Helical magnetic state in the vicinity of the pressure-induced superconducting phase in MnP

Sachith E. Dissanayake, Masaaki Matsuda, Kazuyoshi Yoshimi, Shusuke Kasamatsu, Feng Ye, Songxue Chi, William Steinhardt, Gilberto Fabbris, Sara Haravifard, Jinguang Cheng, Jiaqiang Yan, Jun Gouchi, Yoshiya Uwatoko

Research output: Contribution to journalArticlepeer-review

Abstract

MnP is a metal that shows successive magnetic transitions from paramagnetic to ferromagnetic and helical magnetic phases at ambient pressure with decreasing temperature. With applied pressure, the magnetic transition temperatures decrease and superconductivity appears around 8 GPa where the magnetic order is fully suppressed and the quantum critical behavior is observed. These results suggest that MnP is an unconventional superconductor in which magnetic fluctuations may be relevant to the superconducting pairing mechanism. In order to elucidate the magnetic ground state adjacent to the superconducting phase first discovered in Mn-based materials, high-pressure neutron diffraction measurements have been performed in hydrostatic pressure up to 7.5 GPa. The helical magnetic structure with the propagation vector along the b axis, reported previously at 3.8 GPa, was found to be robust up to 7.5 GPa. First-principles and classical Monte Carlo calculations have also been performed to understand how the pressure-driven magnetic phase transitions are coupled with change of the exchange interactions. The calculations, which qualitatively reproduce the magnetic structures as a function of pressure, suggest that the exchange interactions change drastically with applied pressure and the further-neighbor interactions become more influential at high pressures. Combining the experimental and theoretical results, we describe the detail of exchange interactions in the vicinity of the superconducting phase, which is critical to understand the pairing mechanism of the unconventional superconductivity in MnP.

Original languageEnglish
Article number043026
JournalPhysical Review Research
Volume5
Issue number4
DOIs
StatePublished - Oct 2023

Funding

We would like to thank Dr. S. Yano for stimulating discussions. This research used resources at the High Flux Isotope Reactor, a DOE Office of Science User Facility operated by the Oak Ridge National Laboratory. This work was partially supported by MEXT, the Grant-in-Aid for Scientific Research Grant No. 19H00648. This work was supported by JSPS KAKENHI Grant No. 21H01041. This research used resources of the Advanced Photon Source, a U.S. Department of Energy (DOE) Office of Science user facility at Argonne National Laboratory and is based on research supported by the U.S. DOE Office of Science-Basic Energy Sciences, under Contract No. DE-AC02-06CH11357. S.H. acknowledges support provided by funding from the William M. Fairbank Chair in Physics and from the Fritz London Fellowship at Duke University. J.G.C. is supported by the National Natural Science Foundation of China (Grants No. 12025408 and No. 11921004). J.Q.Y. acknowledges the support by the U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division. A part of the computation in this work has been done using the facilities of the Supercomputer Center, the Institute for Solid State Physics, the University of Tokyo.

FundersFunder number
U.S. DOE Office of Science-Basic Energy SciencesDE-AC02-06CH11357
U.S. Department of Energy
Office of Science
Basic Energy Sciences
Duke University
Division of Materials Sciences and Engineering
Japan Society for the Promotion of Science21H01041
Ministry of Education, Culture, Sports, Science and Technology19H00648
National Natural Science Foundation of China12025408, 11921004

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