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Probing the origin of the giant magnetic anisotropy in trigonal bipyramidal Ni(ii) under high pressure† †Electronic supplementary information (ESI) available. CCDC 1579468–1579472. For ESI and crystallographic data in CIF or other electronic format see DOI: 10.1039/c7sc04460g

Authors :
Craig, Gavin A.
Sarkar, Arup
Woodall, Christopher H.
Hay, Moya A.
Marriott, Katie E. R.
Kamenev, Konstantin V.
Moggach, Stephen A.
Brechin, Euan K.
Parsons, Simon
Rajaraman, Gopalan
Murrie, Mark
Source :
Chemical Science
Publication Year :
2017
Publisher :
Royal Society of Chemistry, 2017.

Abstract

The synergistic combination of high pressure techniques with ab initio methods creates a powerful tool to understand giant magnetic anisotropy.<br />Understanding and controlling magnetic anisotropy at the level of a single metal ion is vital if the miniaturisation of data storage is to continue to evolve into transformative technologies. Magnetic anisotropy is essential for a molecule-based magnetic memory as it pins the magnetic moment of a metal ion along the easy axis. Devices will require deposition of magnetic molecules on surfaces, where changes in molecular structure can significantly alter magnetic properties. Furthermore, if we are to use coordination complexes with high magnetic anisotropy as building blocks for larger systems we need to know how magnetic anisotropy is affected by structural distortions. Here we study a trigonal bipyramidal nickel(ii) complex where a giant magnetic anisotropy of several hundred wavenumbers can be engineered. By using high pressure, we show how the magnetic anisotropy is strongly influenced by small structural distortions. Using a combination of high pressure X-ray diffraction, ab initio methods and high pressure magnetic measurements, we find that hydrostatic pressure lowers both the trigonal symmetry and axial anisotropy, while increasing the rhombic anisotropy. The ligand–metal–ligand angles in the equatorial plane are found to play a crucial role in tuning the energy separation between the dx2–y2 and dxy orbitals, which is the determining factor that controls the magnitude of the axial anisotropy. These results demonstrate that the combination of high pressure techniques with ab initio studies is a powerful tool that gives a unique insight into the design of systems that show giant magnetic anisotropy.

Details

Language :
English
ISSN :
20416539 and 20416520
Volume :
9
Issue :
6
Database :
OpenAIRE
Journal :
Chemical Science
Accession number :
edsair.pmid..........9fd3750f3f945ca268b90f1391ec14d5