Grain size in low loss superconducting Ta thin films on c axis sapphire

Author:

Jones Sarah Garcia12ORCID,Materise Nicholas3ORCID,Leung Ka Wun4ORCID,Weber Joel C.5ORCID,Isakov Brian D.1,Chen Xi4,Zheng Jiangchang4,Gyenis András1ORCID,Jaeck Berthold46ORCID,McRae Corey Rae H.125ORCID

Affiliation:

1. Department of Electrical, Computer, and Energy Engineering, University of Colorado Boulder 1 , Boulder, Colorado 80309, USA

2. Department of Physics, University of Colorado 2 , Boulder, Colorado 80309, USA

3. Department of Physics, Colorado School of Mines 3 , Golden, Colorado 80401, USA

4. Department of Physics, The Hong Kong University of Science and Technology 4 , Clear Water Bay, Kowloon, Hong Kong, China

5. National Institute of Standards and Technology 5 , Boulder, Colorado 80305, USA

6. HKUST IAS Center for Quantum Technologies, The Hong Kong University of Science and Technology 6 , Clear Water Bay, Kowloon, Hong Kong, China

Abstract

In recent years, the implementation of thin-film Ta has led to improved coherence times in superconducting circuits. Efforts to further optimize this materials set have become a focus of the subfield of materials for superconducting quantum computing. It has been previously hypothesized that grain size could be correlated with device performance. In this work, we perform a comparative grain size experiment with α-Ta on c axis sapphire. Our evaluation methods include both room-temperature chemical and structural characterization and cryogenic microwave measurements, and we report no statistical difference in device performance between smaller- and larger-grain-size devices with grain sizes of 924 and 1700 nm2, respectively. These findings suggest that grain size is not correlated with loss in the parameter regime of interest for Ta grown on c axis sapphire, narrowing the parameter space for optimization of this materials set.

Funder

Graduate Fellowship for STEM Diversity

Croucher Foundation

University of Colorado Research & Innovation Seed Grant

Publisher

AIP Publishing

Subject

General Physics and Astronomy

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