Spectral Response of Arrays of Half-wave and Electrically Small Antennas with SINIS Bolometers
Journal article, 2020

Two types arrays of annular half-wave and electrically small antennas with typical sizes of the elements corresponding to 1/10 of the wavelength at SubTHz band with integrated superconductor-insulator-normal metal-insulator-superconductor (SINIS) bolometers have been developed, fabricated and experimentally studied. We performed numerical modeling of the full structure and use additional reference channels in experimental studies to enhance the accuracy of the spectral response estimations of receiving arrays. In experiments three reference channels were used for normalization of the spectral response: a pyroelectric detector outside the cryostat, and two cold channels-a RuO(2)bolometer and on-chip thermometer comprising series array of NIS-junctions.

terahertz radiation

SINIS-bolometers

arrays of planar antennas

Author

A. A. Gunbina

Russian Academy of Sciences

Nizhny Novgorod State Technical University

M. A. Tarasov

Russian Academy of Sciences

S. A. Lemzyakov

Moscow Institute of Physics and Technology

Russian Academy of Sciences

A. M. Chekushkin

Russian Academy of Sciences

R. A. Yusupov

Russian Academy of Sciences

Nagirnaya

Russian Academy of Sciences

M. A. Mansfel'd

Russian Academy of Sciences

Nizhny Novgorod State Technical University

V. F. Vdovin

Russian Academy of Sciences

Nizhny Novgorod State Technical University

Dag Winkler

Chalmers, Microtechnology and Nanoscience (MC2), Quantum Device Physics

Alexei Kalaboukhov

Chalmers, Microtechnology and Nanoscience (MC2), Quantum Device Physics

Sumedh Mahashabde

Chalmers, Microtechnology and Nanoscience (MC2), Quantum Device Physics

V. S. Edel'man

Russian Academy of Sciences

Physics of the Solid State

1063-7834 (ISSN) 1090-6460 (eISSN)

Vol. 62 9 1604-1611

Subject Categories

Fluid Mechanics and Acoustics

Signal Processing

Other Electrical Engineering, Electronic Engineering, Information Engineering

Condensed Matter Physics

DOI

10.1134/S1063783420090097

More information

Latest update

4/5/2022 5