Numerical Methods for Current Mirror Qubit Simulations
ORAL
Abstract
Current Mirror Qubits1 (CMQs) are an example of “noise insensitive” superconducting qubits predicted to exhibit longer coherence times than conventional superconducting qubits even when exposed to the same noise environment. CMQs also have the advantage of not requiring detailed tune-up or fabrication precision2 to achieve noise insensitivity. However, given the large number of circuit components that comprise such qubits, direct numerical diagonalization of the qubit’s Hamiltonian using a product basis is numerically intractable. This presents a challenge for verifying projected noise immunity for realistic circuits that include fabrication imperfections or control offsets. This talk discusses various numerical models for CMQs that address this challenge, and presents initial comparisons between these models and experimental realizations of these qubits.
[1] Alexei Kitaev, arXiv:cond-mat/0609441 (2006)
[2] Dempster et al., PRB 90, 094518 (2014)
[1] Alexei Kitaev, arXiv:cond-mat/0609441 (2006)
[2] Dempster et al., PRB 90, 094518 (2014)
–
Presenters
-
Daniel Weiss
Northwestern Univeristy, Department of Physics and Astronomy, Northwestern University
Authors
-
Daniel Weiss
Northwestern Univeristy, Department of Physics and Astronomy, Northwestern University
-
David Ferguson
Northrop Grumman, Northrop Grumman - Mission Systems, Northrop Grumman Corporation
-
Moe S Khalil
Northrop Grumman, Northrop Grumman Corporation
-
Andy C. Y. Li
Fermilab, Scientific Computing Division, Fermi National Accelerator Laboratory
-
Jens Koch
Department of Physics and Astronomy, Northwestern University, Northwestern University, Northwestern Univeristy