Hot Hydride Superconductivity above 550 K
· Invited
Abstract
The search for room temperature (RT) superconductivity (SC) has accelerated dramatically, driven by theoretical predictions that first indicated alloying dense hydrogen with other elements could produce conventional phonon-mediated SC at very high temperatures and at accessible pressures, and then with the success of structure search methods that have identified specific candidates and pressure-temperature (P-T) conditions for synthesis. As a result, experimental studies of simple binary hydrides under pressure have yielded high critical SC transition temperatures (Tc), of 260K in LaH10, close to RT, at pressures near 180GPa. We successfully synthesized a metallic La based superhydride from La metal and NH3BH3, and find an initial multi-step transition with a Tc of 294K for the highest onset, in line with previous work[1],[2]. Subsequent thermal excursions to higher temperatures promoted a chemical reaction a ternary or higher order system, confirmed by X-ray diffraction. Although the reaction does not appear to be complete, the onset temperature was pushed from 294K to 556K. The results provide evidence for hot superconductivity well above RT, in line with recent predictions for a higher order hydride under P[3].
[1] Somayazulu et al. PRL 122 (2019).
[2] Drozdov et al. Nat. 569, 528–531 (2019).
[3] Sun, Y.et al. PRL 123 (2019)
[1] Somayazulu et al. PRL 122 (2019).
[2] Drozdov et al. Nat. 569, 528–531 (2019).
[3] Sun, Y.et al. PRL 123 (2019)
*Portions of this work were performed at HPCAT (Sector 16), Advanced Photon Source (APS), Argonne National Laboratory (ANL). HPCAT operations are supported by DOE NNSA’s Office of Experimental Sciences. The APS is a U.S. Department of Energy (DOE) Office of Science User Facility operated for the DOE Office of Science by ANL under Contract No. DEAC02-06CH11357. Part of this work was performed at the National High Magnetic Field Laboratory, supported by NSF Cooperative Agreement No. DMR-1157490/1644779 and by the State of Florida. M.A., R.K. and R.H. acknowledge funding from the U.S. National Science Foundation (DMR-1933622)
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Presenters
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Audrey Grockowiak
- National High Magnetic Field Laboratory, Tallahassee and Florida State University
- NHMFL, Florida State University