Development of technology for manufacturing NbN HEB mixers with a small spread of DC and RF parameters for the creation of matrix receivers in the terahertz range
Tretyakov I.V.
1, Kaurova N.S.
2, Ivashenceva I.V.
2, Voronov B.M.
2, Goltsman G.N.
21Astro Space Center of P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow, Russia
2Moscow Pedagogical State University, Moscow, Russia
Email: ivantretykov@mail.ru, nkaurova@yandex.ru
The work is devoted to an experimental study of the influence of the process parameters of magnetron deposition of a thin 4-5 nm superconducting film of niobium nitride NbN and the fabrication technology of NbN HEB mixers on the spread of their main parameters to minimize this spread in the future. The main parameters of the NbN HEB mixer are normal resistance R300, critical temperature Tc, superconducting transition width Tc, noise temperature Tn, conversion bandwidth B and required local oscillator power Pobs. Studies of B and current-voltage IV characteristics of NbN HEB mixers were carried out at different temperatures of the Si substrate, at T near Tc and T much lower than Tc, this made it possible to identify individual interfaces in the mixer due to their different Tc. and study their influence. The uniformity of parameters of NbN HEB mixers, in addition to optimizing the NbN film deposition process, was achieved by preparing the surface of the Si substrate, as well as by using an Au layer deposited in situ with the NbN film - contact with a planar THz antenna. The NbN HEB mixers manufactured according to the optimized route had almost identical R(T) characteristics with a spread of Tc and normal resistance R300 of no more than 0.15 K and 2 Ω, respectively. The noise temperature at the local oscillator frequency of 2.52 THz was 800 K with a variation of 150 K from device to device. The noise bandwidth of the mixers at T=4.5 K averaged 7 GHz. Optimized fabrication technology will make it possible in the future to create multi-pixel heterodyne arrays from NbN HEB mixers with high uniformity of pixel parameters. Keywords: terahertz range, thin film niobium nitride, heterodyne receiver.
- H.M. Pickett, R.L. Poynter, E.A. Cohen, M.L. Delitsky, J.C. Pearson, H.S.P. Muller. J. Quant. Spectrosc. Radiat. Transfer, 60, 883 (1998). DOI: 10.1016/S0022-4073(98)00091-0
- P.L. Richards, T.M. Shen, R.E. Harris, F.L. Lloyd. Appl. Phys. Lett., 34, 345 (1979). DOI: 10.1063/1.90782
- G.J. Dolan, T.G. Phillips, D.P. Woody. Appl. Phys. Lett., 34, 347 (1979). DOI: 10.1063/1.90783
- A. Karpov, D. Miller, J.A. Stern, B. Bumbl, H.G. LeDuc, J. Zmuidzinas. Proc. 19th int. Symp. on Space Terahertz Technology (Groningen, The Netherlands, 2008), p. 68
- I. Tretyakov, S. Ryabchun, M. Finkel, A. Maslennikova, N. Kaurova, A. Lobastova, B. Voronov, G. Gol'tsman. Appl. Phys. Lett., 98, 033507 (2011). DOI: 10.1063/1.3544050
- SOFIA --- Stratospheric Observatory for Infrared Astronomy. http://www.sofia.usra.edu
- Th. de Graauw, F.P. Helmich, T.G. Phillips, J. Stutzki, E. Caux, N.D. Whyborn, P. Dieleman, P.R. Roelfsema, H. Aarts, R. Assendorp, R. Bachiller, W. Baechtold, A. Barcia, D.A. Beintema, V. Belitsky, A.O. Benz, R. Bieber, A. Boogert, C. Borys, B. Bumble, P. Cai s, M. Caris, P. Cerulli-Irelli, G. Chattopadhyay, S. Cherednichenko, M. Ciechanowicz, O. Coeur-Joly, C. Comito, A. Cros, A. de Jonge, G. de Lange, B. Delforges, Y. Delorme, T. den Boggende, J.-M. Desbat, C. Diez-Gonzalez, A.M. Di Giorgio, L. Dubbeldam, K. Edwards, M. Eggens, N. Erickson, J. Evers, M. Fich, T. Finn, B. Franke, T. Gaier, C. Gal, J.R. Gao, J.-D. Gallego, S. Gauffre, J.J. Gill, S. Glenz, H. Golstein, H. Goulooze, T. Gunsing, R. Gusten, P. Hartogh, W.A. Hatch, R. Higgins, E.C. Honingh, R. Huisman, B.D. Jackson, H. Jacobs, K. Jacobs, C. Jarchow, H. Javadi, W. Jellema, M. Justen, A. Karpov, C. Kasemann, J. Kawamura, G. Keizer, D. Kester, T.M. Klapwijk, Th. Klein, E. Kollberg, J. Kooi, P.-P. Kooiman, B. Kopf, M. Krause, J.-M. Krieg, C. Kramer, B. Kruizenga, T. Kuhn, W. Laauwen, R. Lai, B. Larsson, H.G. Leduc, C. Leinz, R.H. Lin, R. Liseau, G.S. Liu, A. Loose, I. Lopez-Fernandez, S. Lord, W. Luinge, A. Marston, J. Marti n-Pintado, A. Maestrini, F.W. Maiwald, C. McCoey, I. Mehdi, A. Megej, M. Melchior, L. Meinsma, H. Merkel, M. Michalska, C. Monstein, D. Moratschke, P. Morris, H. Muller, J.A. Murphy, A. Naber, E. Natale, W. Nowosielski, F. Nuzzolo, M. Olberg, M. Olbrich, R. Orfei, P. Orleanski, V. Ossenkopf, T. Peacock, J.C. Pearson, I. Peron, S. Phillip-May, L. Piazzo, P. Planesas, M. Rataj, L. Ravera, C. Risacher, M. Salez, L.A. Samoska, P. Saraceno, R. Schieder, E. Schlecht, F. Schloder, F. Schmu lling, M. Schultz, K. Schuster, O. Siebertz, H. Smit, R. Szczerba, R. Shipman, E. Steinmetz, J.A. Stern, M. Stokroos, R. Teipen, D. Teyssier, T. Tils, N. Trappe, C. van Baaren, B.-J. van Leeuwen, H. van de Stadt, H. Visser, K.J. Wildeman, C.K. Wafelbakker, J.S. Ward, P. Wesselius, W. Wild, S. Wulff, H.-J. Wunsch, X. Tielens, P. Zaal, H. Zirath, J. Zmuidzinas, F. Zwart. A\& A, 518 (L6), 7 (2010). DOI: 10.1051/0004-6361/201014698
- P. Putz, C.E. Honingh, K. Jacobs, M. Justen, M. Schultz, J. Stutzki. A\& A, 542 (L2), 5 (2012). DOI: 10.1051/0004-6361/201218916
- C. Risacher, R. Gusten, J. Stutzki, H.W. Hubers, D. Buchel, U.U. Graf, S. Heyminck, C.E. Honingh, K. Jacobs, B. Klein, T. Klein, C. Leinz, P. Putz, N. Reyes, O. Ricken, H.J. Wunsch, P.M. Fusco, S.W. Rosner. IEEE Trans. THz Sci. Technol., 6 (2), 199 (2016). DOI: 10.1109/TTHZ.2015.2508005
- S.-C. Shi, S. Paine, Q.-J. Yao, Z.-H. Lin, X.-X. Li, W.-Yi. Duan, H. Matsuo, Q. Zhang, Ji Yang, M.C.B. Ashley, Zh. Shang, Zh.-W. Hu. Nature Astronomy, 1 (1), (2017). DOI: 10.1038/s41550-016-0001
- Proekt Millimetron. http://www.asc.rssi.ru/millimetron/rus/millim.htm
- N.S. Kardashov, I.D. Novikov, V.N> Lukash, S.V. Pilipenko, E.V. Mikheeva, D.V. Bisikalo, D.Z. Vibe, A.G> Doroshkevich, A.V. Zasov, I.I. Zinchenko, P.B. Ivanov, V.I. Kostenko,T.I. Larchenkova, S.F. Likhachev, I.F. Malov, V.M. Malofeev, A.C. Pozanenko, A.V. Smirnov, A.M. Sobolev, A.M. Cherepashchuk, Yu.A. Shchekinov. UFN, 184, 1319 (2014). DOI: 10.3367/UFNe.0184.201412
- I. Tretyakov, S. Ryabchun, M. Finkel, A. Maslennikova, N. Kaurova, A. Lobastova, B. Voronov, G. Gol'tsman. Appl. Phys. Lett., 98, 033507 (2011). DOI: 10.1063/1.3544050
- M. Shcherbatenko, I. Tretyakov, Yu. Lobanov, S.N. Maslennikov, N. Kaurova, M. Finkel, B. Voronov, G. Goltsman, T.M. Klapwijk. Appl. Phys. Lett., 109, 132602 (2016). DOI: 10.1063/1.4963691
- J.J.A. Baselmans, M. Hajenius, J.R. Gao, T.M. Klapwijk, P.A.J. de Korte, B. Voronov, G. Gol'tsman. Appl. Phys. Lett., 84, 1958 (2004). DOI: 10.1063/1.1667012
- H.B. Callen, Th.A. Welton. Phys. Rev., 83, 34 (1951). DOI: 10.1103/PhysRev.83.34
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