Pressure-Induced Magnetic Switching and Linkage Isomerism in K0.4Fe4[Cr(CN)6]2.8 · 16H2O: X-ray Absorption and Magnetic Circular Dichroism Studies
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American Chemical Society
Abstract
The effect of applied pressure on the magnetic properties of the Prussian blue analogue
K0.4Fe4[Cr(CN)6]2.8·16H2O (1) has been analyzed by dc and ac magnetic susceptibility
measurements. Under ambient conditions, 1 orders ferromagnetically at a critical temperature (TC) of
18.5 K. Under application of pressure in the 0−1200 MPa range, the magnetization of the material
decreases and its critical temperature shifts to lower temperatures, reaching TC = 7.5 K at 1200 MPa.
Pressure-dependent Raman and Mössbauer spectroscopy measurements show that this striking behavior
is due to the isomerization of some CrIII−C≡N−FeII linkages to the CrIII−N≡C−FeII form. As a result,
the ligand field around the iron(II) centers increases, and the diamagnetic low-spin state is populated.
As the number of diamagnetic centers in the cubic lattice increases, the net magnetization and critical
temperature of the material decrease considerably. The phenomenon is reversible: releasing the pressure
restores the magnetic properties of the original material. However, we have found that under more
severe pressure conditions, a metastable sample containing 22% CrIII−N≡C−FeII linkages can be
obtained. X-ray absorption spectroscopy and
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This is the Accepted Manuscript of the following article: Coronado, E., Gimenez López, M.C., Korzeniak, T., Levchenko, G., Romero, F.M., Segura, A., García Baonza, V., Cezar, J.C., Groot, F., Milner, A., Paz Pasternak, M., Journal of the American Chemical Society, 2008, DOI:10.1021/ja8047046 CCC
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Eugenio Coronado, M. Carmen Giménez-López, Tomasz Korzeniak, Georgiy Levchenko, Francisco M. Romero, Alfredo Segura, Valentín García-Baonza, Julio C. Cezar, Frank M. F. de Groot, Alla Milner, and Moshe Paz-Pasternak Journal of the American Chemical Society 2008 130 (46), 15519-15532 DOI: 10.1021/ja8047046
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https://doi.org/10.1021/ja8047046Sponsors
We acknowledge financial support from the European Union (NoE Magmanet), the Ministerio de Educación y Ciencia (Projects MAT2004-03849, MAT2007-61584, and CONSOLIDER-INGENIO in Molecular Nanoscience), and Generalitat Valenciana.
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