Pressure-Induced Superconductivity In Polycrystalline La3Ni2O7-δ

We synthesized polycrystalline La3Ni2O7-δ (δ ≈ 0.07) samples by using the sol-gel method without postannealing under high oxygen pressure, and then measured temperature-dependent resistivity under various hydrostatic pressures up to 18 GPa by using the cubic anvil and two-stage multianvil apparatus....

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Veröffentlicht in:Physical review. X 2024-03, Vol.14 (1)
Hauptverfasser: Wang, Gang, Wang, N.  N., Shen, X.  L., Hou, J., Ma, L., Shi, L.  F., Ren, Z.  A., Gu, Y.  D., Ma, H.  M., Yang, P.  T., Liu, Z.  Y., Guo, H.  Z., Sun, J.  P., Zhang, G.  M., Calder, Stuart, Yan, Jiaqiang -Q., Wang, B.  S., Uwatoko, Yoshiya, Cheng, Jinguang -G.
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Sprache:eng
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Zusammenfassung:We synthesized polycrystalline La3Ni2O7-δ (δ ≈ 0.07) samples by using the sol-gel method without postannealing under high oxygen pressure, and then measured temperature-dependent resistivity under various hydrostatic pressures up to 18 GPa by using the cubic anvil and two-stage multianvil apparatus. We find that the density-wave-like anomaly in resistivity is progressively suppressed with increasing pressure and the resistivity drop corresponding to the onset of superconductivity emerges at pressure as low as ~ 6 GPa. Zero resistivity is achieved at 9 GPa below $T^{ZERO}_{c}$ ≈ 6.6 K, which increases quickly with pressure to 41 K at 18 GPa. However, the diamagnetic response was not detected in the ac magnetic susceptibility measurements up to 15 GPa, indicating a filamentary nature of the observed superconductivity in the studied pressure range. The constructed $T$-$P$ phase diagram reveals an intimate relationship between superconductivity, density-wave-like order, and the strange-metal-like behaviors. The observation of zero-resistance state in the polycrystalline La3Ni2O7-δ samples under high pressures not only corroborates the recent report of superconductivity in the pressurized La3Ni2O7 crystals but also facilitates further studies on this emerging family of nickelate high-$T$c superconductors.
ISSN:2160-3308
2160-3308
DOI:10.1103/PhysRevX.14.011040