| Literature DB >> 33902020 |
Chengping He1, Xue Ming1, Qing Li1, Xiyu Zhu1, Jin Si1, Hai-Hu Wen1.
Abstract
Recently, superconductivity at about 9-15 K was discovered in Nd1-xSrxNiO2(Nd-112,x≈ 0.125-0.25) infinite-layer thin films, which has stimulated enormous interests in related rare-earth nickelates. Usually, the first step to synthesize this 112 phase is to fabricate theRNiO3(R-113,R: rare-earth element) phase, however, it was reported that the 113 phase is very difficult to be synthesized successfully due to the formation of unusual Ni3+oxidation state. And the difficulty of preparation is enhanced as the ionic radius of rare-earth element decreases. In this work, we report the synthesis and investigation on multiple physical properties of polycrystalline perovskites Sm1-xSrxNiO3(x= 0, 0.2) in which the ionic radius of Sm3+is smaller than that of Pr3+and Nd3+in related superconducting thin films. The structural and compositional analyses conducted by x-ray diffraction and energy dispersive x-ray spectrum reveal that the samples mainly contain the perovskite phase of Sm1-xSrxNiO3with small amount of NiO impurities. Magnetization and resistivity measurements indicate that the parent phase SmNiO3undergoes a paramagnetic-antiferromagnetic transition at about 224 K on a global insulating background. In contrast, the Sr-doped sample Sm0.8Sr0.2NiO3shows a metallic behavior from 300 K down to about 12 K, while below 12 K the resistivity exhibits a slight logarithmic increase. Meanwhile, from the magnetization curves, we can see that a possible spin-glass state occurs below 12 K in Sm0.8Sr0.2NiO3. Using a soft chemical reduction method, we also obtain the infinite-layer phase Sm0.8Sr0.2NiO2with square NiO2planes. The compound shows an insulating behavior which can be described by the three-dimensional variable-range-hopping model. And superconductivity is still absent in the polycrystalline Sm0.8Sr0.2NiO2.Entities:
Keywords: high-pressure synthesis; magnetic and transport properties; nickelates
Year: 2021 PMID: 33902020 DOI: 10.1088/1361-648X/abfb90
Source DB: PubMed Journal: J Phys Condens Matter ISSN: 0953-8984 Impact factor: 2.333