Presentation Information
[PC8-05]Magnetic Order in S-substituted FeSe1-xSx Thin Films Grown on LaAlO3 Substrates
*Kazuki Miwa1, Yuma Kawai1, Fuyuki Nabeshima2, Andreas Suter3, Zaher Salman3, Thomas Prokscha3, Atsutaka Maeda2, Tadashi Adachi1 (1. Sophia Univ. (Japan), 2. University of Tokyo (Japan), 3. PSI Center for Neutron and Muon Sciences (Switzerland))
Keywords:
Iron-chalcogenide superconductor,FeSe1-xSx,Thin film,Low-energy muon
Iron-chalcogenide superconductor FeSe does not exhibit a magnetic order but a nematic order at ambient pressure, whereas a magnetic order is induced by hydrostatic pressure [1]. In S-substituted FeSe1-xSx in which the nematic transition temperature decreases monotonically with increasing x, it has been suggested that spin fluctuations develop around x = 0.1 [2]. In our former muon spin relaxation (muSR) measurements on FeSe1-xSx thin films, it was observed that a short-range magnetic order was formed at low temperatures for x = 0.3 and 0.4 [3]. Therefore, to investigate spin fluctuations in the low S-concentration regime where the nematic order is formed, we fabricated FeSe1-xSx thin films by pulsed laser deposition and performed muSR measurements using low-energy muons at PSI, Switzerland. For x = 0.1, muon spin precession was observed at low temperatures, indicating the formation of a long-range magnetic order. This is likely because enhanced spin fluctuations are stabilized into a magnetic order by lattice strain originating from the substrate. Figure1 shows the S-concentration dependence of the magnetic transition temperature Tm in FeSe1-xSx thin films. For x = 0, a magnetic transition occurs at 80 K, and Tm decreases with increasing x. However, Tm increases above x = 0.2. This suggests a change in the magnetic state around x = 0.2.
References
1) M. Bendele et al. Phys. Rev. Lett. Vol.104, p087003, 2010
2) P. Wiecki et al. Phys. Rev. B Vol.98, p020507(R), 2018
3) F. Nabeshima et al. Phys. Rev. B Vol.103, p184504, 2021
4) F. Nabeshima et al. J. Phys. Soc. Jpn. Vol.87, p073704, 2018
References
1) M. Bendele et al. Phys. Rev. Lett. Vol.104, p087003, 2010
2) P. Wiecki et al. Phys. Rev. B Vol.98, p020507(R), 2018
3) F. Nabeshima et al. Phys. Rev. B Vol.103, p184504, 2021
4) F. Nabeshima et al. J. Phys. Soc. Jpn. Vol.87, p073704, 2018
