(La,Th)H10: Potential High-Tc (242 K) Superconductors Stabilized Thermodynamically below 200 GPa

Peng Song, Artur P. Durajski, Zhufeng Hou, Abdul Ghaffar, Rohit Dahule, Radosław Szczȩśniak, Kenta Hongo, Ryo Maezono

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18 Scopus citations

Abstract

The recent experimental discovery of high-pressure superconductivity in (La,Y)H10, (La,Ce)H9, (La,Ce)H10, (Y,Ce)H9, and (La,Nd)H10 confirms that ternary rare-earth clathrate hydrides are promising candidates for high-temperature superconductors. This study theoretically demonstrates the ability of actinide-metal thorium (Th), rare-earth-metal lanthanum (La), and hydrogen to form stable ternary hydrides under 200 GPa. Using the evolutionary algorithm combined with the first-principles calculations and strong-coupling Eliashberg approach, we predicted the pressure-dependent ternary phase diagram of LaxThyHz, particularly, the case of (La1-xThx)Hn [or designated as (La,Th)Hn for simplicity]. Our calculations revealed that hydrogen-rich phases such as (La,Th)H10 are thermodynamically stable below 200 GPa, with phase decomposition occurring in (La,Th)H9 above 150 GPa. Moreover, the electron-phonon coupling (EPC) calculations show that the (La,Th)H10 series could function as potential superconductors, of which I4/mmm-La3ThH40 (at 200 GPa) exhibited a large EPC constant of λ = 2.46 with the highest transition temperature (Tc) of 242 K.

Original languageEnglish
Pages (from-to)2656-2665
Number of pages10
JournalJournal of Physical Chemistry C
Volume128
Issue number6
DOIs
StatePublished - Feb 15 2024

Funding

The computations in this study have been performed using the facilities of Research Center for Advanced Computing Infrastructure (RCACI) at JAIST. P.S. is grateful for financial support from Grant-in-Aid for JSPS Research Fellow (JSPS KAKENHI Grant No. 22J10527). K.H. is grateful for financial support from MEXT-KAKENHI, Japan (JP19K05029, JP21K03400, JP23H04623, and JP22H02170), and the Air Force Office of Scientific Research, United States (Award No.: FA2386-22-1-4065). R.M. is grateful for financial support from MEXT-KAKENHI (22H05146, 21K03400, and 19H04692), from the Air Force Office of Scientific Research (AFOSR-AOARD/FA2386-17-1-4049; FA2386-19-1-4015), and from JSPS Bilateral Joint Projects (JPJSBP120197714). A.P.D. is grateful for financial support from the National Science Centre (Poland) through Project No. 2022/47/B/ST3/00622.

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