Effect of maghemization on the magnetic properties of pseudo-single-domain magnetite particles

Thursday, 17 December 2015
Poster Hall (Moscone South)
Trevor Almeida1, Adrian R Muxworthy2, Takeshi Kasama3, Wyn Williams4, Christian Damsgaard3, Cathrine Frandsen3, Timothy J Pennycook5 and Rafal Dunin-Borkowski6, (1)Imperial College London, London, United Kingdom, (2)Imperial College London, Earth Science and Engineering, London, United Kingdom, (3)Technical University of Denmark, Kongens Lyngby, Denmark, (4)University of Edinburgh, Edinburgh, United Kingdom, (5)University of Vienna, Vienna, Austria, (6)Forschungszentrum Julich GmbH, Julich, Germany
During formation, magnetic minerals record the direction and intensity of the Earth’s magnetic field. Paleomagnetists use this information to investigate, for example, past tectonic plate motion and geodynamo evolution. However, subsequent to formation the constituent magnetic minerals are commonly exposed to a range of weathering conditions and environments. One of the most common weathering processes is maghemization, which is the oxidation of magnetite (Fe3O4) at ambient temperatures, i.e., the slow oxidation of Fe3O4 to maghemite (γ-Fe2O3), and is known to alter the original remanent magnetization.

Of the constituent magnetic minerals, particles in the single domain (SD) grain size range (< 100 nm) are regarded as ideal paleomagnetic recorders because of their strong remanence and high magnetic stability, with potential relaxation times greater than that of the age of the Universe. However, magnetic signals from rocks are often dominated by small grains with non-uniform magnetization that exhibit magnetic recording fidelities similar to those of SD grains (termed pseudo-SD (PSD)).

In this context, the effect of maghemization on the magnetic properties of Fe3O4 grains in the PSD size range is investigated as a function of annealing temperature. X-ray diffraction and transmission electron microscopy confirms the precursor grains as Fe3O4 ranging from ~ 150 nm to ~ 250 nm in diameter, whilst Mössbauer spectrometry suggests the grains are initially near-stoichiometric. The Fe3O4 grains are heated to increasing reaction temperatures of 120 – 220 ºC to investigate their oxidation to γ-Fe2O3. High-angle annular dark field imaging and localized electron energy-loss spectroscopy reveals slightly oxidized Fe3O4 grains, heated to 140 ºC, exhibit higher oxygen content at the surface. Off-axis electron holography allows for construction of magnetic induction maps of individual Fe3O4 and γ-Fe2O3 grains, revealing their PSD (vortex) nature, which is supported by magnetic hysteresis measurements, including first-order reversal curve analysis. The coercivity of the grains is shown to increase with reaction temperature up to 180 ºC, but subsequently decreases after heating above 200 ºC; this magnetic behavior is attributed to the growth of a γ-Fe2O3 shell with magnetic properties distinct from the Fe3O4 core.