Superconductivity with High Upper Critical Field in the Cubic Centrosymmetric η-Carbide Nb₄Rh₂C_1-δ

2021/06/24 by KeYuan Ma, Karolina Gornicka, Robin Lefevre +5 · 1 citation
Physics and Astronomy · #cond-mat.supr-con

paper · pdf · doi:10.1021/acsmaterialsau.1c00011

published as ACS Materials Au 2021

arxiv created 2021/06/24 · arxiv updated 2021/06/25

Abstract

The upper critical field is a fundamental measure of the strength of superconductivity in a material. It is also a cornerstone for the realization of superconducting magnet applications. The critical field arises because of the Copper pair breaking at a limiting field, which is due to the Pauli paramagnetism of the electrons. The maximal possible magnetic field strength for this effect is commonly known as the Pauli paramagnetic limit given as μ₀ H_{\rm Pauli} ≈ 1.86\rm [T/K] ⋅ T_{\rm c} for a weak-coupling BCS superconductor. The violation of this limit is only rarely observed. Exceptions include some low-temperature heavy fermion and some strongly anisotropic superconductors. Here, we report on the superconductivity at 9.75 K in the centrosymmetric, cubic η-carbide-type compound Nb₄Rh₂C_1-δ, with a normalized specific heat jump of ΔC/γT_{\rm c} = 1.64. We find that this material has a remarkably high upper critical field of μ₀ H_{\rm c2}\rm (0) =~28.5~T, which is exceeding by far its weak-coupling BCS Pauli paramagnetic limit of μ₀ H_{\rm Pauli}~=~18.1 T. Determination of the origin and consequences of this effect will represent a significant new direction in the study of critical fields in superconductors.

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