A series of photomagnetic coordination
polymer core–shell
heterostructures, based on the light-switchable Prussian blue analogue
Rb
a
Co
b
[Fe(CN)6]
c
·mH2O (RbCoFe-PBA) as the core and the ferromagnetic K
j
Ni
k
[Cr(CN)6]
l
·nH2O (KNiCr-PBA) as the shell, was studied using powder X-ray diffraction,
down to 100 K, and magnetometry, down to 2 K, to investigate the influence
of the shell thickness on light-induced magnetization changes and
gain insight into the mechanism. The core material is known to undergo
a charge-transfer-induced spin transition (CTIST), and synchrotron
powder diffraction was used to monitor structural changes in both
the core and the shell associated with the thermally and optically
induced CTIST of the core. Significant lattice contraction in the
RbCoFe-PBA core upon cooling through the high-spin to the low-spin
state transition near ∼260 K induces strain on the KNiCr-PBA
shells. This lattice strain in the shell can be relieved either by
thermal cycling back to high temperature or by using light to access
the metastable high-spin state of the core at low temperature. The
different extents of strain in the KNiCr-PBA shell are reflected in
low-temperature, low-field magnetization versus temperature data in
the light and dark states. A broader magnetic transition at T
c ≈ 70 K in the dark state relative to
the light state reflects the greater dispersion of nearest-neighbor
contacts and exchange energies induced by the structural distortions
of the strained state. Analyses for different shell thicknesses, coupled
with high-field magnetization data, support a mechanism whereby the
light-induced magnetization changes in the KNiCr-PBA shell are due
to realignment of the local magnetic anisotropy as a result of the
structural changes in the shell associated with the optical CTIST
of the core. Through magnetization and structural analyses, the depth
to which the properties of the shell are influenced by the core–shell
architecture was estimated to be between 40 and 50 nm.