The discovery of superconductivity at 260 K in hydrogen-rich compounds like LaH re-invigorated the quest for room temperature superconductivity. Here, we report the temperature dependence of the upper critical fields μH(T) of superconducting HS under a record-high combination of applied pressures up to 160 GPa and fields up to 65 T. We find that H(T) displays a linear dependence on temperature over an extended range as found in multigap or in strongly-coupled superconductors, thus deviating from conventional Werthamer, Helfand, and Hohenberg (WHH) formalism. The best fit of H(T) to the WHH formalism yields negligible values for the Maki parameter α and the spin-orbit scattering constant λ. However, H(T) is well-described by a model based on strong coupling superconductivity with a coupling constant λ ~ 2. We conclude that HS behaves as a strong-coupled orbital-limited superconductor over the entire range of temperatures and fields used for our measurements.

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http://www.ncbi.nlm.nih.gov/pmc/articles/PMC6555813PMC
http://dx.doi.org/10.1038/s41467-019-10552-yDOI Listing

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The discovery of superconductivity at 260 K in hydrogen-rich compounds like LaH re-invigorated the quest for room temperature superconductivity. Here, we report the temperature dependence of the upper critical fields μH(T) of superconducting HS under a record-high combination of applied pressures up to 160 GPa and fields up to 65 T. We find that H(T) displays a linear dependence on temperature over an extended range as found in multigap or in strongly-coupled superconductors, thus deviating from conventional Werthamer, Helfand, and Hohenberg (WHH) formalism.

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