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International Conference Laser Optics (ICLO)

Statistical features of "elementary" response of superconducting hot-electron bolometer

A. V. Osipenkov, T. I. Novikova, П.А. Прудковский, G. Kh. Kitaeva

Published Jun 1, 2026• 0 citations
Publisher
DOI
10.1109/iclo69056.2026.11624467

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We study the statistical distributions of the output signals of a superconducting hot-electron bolometer (HEB) detector exposed to weak photon pulses of 1 THz (terahertz) frequency. Pulses with variable photon numbers were generated through strongly non-degenerate parametric downconversion (PDC) in a LiNbO3 crystal at 4.8 K. Fundamental differences in histograms are found between two PDC pumping modes, with pulse widths of 28 ps and 10 ns. HEB response to a picosecond THz pulse was detected in the form of a single elementary electrical pulse (SEP), with the average amplitude proportional to radiation intensity and dispersion relative to the bolometer's dark current. HEB responses to extremely weak radiation intensities have been recorded using nanosecond pulsed illumination. We found that nanosecond histograms are asymmetrical and broaden as radiation intensity increases, indicating that the nanosecond response consists of several SEPs. Poisson–Gauss approximation of histograms indicates that not only the average number of SEPs increase but also the average amplitude of a SEP increases with increasing power of incident THz radiation.
Abstract Statistical characteristics of the photoresponse of a superconducting hot-electron bolometer detector were measured under illumination by low-power terahertz pulses of 25 ns duration and 1.5 THz frequency. The pulses were generated via nonlinear-optical effects of parametric down-conversion in Mg:LiNbO 3 crystal, which was cooled to 4.5 K and pumped by a pulsed laser. The asymmetric experimental histograms of the photoresponse values obtained at different levels of incident radiation power were approximated by the Poisson-weighted sum of functions representing the convolutions of varying numbers of Gaussian distributions of elementary photocurrent pulses and the dark current distribution. It was found that the average number, the mean value, and the variance of such elementary pulses change with incident power. Specifically, the mean value and standard deviation of these pulses both grow monotonically with the increase in the mean current response, while their number tends to reach saturation at high powers. Conclusions were made about the fluctuating nature of elementary pulses, which is related to the formation of different configurations of hot spots appearing due to absorption of photons in different areas of the superconducting film. An estimate of the maximum lifetime of a hot spot was made based on the experimental data.