly doped silicon absorber, the second has a highly doped strained-silicon absorber.Using a novel method of cross-correlating the outputs from two parallel amplifiers, we measure noise-equivalent powers of 3.0×10163.0 \times 10^{-16} and 6.6×1017 WHz1/26.6 \times 10^{-17}~\mathrm{W\,Hz^{-1/2}} for the control and strained device, respectively, when observing radiation from a 77-K source. In the case of the strained device, the noise-equivalent power is limited by the photon noise.

Keywords

Cite

@article{arxiv.1603.03309,
  title  = {Optical Response of Strained- and Unstrained-Silicon Cold-Electron Bolometers},
  author = {T. L. R. Brien and P. A. R. Ade and P. S. Barry and C. J. Dunscombe and D. R. Leadley and D. V. Morozov and M. Myronov and E. H. C. Parker and M. J. Prest and M. Prunnila and R. V. Sudiwala and T. E. Whall and P. D. Mauskopf},
  journal= {arXiv preprint arXiv:1603.03309},
  year   = {2016}
}

Comments

Accepted for publication in Journal of Low Tempature Physics