This is a page describing data taken during an experiment at the ISIS Neutron and Muon Source. Information about the ISIS Neutron and Muon Source can be found at https://www.isis.stfc.ac.uk.
The magnetic structure of FeSe superconductor under pressure
Abstract: Magnetism is in general a key ingredient for high-Tc superconductors because the corresponding spin fluctuations could mediate electronic Cooper pairing. FeSe with a nematic order of 90 K exhibits Neel and stripe spin fluctuations with no magnetic phase transition at ambient pressure. The Tc of FeSe can be dramatically enhanced by hydrostatic pressure, accompanied by the development of a magnetic order above ~ 1.2 GPa. Determining the pressure-induced magnetic structure is thus of particular interest, while neutron diffraction measurements are still lacking due to techinal difficulties. Recent muSR study revealed the static magnetism in Fe(Se,S) at lower pressure of 0.6 GPa, we therefore propose a neutron powder diffraction experiment in the helium pressure cell. Our results will be crucial for elucidating the magnetism and its interplay with nematicity and superconductivity in FeSe.
Public release date: 08 August 2027
Principal Investigator: Dr Hongliang Wo
Experimenter: Mr Jun Zhao
Experimenter: Miss Hao Zhang
Experimenter: Miss Yimeng Gu
Local Contact: Dr Fabio Orlandi
Experimenter: Dr Yinghao Zhu
DOI: 10.5286/ISIS.E.RB2220344-3
Parent DOI: 10.5286/ISIS.E.RB2220344
ISIS Experiment Number: RB2220344
Part Number: 3
This dataset is NOT yet publicly available.
The release date is: 08 August 2027
Date of Experiment: 01 August 2024
Publisher: STFC ISIS Neutron and Muon Source
Data format: RAW/Nexus
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Data Citation
The recommended format for citing this dataset in a research
publication is as:
[author], [date], [title], [publisher],
[doi]
For Example:
Dr Hongliang Wo et al; (2024): The magnetic structure of FeSe superconductor under pressure, STFC ISIS Neutron and Muon Source, https://doi.org/10.5286/ISIS.E.RB2220344-3
Data is released under the CC-BY-4.0 license.