Development of FD-SOI cryogenic amplifier for application to STJ readout in COBAND project

• Published in: 2021 International Symposium on VLSI Technology, Systems and Applications (VLSI-TSA) pp. 1 - 2
• Main Authors: Takeuchi, Y., Kim, S.H., Iida, T., Asano, C., Wakasa, R., Maekawa, G., Nakahara, S., Yamane, R., Ikeda, H., Wada, T., Nagase, K., Matsuura, S., Arai, Y., Kurachi, I., Hazumi, M., Yoshida, T., Mima, S., Kiuchi, K., Ishino, H., Kibayashi, A., Kato, Y., Fujii, G., Shiki, S., Ukibe, M., Ohkubo, M., Kawahito, S., Ramberg, E., Rubinov, P., Sergatskov, D., Kim, S.B., Kim, Y.H., Lee, H.J.
• Format: Conference Proceeding
• Language: English
• Published: IEEE 19.04.2021
• Subjects: Cryogenics; Finite impulse response filters; Neutrino sources; Shape; Spectroscopy; Very large scale integration; Wavelength measurement
• DOI: 10.1109/VLSI-TSA51926.2021.9440090

The COBAND is a project of an experimental search for the cosmic background neutrino decay [1] - [9] . The existence of the cosmic background neutrino is predicted as a relic of the big bang in the theoretical cosmology. Since the neutrino is found to have mass generations and mixing between them, a heavier neutrino is possible to decay to a lighter neutrino with a far-infrared photon, even though its lifetime is expected to be much longer than the age of the universe [10] . However, neither the cosmic background neutrino nor the neutrino decay is yet established experimentally. Only a lower limit in the order of 10 12 years is given on the heaviest neutrino lifetime. We, thus, search for photons which come from the cosmic background neutrino decays. The photons from the cosmic background neutrino decays are expected to shape a spectrum of a unique signature with a sharp edge at a wavelength of around 50μm depending on the heaviest neutrino mass. To identify the signature against the overwhelming zodiacal emission foreground as well as the cosmic infrared background, the photodetectors are required to have an ability to measure the FIR spectrum around 50pm with sufficient precision. Thus, we aim at developing a photodetector with capability of FIR photon-by-photon spectrometry. We employ superconducting tunnel junction (STJ) sensors in combination with cryogenic amplifiers for signal readout to maximize the potential of STJ.