We report resistivity measurements of the helimagnet CrAs under pressures. The helimagnetic transition with TN ∼ 265 K at ambient pressure is completely suppressed above a critical pressure of Pc ∼ 0.7 GPa, and superconductivity is observed at ∼ 2.2 K for zero resistance, which exists in a wide pressure range extending beyond 3 GPa. Both the upper critical field Hc2 and the coefficient A in the resistivity increase toward Pc, suggesting that the superconductivity of CrAs is mediated by electronic correlations enhanced in the vicinity of the helimagnetic phase.KEYWORDS: CrAs, superconductivity, helimagnet, pressure 3d electron systems can offer stages that induce intriguing superconductivity such as that realized in cuprates, Fe pnictides, and cobalt oxyhydrate. Superconducting (SC) mechanisms and symmetries are diverse depending on the material, and thus the discovery of superconductivity in a new system is crucial for the development of the field of research on superconductivity. In this paper, we report the discovery of a pressure-induced superconductivity of ∼ 2.2 K in the helimagnet CrAs through resistivity measurements. This is the first example of superconductivity in Cr-based magnetic systems. Very recently, W. Wu and coworkers have independently obtained similar results on the occurrence of superconductivity under high pressure in CrAs through resistivity and susceptibility measurements.
1CrAs has an orthorhombic MnP-type crystal structure with the space group of P nma and shows a firstorder magnetic transition at T N ∼ 265 K. Most research studies of the magnetic property of CrAs have been performed in the 1970s. The magnetic structure of CrAs is a double-helical one represented by a propagation vector of 0.354 · 2πc * and a magnetic moment of ∼ 1.7µ B /Cr that lies in the ab plane.2, 3 The magnetic transition is accompanied by a large magnetostriction of ∆b/b = +5.5%, ∆a/a = −0.3%, and ∆c/c = −0.9% below T N .4, 5 The crystal structure in the helimagnetic phase has been reported to belong to the same space group as the paramagnetic (PM) phase, 4, 5 although the magnetic structure is incommensurate.Single crystals of CrAs were prepared by the Sn-flux method similar to that described in Ref. 6. The resistivity measurements under pressure were performed using samples #1 and #2, which are from different batches. Sample #1 was obtained accidentally from a mixture of Sr:Cr:As:Sn=1:2:2:20, which was prepared with the aim of producing SrCr 2 As 2 ; however, CrAs was obtained as the main product. For sample #2, a mixture of Cr:As:Sn=1:1:10 was prepared. For both samples, the mixture was placed in an alumina crucible and sealed in an evacuated quartz ampoule. The ampoule was heated slowly up to 1050• C, and held there for 2 h, and then cooled to 600