Disentangling superconductor and dielectric microwave losses in sub-micron Nb/ TEOS-SiO2 interconnects using a multi-mode microstrip resonator

Abstract

Understanding the origins of power loss in superconducting interconnects is essential for the energy efficiency and scalability of superconducting digital logic. At microwave frequencies, power dissipates in both the dielectrics and superconducting wires, and these losses can be of comparable magnitude. A novel method to accurately disentangle such losses by exploiting their frequency dependence using a multi-mode transmission line resonator, supported by a geometric factor concept and a 3D superconductor finite element method (FEM) modeling, is described. Using the method we optimized a planarized fabrication process of reciprocal quantum logic (RQL) for the interconnect loss at 4.2 K and GHz frequencies. The interconnects are composed of niobium ( Nb) insulated by silicon dioxide made with a tetraethyl orthosilicate precursor ( TEOS-SiO2). Two process generations use damascene fabrication, and the third one uses Cloisonn\'e fabrication. For all three, TEOS-SiO2 exhibits a dielectric loss tangent δ = 0.0012 0.0001, independent of Nb wire width over 0.25 - 4 \: μ m. The Nb loss varies with both the processing and the wire width. For damascene fabrication, scanning transmission electron microscopy (STEM) and energy dispersive X-ray spectroscopy (EDS) reveal that Nb oxide and Nb grain growth orientation increase the loss above the Bardeen Cooper Schrieffer (BCS) minimum theoretical resistance R BCS. For Cloisonn\'e fabrication, the 0.25 \: μ m wide Nb wires exhibit an intrinsic resistance Rs = 13 1.4 \: μ at 10 GHz, which is below RBCS ≈ 17 \: μ . That is arguably the lowest resistive loss reported for Nb.

0

Turn this paper into a lesson

ArcXiv compiles a structured reading guide from this paper's metadata: plain-English importance, contributions, prerequisite concepts, which sections to read first, flashcards, and a quiz. Grounded in the abstract, never invented.

Discussion (0)

Sign in to join the discussion.

Loading comments…