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Magnetic nanoparticles

Published online by Cambridge University Press:  13 November 2013

Sara A. Majetich*
Affiliation:
Carnegie Mellon University, USA; sara@cmu.edu
Tianlong Wen
Affiliation:
Carnegie Mellon University, USA; halong@andrew.cmu.edu
O. Thompson Mefford*
Affiliation:
Clemson University, USA; mefford@clemson.edu

Abstract

Monodomain magnetic nanoparticles, due to their size, demonstrate physical properties not seen in the bulk materials, such as size-dependent magnetization reversal fields. They can be also made into a magnetic suspension or ferrofluid. There is thus growing interest in the application of these materials to ferrofluids, spintronics, directed assembly, as well as for imaging and therapeutic applications. In this article, we provide an overview of these materials, discuss the fundamental physical properties, describe several routes for the “bottom-up” generation of these materials, and identify major challenges for the future of these fields. The articles in this issue describe various aspects of the characterization and application of magnetic nanoparticles.

Information

Type
Introduction
Copyright
Copyright © Materials Research Society 2013 
Figure 0

Figure 1. (a) A spherical particle has a net magnetic moment with magnitude μ = MsV, where V is the particle volume and Ms is the saturation magnetization, due to the internal alignment of atomic spins. In the case of a perfect sphere, it behaves as a point dipole. (b) The equilibrium direction of the single particle magnetization depends on the external magnetic field H and also on its magnetocrystalline anisotropy easy axis. Note: M is the magnetization, φ is the angle between the magnetization and the easy axis, and θ is the angle between the easy axis and the applied field.

Figure 1

Figure 2. The energy (E) of a magnetic nanoparticle as a function of the magnetic moment orientation relative to the external field direction (H). Because of the magnetocrystalline anisotropy, there will be an energy barrier between “spin up” and “spin down” states (black circles with green arrows), even for an isolated particle. When H = 0, $\Delta E$ = KV. When particles interact, there is still an energy barrier, but its magnitude changes. When the thermal energy is high, relative to the energy barrier height, equilibration is rapid. Note: K is the anisotropy; V is the particle volume, Ms is the saturation magnetization, kB is the Boltzmann constant, Thigh is a higher temperature, and Tlow is a lower temperature.

Figure 2

Figure 3. Magnetization (M) as a function of the applied magnetic field (H). (a) Superparamagnetic particles have zero coercivity. This occurs either when the thermal energy is high, relative to the energy barrier, or when the measurement time (tmeas) is long so that the sample reaches thermal equilibrium. (b) If equilibrium is not reached within the measurement time, then hysteresis will be observed. Note: kB is the Boltzmann constant, Thigh is a higher temperature, and Tlow is a lower temperature.

Figure 3

Figure 4. Threshold diameters for superparamagnetism (dsp) and maximum monodomain (dcr) size for spherical nanoparticles, based on bulk material parameters. (Data taken from References 21 and 40.) The measurement time is assumed to be ∼100 s. The size of the particles has a significant impact on the properties of these materials and should be carefully controlled to meet the needs of a given application.

Figure 4

Figure 5. Comparison of blocking temperature (Tb) and Curie temperature (TC). Below the blocking temperature, there is some net alignment of the particle spins, while above it, the spins are in random directions. Below the Curie temperature, there is some net alignment of the atomic spins within a particle, while above it, they are randomized.