ISIS Neutron and Muon Source Data Journal

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.


Magnetic Coupling and Chiral Structures in Rare Earth Metal Molecular Systems

Abstract: We have observed that the addition of C60 molecules on the surface of rare earth (RE) metal thin films alters magnetic transitions into collinear and non-collinear states. The molecules themselves may become weakly spin polarised. Here, we aim to explore the as yet unexplained origin of this effect and its possible applications. Critically for our systems, PNR is a unique technique in that it allows us to study the magnetic profile of samples composed of elements with very different atomic weights and properties, such as carbon and gadolinium, and without damaging the highly sensitive interfaces. Comparing measurements at the second order transition into the ferromagnetic state between Y/Gd and Y/Gd/C60 samples we will be able to determine the local magnetic moments and the spatial profile of the magnetic interaction.

Principal Investigator: Dr Oscar Cespedes
Experimenter: Dr Tim Moorsom
Experimenter: Mr Alistair Walton
Local Contact: Dr Andrew Caruana
Experimenter: Professor Bryan Hickey
Experimenter: Dr Christy Kinane
Experimenter: Mr Timothy Moorsom

DOI: 10.5286/ISIS.E.RB1820618

ISIS Experiment Number: RB1820618

Part DOI Instrument Public release date Download Link
10.5286/ISIS.E.98020590 POLREF 22 October 2021 Download

Publisher: STFC ISIS Neutron and Muon Source

Data format: RAW/Nexus
Select the data format above to find out more about it.

Data Citation

The recommended format for citing this dataset in a research publication is as:
[author], [date], [title], [publisher], [doi]

For Example:
Dr Oscar Cespedes et al; (2018): Magnetic Coupling and Chiral Structures in Rare Earth Metal Molecular Systems, STFC ISIS Neutron and Muon Source, https://doi.org/10.5286/ISIS.E.RB1820618

Data is released under the CC-BY-4.0 license.



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