Published July 15, 2010 | Version Published
Book Section - Chapter Open

Development of the nano-HEB array for low-background far-IR applications

  • 1. ROR icon Jet Propulsion Lab
  • 2. ROR icon National Institute of Standards and Technology
  • 3. ROR icon Rutgers, The State University of New Jersey
  • 4. ROR icon Star Cryoelectronics (United States)
  • 5. ROR icon Yale University

Abstract

We present an overview of the recent progress made in the development of a far-IR array of ultrasensitive hot-electron nanobolometers (nano-HEB) made from thin titanium (Ti) films. We studied electrical noise, signal and noise bandwidth, single-photon detection, optical noise equivalent power (NEP), and a microwave SQUID (MSQUID) based frequency domain multiplexing (FDM) scheme. The obtained results demonstrate the very low electrical NEP down to 1.5 × 10^(-20) W/Hz^(1/2) at 50 mK determined by the dominating phonon noise. The NEP increases with temperature as ~ T^3 reaching ~10^(-17) W/Hz^(1/2) at the device critical temperature T_C = 330-360 mK. Optical NEP = 8.6 × 10^(-18) W/Hz^(1/2) at 357 mK and 1.4 × 10^(-18) W/Hz^(1/2) at 100 mK respectively, agree with thermal and electrical data. The optical coupling efficiency provided by a planar antenna was greater than 50%. Single 8-μm photons have been detected for the first time using a nano-HEB operating at 50-200 mK thus demonstrating a potential of these detectors for future photon-counting applications in mid-IR and far-IR. In order to accommodate the relatively high detector speed (~μs at 300 mK, ~100 μs at 100 mK), an MSQUID based FDM multiplexed readout with GHz carrier frequencies has been built. Both the readout noise ~2 pA/Hz^(1/2) and the bandwidth > 150 kHz are suitable for nano-HEB detectors.

Additional Information

© 2010 SPIE. This research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration and funded in part through the internal Research and Technology Development program. The research of S.V. Pereverzev was supported by an appointment to the NASA Postdoctoral Program at the Jet Propulsion Laboratory, California Institute of Technology, administered by Oak Ridge Associated Universities through a contract with NASA. The authors thank A. Soibel (JPL) for lending the 8-µm QCL and M. Wanke (Sandia National Laboratories) for lending the 100-µm QCL.

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Identifiers

Eprint ID
65314
Resolver ID
CaltechAUTHORS:20160311-143706778

Funding

NASA/JPL/Caltech
JPL Research and Technology Development Fund
NASA Postdoctoral Program

Dates

Created
2016-03-14
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Updated
2021-11-10
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Caltech Custom Metadata

Caltech groups
Keck Institute for Space Studies
Series Name
Proceedings of SPIE
Series Volume or Issue Number
7741