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José Alberto Nava Aquino

Publications and source records attributed to José Alberto Nava Aquino.

3 recordsLinked to original sources

Nonequilibrium Quasiparticles in Superconducting Circuits: Energy Relaxation, Charge and Flux Noise

The quasiparticle density observed in low-temperature superconducting circuits is several orders of magnitude larger than the value expected at thermal equilibrium. The tunneling of this excess of quasiparticles across Josephson junctions is recognized as one of the main loss and decoherence mechanisms in superconducting qubits. Here, we present a unified impedance theory that accounts for quasiparticle energy loss in circuit regions both far and near (across) junctions. Our theory leverages the recent experimental demonstration that the excess quasiparticles are in \emph{quasiequilibrium} [T. Connolly et al., Phys. Rev. Lett. $\textbf{132}$, 217001 (2024)] and uses a generalized fluctuation-dissipation theorem to predict the amount of charge and flux noise generated by them. We compute the resulting energy relaxation time $T_1$ in transmon qubits with and without junction asymmetric gap engineering, and show that quasiparticles residing away from junctions can play a dominant role in the former case. They also may provide an upper limit for resonator quality factors if the density of amorphous two-level systems is reduced. In addition, we show that charge noise from quasiparticles leads to flux noise that is logarithmic-in-frequency, giving rise to a ``nearly white" contribution that is comparable to the flux noise observed in flux qubits. This contrasts with amorphous two-level systems, whose associated flux noise is shown to be superOhmic. We discuss how this quasiparticle flux noise can limit $T_2^{*}$ coherence times in flux-tunable qubits. The conclusion is that asymmetric gap engineering can greatly reduce noise and increase coherence times in superconducting qubits.

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Model for 1/f Flux noise in Superconducting Aluminum Devices: Impact of External Magnetic Fields

Superconducting quantum interference devices (SQUIDs) and related circuits made of aluminum are known to display $1/ω$ flux noise, where $ω$ is frequency. A recent experiment showed that the application of an external magnetic field in the $10-100$~G range changed the noise to a single Lorentzian peaked at $ω=0$. Here it is shown that a model based on independent impurity spin flips with coexisting cross and direct mechanisms of spin relaxation may explain these experiments. The model shows that application of an external magnetic field can be used to reduce the impact of flux noise in qubits.

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Flux noise in disordered spin systems

Impurity spins randomly distributed at the surfaces and interfaces of superconducting wires are known to cause flux noise in Superconducting Quantum Interference Devices, providing a mechanism for decoherence in superconducting qubits. While flux noise is well characterised experimentally, the microscopic model underlying spin dynamics remains unknown. First-principles theories are too computationally expensive to capture spin diffusion over large length scales, third-principles approaches lump spin dynamics into a single phenomenological spin-diffusion operator that is not able to describe the quantum noise regime and connect to microscopic models and disorder scenarios. Here we propose an intermediate "second principles" method to describe general spin dissipation and flux noise in the quantum regime. It leads to the interpretation that flux noise arises from the density of paramagnon excitations at the edge of the wire, with paramagnon-paramagnon interactions leading to spin diffusion, and interactions between paramagnons and other degrees of freedom leading to spin energy relaxation. At high frequency we obtain an upper bound for flux noise, showing that the (super)Ohmic noise observed in experiments does not originate from interacting spin impurities. We apply the method to Heisenberg models in two dimensional square lattices with random distribution of vacancies and nearest-neighbour spins coupled by constant exchange. Numerical calculations of flux noise show that it follows the observed power law $A/ω^α$, with amplitude $A$ and exponent $α$ depending on temperature and inhomogeneities. These results are compared to experiments in niobium and aluminium devices. The method establishes a connection between flux noise experiments and microscopic Hamiltonians identifying relevant microscopic mechanisms and guiding strategies for reducing flux noise.

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