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Abstract
As quantum coherence times of superconducting circuits have increased from nanoseconds to hundreds of microseconds, they are currently one of the leading platforms for quantum information processing. However, coherence needs to further improve by orders of magnitude to reduce the prohibitive hardware overhead of current error correction schemes. Reaching this goal hinges on reducing the density of broken Cooper pairs, so-called quasiparticles. Here, we show that environmental radioactivity is a significant source of nonequilibrium quasiparticles. Moreover, ionizing radiation introduces time-correlated quasiparticle bursts in resonators on the same chip, further complicating quantum error correction. Operating in a deep-underground lead-shielded cryostat decreases the quasiparticle burst rate by a factor thirty and reduces dissipation up to a factor four, showcasing the importance of radiation abatement in future solid-state quantum hardware.
Background radiation has been identified as a key factor limiting the coherence times of superconducting circuits. Here, the authors measure the impact of environmental and cosmic radiation on a superconducting resonator with varying degrees of shielding, including an underground facility.
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1 INFN Sezione di Roma, Roma, Italy (GRID:grid.470218.8)
2 PHI, Karlsruhe Institute of Technology, Karlsruhe, Germany (GRID:grid.7892.4) (ISNI:0000 0001 0075 5874); IPE, Karlsruhe Institute of Technology, Eggenstein-Leopoldshafen, Germany (GRID:grid.7892.4) (ISNI:0000 0001 0075 5874)
3 JARA Institute for Quantum Information, Forschungszentrum Jülich, Jülich, Germany (GRID:grid.8385.6) (ISNI:0000 0001 2297 375X)
4 PHI, Karlsruhe Institute of Technology, Karlsruhe, Germany (GRID:grid.7892.4) (ISNI:0000 0001 0075 5874)
5 Università di Milano - Bicocca, Dipartimento di Fisica, Milano, Italy (GRID:grid.7563.7) (ISNI:0000 0001 2174 1754); INFN Sezione di Milano - Bicocca, Milano, Italy (GRID:grid.470207.6)
6 INFN Sezione di Roma, Roma, Italy (GRID:grid.470218.8); Sapienza Università di Roma, Istituto di Nanotecnologia, Consiglio Nazionale delle Ricerche, c/o Dip. Fisica, Roma, Italy (GRID:grid.7841.a)
7 Universidad de Zaragoza, Fundación ARAID and Centro de Astropartículas y Física de Altas Energías, Zaragoza, Spain (GRID:grid.11205.37) (ISNI:0000 0001 2152 8769)
8 Institute for Photonics and Nanotechnologies, National Research Council, Rome, Italy (GRID:grid.5326.2) (ISNI:0000 0001 1940 4177)
9 INFN Laboratori Nazionali del Gran Sasso, Assergi, Italy (GRID:grid.466877.c) (ISNI:0000 0001 2201 8832); University of South Carolina, Department of Physics and Astronomy, Columbia, USA (GRID:grid.254567.7) (ISNI:0000 0000 9075 106X)
10 IPE, Karlsruhe Institute of Technology, Eggenstein-Leopoldshafen, Germany (GRID:grid.7892.4) (ISNI:0000 0001 0075 5874)
11 PHI, Karlsruhe Institute of Technology, Karlsruhe, Germany (GRID:grid.7892.4) (ISNI:0000 0001 0075 5874); National University of Science and Technology MISIS, Moscow, Russia (GRID:grid.35043.31) (ISNI:0000 0001 0010 3972); Russian Quantum Center, Skolkovo, Russia (GRID:grid.452747.7)
12 PHI, Karlsruhe Institute of Technology, Karlsruhe, Germany (GRID:grid.7892.4) (ISNI:0000 0001 0075 5874); IQMT, Karlsruhe Institute of Technology, Eggenstein-Leopoldshafen, Germany (GRID:grid.7892.4) (ISNI:0000 0001 0075 5874); Institut Néel, CNRS and Université Joseph Fourier, Grenoble, France (GRID:grid.450308.a) (ISNI:0000 0004 0369 268X)
13 INFN Sezione di Roma, Roma, Italy (GRID:grid.470218.8); Sapienza Università di Roma, Dipartimento di Fisica, Roma, Italy (GRID:grid.7841.a)
14 INFN Laboratori Nazionali del Gran Sasso, Assergi, Italy (GRID:grid.466877.c) (ISNI:0000 0001 2201 8832)
15 PHI, Karlsruhe Institute of Technology, Karlsruhe, Germany (GRID:grid.7892.4) (ISNI:0000 0001 0075 5874); IQMT, Karlsruhe Institute of Technology, Eggenstein-Leopoldshafen, Germany (GRID:grid.7892.4) (ISNI:0000 0001 0075 5874)